http://solar.gmu.edu/heliophysics/index.php?action=history&feed=atom&title=ISEST_2017_Workshop 2026-05-29T21:13:55Z Revision history for this page on the wiki MediaWiki 1.31.0 http://solar.gmu.edu/heliophysics/index.php?title=ISEST_2017_Workshop&diff=2979&oldid=prev 2018-09-18T02:35:29Z

<p>‎<span dir="auto"><span class="autocomment">Working Group Summary (September 22, 2017)</span></span></p> <table class="diff diff-contentalign-left" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="en"> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 02:35, 18 September 2018</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l53" >Line 53:</td> <td colspan="2" class="diff-lineno">Line 53:</td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Working Group Summary (September 22, 2017)==</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Working Group Summary (September 22, 2017)==</div></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG_Summary/ISEST_WG1_summary_2017_Zhang.pdf WG1 <del class="diffchange diffchange-inline">data </del>Group <del class="diffchange diffchange-inline">Report </del>---- by Jie Zhang<del class="diffchange diffchange-inline">*</del>] &lt;br&gt;</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG_Summary/ISEST_WG1_summary_2017_Zhang.pdf WG1 <ins class="diffchange diffchange-inline">Data </ins>Group <ins class="diffchange diffchange-inline">Summary </ins>---- by Jie Zhang] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>*WG2 <del class="diffchange diffchange-inline">Campaign Study </del>Group <del class="diffchange diffchange-inline">Report </del>&lt;br&gt;</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*<ins class="diffchange diffchange-inline">[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG_Summary/WG2_Summary20170922.pdf </ins>WG2 <ins class="diffchange diffchange-inline">Theory </ins>Group <ins class="diffchange diffchange-inline">Summary ---- by Yuming Wang] </ins>&lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>*WG3 <del class="diffchange diffchange-inline">Campaign Study </del>Group <del class="diffchange diffchange-inline">Report </del>&lt;br&gt;</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*<ins class="diffchange diffchange-inline">[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG_Summary/WG3_summery20170922.pdf </ins>WG3 <ins class="diffchange diffchange-inline">Simulation </ins>Group <ins class="diffchange diffchange-inline">Summary ---- by Fang Shen] </ins>&lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>*WG4 Campaign <del class="diffchange diffchange-inline">Study </del>Group <del class="diffchange diffchange-inline">Report </del>&lt;br&gt;</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*<ins class="diffchange diffchange-inline">[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG_Summary/WG4_summary20170922.pdf </ins>WG4 Campaign Group <ins class="diffchange diffchange-inline">Summary ---- by Nariaki Nitta] </ins>&lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG_Summary/wg5_summary.pdf WG5 Bs Challenge Group Report ---- by Spiros Patsourakos]] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG_Summary/wg5_summary.pdf WG5 Bs Challenge Group Report ---- by Spiros Patsourakos]] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>*WG6 SEP Group <del class="diffchange diffchange-inline">Report </del>&lt;br&gt;</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*WG6 SEP Group <ins class="diffchange diffchange-inline">Summary </ins>&lt;br&gt;</div></td></tr> </table>

Jie Zhang http://solar.gmu.edu/heliophysics/index.php?title=ISEST_2017_Workshop&diff=2975&oldid=prev 2018-09-17T05:42:22Z

<p>‎<span dir="auto"><span class="autocomment">Working Group Summary (September 22, 2017)</span></span></p> <table class="diff diff-contentalign-left" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="en"> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 05:42, 17 September 2018</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l53" >Line 53:</td> <td colspan="2" class="diff-lineno">Line 53:</td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; 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white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/<del class="diffchange diffchange-inline">WG_summary</del>/ISEST_WG1_summary_2017_Zhang.pdf WG1 data Group Report ---- by Jie Zhang*] &lt;br&gt;</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/<ins class="diffchange diffchange-inline">WG_Summary</ins>/ISEST_WG1_summary_2017_Zhang.pdf WG1 data Group Report ---- by Jie Zhang*] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*WG2 Campaign Study Group Report &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*WG2 Campaign Study Group Report &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*WG3 Campaign Study Group Report &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*WG3 Campaign Study Group Report &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*WG4 Campaign Study Group Report &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*WG4 Campaign Study Group Report &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/<del class="diffchange diffchange-inline">WG_summary</del>/wg5_summary.pdf WG5 Bs Challenge Group Report ---- by Spiros Patsourakos]] &lt;br&gt;</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/<ins class="diffchange diffchange-inline">WG_Summary</ins>/wg5_summary.pdf WG5 Bs Challenge Group Report ---- by Spiros Patsourakos]] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*WG6 SEP Group Report &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*WG6 SEP Group Report &lt;br&gt;</div></td></tr> </table>

Jie Zhang http://solar.gmu.edu/heliophysics/index.php?title=ISEST_2017_Workshop&diff=2974&oldid=prev 2018-09-17T05:41:22Z

<p></p> <table class="diff diff-contentalign-left" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="en"> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 05:41, 17 September 2018</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l48" >Line 48:</td> <td colspan="2" class="diff-lineno">Line 48:</td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Jinhye_Park.pdf&#160; Forecast of Solar Energetic Particles Depending on CME 3D parameters Using Multiple Spacecraft--- Jinhye Park] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Jinhye_Park.pdf&#160; Forecast of Solar Energetic Particles Depending on CME 3D parameters Using Multiple Spacecraft--- Jinhye Park] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/KS_Lee.pdf&#160; Spectroscopic and Stereoscopic Observation of a Loop-Top Source of An M1.3 Limb Solar Flare--- by Kyoung-Sun Lee] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/KS_Lee.pdf&#160; Spectroscopic and Stereoscopic Observation of a Loop-Top Source of An M1.3 Limb Solar Flare--- by Kyoung-Sun Lee] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;"></del></div></td><td colspan="2">&#160;</td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Nai_Hwa_Chen.pdf&#160; Temperature of Source Region of 3He-rich Impulsive Solar Energetic Particle Events --- Nai-Hwa Chen] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Nai_Hwa_Chen.pdf&#160; Temperature of Source Region of 3He-rich Impulsive Solar Energetic Particle Events --- Nai-Hwa Chen] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Pietro_Zucca.pdf Shock Location and CME 3D Reconstruction of the First Spatial Resolved Solar Type II Radio Burst With LOFAR --- by Pietro Zucca] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Pietro_Zucca.pdf Shock Location and CME 3D Reconstruction of the First Spatial Resolved Solar Type II Radio Burst With LOFAR --- by Pietro Zucca] &lt;br&gt;</div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;"></ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;"></ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">==Working Group Summary (September 22, 2017)==</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG_summary/ISEST_WG1_summary_2017_Zhang.pdf WG1 data Group Report ---- by Jie Zhang*] &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*WG2 Campaign Study Group Report &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*WG3 Campaign Study Group Report &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*WG4 Campaign Study Group Report &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG_summary/wg5_summary.pdf WG5 Bs Challenge Group Report ---- by Spiros Patsourakos]] &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*WG6 SEP Group Report &lt;br&gt;</ins></div></td></tr> </table>

Jie Zhang http://solar.gmu.edu/heliophysics/index.php?title=ISEST_2017_Workshop&diff=2973&oldid=prev 2018-09-17T04:21:41Z

<p>‎<span dir="auto"><span class="autocomment">WG6 SEP Presentations</span></span></p> <table class="diff diff-contentalign-left" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="en"> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 04:21, 17 September 2018</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l44" >Line 44:</td> <td colspan="2" class="diff-lineno">Line 44:</td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==WG6 SEP Presentations==</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==WG6 SEP Presentations==</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/RS_Kim.pdf The Third Class of SEPs--- by Roksoon Kim (Invited)] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/RS_Kim.pdf The Third Class of SEPs--- by Roksoon Kim (Invited)] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Modeling the Solar Energetic Particle Transport in the 3D Background Solar Wind --- by Fang Shen] &lt;br&gt;</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/<ins class="diffchange diffchange-inline">Fang_Shen_SEP0921.pdf&#160; </ins>Modeling the Solar Energetic Particle Transport in the 3D Background Solar Wind --- by Fang Shen] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Hongyu_Liu.pdf A Solar Stationary Type IV Radio Burst and Its Radiation Mechanism --- by Hongyu Liu] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Hongyu_Liu.pdf A Solar Stationary Type IV Radio Burst and Its Radiation Mechanism --- by Hongyu Liu] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Jinhye_Park.pdf&#160; Forecast of Solar Energetic Particles Depending on CME 3D parameters Using Multiple Spacecraft--- Jinhye Park] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Jinhye_Park.pdf&#160; Forecast of Solar Energetic Particles Depending on CME 3D parameters Using Multiple Spacecraft--- Jinhye Park] &lt;br&gt;</div></td></tr> </table>

Jie Zhang http://solar.gmu.edu/heliophysics/index.php?title=ISEST_2017_Workshop&diff=2972&oldid=prev 2018-09-17T04:20:09Z

<p></p> <table class="diff diff-contentalign-left" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="en"> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 04:20, 17 September 2018</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l41" >Line 41:</td> <td colspan="2" class="diff-lineno">Line 41:</td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/Jae-Ok_Lee.pdf Effects of Geometries and Substructures of ICMEs on Geomagnetic Storms --- by Jae-Ok Lee] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/Jae-Ok_Lee.pdf Effects of Geometries and Substructures of ICMEs on Geomagnetic Storms --- by Jae-Ok Lee] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/Schmidt_Cairns_cut.pdf Prediction &amp; Testing of Bz, Local CME Properties, White Light Images, &amp; Type II Radio Emission from Sun to Earth --- by Over H. Cairns] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/Schmidt_Cairns_cut.pdf Prediction &amp; Testing of Bz, Local CME Properties, White Light Images, &amp; Type II Radio Emission from Sun to Earth --- by Over H. Cairns] &lt;br&gt;</div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;"></ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">==WG6 SEP Presentations==</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/RS_Kim.pdf The Third Class of SEPs--- by Roksoon Kim (Invited)] &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Modeling the Solar Energetic Particle Transport in the 3D Background Solar Wind --- by Fang Shen] &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Hongyu_Liu.pdf A Solar Stationary Type IV Radio Burst and Its Radiation Mechanism --- by Hongyu Liu] &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Jinhye_Park.pdf&#160; Forecast of Solar Energetic Particles Depending on CME 3D parameters Using Multiple Spacecraft--- Jinhye Park] &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/KS_Lee.pdf&#160; Spectroscopic and Stereoscopic Observation of a Loop-Top Source of An M1.3 Limb Solar Flare--- by Kyoung-Sun Lee] &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;"></ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Nai_Hwa_Chen.pdf&#160; Temperature of Source Region of 3He-rich Impulsive Solar Energetic Particle Events --- Nai-Hwa Chen] &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Pietro_Zucca.pdf Shock Location and CME 3D Reconstruction of the First Spatial Resolved Solar Type II Radio Burst With LOFAR --- by Pietro Zucca] &lt;br&gt;</ins></div></td></tr> </table>

Jie Zhang http://solar.gmu.edu/heliophysics/index.php?title=ISEST_2017_Workshop&diff=2971&oldid=prev 2018-09-17T04:10:13Z

<p>‎<span dir="auto"><span class="autocomment">WG5 Bz Challenge Presentations</span></span></p> <table class="diff diff-contentalign-left" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="en"> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 04:10, 17 September 2018</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l39" >Line 39:</td> <td colspan="2" class="diff-lineno">Line 39:</td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/FRED_gopalswamy.pptx Flux Rope From Eruption Data (FRED) and Its Interplanetary Counterpart --- by Nat Gopalswamy] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/FRED_gopalswamy.pptx Flux Rope From Eruption Data (FRED) and Its Interplanetary Counterpart --- by Nat Gopalswamy] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/HS_Yang.pdf Observation of the Streaming-Kink Instability in the Solar Prominence --- by Heesu Yang] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/HS_Yang.pdf Observation of the Streaming-Kink Instability in the Solar Prominence --- by Heesu Yang] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/Jae-<del class="diffchange diffchange-inline">Ok\ Lee</del>.pdf Effects of Geometries and Substructures of ICMEs on Geomagnetic Storms --- by Jae-Ok Lee] &lt;br&gt;</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/Jae-<ins class="diffchange diffchange-inline">Ok_Lee</ins>.pdf Effects of Geometries and Substructures of ICMEs on Geomagnetic Storms --- by Jae-Ok Lee] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/Schmidt_Cairns_cut.pdf Prediction &amp; Testing of Bz, Local CME Properties, White Light Images, &amp; Type II Radio Emission from Sun to Earth --- by Over H. Cairns] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/Schmidt_Cairns_cut.pdf Prediction &amp; Testing of Bz, Local CME Properties, White Light Images, &amp; Type II Radio Emission from Sun to Earth --- by Over H. Cairns] &lt;br&gt;</div></td></tr> </table>

Jie Zhang http://solar.gmu.edu/heliophysics/index.php?title=ISEST_2017_Workshop&diff=2970&oldid=prev 2018-09-17T04:08:03Z

<p></p> <table class="diff diff-contentalign-left" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="en"> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 04:08, 17 September 2018</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l34" >Line 34:</td> <td colspan="2" class="diff-lineno">Line 34:</td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG4/Nitta_Stealthy_but_Earth_Affecting_CMEs.pdf Stealthy But Earth-Affecting CMEs --- by Nariaki Nitta] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG4/Nitta_Stealthy_but_Earth_Affecting_CMEs.pdf Stealthy But Earth-Affecting CMEs --- by Nariaki Nitta] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG4/WangYuming.pdf CME Dynamics: Tracing an Interplanetary Magnetic Cloud From Mercury to Venus, Earth and Beyond --- by Yuming Wang] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG4/WangYuming.pdf CME Dynamics: Tracing an Interplanetary Magnetic Cloud From Mercury to Venus, Earth and Beyond --- by Yuming Wang] &lt;br&gt;</div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;"></ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">==WG5 Bz Challenge Presentations==</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/BV_Jackson.pdf&#160; Different Techniques for (and Some Success in) Measurement of Bs--- by B.V. Jackson(Invited)] &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/FRED_gopalswamy.pptx Flux Rope From Eruption Data (FRED) and Its Interplanetary Counterpart --- by Nat Gopalswamy] &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/HS_Yang.pdf Observation of the Streaming-Kink Instability in the Solar Prominence --- by Heesu Yang] &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/Jae-Ok\ Lee.pdf Effects of Geometries and Substructures of ICMEs on Geomagnetic Storms --- by Jae-Ok Lee] &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/Schmidt_Cairns_cut.pdf Prediction &amp; Testing of Bz, Local CME Properties, White Light Images, &amp; Type II Radio Emission from Sun to Earth --- by Over H. Cairns] &lt;br&gt;</ins></div></td></tr> </table>

Jie Zhang http://solar.gmu.edu/heliophysics/index.php?title=ISEST_2017_Workshop&diff=2969&oldid=prev 2018-09-17T03:33:02Z

<p>‎<span dir="auto"><span class="autocomment">WG4 Campaign Group Presentations</span></span></p> <table class="diff diff-contentalign-left" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="en"> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 03:33, 17 September 2018</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l32" >Line 32:</td> <td colspan="2" class="diff-lineno">Line 32:</td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG4/Katsuhide_Marubashi.pdf&#160; What We Can Learn From the ISEST WG4 Campaign Study of Sun-Earth Events? --- by Katsuhide Marubashi (Invited)] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG4/Katsuhide_Marubashi.pdf&#160; What We Can Learn From the ISEST WG4 Campaign Study of Sun-Earth Events? --- by Katsuhide Marubashi (Invited)] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG4/Brigitte_Schmieder.pdf&#160; Solar Events Associated With SSCs in 2002: Propagation and Effects From the Sun to the Earth --- by Brigitte Schmieder] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG4/Brigitte_Schmieder.pdf&#160; Solar Events Associated With SSCs in 2002: Propagation and Effects From the Sun to the Earth --- by Brigitte Schmieder] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG4/<del class="diffchange diffchange-inline">Nitta_Stealth_but_Earth_Affecting_CME</del>.pdf Stealthy But Earth-Affecting CMEs --- by Nariaki Nitta] &lt;br&gt;</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG4/<ins class="diffchange diffchange-inline">Nitta_Stealthy_but_Earth_Affecting_CMEs</ins>.pdf Stealthy But Earth-Affecting CMEs --- by Nariaki Nitta] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG4/WangYuming.pdf CME Dynamics: Tracing an Interplanetary Magnetic Cloud From Mercury to Venus, Earth and Beyond --- by Yuming Wang] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG4/WangYuming.pdf CME Dynamics: Tracing an Interplanetary Magnetic Cloud From Mercury to Venus, Earth and Beyond --- by Yuming Wang] &lt;br&gt;</div></td></tr> </table>

Jie Zhang http://solar.gmu.edu/heliophysics/index.php?title=ISEST_2017_Workshop&diff=2968&oldid=prev 2018-09-17T03:32:23Z

<p>‎<span dir="auto"><span class="autocomment">WG4 Campaign Group Presentations</span></span></p> <table class="diff diff-contentalign-left" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="en"> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 03:32, 17 September 2018</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l30" >Line 30:</td> <td colspan="2" class="diff-lineno">Line 30:</td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==WG4 Campaign Group Presentations==</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==WG4 Campaign Group Presentations==</div></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/<del class="diffchange diffchange-inline">WG2_3</del>/<del class="diffchange diffchange-inline">Christina_Verbeke</del>.pdf <del class="diffchange diffchange-inline">Progress of MHD Simulations For </del>the <del class="diffchange diffchange-inline">Interplanetary Propagation </del>of <del class="diffchange diffchange-inline">Coronal Mass Ejections </del>--- by <del class="diffchange diffchange-inline">Christina Verbeke </del>(Invited)] &lt;br&gt;</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/<ins class="diffchange diffchange-inline">WG4</ins>/<ins class="diffchange diffchange-inline">Katsuhide_Marubashi</ins>.pdf <ins class="diffchange diffchange-inline"> What We Can Learn From </ins>the <ins class="diffchange diffchange-inline">ISEST WG4 Campaign Study </ins>of <ins class="diffchange diffchange-inline">Sun-Earth Events? </ins>--- by <ins class="diffchange diffchange-inline">Katsuhide Marubashi </ins>(Invited)] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/<del class="diffchange diffchange-inline">WG2_3</del>/<del class="diffchange diffchange-inline">Kyungsun_Park</del>.pdf&#160; <del class="diffchange diffchange-inline">Response of </del>the <del class="diffchange diffchange-inline">Earth's Magnetosphere and&#160; Ionosphere </del>to the <del class="diffchange diffchange-inline">Small-scale Magnetic Flux Rope in Solar Wind by the MHD Simulation </del>--- by <del class="diffchange diffchange-inline">Kyung Sun Park</del>] &lt;br&gt;</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/<ins class="diffchange diffchange-inline">WG4</ins>/<ins class="diffchange diffchange-inline">Brigitte_Schmieder</ins>.pdf&#160; <ins class="diffchange diffchange-inline">Solar Events Associated With SSCs in 2002: Propagation and Effects From </ins>the <ins class="diffchange diffchange-inline">Sun </ins>to the <ins class="diffchange diffchange-inline">Earth </ins>--- by <ins class="diffchange diffchange-inline">Brigitte Schmieder</ins>] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/<del class="diffchange diffchange-inline">WG2_3</del>/<del class="diffchange diffchange-inline">Mark_Cheung_</del>.pdf <del class="diffchange diffchange-inline">Data</del>-<del class="diffchange diffchange-inline">driven Evolving Models of the Solar Corona </del>--- by <del class="diffchange diffchange-inline">Mark Cheung</del>] &lt;br&gt;</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/<ins class="diffchange diffchange-inline">WG4</ins>/<ins class="diffchange diffchange-inline">Nitta_Stealth_but_Earth_Affecting_CME</ins>.pdf <ins class="diffchange diffchange-inline">Stealthy But Earth</ins>-<ins class="diffchange diffchange-inline">Affecting CMEs </ins>--- by <ins class="diffchange diffchange-inline">Nariaki Nitta</ins>] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/<del class="diffchange diffchange-inline">WG2_3</del>/<del class="diffchange diffchange-inline">Nishtha_Shachdeva</del>.pdf CME Dynamics: <del class="diffchange diffchange-inline">Relative Importance of Lorentz Force </del>and <del class="diffchange diffchange-inline">Solar Wind Drag </del>--- by <del class="diffchange diffchange-inline">Nishtha Sachdeva</del>] &lt;br&gt;</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/<ins class="diffchange diffchange-inline">WG4</ins>/<ins class="diffchange diffchange-inline">WangYuming</ins>.pdf CME Dynamics: <ins class="diffchange diffchange-inline">Tracing an Interplanetary Magnetic Cloud From Mercury to Venus, Earth </ins>and <ins class="diffchange diffchange-inline">Beyond </ins>--- by <ins class="diffchange diffchange-inline">Yuming Wang</ins>] &lt;br&gt;</div></td></tr> </table>

Jie Zhang http://solar.gmu.edu/heliophysics/index.php?title=ISEST_2017_Workshop&diff=2967&oldid=prev 2018-09-17T02:44:33Z

<p></p> <table class="diff diff-contentalign-left" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="en"> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td> <td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 02:44, 17 September 2018</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l24" >Line 24:</td> <td colspan="2" class="diff-lineno">Line 24:</td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==WG2 Theory Group / WG3 Simulation Group Presentations==</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==WG2 Theory Group / WG3 Simulation Group Presentations==</div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG2_3/Christina_Verbeke.pdf Progress of MHD Simulations For the Interplanetary Propagation of Coronal Mass Ejections --- by Christina Verbeke (Invited)] &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG2_3/Kyungsun_Park.pdf&#160; Response of the Earth's Magnetosphere and&#160; Ionosphere to the Small-scale Magnetic Flux Rope in Solar Wind by the MHD Simulation --- by Kyung Sun Park] &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG2_3/Mark_Cheung_.pdf Data-driven Evolving Models of the Solar Corona --- by Mark Cheung] &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG2_3/Nishtha_Shachdeva.pdf CME Dynamics: Relative Importance of Lorentz Force and Solar Wind Drag --- by Nishtha Sachdeva] &lt;br&gt;</ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;"></ins></div></td></tr> <tr><td colspan="2">&#160;</td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">==WG4 Campaign Group Presentations==</ins></div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG2_3/Christina_Verbeke.pdf Progress of MHD Simulations For the Interplanetary Propagation of Coronal Mass Ejections --- by Christina Verbeke (Invited)] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG2_3/Christina_Verbeke.pdf Progress of MHD Simulations For the Interplanetary Propagation of Coronal Mass Ejections --- by Christina Verbeke (Invited)] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG2_3/Kyungsun_Park.pdf&#160; Response of the Earth's Magnetosphere and&#160; Ionosphere to the Small-scale Magnetic Flux Rope in Solar Wind by the MHD Simulation --- by Kyung Sun Park] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG2_3/Kyungsun_Park.pdf&#160; Response of the Earth's Magnetosphere and&#160; Ionosphere to the Small-scale Magnetic Flux Rope in Solar Wind by the MHD Simulation --- by Kyung Sun Park] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG2_3/Mark_Cheung_.pdf Data-driven Evolving Models of the Solar Corona --- by Mark Cheung] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG2_3/Mark_Cheung_.pdf Data-driven Evolving Models of the Solar Corona --- by Mark Cheung] &lt;br&gt;</div></td></tr> <tr><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG2_3/Nishtha_Shachdeva.pdf CME Dynamics: Relative Importance of Lorentz Force and Solar Wind Drag --- by Nishtha Sachdeva] &lt;br&gt;</div></td><td class='diff-marker'>&#160;</td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG2_3/Nishtha_Shachdeva.pdf CME Dynamics: Relative Importance of Lorentz Force and Solar Wind Drag --- by Nishtha Sachdeva] &lt;br&gt;</div></td></tr> </table>

Jie Zhang