Published February 1976
| Version v1
Journal article
Directivity in the stream-plasma interaction
- 1. Observatoire de Paris, Section de Meudon, 92 (France)
Description
Center-to-limb variations indicate that a type III burst is likely to be emitted in a radial direction while a type IIIb emission is more perpendicular to the stream. (Auth.)
Additional details
Identifiers
- DOI
- 10.1007/bf00149877;
Publishing Information
- Journal Title
- Solar Physics
- Journal Volume
- 46
- Journal Issue
- 2
- Series
- Sol. Phys.
- Journal Page Range
- 505-507
- ISSN
- 0038-0938
Conference
- Title
- Mechanisms for solar type III radio bursts.
- Dates
- 8 May 1975.
- Place
- Berkeley, Calif., USA.
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 8285219
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ELECTRONS; MHZ RANGE 01-100; PLASMA; SOLAR RADIO BURSTS; SOLAR WIND; SUN
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; FREQUENCY RANGE; LEPTONS; MHZ RANGE; RADIATIONS; RADIOWAVE RADIATION; SOLAR ACTIVITY; STARS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent