Model of the chromosphere spicule formation

Details Model of the chromosphere spicule formation Model of the chromosphere spicule formation

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989plap.work..349c&link_type=abstract

In ESA, Proceedings of an International School and Workshop on Plasma Astrophysics, Volume 1 p 349-351 (SEE N89-24910 18-75)

Astronomy and Astrophysics

Astrophysics

Chromosphere, Magnetic Field Configurations, Spicules, Stellar Models, Hydrodynamic Equations, Magnetohydrodynamics, Solar Magnetic Field

Scientific paper

By means of MHD equations and based on a proposed configuration of the magnetic field, a number of spicules per supergranule is estimated and the dependence of this number on a height of a level of the spicule formation and on latitude is obtained. The close relation of the spicule number distribution with chromospheric net (supergranular structure) is explained. The possibility of structuring of diffusive magnetic field (formation of the magnetic tubes) is shown.

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