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Volumn 703, Issue , 2004, Pages 193-202

Aspects of nonlinear magnetohydrodynamics in the solar corona

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EID: 85007241821     PISSN: 0094243X     EISSN: 15517616     Source Type: Conference Proceeding    
DOI: 10.1063/1.1718455     Document Type: Conference Paper
Times cited : (1)

References (17)
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  • 3
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    • Magnetic energy shedding in the solar atmosphere
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    • Parker, E.N.1
  • 5
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    • The viability of ohmic dissipation as a coronal heating source
    • Hendrix, D.L., van Hoven, G., Mikic, Z. and Schnack, D. D., "The Viability of Ohmic Dissipation as a Coronal Heating Source ", Astrophys. J.470, 1192, (1996).
    • (1996) Astrophys. J. , vol.470 , pp. 1192
    • Hendrix, D.L.1    Van Hoven, G.2    Mikic, Z.3    Schnack, D.D.4
  • 8
    • 0142051275 scopus 로고    scopus 로고
    • Coronal heating and reduced MHD
    • E. Falgarone and T. Passot (Eds), Springer-Verlag, Berlin 2003
    • Oughton, S. P. E'Dmitruk, and W.H. Matthaeus 2003, "Coronal heating and reduced MHD", in Turbulence and Magnetic Fields in Astrophysics, E. Falgarone and T. Passot (Eds), Springer-Verlag, Berlin, Vol. 614 (LNP) (2003) p. 28-55.
    • (2003) Turbulence and Magnetic Fields in Astrophysics , vol.614 , pp. 28-55
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  • 10
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    • submitted
    • M. Velli, R. Betta, G. Einaudi and M. Ghiglione, Mhd Turbulence Simulations of Coronal Heating: 2d vs 3d Models, Astrophys. J. submitted, (2003).
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    • Velli, M.1    Betta, R.2    Einaudi, G.3    Ghiglione, M.4
  • 16
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    • Evolution of wake instabilities and the acceleration of the slow solar wind: Melon seed and expansion effects
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    • Rappazzo, A. F., Velli, M., Einaudi, G., and Dahlburg, R. B., "Evolution of wake instabilities and the acceleration of the slow solar wind: melon seed and expansion effects," in Solar Wind 10, M. Velli, R. Bruno and F. Malara (Eds), AIP Conference Proceedings 679, American Institute of Physics, New York, (2003), pp. 371-374.
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.