Published 1986
| Version v1
Journal article
Typical development of solar flares with cosmic rays
Description
A synthesis of the typical development of big energetic flares with cosmic and subcosmic rays is given. The courses of many emissions, temperature Te and the emission measure are also presented. A model of various phases of the events in the magnetic topology based on the emergence of a new opposite field in the pre-existing old field is presented. (author)
Additional details
Publishing Information
- Journal Title
- Bull. Astron. Inst. Czech.
- Journal Volume
- 37
- Journal Issue
- 5
- Series
- Bull. Astron. Inst. Czech.
- Journal Page Range
- 314-315
- ISSN
- 0004-6248
- CODEN
- BAICA
INIS
- Country of Publication
- Czech Republic
- Country of Input or Organization
- Serbia and Montenegro
- INIS RN
- 18096952
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMIC RADIATION; GEOMAGNETIC FIELD; GHZ RANGE 01-100; HARD X RADIATION; SOFT X RADIATION; SOLAR FLARES; SUN
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; FREQUENCY RANGE; GHZ RANGE; IONIZING RADIATIONS; MAGNETIC FIELDS; MAIN SEQUENCE STARS; RADIATIONS; SOLAR ACTIVITY; STARS; STELLAR ACTIVITY; STELLAR FLARES; X RADIATION