Compression of the current sheet and its impact into the reconnection rate

Details Compression of the current sheet and its impact into the reconnection rate Compression of the current sheet and its impact into the reconnection rate

2007-11-11

arxiv.org/abs/0711.1666v3

Astronomy and Astrophysics

Astrophysics

24 pages 10 figures, typos corrected

Scientific paper

Numerical simulations of strongly compressible MHD corresponding to a stellar
atmosphere with substantial gravity and near force-free magnetic fields show
that the current sheet collapses (its width decreasing substantially). As a
result, the reconnection rate increases dramatically.

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