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
20 papers · 1 filter
Magnetic fields in Accretion Discs around Neutron Stars - Consequences for the change of spin
Luca Naso, John Miller, Wlodek Kluzniak
Accretion disks are ubiquitous in the universe and it is generally accepted that magnetic fields play a pivotal role in accretion-disk physics. The spin history of millisecond puls…
Properties of Solar Ephemeral Regions at the Emergence Stage
Shuhong Yang, Jun Zhang
For the first time, we statistically study the properties of ephemeral regions (ERs) and quantitatively determine their parameters at the emergence stage based on a sample of 2988…
Statistics and Classification of the Microwave Zebra Patterns Associated with Solar Flares
Baolin Tan, Chengming Tan, Yin Zhang +2
The microwave zebra pattern (ZP) is the most interesting, intriguing, and complex spectral structure frequently observed in solar flares. A comprehensive statistical study will cer…
Magnetic helicity and energy spectra of a solar active region
Hongqi Zhang, Axel Brandenburg, D. D. Sokoloff
We compute for the first time magnetic helicity and energy spectra of the solar active region NOAA 11158 during 11-15 February 2011 at 20^o southern heliographic latitude using obs…
Homologous Flux Ropes Observed by SDO/AIA
Ting Li, Jun Zhang
We firstly present the Solar Dynamics Observatory observations of four homologous flux ropes in active region (AR) 11745 on 2013 May 20-22. The four flux ropes are all above the ne…
Quasi-periodic wiggles of microwave zebra structures in a solar flare
Sijie Yu, V. M. Nakariakov, L. A. Selzer +2
Quasi-periodic wiggles of microwave zebra pattern structures with period range from about 0.5 s to 1.5 s are found in a X-class solar flare on 2006 December 13 at the 2.6-3.8 GHz w…
Limits to solar cycle predictability: Cross-equatorial flux plumes
R. H. Cameron, M. Dasi-Espuig, J. Jiang +3
Within the Babcock-Leighton framework for the solar dynamo, the strength of a cycle is expected to depend on the strength of the dipole moment or net hemispheric flux during the pr…
Observations of a Quasi-Periodic Fast Propagating Magnetosonic Wave in Multi-Wavelength and Its Interaction with Other Magnetic Structures
Y. D. Shen, Y. Liu, J. T. Su +5
We present an observational study of a quasi-periodic fast propagating (QFP) magnetosonic wave on 2012, April 23. The multiple wave trains were observed along an active region open…
Diffraction, Refraction, and Reflection of An Extreme-Ultraviolet Wave Observed during Its Interactions with Remote Active Regions
Yuandeng Shen, Yu Liu, Jiangtao Su +5
We present observations of the diffraction, refraction, and reflection of a global extreme-ultraviolet (EUV) wave propagating in the solar corona. These intriguing phenomena are ob…
SDO/AIA and Hinode/EIS Observations of Interaction Between an EUV Wave and Active Region Loops
Liheng Yang, Jun Zhang, Wei Liu +2
We present detailed analysis of an extreme ultraviolet (EUV) wave and its interaction with active region (AR) loops observed by the Solar Dynamics Observatory/Atmospheric Imaging A…
Magnetic Nonpotentiality in Photospheric Active Regions as a Predictor of Solar Flares
Xiao Yang, GangHua Lin, HongQi Zhang +1
Based on several magnetic nonpotentiality parameters obtained from the vector photospheric active region magnetograms obtained with the Solar Magnetic Field Telescope at the Huairo…
Coronal magnetic topology and the production of solar impulsive energetic electrons
C. Li, L. P. Sun, X. Y. Wang +1
We investigate two candidate solar sources or active regions (ARs) in association with a solar impulsive energetic electron (SIEE) event on 2002 October 20. The solar particle rele…
Small Scale Microwave Bursts in Long-duration Solar Flares
Baolin Tan
Solar small scale microwave bursts (SMBs), including microwave dot, spike, and narrow band type III bursts, are characterized with very short timescales, narrow frequency bandwidth…
A Peculiar Microwave Quasi-periodic Pulsation with Zigzag Pattern in a CME-related Flare on 2005-01-15
Baolin Tan
A peculiar microwave quasi-periodic pulsation with zigzag pattern (Z-QPP) is observed first by the Chinese Solar Broadband Spectrometer in Huairou (SBRS/Huairou) at 1.10-1.34 GHz i…
Fine-scale Structures of Flux Ropes Tracked by Erupting Material
Ting Li, Jun Zhang
We present the Solar Dynamics Observatory observations of two flux ropes respectively tracked out by material from a surge and a failed filament eruption on 2012 July 29 and August…
Internal-cycle variation of solar differential rotation
K. J. Li, J. L. Xie, X. J. Shi
The latitudinal distributions of the yearly mean rotation rates measured respectively by Suzuki in 1998 and 2012 and Pulkkinen Tuominen in 1998 are utilized to investigate int…
Modeling Solar Cycles 15 to 21 Using a Flux Transport Dynamo
J. Jiang, R. H. Cameron, D. Schmitt +1
Context: The Sun's polar fields and open flux around the time of activity minima have been considered to be strongly correlated with the strength of the subsequent maximum of solar…
Eruption of the magnetic flux rope in a fast decayed active region
Shangbin Yang, Wenbin Xie, Jihong Liu
An isolated and fast decayed active region (NOAA 9729) was observed when passing through solar disk. There is only one CME related with it that give us a good opportunity to invest…
The Induced Electric Field Distribution in Solar Atmosphere
Rong Chen, Zhiliang Yang, Yuanyong Deng
A method of calculating induced electric field is presented in this paper. Induced electric field in solar atmosphere is derived by the time variation of magnetic field when the ch…
A brief report on statistical study of net electric current in solar active regions with longitudinal fields of opposite polarity
Yu Gao
Dynamic processes occurring in solar active regions are dominated by the solar magnetic field. As of now, observations using a solar magnetograph have supplied us with the vector c…