the University Grants Commission,India for providing a Non-NET fellowship。
We study the nonlinear coupling of kinetic Alfvén waves with ion acoustic waves applicable to the Earth’s radiation belt and near-Sun streamer belt solar wind using dynamical equations in the form of modified Zakhar...
supported by Yunnan Revitalization Talent Support Program(202305AS350029 and 202305AT350005);Yunnan Key Laboratory of Solar Physics and Space Science(202205AG070009)。
The near-infrared imaging channel constitutes a crucial component of the multichannel high-resolution imaging system of the New Vacuum Solar Telescope(NVST). We have successfully achieved high-resolution, narrowband i...
supported by the National Key R&D Program of China under grants 2022YFF0503003(2022YFF0503000)and 2018YFA0404200;the National Natural Science Foundation of China(NSFC,Grant Nos.11921003,11973012,and 11820101002);CAS Strategic Pioneer Program on Space Science(Grant Nos.XDA15018300,XDA15052200,XDA15320103,and XDA15320301);the mobility program(M-0068)of the Sino-German Science Center。
Lyα(Lyα,1216 A)is the strongest emission line in the solar ultraviolet spectrum.In the present work,we obtained a Lyαenhancement catalog covering flares larger than B1 class from the GOES/EUVS data during 2010-2016...
supported by the International Space Science Institute (ISSI),Bern,Switzerland and ISSI-Beijing,China。
A combined uniform and long-time series of Ca-K images from the Kodaikanal Observatory,Mount Wilson Observatory and Mauna Loa Solar Observatory was used to identify and study the Ca-K small-scale features and their so...
sponsored by the National Natural Science Foundation of China (NSFC) under Grant Nos.11873027, U2031140, 12073077, 11833010 and 11973088;West Light Foundation of the Chinese Academy of Sciences (Y9XB01A and Y9XB019)。
Suppressing the interference of atmospheric turbulence and obtaining observation data with a high spatial resolution are an issue to be solved urgently for ground observations. One way to solve this problem is to perf...
We present findings from an analysis of the fractal dimension of solar supergranulation as a function of latitude,supergranular cell size and solar rotation, employing spectroheliographic data in the Ca II K line of s...
the National Natural Science Foundation of China(NSFC,Grant Nos.11527804,U1931206,11373065,11078005,10943002 and 12003066)。
This paper presents the analytical results of solar MgⅠb_(2)flash spectra,obtained by the prototype Fiber Arrayed Solar Optic Telescope in process of the 2013 Gabon total solar eclipse.The analysis reveals irregular ...
the National Key R&D Program of China (Grant No. 2021YFA1600500) and mobility program (Grant No. M-0068) of the Sino-German Science Center;financial support by the UKs Science and Technology Facilities Council (STFC) (Grant Nos. ST/S000402/1 and ST/W001195/1) financial support by DLR-grant 50 OC 2101。
Understanding structures and evolutions of the magnetic fields and plasma in multiple layers on the Sun is very important. A force-free magnetic field which is an accurate approximation of the solar corona due to the ...
supported by China National Space Administration(CNSA)。
The Chinese Hα Solar Explorer(CHASE), dubbed “Xihe”—Goddess of the Sun, was launched on October 14, 2021 as the first solar space mission of China National Space Administration(CNSA). The CHASE mission is designed...
The Hα line is an important optical line in solar observations containing the information from the photosphere to the chromosphere. To study the mechanisms of solar eruptions and the plasma dynamics in the lower atmo...