Published 1984 | Version v1
Journal article

Magnetic reconnection in a high-temperature plasma of solar flares

  • 1. Fizicheskii Institut, Moscow, USSR

Description

In the framework of a simple self-consistent model for high-temperature turbulent-current sheet (HTCS), three effects are considered. Gradient instabilities create anomalous plasma diffusion across magnetic field and increase the power of energy release in HTCS. Moreover, penetration of a small transverse component of magnetic field into HTCS can also significantly increase the energy output of HTCS. Electric current appears to circulate around a current sheet at a compression of longitudinal magnetic field. This current induces Joule heat however, a total flux of the longitudinal field remains constant. 9 references

Additional details

Publishing Information

Journal Title
Adv. Space Res.
Journal Volume
4
Series
Adv. Space Res.
Journal Page Range
183-185
ISSN
0273-1177
CODEN
ASRSD

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
17014636
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ENERGY TRANSFER; HOT PLASMA; MAGNETIC FIELDS; MAGNETIC FLUX; MAGNETOHYDRODYNAMICS; SOLAR FLARES
Descriptors DEC
FLUID MECHANICS; HYDRODYNAMICS; MECHANICS; PLASMA; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR FLARES