Contributed by Sonja Jejčič. Posted on November 30, 2018
A strong limb flare observed simultaneously by the SDO/AIA and SDO/HMI, which is very rare, allows the authors to study the emission mechanism for white-light flare loops, as well as estimate the electron densities along the flare loop.
Contributed by J. Kašparová and P. Heinzel. Posted on October 31, 2017
What makes the limb flares detectable in visible lights, hydrogen recombination or Thomson scattering?
Contributed by Chang Liu. Posted on October 27, 2014
By synthesizing the results of photospheric field change indicated by HMI observations and coronal field variation suggested by the NLFFF modeling, we study the flare-related 3D magnetic restructuring and find it consistent with the coronal implosion scenario in the low solar atmosphere.