๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Recurrence of flare energy releases in solar active regions (Cycle 23)

โœ Scribed by Nagovitsyn, Yu. A.; Kuleshova, A. I.

Book ID
121592311
Publisher
SP MAIK Nauka/Interperiodica
Year
2013
Tongue
English
Weight
202 KB
Volume
53
Category
Article
ISSN
0016-7932

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

The correlation of solar flare productio
The correlation of solar flare production with magnetic energy in active regions
โœ E. B. Mayfield; John K. Lawrence ๐Ÿ“‚ Article ๐Ÿ“… 1985 ๐Ÿ› Springer ๐ŸŒ English โš– 677 KB

An investigation of 531 active regions was made to determine the correlation between energy released by flares and the available energy in magnetic fields of the regions. Regions with magnetic flux greater than 102~ maxwell during the years 1967-1969, which included sunspot maximum, were selected fo

Plasma radiation diagnostics of the prim
Plasma radiation diagnostics of the primary energy release region in solar flares
โœ Dean F. Smith; Daniel S. Spicer ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Springer ๐ŸŒ English โš– 854 KB

The possibility is investigated that the plasma turbulence used in many recent models of the primary energy release and acceleration in solar flares should be detectable by radiation near the fundamental and second harmonic of the plasma frequency. Formulae are derived for fundamental emission due t

Laboratory simulation of energy release
Laboratory simulation of energy release in solar flares
โœ A. T. Altyntsev; V. M. Bardakov; V. I. Krasov; N. V. Lebedev; V. L. Paperny; V. ๐Ÿ“‚ Article ๐Ÿ“… 1986 ๐Ÿ› Springer ๐ŸŒ English โš– 810 KB

A laboratory simulation method is proposed for energy release processes occurring in a fragment of the flare current sheet on the Sun. The method relies on the assumption that the spatial scale of such processes is represented by the current sheet's thickness whose values can be close for both the s