Published March 1981
| Version v1
Journal article
Possibility of predicting solar flares from radio emission characteristics
Description
The possibility of predicting solar flares from radio emission characteristics is examined. Within the framework of S. I. Syrovatskii's model a criterion is derived which allows one, using quantities observed in the radio range, to determine the onset of thermal instability of a current sheet as the start of the explosive phase of a solar flare
Additional details
Publishing Information
- Journal Title
- Sov. Astron. (Engl. Transl.)
- Journal Volume
- 25
- Journal Issue
- 2
- Series
- Sov. Astron. (Engl. Transl.).
- Journal Page Range
- 220-225
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 13701472
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- MAGNETIC FIELDS; PLASMA INSTABILITY; PLASMA SHEET; RADIOWAVE RADIATION; SOLAR FLARES; SOLAR RADIATION
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; INSTABILITY; RADIATIONS; SOLAR ACTIVITY; STELLAR RADIATION