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On the magnetic flux conservation in the partially ionized plasma

Published online by Cambridge University Press:  18 July 2013

Yuriy Tsap
Yuriy Tsap*
Affiliation:
Crimean Astrophysical Observatory, Nauchny, 98409 Crimea, Ukraine email: [email protected]
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Abstract

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Ohm, Hall, and ambipolar diffusions in the partially ionized plasma are considered. The statement of Pandey & Wardle (2011,2012) that only Ohmic diffusion is capable of destroying the magnetic flux is not sufficiently correct due to the formal dependence of the magnetic diffusion on a frame of reference.

Keywords

Plasmasdiffusionmagnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S294: Solar and Astrophysical Dynamos and Magnetic Activity , August 2012 , pp. 371 - 372
Copyright
Copyright © International Astronomical Union 2013 

References

Pandey, B. P. & Wardle, M. 2011, Hall instability of solar flux tubes, eprint arXiv:1108.3169.Google Scholar
Pandey, B. P. & Wardle, M. 2012, MNRAS, 423, 222 Google Scholar
Nickeler, D. H. & Karlicky, M. 2006 Astrophys. Space Sci. Trans. 2 63 Google Scholar