the support received from the National Natural Science Foundation of China (Nos. 11573012, 11303011, 11263004, 11163004 and U1231205);the Open Research Program of the Key Laboratory of Solar Activity of the Chinese Academy of Sciences (Nos. KLSA201414 and KLSA201505)
Six high-resolution TiO-band image sequences from the New Vacuum Solar Telescope (NVST) are used to investigate the properties of intergranular bright points (igBPs). We detect the igBPs using a Laplacian and morp...
supported by the National Natural Science Foundation of China (Nos. U1231205,11163004,11263004 and 11303011);the Open Research Program of Key Laboratory of Solar Activity of Chinese Academy of Sciences (No. KLSA201309);supported by the Opening Project of Key Laboratory of Astronomical Optics&Technology,Nanjing Institute of Astronomical Optics & Technology,Chinese Academy of Sciences (No. CAS-KLAOT-KF201306)
The emission sources of umbral flashes (UFs) are believed to be closely related to running umbral and penumbral waves, and are concluded to be associated with umbral dots in the solar photosphere. Accurate identific...