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The Physics of Solar Flares || High-Temperature Plasma in Solar Flares

โœ Scribed by G. A. Doschek

Book ID
123645500
Publisher
The Royal Society
Year
1991
Tongue
English
Weight
261 KB
Volume
336
Category
Article
ISSN
0264-3952

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๐Ÿ“œ SIMILAR VOLUMES

Magnetic reconnection in high-temperatur
Magnetic reconnection in high-temperature plasma of solar flares
โœ B. V. Somov; A. I. Verneta ๐Ÿ“‚ Article ๐Ÿ“… 1988 ๐Ÿ› Springer ๐ŸŒ English โš– 327 KB

Quasi-steady high-temperature current sheets are an energy source during the 'main' or 'hot' phase of solar flares. Such sheets are shown to be stabilized with respect to the tearing instability by a small transverse component of magnetic field existing in the sheets. \* Send offprint requests to B.

The structure of high-temperature solar
The structure of high-temperature solar flare plasma in non-thermal flare models
โœ A. Gordon Emslie ๐Ÿ“‚ Article ๐Ÿ“… 1985 ๐Ÿ› Springer ๐ŸŒ English โš– 492 KB

We solve the energy equation for the high-temperature (coronal) component of flare plasma for two models of energy input: (i) direct collisional heating by a beam of suprathermal electrons, and (ii) ohmic heating by the beam-neutralizing reverse current. We discuss the regimes where each case is app