Difference between revisions of "ISEST 2017 Workshop"

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(WG5 Bz Challenge Presentations)
(Working Group Summary (September 22, 2017))
 
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*[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] <br>
 
*[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] <br>
 
*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/Schmidt_Cairns_cut.pdf Prediction & Testing of Bz, Local CME Properties, White Light Images, & Type II Radio Emission from Sun to Earth --- by Over H. Cairns] <br>
 
*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG5/Schmidt_Cairns_cut.pdf Prediction & Testing of Bz, Local CME Properties, White Light Images, & Type II Radio Emission from Sun to Earth --- by Over H. Cairns] <br>
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==WG6 SEP Presentations==
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*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/RS_Kim.pdf The Third Class of SEPs--- by Roksoon Kim (Invited)] <br>
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*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Fang_Shen_SEP0921.pdf  Modeling the Solar Energetic Particle Transport in the 3D Background Solar Wind --- by Fang Shen] <br>
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*[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] <br>
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*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Jinhye_Park.pdf  Forecast of Solar Energetic Particles Depending on CME 3D parameters Using Multiple Spacecraft--- Jinhye Park] <br>
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*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/KS_Lee.pdf  Spectroscopic and Stereoscopic Observation of a Loop-Top Source of An M1.3 Limb Solar Flare--- by Kyoung-Sun Lee] <br>
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*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG6/Nai_Hwa_Chen.pdf  Temperature of Source Region of 3He-rich Impulsive Solar Energetic Particle Events --- Nai-Hwa Chen] <br>
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*[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] <br>
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==Working Group Summary (September 22, 2017)==
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*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG_Summary/ISEST_WG1_summary_2017_Zhang.pdf WG1 Data Group Summary ---- by Jie Zhang] <br>
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*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG_Summary/WG2_Summary20170922.pdf WG2 Theory Group Summary ---- by Yuming Wang] <br>
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*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG_Summary/WG3_summery20170922.pdf WG3 Simulation Group Summary ---- by Fang Shen] <br>
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*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG_Summary/WG4_summary20170922.pdf WG4 Campaign Group Summary ---- by Nariaki Nitta] <br>
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*[http://solar.gmu.edu/wiki/presentations/ISEST_2017_workshop/WG_Summary/wg5_summary.pdf WG5 Bs Challenge Group Report ---- by Spiros Patsourakos]] <br>
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*WG6 SEP Group Summary <br>

Latest revision as of 22:35, 17 September 2018

This page contains presentations given at the 2017 ISEST Workshop. The 2017 ISEST Workshop was held in September 18-22, 2017, Jeju, Korea. Here is the link to the meeting website

WG Report (Sep. 18, 2017)

WG1 Data Group Presentations

WG2 Theory Group / WG3 Simulation Group Presentations

WG4 Campaign Group Presentations

WG5 Bz Challenge Presentations

WG6 SEP Presentations


Working Group Summary (September 22, 2017)