๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Flare loops heated by thermal conduction

โœ Scribed by David M. Rust; Boris V. Somov


Book ID
104647227
Publisher
Springer
Year
1984
Tongue
English
Weight
753 KB
Volume
93
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

โœฆ Synopsis


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 10 j~ cm, rose to temperatures of 21.5 x 10 6 K and 30 x 10 6 K, respectively, in 30 s. Assuming equal heat flux Finto 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 = (~(FL,'/r 2 7, which gives a loop temperture 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 ~ 5 x 10 9 ergs cm-z s -~. 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.


๐Ÿ“œ SIMILAR VOLUMES


A model of impulsive loop flares caused
โœ T. Takakura ๐Ÿ“‚ Article ๐Ÿ“… 1992 ๐Ÿ› Springer ๐ŸŒ English โš– 541 KB

Numerical simulation is made of the impulsive loop flare caused by transient heat conduction along the loop with an applied axial electric current. It is assumed that a segment near the top of the coronal loop is heated to above 107 K by a heat input that is small compared with the total flare ener

The effect of nonlinear conduction on th
โœ K. R. Krall ๐Ÿ“‚ Article ๐Ÿ“… 1977 ๐Ÿ› Springer ๐ŸŒ English โš– 180 KB

Attention is drawn to consequences of the non-linear nature of thermal conductivity on the cooling rate of solar flares.

Effect of thermal conduction and radiati
โœ S. T. Wu; L. C. Kan; Y. Nakagawa; E. Tandberg-Hanssen ๐Ÿ“‚ Article ๐Ÿ“… 1981 ๐Ÿ› Springer ๐ŸŒ English โš– 562 KB

A systematic study of the effects of thermal conduction and radiation (Cox-Tucker type) on the dynamic response of a coronal loop is presented. The study is based on a one-fluid hydrodynamic description of a magnetic flux loop subject to a sudden localized heating, simulating the flare energy releas

Influence of magnetic field structure on
โœ S. K. Antiochos; P. A. Sturrock ๐Ÿ“‚ Article ๐Ÿ“… 1976 ๐Ÿ› Springer ๐ŸŒ English โš– 388 KB

A simple model facilitates calculation of the influence of magnetic field configuration on the conduction cooling rate of a hot post-flare coronal plasma. The magnetic field is taken to be that produced by a line dipole or point dipole at an arbitrary depth below the chromosphere. For the high tempe

The effects of magnetic structure on the
โœ Gerard Hoven ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Springer ๐ŸŒ English โš– 302 KB

A model of the sheared magnetic field in a coronal loop is used to evaluate the average cross-field suppression of axial thermal conduction. If the energy source is uniform in radius, this can lead to heat-flux reduction by a factor greater than three. When the source is annular, in a region of radi