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Title: Possible Mechanism of Enhancement of Diamagnetic Current Dissipation during the Heating of Magnetic Flux Tubes in the Solar Corona

Abstract

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.

Authors:
 [1]
  1. Russian Academy of Sciences, Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (Russian Federation)
Publication Date:
OSTI Identifier:
22763300
Resource Type:
Journal Article
Journal Name:
Plasma Physics Reports
Additional Journal Information:
Journal Volume: 44; Journal Issue: 2; Other Information: Copyright (c) 2018 Pleiades Publishing, Ltd.; Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 1063-780X
Country of Publication:
United States
Language:
English
Subject:
70 PLASMA PHYSICS AND FUSION TECHNOLOGY; HEATING; MAGNETIC FLUX; MICROSTRUCTURE; PLASMA; SOLAR CORONA

Citation Formats

Kovalev, V. A., E-mail: vic.kov@yandex.ru. Possible Mechanism of Enhancement of Diamagnetic Current Dissipation during the Heating of Magnetic Flux Tubes in the Solar Corona. United States: N. p., 2018. Web. doi:10.1134/S1063780X18020083.
Kovalev, V. A., E-mail: vic.kov@yandex.ru. Possible Mechanism of Enhancement of Diamagnetic Current Dissipation during the Heating of Magnetic Flux Tubes in the Solar Corona. United States. doi:10.1134/S1063780X18020083.
Kovalev, V. A., E-mail: vic.kov@yandex.ru. Thu . "Possible Mechanism of Enhancement of Diamagnetic Current Dissipation during the Heating of Magnetic Flux Tubes in the Solar Corona". United States. doi:10.1134/S1063780X18020083.
@article{osti_22763300,
title = {Possible Mechanism of Enhancement of Diamagnetic Current Dissipation during the Heating of Magnetic Flux Tubes in the Solar Corona},
author = {Kovalev, V. A., E-mail: vic.kov@yandex.ru},
abstractNote = {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.},
doi = {10.1134/S1063780X18020083},
journal = {Plasma Physics Reports},
issn = {1063-780X},
number = 2,
volume = 44,
place = {United States},
year = {2018},
month = {2}
}