期刊： SOLAR PHYSICS, 2021; 296 (8)
We report quasi-periodic pulsations (QPPs) with double periods during three solar flares (viz. SOL2011-Feb-15T01:44, SOL2011-Sep-25T04:31, SOL2012-May......
期刊： SOLAR PHYSICS, 2021; 296 (4)
In this study, we investigate the energy partition of four confined circular-ribbon flares (CRFs) that occurred close to solar disk center. The flares......
期刊： SOLAR PHYSICS, 2021; 296 (4)
Solar coronal mass ejections (CMEs) are known for their space-weather and geomagnetic consequences. Among all CMEs, the so-called radio-loud (RL) and ......
期刊： SOLAR PHYSICS, 2021; 296 (6)
We examine resonantly damped kink modes in straight coronal slabs, paying special attention to the effects of the formulation for the transverse densi......
期刊： SOLAR PHYSICS, 2021; 296 (7)
Coronal mass ejections (CMEs) belong to the most energetic explosions in the solar atmosphere, and their occurrence rates exhibit obvious solar cycle ......
期刊： SOLAR PHYSICS, 2021; 296 (9)
The solar activity cycle varies in amplitude. The last Solar Cycle 24 is the weakest in the past century. Sun's activity dominates Earth's space envir......
期刊： SOLAR PHYSICS, 2021; 296 (4)
The National Science Foundation's Daniel K. Inouye Solar Telescope (DKIST) will revolutionize our ability to measure, understand, and model the basic ......
期刊： SOLAR PHYSICS, 2021; 296 (5)
This article proposes a new model for predicting sunspot activity based on the inverse number and intelligent fixed point. Firstly, in the training ph......
期刊： SOLAR PHYSICS, 2021; 296 (4)
We use Delta SYM-H to capture the variation in the SYM-H index during the main phase of a geomagnetic storm. We define great geomagnetic storms as tho......
期刊： SOLAR PHYSICS, 2021; 296 (3)
The Joint Total Solar Irradiance Monitor (JTSIM) is due to fly onboard the Fengyun-3E spacecraft and aims to measure the Total Solar Irradiance (TSI) ......
期刊： SOLAR PHYSICS, 2021; 296 (3)
Spectroscopic observations at extreme- and far-ultraviolet wavelengths have revealed systematic upflows in the solar transition region and corona. The......
期刊： SOLAR PHYSICS, 2021; 296 (3)
The Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory (SDO) (launched in February 2010) provides uninterrupted full-disk sola......
期刊： SOLAR PHYSICS, 2021; 296 (1)
We studied the statistical and solar cycle distribution of daily flux >= 109 cm-2d(-1)sr(-1) for E>2 MeV electrons Observed by GOES from 1987 to......
期刊： SOLAR PHYSICS, 2021; 296 (1)
Coronal holes are well accepted to be source regions of the fast solar wind. As one of the common structures in coronal holes, coronal plumes might co......
期刊： SOLAR PHYSICS, 2021; 296 (1)
The solar chromosphere data products of the New Vacuum Solar Telescope (NVST) have been affected by the interference fringes since its first operation......
