Published July 1981 | Version v1
Journal article

Two observable effects in the radio bremsstrahlung of nonsteady solar sources

Creators

  • 1. Inst. of Terrestrial Magnetism, the Ionosphere, and Radio-Wave Propagation, USSR Academy of Sciences, Troitsk, Moscow Oblast'

Description

The excess in the rate of change of circularly polarized radiation compared with the rate of change of the intensity in the microwave range can serve as a criterion (a sufficiency condition) for the presence of time variations in the longitudinal magnetic field component in a nonsteady solar source. Heating of an optically thin source in a magnetic loop could produce a dip in the observed radio emission

Additional details

Publishing Information

Journal Title
Sov. Astron. Lett. (Engl. Transl.)
Journal Volume
7
Journal Issue
4
Series
Sov. Astron. Lett. (Engl. Transl.).
Journal Page Range
272-274

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
14744483
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
BREMSSTRAHLUNG; BRIGHTNESS; MAGNETIC FIELDS; MICROWAVE RADIATION; POLARIZATION; RADIOWAVE RADIATION; SOLAR RADIATION; VARIATIONS
Descriptors DEC
ELECTROMAGNETIC RADIATION; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS; STELLAR RADIATION