Splinter: SSA Space Weather Service Network Splinter: SSA Space Weather Service Network Tuesday 18th, 15:30 - 17:00 1.Overview of the P2-SSA activities.
A solar eruption driven by rapid sunspot rotation Guiping Ruan, Yao Chen, Shuo Wang, Hongqi Zhang, Gang Li, Ju Jing, Xing Li, Haiqing Xu, and Haimin Wang.
Evolution of the Filament’s Shape. Fig. 1a shows the filament (in absorption) almost one hour before eruption. Once the filament begins to erupt, it takes.
A comparison of CME-associated atmospheric waves observed in coronal (Fe XII 195A) and chromospheric ( He I 10830A) lines Holly R. Gilbert, Thomas E. Holzer,
Future Plans for Space Weather Observations – U.S. NOAA Perspective Terry Onsager National Oceanic and Atmospheric Administration Space Weather Prediction.
Magnetic Helicity and Energetics in Solar Active Regions: Can we calculate them – why do we need them? Manolis K. Georgoulis JHU/APL Whistler, CA, 08/01/07.
The CME Link to Filaments and Filament Channels
Abstract
High-Energy Emission from a Solar Flare in Hard X-Rays and Microwaves M R Kundu 1, V V Grechnev 2, S M White 1, E J Schmahl 1, N S Meshalkina 2, L K Kashapova.
Flare Energy Build-Up in a Decaying Active Region Near a Coronal Hole
Low atmospheric reconnections associated with an eruptive flare
KASI - 0 - Low atmospheric reconnections associated with an eruptive flare Yong-Jae Moon(1), Jongchul Chae(2), Young-Deuk Park(1) 1: Korea Astronomy and.
