Plasma flow in weakly diverging coronal structures

Details Plasma flow in weakly diverging coronal structures Plasma flow in weakly diverging coronal structures

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68..602b&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, May-June 1991, p. 602-611. In Russian.

Other

4

Gravitational Fields, Magnetohydrodynamic Flow, Solar Corona, Solar Wind, Thermal Plasmas, Isothermal Processes, Solar Activity, Stellar Luminosity

Scientific paper

The outflow of a hot isothermal plasma in a gravity field in structures having a divergence less than the radial one is studied theoretically. A solution which passes through the critical point is obtained, and the dependence of the solution on the problem's parameters is investigated. In such structures, velocities were found to be lower than in a spherically symmetric flow under the same physical conditions. It is inferred that a great outflow of gas is possible in streamers.

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