Longitudinal motion of matter in the solar atmosphere due to magnetic compression

Details Longitudinal motion of matter in the solar atmosphere due to magnetic compression Longitudinal motion of matter in the solar atmosphere due to magnetic compression

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993azh....70.1086f&link_type=abstract

Astronomicheskij Zhurnal, vol. 70, p. 1086

Astronomy and Astrophysics

Astronomy

Solar Atmosphere, Magnetic Compression, Field Aligned Currents, Chromosphere, Hydrodynamic Equations, Ideal Gas

Scientific paper

An analysis is made of the formation of a directional motion of matter along the magnetic field lines associated with an increase of the field in the chromosphere. A system of hydrodynamic equations for an ideal gas in a flux tube is solved numerically. A increase in the field with a time constant of less than 300 s is shown to be necessary for the efficient formation of a jet with characteristics of a typical surge.

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