Published February 2018
| Version v1
Journal article
Possible Mechanism of Enhancement of Diamagnetic Current Dissipation during the Heating of Magnetic Flux Tubes in the Solar Corona
Creators
- 1. Russian Academy of Sciences, Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (Russian Federation)
Description
It is shown that dissipation of the diamagnetic current heating the coronal plasma with the classical conductivity in the absence of a longitudinal current can increase significantly due to the cellular transverse microstructure of the flux tube, thereby compensating for intense radiative losses.
Additional details
Identifiers
Publishing Information
- Journal Title
- Plasma Physics Reports
- Journal Volume
- 44
- Journal Issue
- 2
- Journal Page Range
- p. 267-269
- ISSN
- 1063-780X
- CODEN
- PPHREM
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 50006445
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- HEATING; MAGNETIC FLUX; MICROSTRUCTURE; PLASMA; SOLAR CORONA
- Descriptors DEC
- ATMOSPHERES; SOLAR ATMOSPHERE; STELLAR ATMOSPHERES; STELLAR CORONAE
Optional Information
- Copyright
- Copyright (c) 2018 Pleiades Publishing, Ltd.