A new plasma emission model for bright, slowly moving type IV solar radio bursts
Abstract
As a model of bright, slowly moving type IV bursts, coalescence of oblique Bernstein modes into predominantly o-mode waves is proposed. Bernstein mode instability is supposed in an adiabatically compressed plasma within the current sheet associated with the underlying traveling coronal disturbance.
- Publication:
-
Contributions of the Astronomical Observatory Skalnate Pleso
- Pub Date:
- 1986
- Bibcode:
- 1986CoSka..15..709K