partly supported by RFBR projects 13-02-91165 and 15-32-21078;MOST (973 program,2011CB811402);National Natural Science Foundation of China (11233008 and 11427803)
From the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESS1) catalog we select events which have approximately the same GOES class (high C - low M or 500-1200 counts s-1 within the RHESSI 6-12 keV energy ...
supported by the National Natural Science Foundation of China (Grant Nos. 11111120071, 10833007, 11173062, 11221063 and 11178002);the National Basic Research Program of China (973 Program, 2011CB811402);supported by the Chinese Academy of Sciences visiting professorship for senior international scientists (Grant No. 2010t2j36);by the joint RFBR-CNSF (Grant No. 11-02-91175)
We carry out a detailed analysis of the X3.5 solar flare that occurred on 2002 July 20, which is the strongest partially limb-occulted flare ever observed by the RHESSI satellite. The main results are: (1) during t...
supported by the National Natural Science Foundation of China(Grant Nos.10833007,11173062,10921303,11178002,10928307and11111120071);the National Basic Research Program of China(973program,Grant No.2011CB811402);supported by the Chinese Academy of Sciences via a visiting professorship for senior international scientists with grant No.2010t2j36;by the joint RFBR-CNSF(Grant No.11-02-91175);supported by the Open Research Program of the Key Laboratory of Solar Activity ofNational Astronomical Observatories;the Scientific Research Foundation of Nanjing Universityof Information Science and Technology(Grant Nos.S8110136001and N1081005072)
With the aim of studying the relationship between the relative motions of the loop-top (LT) source and footpoints (FPs) during the rising phase of solar flares, we give a detailed analysis of the X7.1 class flare ...
Supported by the National Natural Science Foundation of China(Grant Nos. 10773032,11073058 and 10833007);the National Basic Research Program of China (973 program,No. 2011CB811402)
Based on Dulk and Marsh's approximate theory about nonthermal gyrosyn- chrotron radiation, one simple impulsive microwave burst with a loop-like structure is selected for radio diagnostics of the coronal magnetic fie...
supported by the National Natural Science Foundation of China(Grant Nos.10873038 and 10833007);the National Basic Research Program of China(973Program,2011CB811402).
We statistically study the properties of emerging flux regions(EFRs)and response of the upper solar atmosphere to the flux emergence using data from the Helioseismic and Magnetic Imager and the Atmospheric Imaging A...