๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Polarization of radio emission of the turbulent plasma of solar flares

โœ Scribed by V. V. Tirskii; V. M. Tomozov

Book ID
112718508
Publisher
Springer US
Year
1996
Tongue
English
Weight
149 KB
Volume
39
Category
Article
ISSN
0033-8443

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

The role of plasma turbulence in the dev
The role of plasma turbulence in the development of solar flares
โœ M. Kuperus ๐Ÿ“‚ Article ๐Ÿ“… 1976 ๐Ÿ› Springer ๐ŸŒ English โš– 653 KB

The amount of energy released during a solar flare and the relatively short timescale in which all the flare associated events occur lead to the conclusion that a solar flare is a magnetohydrodynamic instability taking place in a strongly turbulent plasma. The main effect of the plasma turbulence i

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 %