Dissipative structure and weak turbulence in the solar corona

Advances in Space Research

Volumn 20, Issue 12, 1997, Pages 2303-2308

  Rosa, R R ^a   Sawant, H S ^a   Valdivia, J A ^b   Sharma, A S ^b  

^a INSTITUTO NACIONAL DE PESQUISAS ESPACIAIS   (Brazil)

^b UNIVERSITY OF MARYLAND   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0008187988     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(97)00910-1     Document Type: Article

References (11)

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7. Rosa, R.R.; Sharma, A.S., Spatial fragmentation in nonlinear dissipative systems: an application to solar plasma processes EOS, Trans. AGU# 76 S219 (1995b).
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9. Rosa, R.R., Vinhas, L., A matrix computational operator for characterization of assimetric energy fragmentation in extended systems, in submission to Journal of Computational Physics, (1996).
10. Tsuneta, S.; Lemen, J.R., Dynamics of the solar corona observed with the Yohkoh soft X-ray telescope, in Physics of Solar and Stellar Corona, eds. J.F. Linsky and S. Serio, pp. 113-130, Kluwer Ac. Publ. (1993).
11. Vassilicus, J.C. Turbulence and Intermittency, Nature, 374:408-409 (1995).