Abstract
There is some similitude in physical conditions between the system “disk — corona” of compact stars (such as white dwarfs or neutron stars) and the system “photosphere — corona” of the Sun (e.g. [1], [2]). This is a basic idea of our study.
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References
Somov, B.V., 2000, Cosmic Plasma Physics, Kluwer Academic Publishers, Dordrecht.
Liu, B.F., Mineshige, S., Shibata, K. 2002, ApJ, 572, L173.
Heyvaerts, J. 1991, in E. R. Priest and A.W. Hood (eds.), Advances in Solar System Magnetohydrodynamics, Cambridge Univ. Press.
Mukerjee, K. et al. 2001, ApJ, 548, 368.
Oreshina, A.V. and Somov, B.V. 2000, Astronomy Letters, 26(11), 750.
Barret, D., Olive, J.F., Boirin, L. 2000, ApJ, 533, 329.
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Oreshina, A.V., Oreshina, I.V., Somov, B.V. (2003). Magnetic Reconnection in the Accretion-Disk Corona of Compact Stars. In: de Martino, D., Silvotti, R., Solheim, JE., Kalytis, R. (eds) White Dwarfs. NATO Science Series, vol 105. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0215-8_63
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DOI: https://doi.org/10.1007/978-94-010-0215-8_63
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