High-order shock-capturing methods for modeling dynamics of the solar atmosphere-Reference-Cited by-同舟云学术

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High-order shock-capturing methods for modeling dynamics of the solar atmosphere

Published:2005-02 Issue:1-2 Volume:201 Page:1-26
ISSN:0167-2789
Container-title:Physica D: Nonlinear Phenomena
language:en
Short-container-title:Physica D: Nonlinear Phenomena

Author:

Bryson Steve,Kosovichev Alexander,Levy Doron

Publisher

Elsevier BV

Subject

Condensed Matter Physics,Statistical and Nonlinear Physics

Reference17 articles.

1. On a mechanism of spicule formation by shock waves in magnetic tubes;Andreev;Astron. Lett.,1994

2. The detection of 3 & 5 minute period oscillations in coronal loops;De Moortel;Astron. Astrophys.,2002

3. B. de Pontieu, Ph.D. Thesis, University of Ghent, Belgium, 1996.

4. A semi-empirical model of sunspot penumbra;Ding;Astron. Astrophys.,1989

5. On the origin of solar spicules;Hollweg;ApJ,1982

Cited by 4 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Sunquakes and starquakes;Proceedings of the International Astronomical Union;2013-08

2. Variability of Solar Five-Minute Oscillations in the Corona as Observed by the Extreme Ultraviolet Spectrophotometer (ESP) on the Solar Dynamics Observatory/Extreme Ultraviolet Variability Experiment (SDO/EVE);Solar Physics;2012-11-23

3. Reflectionless propagation of acoustic waves in the solar atmosphere;Astronomy Letters;2012-06

4. NUMERICAL SIMULATIONS OF IMPULSIVELY EXCITED ACOUSTIC-GRAVITY WAVES IN A STELLAR ATMOSPHERE;Acta Physica Polonica B;2011

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