Published August 1972
| Version v1
Journal article
Plasma emission processes in a magnetoactive plasma
Description
Plasma emission (i.e. emission at about the plasma frequency and twice this frequency) is treated taking into account the effects of the magnetic field on the electron plasma waves, on the conversion processes, and on the escaping radiation. The expected degrees of polarization of the fundamental and second harmonic are calculated in the weak field limit. The results are used to estimate the magnetic field strength B at the 80 MHz level from the observed polarization of type III bursts; the result B < 0·04 G is smaller than previous estimates. The possible importance of electron-cyclotron waves in an application to type I bursts is noted.
Additional details
Identifiers
- DOI
- 10.1071/ph720387;
Publishing Information
- Journal Title
- Australian Journal of Physics
- Journal Volume
- 25
- Journal Issue
- 4
- Series
- Aust. J. Phys.
- Journal Page Range
- 387-402
- ISSN
- 0004-9506
INIS
- Country of Publication
- Australia
- Country of Input or Organization
- Australia
- INIS RN
- 3032827
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CONVERSION; ELECTRONS; EMISSION; LANGMUIR FREQUENCY; MAGNETIC FIELDS; MHZ RANGE 01-100; PLASMA; PLASMA WAVES; POLARIZATION; SCATTERING; SOLAR RADIO BURSTS
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; FREQUENCY RANGE; LEPTONS; MHZ RANGE; RADIATIONS; RADIOWAVE RADIATION; SOLAR ACTIVITY
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent