Dissipative structure and weak turbulence in the solar corona-Reference-Cited by-同舟云学术

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Dissipative structure and weak turbulence in the solar corona

Published:1997-01 Issue:12 Volume:20 Page:2303-2308
ISSN:0273-1177
Container-title:Advances in Space Research
language:en
Short-container-title:Advances in Space Research

Author:

Rosa R.R.,Sawant H.S.,Valdivia J.A.,Sharma A.S.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference11 articles.

1. Geometric algorithms;Adelsbrunner,1993

2. Particle acceleration in an evolving active region by an esemble of shock waves;Anastasiadis;The Astrophysical Journal,1994

3. Solar radio signatures suggestive of proton beams;Benz;Nature,1986

4. A mechanism for localized turbulence;Bohr;Physica D,1991

5. Intermittent transition to turbulence in dissipative dynamical systems;Pomeau;Comm. Math. Phys.,1980

Cited by 3 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. Spectral and polarization analysis of geomagnetic pulsations data using a multitaper method;Computers & Geosciences;2004-10

2. Characterization of local self-similarity and criticality in the solar active regions;Advances in Space Research;2002-01

3. Phenomenological dynamics of coronal loops using a neural network approach;Advances in Space Research;2000-01

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