Generation of Flows in the Solar Chromosphere Due to Magnetofluid Coupling

Details Generation of Flows in the Solar Chromosphere Due to Magnetofluid Coupling Generation of Flows in the Solar Chromosphere Due to Magnetofluid Coupling

2002-04-18

arxiv.org/abs/astro-ph/0204311v1

Astrophys.J. 576 (2002) L161-L164

Astronomy and Astrophysics

Astrophysics

11 pages of text and 2 figures. Submitted to The Astrophysical Journal Letters

Scientific paper

10.1086/343727

It is shown that a generalized magneto-Bernoulli mechanism can effectively
generate high velocity flows in the Solar chromosphere by transforming the
plasma pressure energy into kinetic energy. It is found that at reasonable
heights and for realistic plasma parameters, there is a precipitous pressure
fall accompanied by a sharp amplification of the flow speed.

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