Published 1984
| Version v1
Journal article
Interpretation of hard X-ray images during the impulsive phase of a limb flare
Creators
- 1. Observatorio Nacional de Fisica Cosmica, San Miguel, Argentina
Description
It is shown that the observations of a limb flare, in which a hard X-ray (16-30 keV) source is seen at the boundary between two interacting magnetic structures, indicate the presence of hot (T approximately equal to or greater than 10 to the 7th K) plasma within the region. Nonthermal bremsstrahlung processes do not agree with these observations. The possible causes of the heating are discussed. 5 references
Additional details
Publishing Information
- Journal Title
- Adv. Space Res.
- Journal Volume
- 4
- Series
- Adv. Space Res.
- Journal Page Range
- 237-241
- ISSN
- 0273-1177
- CODEN
- ASRSD
Conference
- Title
- 25. plenary session of COSPAR.
- Dates
- 25 Jun - 7 Jul 1984.
- Place
- Graz (Austria).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 17014577
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BREMSSTRAHLUNG; HARD X RADIATION; SOLAR FLARES; X RADIATION
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; RADIATIONS; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR FLARES
Optional Information
- Secondary number(s)
- CONF-8406167--.