The top documents tagged [filament eruption]

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
Documents 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

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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
Documents 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

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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
Documents 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

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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,
Documents 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,

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Future Plans for Space Weather Observations – U.S. NOAA Perspective Terry Onsager National Oceanic and Atmospheric Administration Space Weather Prediction
Documents Future Plans for Space Weather Observations – U.S. NOAA Perspective Terry Onsager National Oceanic and Atmospheric Administration Space Weather Prediction

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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
Documents 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

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The CME Link to Filaments and Filament Channels
Documents The CME Link to Filaments and Filament Channels

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Abstract
Documents Abstract

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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
Documents 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

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Flare Energy Build-Up in a Decaying Active Region Near a Coronal Hole
Documents Flare Energy Build-Up in a Decaying Active Region Near a Coronal Hole

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Low atmospheric reconnections associated with an eruptive flare
Documents Low atmospheric reconnections associated with an eruptive flare

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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
Documents 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

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