On the Observation of Scattered Radio Emission from Sources in the Solar Corona
Abstract
The effects of scattering and refraction on radio waves in the solar corona are considered for several different coronal models. By considering a source near the plasma level in a spherically symmetric corona and in a streamer enhancement superimposed on a spherically symmetric corona we obtain results relating to bursts of types I, II and III.
- Publication:
-
Solar Physics
- Pub Date:
- March 1974
- DOI:
- 10.1007/BF00156964
- Bibcode:
- 1974SoPh...35..153R
- Keywords:
-
- Radiation;
- Plasma Level;
- Refraction;
- Source Radiation;
- Radio Wave