๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Steady models for the hard X-ray loops in the solar corona

โœ Scribed by T. Takakura


Publisher
Springer
Year
1984
Tongue
English
Weight
592 KB
Volume
91
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


X-ray temperature-emission measure model
โœ G. G. Cohen; D. W. Keith ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Springer ๐ŸŒ English โš– 383 KB

Several problems related to the calculation of an emission measure differential in temperature are resolved using a new calculation technique. The analysis of a flare on 20 April, 1976, is used to evaluate the usefulness of this new approach and to estimate its future value.

Soft x-ray emitting regions in the solar
โœ M. Landini; B. C. Monsignori Fossi ๐Ÿ“‚ Article ๐Ÿ“… 1971 ๐Ÿ› Springer ๐ŸŒ English โš– 485 KB

The soft X-ray emission of the solar corona is investigated by comparison of the signals of several broad band photometers carried on the Solrad 9 satellite, and sensitive to the region 0.5-20 A. Temperature from 1.5 โ€ข 106 to 25 โ€ข 106 K have been measured with 'emission measure' S N~2 dVranging betw

Time delays in large and small loop ther
โœ Dean F. Smith; Lorant A. Muth ๐Ÿ“‚ Article ๐Ÿ“… 1984 ๐Ÿ› Springer ๐ŸŒ English โš– 568 KB

The time histories of the emission at 10, 30, and 100 keV averaged over the loop from small and large loop thermal models of hard X-ray emission are studied. The small (15 000 km) loop cases show a characteristic delay in the peak of the 100 keV emission relative to the 30 keV emission of about 1.5

On the production of hard X-rays in sola
โœ G. M. Simnett; M. G. Haines ๐Ÿ“‚ Article ๐Ÿ“… 1990 ๐Ÿ› Springer ๐ŸŒ English โš– 613 KB

The problem of producing the hard X-ray burst at the onset of solar flares may be thought of in terms of the problem of producing the non-thermal electrons which emit the X-rays via bremsstrahlung. Electron acceleration to relativistic energies without similar ion acceleration is difficult to achiev