ISEST 2017 Workshop

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)

• Introduction to ISEST Project ---- by Jie Zhang*
  
• WG1 data Group Report ---- by Jie Zhang
  
• WG2 Theory Group Report ---- by Yuming Wang on behalf of Bojan Vrsnak
  
• WG3 Simulation Group Report ---- by Fang Shen
  
• WG4 Campaign Study Group Report ---- by Nariaki Nitta & David Webb
  
• WG5 Bs Challenge Group Report ---- by Spiros Patsourakos
  
• WG6 SEP Group Report ---- by Nat Gopalswamy on behalf of Olga Malandraki
  
• WG7 MiniMax Report ---- by Nat Gopalswamy on behalf of Manuela Temmer
  

WG1 Data Group Presentations

• Key Problems in the Forecasting of the Geoeffectiveness of CMEs --- by Chenglong Shen* (Invited)
  
• Development of a Daily Solar Major Flare Occurrence Probability Model Based on Vector Parameters From SOHO/HMI --- by Date Lim
  
• Application of Convolutional Neutral Network to the Forecasts of Flare Classification and Occurrence Using SOHO MDI Data --- by Eunsu Park
  
• Heating of an Erupting Prominence Associated With a Solar Coronal Mass Ejection on 2012 Jan. 27 --- by Jin-Yi Lee
  
• PC Index as a Proxy of the Solar Wind Energy Incoming Into the Magnetosphere --- by Oleg Troshichev
  
• Study of Filament Eruption During 2015 March 14-15 --- by Ramesh Chandra
  
• Statistical Study on the Kinematic Distribution of CMEs from 1996 to 2015 --- by Seong-Gyeong Jeon
  
• Two Distinct Types of CME-flare Relationships Based on SOHO and STEREO Observations --- by Soojeong Jang
  
• Assesssing the Collusion Nature of Coronal Mass Ejections in the Inner Heliosphere --- by Wageesh Mishra
  
• Progress on Solar Activity (Flares and Coronal Mass Ejections) Prediction in Space Weather Science --- by Jie Zhang
  

WG2 Theory Group / WG3 Simulation Group Presentations

• Progress of MHD Simulations For the Interplanetary Propagation of Coronal Mass Ejections --- by Christina Verbeke (Invited)
  
• Response of the Earth's Magnetosphere and Ionosphere to the Small-scale Magnetic Flux Rope in Solar Wind by the MHD Simulation --- by Kyung Sun Park
  
• Data-driven Evolving Models of the Solar Corona --- by Mark Cheung
  
• CME Dynamics: Relative Importance of Lorentz Force and Solar Wind Drag --- by Nishtha Sachdeva
  

WG4 Campaign Group Presentations

• What We Can Learn From the ISEST WG4 Campaign Study of Sun-Earth Events? --- by Katsuhide Marubashi (Invited)
  
• Solar Events Associated With SSCs in 2002: Propagation and Effects From the Sun to the Earth --- by Brigitte Schmieder
  
• Stealthy But Earth-Affecting CMEs --- by Nariaki Nitta
  
• CME Dynamics: Tracing an Interplanetary Magnetic Cloud From Mercury to Venus, Earth and Beyond --- by Yuming Wang
  

WG5 Bz Challenge Presentations

• Different Techniques for (and Some Success in) Measurement of Bs--- by B.V. Jackson(Invited)
  
• Flux Rope From Eruption Data (FRED) and Its Interplanetary Counterpart --- by Nat Gopalswamy
  
• Observation of the Streaming-Kink Instability in the Solar Prominence --- by Heesu Yang
  
• Effects of Geometries and Substructures of ICMEs on Geomagnetic Storms --- by Jae-Ok Lee
  
• Prediction & Testing of Bz, Local CME Properties, White Light Images, & Type II Radio Emission from Sun to Earth --- by Over H. Cairns
  

WG6 SEP Presentations

• The Third Class of SEPs--- by Roksoon Kim (Invited)
  
• Modeling the Solar Energetic Particle Transport in the 3D Background Solar Wind --- by Fang Shen
  
• A Solar Stationary Type IV Radio Burst and Its Radiation Mechanism --- by Hongyu Liu
  
• Forecast of Solar Energetic Particles Depending on CME 3D parameters Using Multiple Spacecraft--- Jinhye Park
  
• Spectroscopic and Stereoscopic Observation of a Loop-Top Source of An M1.3 Limb Solar Flare--- by Kyoung-Sun Lee
  

• Temperature of Source Region of 3He-rich Impulsive Solar Energetic Particle Events --- Nai-Hwa Chen
  
• Shock Location and CME 3D Reconstruction of the First Spatial Resolved Solar Type II Radio Burst With LOFAR --- by Pietro Zucca