169 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Chinese Academy of SciencesCN124 papers
- National Space Science CenterCN91 papers
- University of Chinese Academy of SciencesCN32 papers
- University of Science and Technology of ChinaCN15 papers
- National Astronomical ObservatoriesCN14 papers
- Harbin Institute of TechnologyCN11 papers
- Institute of Theoretical PhysicsCN11 papers
- Purple Mountain ObservatoryCN11 papers
- Yunnan ObservatoriesCN11 papers
- Key Laboratory of Solar Activities, Chinese Academy of SciencesCN10 papers
- Shandong UniversityCN10 papers
- Space Sciences LaboratoryUS10 papers
5 papers · 2 filters
Are IRIS bombs connected to Ellerman bombs?
Hui Tian, Zhi Xu, Jiansen He +1
Recent observations by the Interface Region Imaging Spectrograph (IRIS) have revealed pockets of hot gas (2--810 K) potentially resulting from magnetic reconnec…
Dark Post-Flare Loops Observed by Solar Dynamics Observatory
Qiao Song, Jing-Song Wang, Xueshang Feng +1
Solar post-flare loops (PFLs) are arcade-like loop systems that appear during the gradual phases of eruptive flares. The extreme ultraviolet (EUV) observations from the Atmospheric…
Spectral Anisotropy of Elsässer Variables in Two Dimensional Wave-vector Space as Observed in the Fast Solar Wind Turbulence
Limei Yan, Jiansen He, Lei Zhang +6
Intensive studies have been conducted to understand the anisotropy of solar wind turbulence. However, the anisotropy of Elsässer variables () in 2D wave-vector spac…
Ultra-narrow Negative Flare Front Observed in Helium-10830~Å using the 1.6 m New Solar Telescope
Yan Xu, Wenda Cao, Mingde Ding +10
Solar flares are sudden flashes of brightness on the Sun and are often associated with coronal mass ejections and solar energetic particles which have adverse effects in the near E…
Kinetic Simulation of Slow Magnetosonic Waves and Quasi-periodic Upflows in the Solar Corona
Wenzhi Ruan, Jiansen He, Lei Zhang +5
Quasi-periodic disturbances of emission-line parameters are frequently observed in the corona. These disturbances propagate upward along the magnetic field with speeds $\sim100~\rm…