Flare loops heated by thermal conduction
Creators
- 1. American Science and Engineering, Inc., Cambridge, MA
- 2. AN SSSR, Moscow. Fizicheskij Inst.
Description
A flare observed with the Hard X-Ray Imaging Spectrometer (HXIS) was studied during its rise to maximum temperature and X-ray emission rate. Two proximate flare loops, of lengths 2.8 x 109 cm and 1.1 x 1010 cm, rose to temperatures of 21.5 x 106 K and 30x106 K, respectively, in 30 s. Assuming equal heat flux F into each loop from a thermal source at the point where they met, we derive a simple relationship between temperature T and loop length L: T = (7/2 (FL/K))sup(2/7), which gives a loop temperature ratio of 0.68, in close agreement with the observed ratio of 0.72. The observations imply that heating in each loop was maintained by a thermal flux of approx.= 5 x 109 ergs cm-2 s-1. It is suggested that conductive heating adequately describes the rise and maximum phase emissions in the loops and that long flare loops reach higher temperatures than short loops during the impulsive phase because of an equipartition of energy between them at their point of interaction. (orig.)
Additional details
Publishing Information
- Journal Title
- Sol. Phys.
- Journal Volume
- 93
- Journal Issue
- 1
- Series
- CODEN: SLPHA.;Sol. Phys.
- Journal Page Range
- 95-104
- ISSN
- 0038-0938
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 16008395
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BALMER LINES; DIAGRAMS; HARD X RADIATION; HEAT FLUX; IMAGES; SOLAR FLARES
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; INFORMATION; IONIZING RADIATIONS; RADIATIONS; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR FLARES; X RADIATION