Published 1989
| Version v1
Book
Classification of solar flares
Creators
- 1. California Univ., Berkeley (USA)
- 2. Harvard College Observatory, Cambridge, MA (USA)
- 3. California Univ., San Diego (USA)
Description
The historical background of solar flare classification before the SMM launch is reviewed along with recent developments made by observations with SMM, Hinotori, and other contemporary satellite and ground-based observations. Based on these recent findings, solar flares are grouped into five classes: thermal hard X-ray flares, nonthermal hard X-ray flares, impulsive gamma-ray/proton flares, gradual gamma-ray/proton flares, and quiescent filament-eruption flares. The roles of filament eruptions in flare development are examined, and theoretical ideas related to processes occurring in different flare classes are discussed. 204 refs
Additional details
Publishing Information
- Publisher
- Annual Reviews, Inc.
- Imprint Place
- Palo Alto, CA (USA)
- Imprint Title
- Annual review of astronomy and astrophysics. Volume 27
- Imprint Pagination
- 784 p.
- Journal Page Range
- p. 421-467.
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 21069289
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- GAMMA RADIATION; HARD X RADIATION; HISTORICAL ASPECTS; ORGANIZING; SATELLITES; SKYLAB; SOLAR ATMOSPHERE; SOLAR FLARES; SOLAR PROMINENCES; SOLAR RADIO BURSTS; X RADIATION
- Descriptors DEC
- ATMOSPHERES; ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; RADIATIONS; RADIOWAVE RADIATION; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR ATMOSPHERES; STELLAR FLARES