funded by the SinoSouth Africa Joint Research on Polar Space Environment(2021YFE0106400);International Cooperation Project on Scientific and Technological Innovation Between Governments;National Key Plans on Research and Development,Ministry of Science and Technology,China;the Special Fund of the Institute of Geophysics,China Earthquake Administration(Grant No.DQJB21X26);CAS Key Laboratory of Solar Activity under No.KLSA202109;the National Natural Science Foundation of China(Grant Nos.41074132,41474166,41774195 and 41774085)。
We studied the properties of the main phases of 24 super geomagnetic storms(SGSs)(ΔSYM-H≤-250 nT)since 1981.We divided the SGSs into two subgroups:SGSs-Ⅰ(-400 nT<ΔSYM-H≤-250 nT)and SGSs-Ⅱ(ΔSYM-H≤-400 nT).Of th...
supported by Sino-South Africa Joint Research on Polar Space Environment (2021YFE0106400);International Cooperation Project on Scientific and Technological Innovation Between Governments;National Key Plans on Research and Development,Ministry of Science and Technology,China;CAS Key Laboratory of Solar Activity under number KLSA (grant No.KLSA202109);the National Natural Science Foundation of China (grant Nos.41074132,41274193,41474166,41774195 and 41874187)。
An interplanetary shock and a magnetic cloud(MC) reached the Earth on 2012 July 14 and 15 one after another.The shock sheath and the MC triggered an intense geomagnetic storm.We find that only small part of the MC fro...
This work was supported by the National Natural Science Foundation of China(Grant Nos.41774085,41074132,41274193,41474166,41774195 and 41874187).
Extreme space weather events including≥X5.0 flares,ground level enhancement(GLE)events and super geomagnetic storms(Dst≥-250 nT)caused by super active regions(SARs)during solar cycles 21-24 were studied.The total nu...
funded by the National Natural Science Foundation of China(Grant Nos.41674166,41074132,41274193 and 41304144);the National Standard Research Program(Grant 200710123)
According to the solar proton data observed by Geostationary Operational Environmental Satellites (GOES), ground-based neutron monitors on Earth and near-relativistic electron data measured by the ACE spacecraft, th...
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...
supported by the National Basic Research Program of China (973 Program,Grant No.2012CB957801);the National Natural Science Foundation of China (Grant Nos.41074132,41274193,41674166,41031064 and 11303017);the National Standard Research Program (Grant No.200710123);the project 985 of Nanjing University,the Advanced Discipline Construction Project of Jiangsu Province and the NKBRSF (Grant No.2014CB744203)
The intensity-time profiles of solar proton events(SPEs) are grouped into three types in the present study. The Type-I means that the intensity-time profile of an SPE has one peak, which occurs shortly after the ass...
Supported by the National Natural Science Foundation of China (Grant Nos. 41074132, 41274193, 40931056 and 41031064);the National Basic Research Program of China (973 Program, Grant Nos. 2012CB957801 and 2011CB811406);the National Standard Research Program (Grant No. 10-123);the program SOA Key Laboratory for Polar Science, Polar Research Institute of China (Grant No. KP201206)
This is a study designed to analyze the relationship between ground level enhancements(GLEs)and their associated solar active regions during solar cycles 22and 23.Results show that 90.3%of the GLE events that are in...
supported by the National Basic Research Program of China (973 Program, Grant Nos. 2012CB957801 and 2011CB811406);the National Natural Science Foundation of China (Grant Nos. 41074132, 41274193 and 40931056);the National Standard Research Program (Grant No. 10-123)
We examine the solar cycle distribution of major geomagnetic storms (Dst ≤ -100 nT), including intense storms at the level of -200 nT〈 Dst ≤ -100 nT, great storms at -300 nT〈 Dst ≤-200 nT, and super storms at D...
supported by the National Natural Science Foundation of China(41074132,40931056);the Foundation for Standout Youth of Anhui Province(2010SQRL039)
A range of analysis approaches,namely continuous wavelet,cross wavelet,and wavelet coherence analyses,are employed to clarify the phase relationship between the smoothed monthly mean sunspot number and solar 10.7 cm f...