6 citations · 8 across the 6 of their papers we have counts for
6 papers
Chromospheric modeling of the active M3V star G 80-21 with RH1.5D
Shuai Liu, Huigang Wei, Jianrong Shi +4
This study investigates the active regions of the M3.0V star G 80-21 using the observed data from the CARMENES project with synthetic spectra generated by the RH1.5D radiative tran…
Magnetic helicity evolution during active region emergence and subsequent flare productivity
Zheng Sun, Ting Li, Quan Wang +3
Aims. Solar active regions (ARs), which are formed by flux emergence, serve as the primary sources of solar eruptions. However, the specific physical mechanism that governs the eme…
Study of Reconnection Dynamics and Plasma Relaxation in MHD simulation of a Solar Flare
Satyam Agarwal, Ramit Bhattacharyya, Shangbin Yang
Self-organization in continuous systems is associated with dissipative processes. In particular, for magnetized plasmas, it is known as magnetic relaxation, where the magnetic ener…
An Automatic Approach for Grouping Sunspots and Calculating Relative Sunspot Number on SDO/HMI Continuum Images
Cui Zhao, Shangbin Yang, Tingmei Wang +4
Relative Sunspot Number is one of the major parameters for the study of long-term solar activity. The automatic calculation of the Relative Sunspot Number is more stable and accura…
Observations of Magnetic Helicity Proxies in Solar Photosphere: Helicity with Solar Cycles
Hongqi Zhang, Shangbin Yang, Haiqing Xu +3
Observations of magnetic helicity transportation through the solar photosphere reflect the interaction of turbulent plasma movements and magnetic fields in the solar dynamo process…
Change ratios of magnetic helicity and magnetic free energy during major solar flares
Quan Wang, Mei Zhang, Shangbin Yang +2
Magnetic helicity is an important concept in solar physics, with a number of theoretical statements pointing out the important role of magnetic helicity in solar flares and coronal…