funded by the National Basic Research Program of China (973 Program,Grants 2012CB957801 and 2014CB744203);the National Natural Science Foundation of China (Grant Nos.41074132,41274193,41474166,41304144,11303017 and 11533005);the National Standard Research Program (Grant 200710123)
To investigate the dependence of large gradual solar energetic particle(SEP) events on the associated flares and coronal mass ejections(CMEs), the correlation coefficients(CCs) between peak intensities of E 〉 1...
jointly funded by the National Basic Research Program of China (973 Program, Grants 2012CB957801 and 2014CB744203);the National Natural Science Foundation of China (Grants 41074132, 41274193, 41474166, 41304144, 11303017 and 11533005);the National Standard Research Program (Grant 200710123)
To investigate the possible solar source of high-energy protons, correlation coefficients between the peak intensities of E ≥ 100 MeV protons, I100, and the peak flux and fluence of solar soft X-ray(SXR) emission, ...
Supported by the National Natural Science Foundation of China;supported by the Natural Science Foundation of China (Grant No. 11133001);the National Basic Research Program of China (973 Program, 2009CB824800);the Qinglan project of Jiangsu Province
We perform numerical calculations to simulate the evolution of low-mass X-ray binary systems. For the accreting compact object we consider the initial mass of 1.4, 10, 20, 100, 200, 500 and 1000 Mo, corresponding to n...
Supported by National Basic Research Program of China (973 Program) (2007CB815004);Shanghai Development Foundation from Science and Technology (06JC14082, 06QA14062);National Natural Science Foundation of China (10535010, 10775167)
Hard photon emitted from energetic heavy ion collisions is of very interesting since it does not experience the late-stage nuclear interaction, therefore it is useful to explore the early-stage information of matter p...