๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

X-ray heating of a low-temperature region in chromospheric flares

โœ Scribed by B. V. Somov

Publisher
Springer
Year
1975
Tongue
English
Weight
668 KB
Volume
42
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

On the low-temperature region of chromos
On the low-temperature region of chromospheric flares
โœ B. V. Somov; S. I. Syrovatskii ๐Ÿ“‚ Article ๐Ÿ“… 1974 ๐Ÿ› Springer ๐ŸŒ English โš– 924 KB

Most of the energy of particles accelerated in a flare is used for the creation of a hightemperature flare region, the structure of which is determined by the heat conduction . However, as the temperature drops with the depth in the chromosphere, the heat flux decreases quickly and in the low-temper

The heating of the temperature minimum r
The heating of the temperature minimum region in solar flares โ€” A reassessment
โœ A. Gordon Emslie; Marcos E. Machado ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Springer ๐ŸŒ English โš– 320 KB

As a sequel to the work by Machado et al. (1978), we discuss and evaluate the suggestions made by these authors on how to possibly reconcile the observed temperature enhancements at temperatureminimum levels in solar flares with some form of theoretical heating mechanism. After establishing the H-LT

Soft X-ray and microwave observations of
Soft X-ray and microwave observations of hot regions in solar flares
โœ H. S. Hudson; K. Ohki ๐Ÿ“‚ Article ๐Ÿ“… 1972 ๐Ÿ› Springer ๐ŸŒ English โš– 696 KB

Hot regions in solar flares produce X-radiation and microwaves by thermal processes. Recent X-ray data make it possible to specify the temperature and emission measure of the soft X-ray source, by using, for instance, a combination of the 1-8 A (peak response at about 2 keV) and the 0.5-3 ]k (peak r

The relation between hard X-ray and tran
The relation between hard X-ray and transition-region line emission in solar flares
โœ John T. Mariska; A. I. Poland ๐Ÿ“‚ Article ๐Ÿ“… 1985 ๐Ÿ› Springer ๐ŸŒ English โš– 810 KB

Observational evidence suggests that both the hard X-ray and ultraviolet emission from the impulsive phase of flares result from an electron beam. We present the results of model calculations that are consistent with this theory. The impulsive phase is envisioned as occurring in many small magnetica