Date
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Discussion
leader
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Article
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01/23
|
Silvina
|
S. J. Bradshaw, G. AUlanier, G. Del Zanna, A Reconnection-Driven Rarefaction Wave Model for Coronal Outflows
|
01/30
|
Tom
|
Jess et. al., The Origin of Type I Spicule Oscillations
|
02/06
|
Ying
|
Milligan et. al., Observations of Enhanced EUV Continua During an X-class Solar Flare Using SDO/EVE
|
02/13
|
Jake
|
P. Judge, B. dePontieu, S. McIntosh, and K. Olluri, The Connection of Type II Spicules to the Corona
|
02/27
|
Sean
|
Wang et al, Response of the Photospheric Magnetic Field to the X2.2 Flare on 2011 February 15
|
03/05
|
Ernest
|
Hathaway, D.H. A Standard Law for the Equatorward Drift of the Sunspot Zones
|
03/19
|
Roger
|
De Moortel, I. et al, The damping of slow MHD waves in solar coronal magnetic fields. III. The effect of mode coupling
|
03/26
|
Alec
|
Cheung, M.C.M. Simulation of the Formation of a Solar Active Region
|
04/02
|
Lucas
|
Sun, Xudong Evolution of Magnetic Field and Energy in a Major Eruptive Active Region Based on SDO/HMI Observation
|
04/09
|
Anna
|
Non-Linear Force-Free Modeling of the
Solar Corona Using Information Contained in Coronal Loops
|
04/16
|
Wenjuan
|
Asai et al, First Simultaneous Observation of an H_alpha Moreton Wave, EUV Wave, and Filament/Prominence Oscillations
|
04/23
|
Chris
|
Sheeley, N. R., Jr.; Warren, H. P. Coronal Cells
|