国家自然科学基金(10673004)

作品数：8被引量：21H指数：3
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MHD Seismology of a loop-like filament tube by observed kink waves被引量：1
《Research in Astronomy and Astrophysics》2015年第10期1713-1724,共12页Vaibhav Pant Abhishek K Srivastava Dipankar Banerjee Marcel Goossens Peng-Fei Chen Navin Chandra Joshi Yu-Hao Zhou 
support from KU Leuven via GOA/2009-009;support from the Interuniversity Attraction Poles Programme initiated by the Belgian Science Policy Office(IAP P7/08 Charm);supported by the Chinese foundations2011CB811402;the National Natural Science Foundation of China(Grant Nos.11025314,10933003 and 10673004)
We report and analyze observational evidence of global kink oscillations in a solar filament as observed in Ha by instruments administered by National Solar Observatory （NSO）/Global Oscillation Network Group （GONG...
关键词：Sun： oscillations -- Sun： magnetic fields -- Sun： filament 
Diagnostics of Ellerman bombs with high-resolution spectral data被引量：1
《Research in Astronomy and Astrophysics》2015年第9期1513-1524,共12页Zhen Li Cheng Fang Yang Guo Peng-Fei Chen Zhi Xu Wen-Da Cao 
supported by the National Natural Science Foundation of China (NSFC, Grants 10878002, 10933003, 11025314, 10673004, 11203014 and 11103075);NKBRSF (Grant Nos. 2011CB811402 and 2014CB744203);the support of the US NSF (AGS0847126 and AGS-1250818);NASA (NNX13AG14G)
Ellerman bombs （EBs） are tiny brightenings often observed near sunspots. The most impressive characteristic of EB spectra is the two emission bumps in both wings of the Hα and Ca II 8542 A lines. High-resolution sp...
关键词：Sun： chromosphere -- Sun： photosphere -- line profiles -- magnetic reconnection 
Hαcounterparts of X-ray bright points in the solar atmosphere
《Science China(Physics,Mechanics & Astronomy)》2012年第5期907-914,共8页ZHANG Ping FANG Cheng ZHANG QingMin 
supported by the National Basic Research Program of China (Grant No.2011CB811402);the National Natural Science Foundation of China (Grant Nos.10878002,10610099,10933003,10673004,10073005,10403003,and 11025314)
X-ray bright points （XBPs） are small-scale brightenings in the solar corona. Their counterparts in the lower atmosphere, how- ever, are poorly investigated. In this paper, we study the counterparts of XBPs in the up...
关键词：solar activity bright points small-scale brightenings 
Recent progress of solar physics research in China被引量：14
《Research in Astronomy and Astrophysics》2011年第12期1377-1402,共26页Cheng Fang 1 School of Astronomy and Space Science,Nanjing University,Nanjing 210093,China 2 Key Laboratory of Modern Astronomy and Astrophysics(Nanjing University),Ministry of Education,China 
supported by the National Natural Science Foundation of China (NSFC, Grant Nos. 10878002, 10610099, 10933003 and 10673004);the National Basic Research Program of China (973 program, 2011CB811402)
Owing to the largely improved facilities and working conditions, solar physics research in China has recently shown marked development. This paper reports on the recent progress of solar physics research in China's Ma...
关键词：Sun： general -- Sun： coronal mass ejections （CMEs） -- solar physics：recent progress 
Detailed analysis of fan-shaped jets in three dimensional numerical simulation被引量：2
《Research in Astronomy and Astrophysics》2011年第6期701-724,共24页Rong-Lin Jiang K.Shibata H.Isobe Cheng Fang 
Supported by the National Natural Science Foundation of China (NSFC,Grant Nos. 10878002,10610099,10933003 and10673004);a grant from the National Basic Research Program of China (973 project,No. 2011CB811402);support and under the auspices of the NIFS Collaboration Research program (NIFS07KTBL005);performed with the KDK system of the Research Institute for Sustainable Humanosphere (RISH) at Kyoto University, as a collaborative research project
We performed three dimensional resistive magnetohydrodynamic simulations to study the magnetic reconnection using an initially shearing magnetic field configuration（force free field with a current sheet in the middle...
关键词：MAGNETOHYDRODYNAMICS MHD-methods NUMERICAL 
Numerical simulations of magnetic reconnection in the lower solar atmosphere被引量：4
《Research in Astronomy and Astrophysics》2011年第2期225-236,共12页Xiao-Yan Xu 1,2,Cheng Fang 2,Ming-De Ding 2 and Dan-Hui Gao 2 1 Purple Mountain Observatory,Chinese Academy of Science,Nanjing 210008,China 2 Department of Astronomy,Nanjing University,Nanjing 210093,China 
supported by the National Natural Science Foundation of China (Grant Nos. 10221001,10333040,10403003,10620150099,10610099 and 10673004);by the Major State Basic Research Development Program (973 project 2006CB806302)
Observations indicate that Ellerman bombs （EBs） and chromospheric microflares both occur in the lower solar atmosphere,and share many common features,such as temperature enhancements,accompanying jet-like mass motio...
关键词：Sun： chromosphere-- Sun： photosphere -- Sun： magnetic reconnection-- Sun： numerical simulation 
The inversion of the real kinematic properties of coronal mass ejections by forward modeling被引量：3
《Research in Astronomy and Astrophysics》2011年第2期237-244,共8页You Wu 1 and Peng-Fei Chen 1,2 1 Department of Astronomy,Nanjing University,Nanjing 210093,China 2 Key Lab of Modern Astron.and Astrophys.,Ministry of Education,Nanjing 210093,China 
supported by the National Basic Research Program of China(No.2011CB811402);the National Natural Science Foundation of China (Grant Nos.11025314,10403003,10933003 and 10673004)
Kinematic properties of coronal mass ejections （CMEs） suffer from projection effects,and it is expected that the real velocity should be larger and the real angular width should be smaller than the apparent values.S...
关键词：Sun： coronal mass ejections （CMEs） -- methods： statistical -- methods：numerical 
Why are halo coronal mass ejections faster?被引量：3
《Research in Astronomy and Astrophysics》2010年第5期461-472,共12页Qing-Min Zhang Yang Guo Peng-Fei Chen Ming-De Ding Cheng Fang 
Supported by the National Natural Science Foundation of China;supported by the Chinese foundations (GYHY200706013, 2006CB806302);the National Natural Science Foundation of China (Grant Nos. 10403003, 10933003 and 10673004);SOHO is a project of international cooperation between ESA and NASA
Halo coronal mass ejections （CMEs） have been to be significantly faster than normal CMEs, which is a long-standing puzzle. In order to solve the puzzle, we first investigate the observed properties of 31 limb CMEs t...
关键词：Sun： coronal mass ejections （CMEs） — Sun： activity — methods： nu-merical — solar-terrestrial relations 
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