Observations of solar radio bursts from meter to kilometer wavelengths
Description
New results obtained with the Clark Lake multifrequency radioheliograph at meter-decameter wavelengths and from satellite multifrequency directive observations at hectometer and kilometer wavelengths are reviewed. Evidence is presented that type III electrons propagate in dense coronal streamers and that frequently observed microbursts (presumably type III) at meter-decameter wavelengths are due to plasma radiation. Observations of hectometer and kilometer type III radio storms which reveal information about active region structures, the interplanetary magnetic field configuration, and solar wind acceleration are discussed. Kilometer type II bursts and interactions between type III electrons and interplanetary shocks are examined, and some new results on shock-associated events are presented. 23 references
Additional details
Publishing Information
- Journal Title
- Adv. Space Res.
- Journal Volume
- 4
- Series
- Adv. Space Res.
- Journal Page Range
- 261-270
- ISSN
- 0273-1177
- CODEN
- ASRSD
Conference
- Title
- 25. plenary session of COSPAR.
- Dates
- 25 Jun - 7 Jul 1984.
- Place
- Graz (Austria).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 17014582
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- LONG WAVE RADIATION; SOLAR CORONA; SOLAR ELECTRONS; SOLAR RADIO BURSTS; SOLAR WIND
- Descriptors DEC
- ATMOSPHERES; ELECTROMAGNETIC RADIATION; ELECTRONS; ELEMENTARY PARTICLES; FERMIONS; LEPTONS; RADIATIONS; RADIOWAVE RADIATION; SOLAR ACTIVITY; SOLAR ATMOSPHERE; SOLAR PARTICLES; SOLAR RADIATION; STELLAR ACTIVITY; STELLAR ATMOSPHERES; STELLAR CORONAE; STELLAR RADIATION; STELLAR WINDS
Optional Information
- Secondary number(s)
- CONF-8406167--.