activity
20152022
most citedObservational Evidence of Magnetic Reconnection for Brightenings and Transition Region Arcades in IRIS observations

41 citations · 125 across the 11 of their papers we have counts for

collaborators

20 papers

astro-ph.SR20225 cited

Spatially Resolved Moving Radio Burst in Association with an EUV Wave

Lei Lu, Li Feng, Weiqun Gan

Coronal mass ejections (CMEs) are large clouds of magnetized plasma ejected from the Sun, and are often associated with acceleration of electrons that can result in radio emission…

astro-ph.SR20228 cited

Three-dimensional analyses of an aspherical coronal mass ejection and its driven shock

Beili Ying, Li Feng, Bernd Inhester +4

Context. Observations reveal that shocks can be driven by fast coronal mass ejections (CMEs) and play essential roles in particle accelerations. A critical ratio, , derived from…

astro-ph.SR202219 cited

Observational Signatures of Tearing Instability in the Current Sheet of a Solar Flare

Lei Lu, Li Feng, Alexander Warmuth +7

Magnetic reconnection is a fundamental physical process converting magnetic energy into not only plasma energy but also particle energy in various astrophysical phenomena. In this…

astro-ph.SR2021

Quasi-Periodic Pulsations Detected in Ly and Nonthermal Emissions During Solar Flares

Lei Lu, Dong Li, Zongjun Ning +2

We report quasi-periodic pulsations (QPPs) with double periods during three solar flares (viz. SOL2011-Feb-15T01:44, SOL2011-Sep-25T04:31, SOL2012-May-17T01:25). The flare QPPs wer…

astro-ph.SR2021

Analysis of type II and type III radio bursts associated with SEPs from non-interacting/interacting radio-loud CMEs

P Pappa Kalaivani, O Prakash, A Shanmugaraju +4

We analyze radio bursts observed in events with interacting/non-interacting CMEs that produced major SEPs (Ip 10 MeV) fromApril 1997 to December 2014.We compare properties of m…

astro-ph.SR20214 cited

Population of Bright Plume Threads in Solar Polar Coronal Holes

Zhenghua Huang, Quanhao Zhang, Lidong Xia +8

Coronal holes are well accepted to be source regions of the fast solar wind. As one of the common structures in coronal holes, coronal plumes might contribute to the origin of the…