Heating and activity of the solar corona 3. Dynamics of a low beta plasma with three-dimensional null points

Journal of Geophysical Research: Space Physics

Volumn 102, Issue A1, 1997, Pages 231-248

  Galsgaard, Klaus ^a,b   Nordlund, Åke ^a  

^a Physics and Geophysics ^*  (Denmark)

^b UNIVERSITY OF ST ANDREWS   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 24644514657     PISSN: 01480227     EISSN: None     Source Type: Journal    
DOI: 10.1029/96JA02680     Document Type: Article

References (6)

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2. Berger, M. A., Generation of coronal magnetic fields by random surface motions, Astron. Astrophys., 252, 367, 1991.
3. Biskamp, D., Nonlinear Magnetohydrodynamics in Cambridge Monogr. Plasma Phys. 1, Cambridge University Press, 1993.
4. Green, J. M., Geometrical properties of 3D reconnecting magnetic fields with nulls, J. Geophys. Res., 93, 8583, 1989.
5. Heyvaerts, J., and E. R. Priest, Coronal heating by reconnection in DC current systems: A theory based on a Taylor's hypothesis, Astron. Astrophys., 137, 63, 1984.
6. Heyvaerts, J., and E. R. Priest, A self-consistent turbulent model for solar coronal heating, Astrophys. J., 390, 297, 1992