322 citations · 1.3k across the 31 of their papers we have counts for
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astro-ph.SR2015★ 32 cited
Why does the apparent mass of a coronal mass ejection increase?
Li Feng, Yuming Wang, Fang Shen +4
Mass is one of the most fundamental parameters characterizing the dynamics of a coronal mass ejection (CME). It has been found that CME apparent mass measured from the brightness e…
astro-ph.SR2015★ 50 cited
Electron acceleration by cascading reconnection in the solar corona I Magnetic gradient and curvature effects
X. Zhou, J. Büchner, M. Barta +2
Aims: We investigate the electron acceleration in convective electric fields of cascading magnetic reconnection in a flaring solar corona and show the resulting hard X-ray (HXR) ra…
astro-ph.SR2015
Radial Flow Pattern of a Slow CME
Li Feng, Bernd Inhester, Weiqun Gan
Height-time plots of the leading edge of coronal mass ejections (CME) have often been used to study CME kinematics. We propose a new method to analyze the CME kinematics in more de…