Comments on the photospheric dynamo model of Henoux and Somov

Details Comments on the photospheric dynamo model of Henoux and Somov Comments on the photospheric dynamo model of Henoux and Somov

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...219..308m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 219, no. 1-2, July 1989, p. 308-312.

Astronomy and Astrophysics

Astrophysics

10

Dynamo Theory, Photosphere, Plasma Currents, Solar Corona, Solar Flares, Solar Magnetic Field, Scattering Cross Sections, Solar Atmosphere, Thermodynamic Equilibrium, Two Fluid Models

Scientific paper

A detailed model for a photospheric dynamo has been presented by Henoux and Somov (1987), who used the three-fluid model to treat the properties of the weakly ionized plasma. Only the equations for the two ionized components were solved. The equation for the neutral component is considered, and it is argued that the model is unacceptable becaused of an implied impossibly large unbalanced stress on the neutral gas. It is argued more generally that all existing photospheric dynamo models are untenable.

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