Analysis of solar radio imaging-spectroscopic observations
- 1National Astronomical Observatories, Chinese Academy of Sciences, CAS Key Lab of Solar Activity, Beijing, China (yyh@nao.cas.cn)
- 2University of Chinese Academy of Sciences, School of Astronomy & Space Science, Beijing, China
Solar radio fine structures observed in wide frequency ranges are manifestations of the physical processes related to the energy release, particle accelerations and propagations, etc. The locations of these fine structures are mostly not clear so it is important to have imaging spectroscopic observations to address these problems.
Mingantu Spectral Radioheliograph (MUSER) is an aperture-synthesis imaging telescope, dedicated to observe the Sun, operating on multiple frequencies in dm to cm range. The ability of MUSER allows one to diagnose coronal magnetic field and the plasma parameters such as electron beam velocity, density, spectral index, etc.
During 2014 to 2019, MUSER has registered a number of solar radio bursts corresponding to 2 X-class, 15 M-class, 38 C-class, 19 B-class, 4 A-class and 5 below A-class flares as well as quiet Sun observations. Here we demonstrate some interesting events from MUSER imaging-spectroscopic observations.
How to cite: Yan, Y., Zhang, M., Zhou, Z., Chen, X., Tan, C., Tan, B., Wang, W., Chen, L., Liu, F., Geng, L., Chen, Z., Zhang, Y., and Team, M.: Analysis of solar radio imaging-spectroscopic observations, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-21394, https://doi.org/10.5194/egusphere-egu2020-21394, 2020
