Type IV dm bursts: onset and sudden reduction
Description
The effect of collisions of suprathermal electrons with a thermal background plasma is investigated and is shown to cause flattening of a monotonically descending velocity distribution of fast particles. As a result flare-produced energetic electrons that are trapped in a coronal magnetic arch and that are initially distributed in energy according to a power-law, can give rise to an instability of Langmuir waves in the background plasma and the subsequent emission of continuum radiation as observed in type IV dm bursts. To explain the appearance of 'sudden reductions' observed in type IV dm outbursts the effects both of magnetic compressions of the source region and of renewed injections of fast particles on the continuum source are investigated. It is found that the latter process can explain the observed reductions. (Auth.)
Additional details
Identifiers
- DOI
- 10.1007/bf00149857;
Publishing Information
- Journal Title
- Solar Physics
- Journal Volume
- 46
- Journal Issue
- 2
- Series
- Sol. Phys.
- Journal Page Range
- 275-290
- ISSN
- 0038-0938
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 8285076
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- DISTRIBUTION; DISTRIBUTION FUNCTIONS; ELECTRON DENSITY; ELECTRONS; ENERGY SPECTRA; KINETIC ENERGY; LOSS CONE; LOSS CONE INSTABILITY; PLASMA; PLASMA WAVES; SOLAR RADIO BURSTS; SUN; VELOCITY
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; ENERGY; FERMIONS; INSTABILITY; LEPTONS; PLASMA INSTABILITY; PLASMA MICROINSTABILITIES; RADIATIONS; RADIOWAVE RADIATION; SOLAR ACTIVITY; SPECTRA; STARS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent