supported by the National Natural Science Foundation of China(Grant Nos.10611120338,10673016,10733020,10921303,41174153 and 11103041);the National Basic Research Program of China(973 Program)(Grant No.2006CB806301)
We analyzed the correlation of the solar magnetograms and Dopplergrams from SOHO/MDI and SDO/HMI respectively. It is found that the full disk correlation coefficient of Dopplergrams is more than 0.80 between SOHO/MDI ...
supported by the National Basic Research Program of China (973 Program, Grant No. 2011CB811406);the National Natural Science Foundation of China(Grant Nos.11273031,10733020,10921303 and 11078010);the China Meteorological Administration grant (No. GYHY201106011)
Three new longitudinal magnetic field parameters are extracted from SOHO/MDI magnetograms to characterize properties of the stressed magnetic field in active regions, and their flare productivities are calculated for ...
supported by the National Basic Research Program of China(Grant No. 2011CB811406);the National Natural Science Foundation of China (Grant Nos. 10921303,10733020,10803011,40890161 and10973020)
ZEUS is a magnetohydrodynamics simulation code widely used in astrophysical research.However,it was recently found that the code may produce artificial shocks in the rarefaction region in some numerical tests since it...
supported by the National Basic Research Program of China(973 Program,No.2011CB811406);the China Meteorological Administration through grant GYHY201106011;the National Natural Science Foundation of China(Grant Nos.10921303, 10733020,10803011,10973020 and 40890161)
Ever since the magnetohydrodynamic (MHD) method for extrapolation of the solar coronal magnetic field was first developed to study the dynamic evolution of twisted magnetic flux tubes, it has proven to be efficient ...
supported by the Young Researcher Grant of National Astronomical Observatories, Chinese Academy of Sciences, the National Basic Research Program of China (973 Program, Grant No. 2011CB811406);the National Natural Science Foundation of China (Grant Nos. 10733020, 10921303, 11003026 and 11078010)
An ensemble prediction model of solar proton events (SPEs), combining the information of solar flares and coronal mass ejections (CMEs), is built. In this model, solar flares are parameterized by the peak flux, th...
Supported by the Important Directional Project of Chinese Academy of Sciences (Grant No. KJCX2-YW-T04);the National Basic Research Program of China (Grant No. 2006CB806301);the National Natural Science Foundation of China (Grant Nos. 10878004, 10733020, and10673016)
In this paper we will summarize the progress in the development of the Chinese Space Solar Telescope (SST) during the past few years. The main scientific objective of SST is to observe the fundamental structure of sol...
Supported by the National Natural Science Foundation of China (Grant Nos. 10611120338, 10473016, 10673016, 60673158, 10733020, and10978015);the National Basic Research Program of China (Grant No. 2006CB806301);the Important Directional Project of Chinese Academy of Sciences (Grant No. KLCX2-YW-T04)
This paper summarizes current helicity measurements in the solar active regions (ARs). There is a basic agreement with the "hemispheric sign rule (HSR)" of the current helicity among different vector magnetographs thr...
Supported by the CAS-NSFC Key Project (Grant No. 10778605);the National Natural Science Foundation of China (Grant Nos. 10733020,10843002, and 10873021);the MOST (Grant No. 2006CB806301);the Young Researcher Grant of National Astronomical Observatories, CAS;the Heavy Rain Research Open Project of IHR, CMA (Grant No. IHR2007G01)
This paper shows some improvements and new results of calibration of Chinese solar radio spectrometer by analyzing the daily calibration data recorded in the period of 1997-2007. First, the calibration coefficient is ...
Supported by the CAS-NSFC Key Project (Grant No. 10778605);the National Natural Science Foundation of China (Grant Nos. 10733020,10843002, and 10873021);the MOST (Grant No. 2006CB806301)
Based on the joint-observations of the radio broadband spectral emissions of the solar eclipse on August 1, 2008 at Jiuquan (total eclipse) and Huairou (partial eclipse) at the frequencies of 2.00-5.60 GHz (Jiuquan), ...