Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles-Reference-Cited by-同舟云学术

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Stability and mode analysis of solar coronal loops using thermodynamic irreversible energy principles

Published:2006-09-12 Issue:3 Volume:458 Page:953-963
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Costa A.,González R.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20065206/pdf

Reference44 articles.

1. Relative Timing of Soft X-Ray Nonthermal Line Broadening and Hard X-Ray Emission in Solar Flares

2. Arfken, G., & Weber, H. 1995, Mathematical methods for physicists (San Diego: Academic Press)

3. The Differential Emission Measure Distribution in the Multiloop Corona

4. Aschwanden, M. J. 2004, Physics of the Solar Corona (New York: Springer-Verlag)

5. Three‐dimensional Stereoscopic Analysis of Solar Active Region Loops. I.SOHO/EIT Observations at Temperatures of (1.0–1.5) x 106K

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2. Exploring the Kipenhahn-Schlüter model;Journal of Physics: Conference Series;2018-05

3. Corrugation Instability of a Coronal Arcade;Solar Physics;2017-11-28

4. Numerical simulation of the internal plasma dynamics of post-flare loops;Monthly Notices of the Royal Astronomical Society;2009-12-21

5. Stability and mode analysis of solar low-coronal structures using irreversible energy principles;Physica Scripta;2008-10

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