Diagnostics of Coronal Magnetic Field in Terms of Radio Burst and Fine Structures
Abstract
A complex solar radio burst was observed on 19 October 2001 with the spectrometers of NAOC (National Astronomical Observatory of China) and Nobeyama Radioheliograph (NoRH). Basing on the analysis of brightness temperature spectra of radio sources and various fine spectral structures, we get a diagnosis of magnetic field of radio active region.
- Publication:
-
Coronal and Stellar Mass Ejections
- Pub Date:
- 2005
- DOI:
- 10.1017/S1743921305000372
- Bibcode:
- 2005IAUS..226..137W