207 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Chinese Academy of SciencesCN179 papers
- National Astronomical ObservatoriesCN175 papers
- University of Chinese Academy of SciencesCN55 papers
- Yunnan ObservatoriesCN32 papers
- Purple Mountain ObservatoryCN22 papers
- Max Planck Institute for Solar System ResearchDE16 papers
- Shandong UniversityCN14 papers
- Nanjing UniversityCN12 papers
- State Key Laboratory of Space Weather10 papers
- Institute of Solar-Terrestrial PhysicsRU9 papers
- Kunming University of Science and TechnologyCN9 papers
- Russian Academy of SciencesRU7 papers
9 papers · 2 filters
A Catalog of LAMOST Variable Sources Based on Time-domain Photometry of ZTF
Tingting Xu, Chao Liu, Feng Wang +4
The identification and analysis of different variable sources is a hot issue in astrophysical research. The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) spect…
Comparison of Helium Abundance between ICMEs and Solar Wind near 1 AU
Hongqiang Song, Xin Cheng, Leping Li +2
The Helium abundance, defined as , is 8.5 in the photosphere and seldom exceeds 5 in fast solar wind. Previous statistics have demonstrated tha…
Common origin of quasi-periodic pulsations in microwave and decimetric solar radio bursts
Larisa Kashapova, Dmitrii Kolotkov, Elena Kupriyanova +3
We analyse quasi-periodic pulsations (QPP) detected in the microwave and decimeter radio emission of the SOL2017-09-05T07:04 solar flare, using simultaneous observations by the Sib…
Active region chromospheric magnetic fields
G. J. M. Vissers, S. Danilovic, X. Zhu +5
Context. A proper estimate of the chromospheric magnetic fields is believed to improve modelling of both active region and coronal mass ejection evolution. Aims. We investigate the…
Energy and spectral analysis of confined solar flares from radio and X-ray observations
Chengming Tan, Karl-Ludwig Klein, Yihua Yan +4
The energy and spectral shape of radio bursts may help us understand the generation mechanism of solar eruptions, including solar flares, CMEs, eruptive filaments, and various scal…
Spotless days and geomagnetic index as the predictors of solar cycle 25
Dipali S. Burud, Rajmal Jain, Arun K. Awasthi +6
We study the sunspot activity in relation to spotless days (SLDs) during the descending phase of solar cycle -- to predict the amplitude of sunspot cycle . For this pur…
Three-dimensional magnetic reconnection in astrophysical plasmas
Ting Li, Eric Priest, Ruilong Guo
Magnetic reconnection is a fundamental process in a laboratory, magnetospheric, solar and astrophysical plasma, whereby magnetic energy is converted into heat, bulk kinetic energy…
Energy partition in a confined flare with an extreme-ultraviolet late phase
Q. M. Zhang, J. X. Cheng, Y. Dai +2
In this paper, we reanalyze the M1.2 confined flare with a large extreme-ultraviolet (EUV) late phase on 2011 September 9, focusing on its energy partition. The radiation (5.…
Flare Activity and Magnetic Feature Analysis of the Flare Stars II: Sub-Giant Branch
Hadis Goodarzi, Ahmad Mehrabi, Habib G. Khosroshahi +1
We present an investigation of the magnetic activity and flare characteristics of the sub-giant stars mostly from F and G spectral types and compare the results with the main-seque…