http://solar.gmu.edu/heliophysics/api.php?action=feedcontributions&feedformat=atom&user=Dodstrci heliophysics - User contributions [en] 2026-07-21T22:04:06Z User contributions MediaWiki 1.31.0 http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1312 Working Group 3 2013-06-12T17:34:14Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> <br /> {| class=&quot;wikitable&quot;<br /> | [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|204px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20100729/]<br /> |}<br /> <br /> <br /> * February 2011<br /> <br /> <br /> * Early March 2012<br /> <br /> {| class=&quot;wikitable&quot;<br /> | [[File:2012-03-01.tim1-coho3-vel-1.7.0144.gif|255px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20120301/]<br /> |}<br /> <br /> <br /> * July 2012<br /> <br /> {| class=&quot;wikitable&quot;<br /> | [[File:2012-07-17.tim1-coho3-vel-1.7.0168.gif|255px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20120717/]<br /> |}<br /> <br /> {| class=&quot;wikitable&quot;<br /> | figure<br /> | COIN-TVD model<br /> |}<br /> <br /> &lt;br&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1311 Working Group 3 2013-06-12T17:28:59Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> <br /> {| class=&quot;wikitable&quot;<br /> | [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|204px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20100729/]<br /> |}<br /> {| class=&quot;wikitable&quot;<br /> | [[File:anim.gif|204px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20100729/]<br /> |}<br /> <br /> <br /> * February 2011<br /> <br /> <br /> * Early March 2012<br /> <br /> {| class=&quot;wikitable&quot;<br /> | [[File:2012-03-01.tim1-coho3-vel-1.7.0144.gif|255px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20120301/]<br /> |}<br /> <br /> <br /> * July 2012<br /> <br /> {| class=&quot;wikitable&quot;<br /> | [[File:2012-07-17.tim1-coho3-vel-1.7.0168.gif|255px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20120717/]<br /> |}<br /> <br /> {| class=&quot;wikitable&quot;<br /> | figure<br /> | COIN-TVD model<br /> |}<br /> <br /> &lt;br&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1310 Working Group 3 2013-06-12T17:23:44Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> <br /> {| class=&quot;wikitable&quot;<br /> | [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|204px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20100729/]<br /> |}<br /> <br /> <br /> * February 2011<br /> <br /> <br /> * Early March 2012<br /> <br /> {| class=&quot;wikitable&quot;<br /> | [[File:2012-03-01.tim1-coho3-vel-1.7.0144.gif|255px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20120301/]<br /> |}<br /> <br /> <br /> * July 2012<br /> <br /> {| class=&quot;wikitable&quot;<br /> | [[File:2012-07-17.tim1-coho3-vel-1.7.0168.gif|255px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20120717/]<br /> |}<br /> <br /> {| class=&quot;wikitable&quot;<br /> | figure<br /> | COIN-TVD model<br /> |}<br /> <br /> &lt;br&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1309 Working Group 3 2013-06-12T17:19:08Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> <br /> {| class=&quot;wikitable&quot;<br /> | [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|255px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20100729/]<br /> |}<br /> <br /> <br /> * February 2011<br /> <br /> <br /> * Early March 2012<br /> <br /> {| class=&quot;wikitable&quot;<br /> | [[File:2012-03-01.tim1-coho3-vel-1.7.0144.gif|255px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20120301/]<br /> |}<br /> <br /> <br /> * July 2012<br /> <br /> {| class=&quot;wikitable&quot;<br /> | [[File:2012-07-17.tim1-coho3-vel-1.7.0168.gif|255px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20120717/]<br /> |}<br /> <br /> {| class=&quot;wikitable&quot;<br /> | figure<br /> | COIN-TVD model<br /> |}<br /> <br /> &lt;br&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1308 Working Group 3 2013-06-12T17:17:01Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> {| class=&quot;wikitable&quot;<br /> | [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|255px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20100729/]<br /> |}<br /> <br /> <br /> * February 2011<br /> <br /> <br /> * Early March 2012<br /> {| class=&quot;wikitable&quot;<br /> | [[File:2012-03-01.tim1-coho3-vel-1.7.0144.gif|255px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20120301/]<br /> |}<br /> <br /> <br /> * July 2012<br /> {| class=&quot;wikitable&quot;<br /> | [[File:2012-07-17.tim1-coho3-vel-1.7.0168.gif|255px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20120717/]<br /> |}<br /> {| class=&quot;wikitable&quot;<br /> | figure<br /> | COIN-TVD model<br /> |}<br /> <br /> &lt;br&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1307 Working Group 3 2013-06-12T17:16:34Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> {| class=&quot;wikitable&quot;<br /> | [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|255px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20100729/]<br /> |}<br /> <br /> <br /> * February 2011<br /> <br /> <br /> * Early March 2012<br /> {| class=&quot;wikitable&quot;<br /> | [[File:2012-03-01.tim1-coho3-vel-1.7.0144.gif|255px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20120301/]<br /> |}<br /> <br /> <br /> * July 2012<br /> {| class=&quot;wikitable&quot;<br /> | [[File:2012-07-17.tim1-coho3-vel-1.7.0168.gif|255px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20120717/]<br /> |}<br /> {| class=&quot;wikitable&quot;<br /> | fig<br /> | COIN-TVD model<br /> |}<br /> <br /> &lt;br&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1306 Working Group 3 2013-06-12T15:37:48Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> ** [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|255px]] WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20100729/]<br /> {|<br /> | [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|255px]]<br /> | WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20100729/]<br /> |}<br /> <br /> <br /> * February 2011<br /> <br /> <br /> * Early March 2012<br /> ** [[File:2012-03-01.tim1-coho3-vel-1.7.0144.gif|255px]] WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20120301/]<br /> <br /> <br /> * July 2012<br /> ** [[File:2012-07-17.tim1-coho3-vel-1.7.0168.gif|255px]] WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20120717/]<br /> ** COIN-TVD model<br /> <br /> &lt;br&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1305 Working Group 3 2013-06-12T15:22:31Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> ** [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|255px]] WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20100729/]<br /> <br /> <br /> * February 2011<br /> <br /> <br /> * Early March 2012<br /> ** [[File:2012-03-01.tim1-coho3-vel-1.7.0144.gif|255px]] WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20120301/]<br /> <br /> <br /> * July 2012<br /> ** [[File:2012-07-17.tim1-coho3-vel-1.7.0168.gif|255px]] WSA-ENLIL-Cone run by HelioWeather. More data at [http://solar.gmu.edu/wiki/upload/Dodstrci/20120717/]<br /> ** COIN-TVD model<br /> <br /> &lt;br&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1226 Working Group 3 2013-06-10T14:52:09Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> ** [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|255px]] WSA-ENLIL-Cone run by HelioWeather<br /> <br /> <br /> * February 2011<br /> <br /> <br /> * Early March 2012<br /> ** [[File:2012-03-01.tim1-coho3-vel-1.7.0144.gif|255px]] WSA-ENLIL-Cone run by HelioWeather<br /> <br /> <br /> <br /> * July 2012<br /> ** [[File:2012-07-17.tim1-coho3-vel-1.7.0168.gif|255px]] WSA-ENLIL-Cone run by HelioWeather<br /> ** COIN-TVD model<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1225 Working Group 3 2013-06-10T14:47:09Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> ** [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|255px]] WSA-ENLIL-Cone run by HelioWeather<br /> <br /> <br /> * February 2011<br /> <br /> <br /> * Early March 2012<br /> ** [[File:2012-03-01.tim1-coho3-vel-1.7.0144.gif|255px]] WSA-ENLIL-Cone run by HelioWeather<br /> <br /> <br /> <br /> * July 2012<br /> ** [[File:2012-07-17.tim1-coho3-vel-1.7.0168.gif|255px]] WSA-ENLIL-Cone run by HelioWeather<br /> <br /> ** COIN-TVD model<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1224 Working Group 3 2013-06-10T14:42:51Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> ** [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|255px|<br /> WSA-ENLIL-Cone run by HelioWeather&lt;br/&gt;<br /> July 29 - August 13]]<br /> <br /> <br /> * February 2011<br /> <br /> <br /> * Early March 2012<br /> ** [[File:2012-03-01.tim1-coho3-vel-1.7.0144.gif|255px|caption]]<br /> WSA-ENLIL-Cone run by HelioWeather&lt;br/&gt;<br /> March 1 - March 21<br /> <br /> <br /> <br /> * July 2012<br /> ** [[File:2012-07-17.tim1-coho3-vel-1.7.0168.gif|255px]]<br /> WSA-ENLIL-Cone run by HelioWeather&lt;br/&gt;<br /> July 17 - July 31<br /> <br /> ** COIN-TVD model<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1223 Working Group 3 2013-06-10T14:40:44Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> ** [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|255px|caption]]<br /> WSA-ENLIL-Cone run by HelioWeather&lt;br/&gt;<br /> July 29 - August 13<br /> <br /> <br /> * February 2011<br /> <br /> <br /> * Early March 2012<br /> ** [[File:2012-03-01.tim1-coho3-vel-1.7.0144.gif|255px]]<br /> WSA-ENLIL-Cone run by HelioWeather&lt;br/&gt;<br /> March 1 - March 21<br /> <br /> <br /> <br /> * July 2012<br /> ** [[File:2012-07-17.tim1-coho3-vel-1.7.0168.gif|255px]]<br /> WSA-ENLIL-Cone run by HelioWeather&lt;br/&gt;<br /> July 17 - July 31<br /> <br /> ** COIN-TVD model<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=File:2012-07-17.tim1-coho3-vel-1.7.0168.gif&diff=1222 File:2012-07-17.tim1-coho3-vel-1.7.0168.gif 2013-06-10T14:29:53Z <p>Dodstrci: </p> <hr /> <div></div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1221 Working Group 3 2013-06-10T14:29:23Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|255px|caption]]<br /> <br /> <br /> * February 2011<br /> <br /> <br /> * Early March 2012<br /> **[[File:2012-03-01.tim1-coho3-vel-1.7.0144.gif|255px|WSA-ENLIL-Cone run by HelioWeather]]<br /> <br /> <br /> <br /> * July 2012<br /> ** [[File:2012-07-17.tim1-coho3-vel-1.7.0168.gif|255px|caption]] WSA-ENLIL-Cone run by HelioWeather<br /> <br /> ** COIN-TVD model<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=File:2012-03-01.tim1-coho3-vel-1.7.0144.gif&diff=1220 File:2012-03-01.tim1-coho3-vel-1.7.0144.gif 2013-06-10T14:25:43Z <p>Dodstrci: </p> <hr /> <div></div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1219 Working Group 3 2013-06-10T14:24:21Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|right|255px|caption]]<br /> <br /> <br /> * February 2011<br /> <br /> <br /> * Early March 2012<br /> **[[File:2012-03-01.tim1-coho3-vel-1.7.0144.gif|204px|WSA-ENLIL-Cone run by HelioWeather]]<br /> <br /> <br /> <br /> * July 2012<br /> ** [[File:2012-07-17.tim1-coho3-vel-1.7.0168.gif|204px|caption]]<br /> WSA-ENLIL-Cone run by HelioWeather<br /> <br /> ** COIN-TVD model<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1218 Working Group 3 2013-06-10T14:22:21Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|right|255px|caption]]<br /> <br /> <br /> * February 2011<br /> <br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> [[File:2012-03-01.tim1-coho3-vel-1.7.0144.gif|204px|caption]]<br /> <br /> <br /> <br /> * July 2012<br /> ** [[File:2012-07-17.tim1-coho3-vel-1.7.0168.gif|204px|caption]]<br /> WSA-ENLIL-Cone run by HelioWeather<br /> <br /> ** COIN-TVD model<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1217 Working Group 3 2013-06-10T14:16:15Z <p>Dodstrci: </p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> <br /> * February 2011<br /> <br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> <br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> ** COIN-TVD model<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=File:2010-07-29.tim1-coho3-vel-1.7.0120.gif&diff=1216 File:2010-07-29.tim1-coho3-vel-1.7.0120.gif 2013-06-10T14:03:58Z <p>Dodstrci: </p> <hr /> <div></div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1215 Working Group 3 2013-06-10T14:02:13Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> ** [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|left|255px]]<br /> WSA-ENLIL-Cone run by HelioWeather<br /> <br /> <br /> * February 2011<br /> <br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> [[File:2012-03-01.tim1-coho3-vrl-1.7.0144.gif|center|255px]]<br /> <br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> [[File:2012-07-17.tim1-coho3-vel-1.7.0168.gif|right|255px]]<br /> ** COIN-TVD model<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1214 Working Group 3 2013-06-10T13:54:53Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> [[File:2010-07-29.tim1-coho3-vel-1.7.0120.gif|left|255px]]<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> [[File:2012-03-01.tim1-coho3-vrl-1.7.0144.gif|center|255px]]<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather [[File:2012-07-17.tim1-coho3-vel-1.7.0168.gif|right|255px]]<br /> ** COIN-TVD model<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=File:WG3-HW-2012-jul.gif&diff=1213 File:WG3-HW-2012-jul.gif 2013-06-10T13:49:23Z <p>Dodstrci: </p> <hr /> <div></div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=File:WG3-HW-2012-mar.png&diff=1212 File:WG3-HW-2012-mar.png 2013-06-10T13:47:53Z <p>Dodstrci: </p> <hr /> <div></div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1211 Working Group 3 2013-06-10T13:45:58Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> [[File:wg3-hw-2010-aug.png|center|255px]]<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> [[File:wg3-hw-2012-mar.png|center|255px]]<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> [[File:wg3-hw-2012-jul.png|center|255px]]<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> ** COIN-TVD model<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=File:Wg3-hw-2010-aug.png&diff=1210 File:Wg3-hw-2010-aug.png 2013-06-10T13:43:45Z <p>Dodstrci: </p> <hr /> <div></div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1209 Working Group 3 2013-06-10T13:42:32Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1 Data) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> [[File:wg3-hw-2010-aug.png|center|255px]]<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> [[File:wg3-hw-2012-mar.png|center|204px]<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> [[File:wg3-hw-2012-jul.png|center|510px]<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> ** COIN-TVD model<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1207 Working Group 3 2013-06-07T11:07:51Z <p>Dodstrci: /* Forecasting the CME Arrival and Impact (with WG4) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4 Campaign Events) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1206 Working Group 3 2013-06-07T11:07:08Z <p>Dodstrci: /* Investigation of Mechanisms, Processes, and Forces (with WG2) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2 Theory) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1205 Working Group 3 2013-06-07T11:06:48Z <p>Dodstrci: /* Simulation of the ISEST Event Periods (with WG1) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1 Data) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1204 Working Group 3 2013-06-07T11:06:02Z <p>Dodstrci: /* Simulation of ISEST Event Periods (with WG1) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of the ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1203 Working Group 3 2013-06-07T10:54:32Z <p>Dodstrci: /* Scientific Questions */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1202 Working Group 3 2013-06-07T10:53:04Z <p>Dodstrci: /* Presentations at the Hvar Workshop 2013 */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and Interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1201 Working Group 3 2013-06-07T10:52:18Z <p>Dodstrci: /* Presentations at the Hvar Workshop 2013 */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and Interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> <br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> <br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> <br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> <br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1200 Working Group 3 2013-06-07T10:50:30Z <p>Dodstrci: /* Forecasting the CME Arrival and Impact (with WG4) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and Interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> <br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> <br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> <br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> <br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1199 Working Group 3 2013-06-07T10:50:21Z <p>Dodstrci: /* Investigation of Mechanisms, Processes, and Forces (with WG2) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and Interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> == Forecasting the CME Arrival and Impact (with WG4) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> <br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> <br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> <br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> <br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1198 Working Group 3 2013-06-07T10:50:12Z <p>Dodstrci: /* Simulation of ISEST Event Periods (with WG1) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and Interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> &lt;br/&gt;<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Forecasting the CME Arrival and Impact (with WG4) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> <br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> <br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> <br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> <br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1197 Working Group 3 2013-06-07T10:50:01Z <p>Dodstrci: /* Scientific Objective */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and Interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Forecasting the CME Arrival and Impact (with WG4) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> <br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> <br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> <br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> <br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1196 Working Group 3 2013-06-07T10:49:43Z <p>Dodstrci: /* Scientific Questions */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and Interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Forecasting the CME Arrival and Impact (with WG4) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> <br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> <br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> <br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> <br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1195 Working Group 3 2013-06-07T10:49:22Z <p>Dodstrci: /* Scientific Objective */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and Interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Forecasting the CME Arrival and Impact (with WG4) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> <br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> <br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> <br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> <br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1194 Working Group 3 2013-06-07T10:48:44Z <p>Dodstrci: /* Scientific Objective */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and Interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Forecasting the CME Arrival and Impact (with WG4) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> <br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> <br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> <br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> <br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1193 Working Group 3 2013-06-07T10:45:23Z <p>Dodstrci: Undo revision 1192 by Dodstrci (talk)</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> ==Scientific Questions==<br /> <br /> * Initiation<br /> <br /> * Propagation and Interaction<br /> <br /> * Impact<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Forecasting the CME Arrival and Impact (with WG4) ==<br /> <br /> * Arrival time<br /> <br /> * Geo-effectiveness<br /> <br /> * Energetic particles<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Presentations at the Hvar Workshop 2013 ==<br /> <br /> * &lt;u&gt;WG3 - 1st Choice:&lt;/u&gt;<br /> <br /> ** Dusan Odstrcil - Helio Weather Project and Numerical Simulation of Multi-CME Events (WG3)<br /> ** Fang Shen - Could the collision of CMEs in the heliosphere be super-elastic? (WG3)<br /> <br /> * &lt;u&gt;WG3 - 2nd Choice:&lt;/u&gt;<br /> <br /> ** Bojan Vrsnak - Drag Based Model for ICME Propagation<br /> <br /> ** Yuming Wang - Do we need to correct projection effect for halo CMEs in terms of space weather forecasting?<br /> <br /> ** Roberto Susino - Study of a geoeffective Coronal Mass Ejection with UV spectroscopy and stereoscopic data<br /> <br /> &lt;br/&gt;<br /> <br /> <br /> == Future Plan ==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1192 Working Group 3 2013-06-07T10:28:55Z <p>Dodstrci: /* Scientific Objective */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> &lt;br/&gt;<br /> &lt;br/&gt;<br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> ===''Initiation''===<br /> <br /> ===''Propagation and Interaction''===<br /> <br /> ===''Impact''===<br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> ==Forecasting the CME Arrival and Impact (with WG4)==<br /> <br /> * Arrival time<br /> * Geo-effectiveness<br /> * Energetic particles<br /> <br /> ==Future Plan==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1191 Working Group 3 2013-06-07T10:28:20Z <p>Dodstrci: /* Scientific Objective */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> &lt;br/&gt;<br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> ===''Initiation''===<br /> <br /> ===''Propagation and Interaction''===<br /> <br /> ===''Impact''===<br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> ==Forecasting the CME Arrival and Impact (with WG4)==<br /> <br /> * Arrival time<br /> * Geo-effectiveness<br /> * Energetic particles<br /> <br /> ==Future Plan==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1190 Working Group 3 2013-06-07T10:27:55Z <p>Dodstrci: /* Scientific Objective */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> ===''Initiation''===<br /> <br /> ===''Propagation and Interaction''===<br /> <br /> ===''Impact''===<br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> ==Forecasting the CME Arrival and Impact (with WG4)==<br /> <br /> * Arrival time<br /> * Geo-effectiveness<br /> * Energetic particles<br /> <br /> ==Future Plan==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1189 Working Group 3 2013-06-07T10:27:33Z <p>Dodstrci: /* Scientific Objective */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> &lt;br/&gt;<br /> &lt;br/&gt;<br /> <br /> ==Scientific Questions==<br /> <br /> ===''Initiation''===<br /> <br /> ===''Propagation and Interaction''===<br /> <br /> ===''Impact''===<br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> ==Forecasting the CME Arrival and Impact (with WG4)==<br /> <br /> * Arrival time<br /> * Geo-effectiveness<br /> * Energetic particles<br /> <br /> ==Future Plan==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1188 Working Group 3 2013-06-07T10:26:13Z <p>Dodstrci: /* Scientific Objective */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> ;<br /> ;<br /> ;<br /> <br /> ==Scientific Questions==<br /> <br /> ===''Initiation''===<br /> <br /> ===''Propagation and Interaction''===<br /> <br /> ===''Impact''===<br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> ==Forecasting the CME Arrival and Impact (with WG4)==<br /> <br /> * Arrival time<br /> * Geo-effectiveness<br /> * Energetic particles<br /> <br /> ==Future Plan==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1187 Working Group 3 2013-06-07T10:25:53Z <p>Dodstrci: /* Scientific Objective */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> ;<br /> <br /> ==Scientific Questions==<br /> <br /> ===''Initiation''===<br /> <br /> ===''Propagation and Interaction''===<br /> <br /> ===''Impact''===<br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> ==Forecasting the CME Arrival and Impact (with WG4)==<br /> <br /> * Arrival time<br /> * Geo-effectiveness<br /> * Energetic particles<br /> <br /> ==Future Plan==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1186 Working Group 3 2013-06-07T10:25:10Z <p>Dodstrci: /* Scientific Objective */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to ''&quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;''.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> ==Scientific Questions==<br /> <br /> ===''Initiation''===<br /> <br /> ===''Propagation and Interaction''===<br /> <br /> ===''Impact''===<br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> ==Forecasting the CME Arrival and Impact (with WG4)==<br /> <br /> * Arrival time<br /> * Geo-effectiveness<br /> * Energetic particles<br /> <br /> ==Future Plan==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1185 Working Group 3 2013-06-07T10:24:06Z <p>Dodstrci: /* Scientific Objective */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to &quot;''improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth''&quot;.<br /> <br /> &lt;u&gt;The WG3 (Simulation Group) will:&lt;/u&gt;<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> ==Scientific Questions==<br /> <br /> ===''Initiation''===<br /> <br /> ===''Propagation and Interaction''===<br /> <br /> ===''Impact''===<br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> ==Forecasting the CME Arrival and Impact (with WG4)==<br /> <br /> * Arrival time<br /> * Geo-effectiveness<br /> * Energetic particles<br /> <br /> ==Future Plan==<br /> TBD</div> Dodstrci http://solar.gmu.edu/heliophysics/index.php?title=Working_Group_3&diff=1184 Working Group 3 2013-06-07T10:19:23Z <p>Dodstrci: /* Simulation of Event Periods (with WG1) */</p> <hr /> <div>Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)<br /> <br /> == Scientific Objective ==<br /> <br /> The main ISEST objective is to &quot;improve the scientific understanding of the origin and propagation of solar transients, and develop the prediction capacity of these transients' arrival and potential impact on the Earth&quot;.<br /> <br /> '''The WG3 (Simulation Group) will:'''<br /> * Provide global context for all CME events investigated by the ISEST team<br /> * Investigate processes of the CME initiation, heliospheric propagation, and CMEs interaction<br /> * Develop tools to assist collaboration of numerical modelers, theoreticians, and observers<br /> <br /> ==Scientific Questions==<br /> <br /> ===''Initiation''===<br /> <br /> ===''Propagation and Interaction''===<br /> <br /> ===''Impact''===<br /> <br /> == Simulation of ISEST Event Periods (with WG1) ==<br /> <br /> * Late July to early August 2010<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * February 2011<br /> <br /> * Early March 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> * July 2012<br /> ** WSA-ENLIL-Cone run by HelioWeather<br /> <br /> == Investigation of Mechanisms, Processes, and Forces (with WG2) ==<br /> <br /> * Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?<br /> * How does energy transform during ICMEs propagation and interaction?<br /> * How much variable ambient conditions affect ICMEs?<br /> * How SEPs are accelerated by shocks and how they transport in heliosphere?<br /> <br /> ==Forecasting the CME Arrival and Impact (with WG4)==<br /> <br /> * Arrival time<br /> * Geo-effectiveness<br /> * Energetic particles<br /> <br /> ==Future Plan==<br /> TBD</div> Dodstrci