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The polarization of X-ray emission of some solar flares in July 1974

โœ Scribed by I. P. Tindo; A. I. Shuryghin; W. Steffen

Publisher
Springer
Year
1976
Tongue
English
Weight
443 KB
Volume
46
Category
Article
ISSN
0038-0938

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๐Ÿ“œ SIMILAR VOLUMES

Further polarization measurements of the
Further polarization measurements of the solar flare X-ray emission
โœ I. P. Tindo; S. L. Mandel'stam; A. I. Shuryghin ๐Ÿ“‚ Article ๐Ÿ“… 1973 ๐Ÿ› Springer ๐ŸŒ English โš– 273 KB

An improved X-ray polarimeter is briefly described and preliminary results of the measurements carried out on the satellite 'Intercosmos-7' are presented. One flare with considerable polarization (P~> 16%) was observed on 1972 August 4. Two other flares with rather low polarization (P ~ 4 %; P/> 2 %

New measurements of the polarization of
New measurements of the polarization of X-ray solar flares
โœ I. P. Tindo; V. D. Ivanov; S. L. Mandel'stam; A. I. Shuryghin ๐Ÿ“‚ Article ๐Ÿ“… 1972 ๐Ÿ› Springer ๐ŸŒ English โš– 185 KB

Measurements of three X-ray flares in October/November 1970 abord the Intercosmos 4 satellite confirm the existence of polarization in the initial phase of the X-ray bursts. The polarization can be observed for a few up to ten minutes, and an increase in polarization is observed during secondary max

Polarization of hard X-rays from solar f
Polarization of hard X-rays from solar flares
โœ Eberhard Haug ๐Ÿ“‚ Article ๐Ÿ“… 1972 ๐Ÿ› Springer ๐ŸŒ English โš– 453 KB

The polarization of hard solar X-radiation (> l0 keV) is calculated on the assumption that electrons get a non-isotropic velocity distribution in the initial phase of a flare. The bremsstrahlung generated by nonthermal electrons spiralling around magnetic field lines with discrete pitch angles is co