Published June 1984 | Version v1
Journal article

Flare loops heated by thermal conduction

  • 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