A study of type V solar radio bursts. II. A theoretical model.
Abstract
A model for the solar Type V event is developed. This model assumes that the basic difference between Type III and Type V bursts is the evolution of the electron beam. For a Type V this beam rapidly elongates, so that it takes progressively longer times to pass higher plasma levels. Physical process influencing the beam development, including Coulomb collisions, non-linear interactions with Langmuir waves and wave-particle scattering from various hydromagnetic wave modes is discussed. The model is compared with previously derived models and with observations.
- Publication:
-
Solar Physics
- Pub Date:
- February 1978
- DOI:
- 10.1007/BF00152480
- Bibcode:
- 1978SoPh...56..405R
- Keywords:
-
- Electron Beams;
- Type 5 Bursts;
- Circular Polarization;
- Coulomb Collisions;
- Electron Distribution;
- Plasma Waves;
- Polarization Characteristics;
- Type 3 Bursts;
- Wave Interaction;
- Wave Scattering;
- Solar Physics;
- Electron Beam;
- Physical Process;
- High Plasma;
- Type Versus;
- Wave Mode;
- Solar Radio Bursts:Models