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Uspekhi Fizicheskikh Nauk, 2008, Volume 178, Number 11, Pages 1165–1204
DOI: https://doi.org/10.3367/UFNr.0178.200811b.1165
(Mi ufn664)
 

This article is cited in 74 scientific papers (total in 74 papers)

REVIEWS OF TOPICAL PROBLEMS

Coronal magnetic loops

V. V. Zaitseva, A. V. Stepanovb

a Institute of Applied Physics, Russian Academy of Sciences
b Central Astronomical Observatory at Pulkovo, Russian Academy of Sciences
References:
Abstract: The goal of this review is to outline some new ideas in the physics of coronal magnetic loops, the fundamental structural elements of the atmospheres of the Sun and flaring stars, which are involved in phenomena such as stellar coronal heating, flare energy release, charged particle acceleration, and the modulation of optical, radio, and X-ray emissions. The Alfvén–Carlqvist view of a coronal loop as an equivalent electric circuit allows a good physical understanding of loop processes. Describing coronal loops as MHD-resonators explains various ways in which flaring emissions from the Sun and stars are modulated, whereas modeling them by magnetic mirror traps allows one to describe the dynamics and emission of high-energy particles. Based on these approaches, loop plasma and fast particle parameters are obtained and models for flare energy release and stellar corona heating are developed.
Received: May 16, 2008
Revised: June 28, 2008
English version:
Physics–Uspekhi, 2008, Volume 51, Issue 11, Pages 1123–1160
DOI: https://doi.org/10.1070/PU2008v051n11ABEH006657
Bibliographic databases:
Document Type: Article
PACS: 52.35.-g, 96.60.-j, 97.10.Sj
Language: Russian
Citation: V. V. Zaitsev, A. V. Stepanov, “Coronal magnetic loops”, UFN, 178:11 (2008), 1165–1204; Phys. Usp., 51:11 (2008), 1123–1160
Citation in format AMSBIB
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  • This publication is cited in the following 74 articles:
    Citing articles in Google Scholar: Russian citations, English citations
    Related articles in Google Scholar: Russian articles, English articles
    Успехи физических наук Physics-Uspekhi
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