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
182 papers
The deformation of an erupting magnetic flux rope in a confined solar flare
Ruisheng Zheng, Yihan Liu, Liang Zhang +7
Magnetic flux ropes (MFRs), sets of coherently twisted magnetic field lines, are believed as core structures of various solar eruptions. Their evolution plays an important role to…
On the Nature of the Three-part Structure of Solar Coronal Mass Ejections
Hongqiang Song, Jie Zhang, Leping Li +4
Coronal mass ejections (CMEs) result from eruptions of magnetic flux ropes (MFRs) and can possess a three-part structure in white-light coronagraphs, including a bright front, dark…
Diagnostic functions of solar coronal magnetic fields from radio observations
Baolin Tan
In solar physics, it is a big challenge to measure the magnetic fields directly from observations in the upper solar atmosphere, including the chromosphere and corona. Radio observ…
Toward a Unified Explanation for the Three-part Structure of Solar Coronal Mass Ejections
Hongqiang Song, Leping Li, Yao Chen
Coronal mass ejections (CMEs) are associated with the eruption of magnetic flux ropes (MFRs), which usually appear as hot channels in active regions and coronal cavities in quiet-S…
Birth places of extreme ultraviolet waves driven by impingement of solar jets upon coronal loops
Liang Zhang, Ruisheng Zheng, Huadong Chen +1
Solar extreme ultraviolet (EUV) waves are large-scale propagating disturbances in the corona. It is generally believed that the vital key for the formation of EUV waves is the rapi…
Formation and Immediate Deformation of a Small Filament Through Intermittent Magnetic Interactions
Ruisheng Zheng, Liang Zhang, Changhui Rao +4
It is generally believed that filament formation involves a process of the accumulation of magnetic energy. However, in this paper we discuss the idea that filaments will not erupt…
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…
Magnetic Reconnection Invoked by Sweeping of the CME-Driven Fast-Mode Shock
Guiping Zhou, Guannan Gao, Jingxiu Wang +4
Coronal waves exist ubiquitously in the solar atmosphere. They are important not only in their own rich physics but also essential candidates of triggering magnetic eruptions in th…
Doppler shift oscillations of a sunspot detected by CYRA and IRIS
D. Li, X. Yang, X. Y. Bai +4
Context. The carbon monoxide (CO) molecular line at around 46655 A in solar infrared spectra is often used to investigate the dynamic behavior of the cold heart of the solar atmosp…
An investigation of flare emissions at multiple wavelengths
Dong Li, Alexander Warmuth, Lei Lu +1
We report multi-wavelength observations of four solar flares on 2014 July 07. We firstly select these flares according to the soft X-ray (SXR) and extreme ultraviolet (EUV) emissio…
Photometric and Spectroscopic Study of Flares on Ross 15
Jian-Ying Bai, Ali Esamdin, Xing Gao +2
We conducted photometric and spectroscopic observations for Ross 15 in order to further study the flare properties of this less observed flare star. A total of 28 B-band flares are…
Estimates of current helicity and tilt of solar active regions and Joy's law
K. Kuzanyan, N. Kleeorin, I. Rogachevskii +2
The tilt angle, current helicity and twist of solar magnetic fields can be observed in solar active regions. We carried out estimates of these parameters by two ways. Firstly, we c…
A White-light Flare Powered by Magnetic Reconnection in the Lower Solar Atmosphere
Yongliang Song, Hui Tian, Xiaoshuai Zhu +3
White-light flares (WLFs), first observed in 1859, refer to a type of solar flares showing an obvious enhancement of the visible continuum emission. This type of enhancement often…
Observations of a quasi-periodic pulsation in the coronal loop and microwave flux during a solar preflare phase
Dong Li, Ying Li, Lei Lu +3
We report a quasi-periodic pulsation (QPP) event simultaneously detected from the spatial displacements of coronal loop at both EUV images and microwave emission during the preflar…
Dynamics of descending knots in a solar prominence and their possible contributions to the heating of the local corona
Yi Bi, Bo Yang, Tng Li +2
The knots in solar prominences are often observed to fall with nearly constant velocity, but the associated physical mechanism is currently not well understood. In this letter, we…
Quasi-periodic pulsation detected in Lyman-alpha emission during solar flares
Dong Li, Lei Lu, Zongjun Ning +3
We investigated the quasi-periodic pulsation (QPP) in Lyman-alpha, X-ray and extreme-ultraviolet (EUV) emissions during two solar flares, i.e., an X-class (SOL2012-01-27T) and a C-…