Published March 1972 | Version v1
Journal article

The effect of scattering on solar radio sources at 80 MHz

Creators

  • 1. Commonwealth Scientific and Industrial Research Organization, Epping (Australia). Div. of Radiophysics

Description

Scattering of radiation from solar radio sources by in homogeneities in the electron density structure of the corona can have marked effects on the observed time profile and the brightness distribution. These effects are appreciable for any localized source emitting a brief burst of radiation and are most pronounced when the radiation propagates close to the plasma level; it is such sources, illustrated here by those of type III bursts, that will be considered in this paper.

Additional details

Identifiers

Publishing Information

Journal Title
Publications of the Astronomical Society of Australia
Journal Volume
2
Journal Issue
2
Series
Proc. Astron. Soc. Aust.
Journal Page Range
98-100
ISSN
1323-3580

Conference

Title
Meeting of the Astronomical Society of Australia.
Dates
13 Dec 1971.
Place
Adelaide, Australia.

INIS

Country of Publication
Australia
Country of Input or Organization
Australia
INIS RN
3033060
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ELECTRON DENSITY; ELECTRONS; EMISSION; ISOTROPY; MHZ RANGE 01-100; REFRACTION; SCATTERING; SOLAR CORONA; SOLAR RADIO BURSTS; SUN
Descriptors DEC
ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; FREQUENCY RANGE; LEPTONS; MHZ RANGE; RADIATIONS; RADIOWAVE RADIATION; SOLAR ACTIVITY; STARS

Optional Information

Notes
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