Stellar dynamic spectroscopy
Abstract
The dynamic spectrum, a three dimensional record of the radio intensity as a function both of time and frequency, has long been used as a probe of plasma processes in the solar corona. Beginning with the work of Wild and McCready (1950) dynamic spectroscopy has been used to distinguish between the multitude of radio wave emitting phenomena which occur in the solar corona and to infer the physical mechanisms responsible.
- Publication:
-
Solar Physics
- Pub Date:
- January 1987
- DOI:
- 10.1007/BF00147709
- Bibcode:
- 1987SoPh..113..289B
- Keywords:
-
- Flare;
- Temporal Resolution;
- Radio Wave;
- Solar Corona;
- Dynamic Spectrum