Difference between revisions of "ISEST Presentations"
(→Tuesday, June 18) |
|||
| (5 intermediate revisions by one other user not shown) | |||
| Line 1: | Line 1: | ||
| − | This page | + | This page contains presentations given at the 2013 ISEST Workshop. The 2013 ISEST Workshop was held in June 17-20, 2013, Hvar, Croatia. [http://spaceweather.gmu.edu/meetings/ISEST/ Here is the link to the meeting website] |
=Monday, June 17= | =Monday, June 17= | ||
| Line 10: | Line 10: | ||
Could the Collision of CMEs in the Heliosphere be Super-Elastic-Fang Shen <br> | Could the Collision of CMEs in the Heliosphere be Super-Elastic-Fang Shen <br> | ||
[http://solar.gmu.edu/wiki/presentations/ISEST2013_ruffenach.pdf Statistical Analysis of Magnetic Cloud Erosion By Magnetic Reconnection]-Alexis Ruffenach <br> | [http://solar.gmu.edu/wiki/presentations/ISEST2013_ruffenach.pdf Statistical Analysis of Magnetic Cloud Erosion By Magnetic Reconnection]-Alexis Ruffenach <br> | ||
| − | Solar Eruptions Observed by the Atmospheric Imaging Assembly-Ewa Chmielewska <br> | + | [http://solar.gmu.edu/wiki/presentations/chmielewska/ Solar Eruptions Observed by the Atmospheric Imaging Assembly]-Ewa Chmielewska <br> |
ARTEMIS II: A Second Generation Catalog of LASCO Coronoal Mass Ejections-Philippe Lamy <br> | ARTEMIS II: A Second Generation Catalog of LASCO Coronoal Mass Ejections-Philippe Lamy <br> | ||
[http://solar.gmu.edu/wiki/presentations/ISEST_workshop_nandita.pdf Estimating the Arrival Time of Earth-Directed CMEs at In Situ Spacecraft Using COR and HI Observations from STEREO]-Nandita Srivastava <br> | [http://solar.gmu.edu/wiki/presentations/ISEST_workshop_nandita.pdf Estimating the Arrival Time of Earth-Directed CMEs at In Situ Spacecraft Using COR and HI Observations from STEREO]-Nandita Srivastava <br> | ||
| Line 20: | Line 20: | ||
[http://solar.gmu.edu/wiki/presentations/Valbona_ISEST2013Croatia.pptx 3-D Geometry, Profiles of B(1 AU) and CME Arrival Time]-Valbona Kunkel <br> | [http://solar.gmu.edu/wiki/presentations/Valbona_ISEST2013Croatia.pptx 3-D Geometry, Profiles of B(1 AU) and CME Arrival Time]-Valbona Kunkel <br> | ||
[http://solar.gmu.edu/wiki/presentations/ISEST%20workshop%20-%20COMESEP%20vs2.pdf Alert System for Arrival and Geo-Effectiveness of CMEs]-Andy Devos <br> | [http://solar.gmu.edu/wiki/presentations/ISEST%20workshop%20-%20COMESEP%20vs2.pdf Alert System for Arrival and Geo-Effectiveness of CMEs]-Andy Devos <br> | ||
| − | Magnetic Storm Generation by Various Types of Solar wind; event catalog, modeling and prediction-Nadia Nikolaeva | + | [http://solar.gmu.edu/wiki/presentations/Nikolaeva-ISEST-2013.ppt Magnetic Storm Generation by Various Types of Solar wind; event catalog, modeling and prediction]-Nadia Nikolaeva |
=Wednesday, June 19= | =Wednesday, June 19= | ||
| Line 26: | Line 26: | ||
[http://solar.gmu.edu/wiki/presentations/hess/ Comparison of the Drag Model, ENLIL Model and Observations for the July 12, 2012 CME+Shock Event]-Phillip Hess <br> | [http://solar.gmu.edu/wiki/presentations/hess/ Comparison of the Drag Model, ENLIL Model and Observations for the July 12, 2012 CME+Shock Event]-Phillip Hess <br> | ||
[http://solar.gmu.edu/wiki/presentations/Lavraud_MEGACME_ISEST_June_2013.pdf The Mega CME of July 2012]-Benoit Lavraud <br> | [http://solar.gmu.edu/wiki/presentations/Lavraud_MEGACME_ISEST_June_2013.pdf The Mega CME of July 2012]-Benoit Lavraud <br> | ||
| + | |||
| + | =Working Group Summaries= | ||
| + | [http://solar.gmu.edu/wiki/presentations/moestl_2013_hvar_WG1_session_summary.pdf Working Group 1] <br> | ||
| + | [http://solar.gmu.edu/wiki/presentations/WG2_summary.pdf Working Group 2] <br> | ||
| + | [http://solar.gmu.edu/wiki/presentations/WG3_summary.pdf Working Group 3] <br> | ||
| + | [http://solar.gmu.edu/wiki/presentations/WG4_Summary_20130620.pdf Working Group 4] <br> | ||
Latest revision as of 10:49, 15 May 2015
This page contains presentations given at the 2013 ISEST Workshop. The 2013 ISEST Workshop was held in June 17-20, 2013, Hvar, Croatia. Here is the link to the meeting website
Monday, June 17
Introduction to SCOSTEP/ISEST-Jie Zhang
Instroduction to SCOSTEP/MiniMax-Manuela Temmer
Drag Based Model for ICME Propagation-Bojan Vrsnak
Eruptive Flux Rope Model for ICME Evolution-Jie Zhang
Connecting Remote and In Situ Observations of 22 Coronal Ejections from the Sun to 1 AU-Christian Moestl
Helio Weather Project and Numerical Simulation of Multi-CME Events-Dusan Odstrcil
Could the Collision of CMEs in the Heliosphere be Super-Elastic-Fang Shen
Statistical Analysis of Magnetic Cloud Erosion By Magnetic Reconnection-Alexis Ruffenach
Solar Eruptions Observed by the Atmospheric Imaging Assembly-Ewa Chmielewska
ARTEMIS II: A Second Generation Catalog of LASCO Coronoal Mass Ejections-Philippe Lamy
Estimating the Arrival Time of Earth-Directed CMEs at In Situ Spacecraft Using COR and HI Observations from STEREO-Nandita Srivastava
Interaction Process of the CME-CME Event from February 14-15, 2011-Manuela Temmer
Deflected Propagation of the 2008 September 13 CME in the Heliosphere-Chenglong Shen
Do We Need to Correct Projection Effect for halo CMEs in Terms of Space Weather Forecasting?-Yuming Wang
Tuesday, June 18
3-D Geometry, Profiles of B(1 AU) and CME Arrival Time-Valbona Kunkel
Alert System for Arrival and Geo-Effectiveness of CMEs-Andy Devos
Magnetic Storm Generation by Various Types of Solar wind; event catalog, modeling and prediction-Nadia Nikolaeva
Wednesday, June 19
Comparison of the Drag Model, ENLIL Model and Observations for the July 12, 2012 CME+Shock Event-Phillip Hess
The Mega CME of July 2012-Benoit Lavraud
Working Group Summaries
Working Group 1
Working Group 2
Working Group 3
Working Group 4
