On the visible shape of the cold plasma jets in the solar chromosphere

Details On the visible shape of the cold plasma jets in the solar chromosphere On the visible shape of the cold plasma jets in the solar chromosphere

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..153..237v&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 153, no. 1-2, p. 237-243

Physics

1

Chromosphere, Cold Plasmas, Light (Visible Radiation), Magnetic Dipoles, Magnetic Field Configurations, Mathematical Models, Optical Thickness, Plasma Jets, Charge Coupled Devices, H Alpha Line, Magnetohydrodynamics, Spicules

Scientific paper

Lines of equal optical thickness are calculated for cold plasma jets propagating in the simplest magnetic configuration. The paraxial approximation is used in the case of jets directed along the axis of a magnetic dipole. The results can explain the apparently convergent as well as divergent shapes of the jets in a divergent magnetic configuration.

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