Filamentary structures in the Sun's atmosphere as singular Alfven waves

Details Filamentary structures in the Sun's atmosphere as singular Alfven waves Filamentary structures in the Sun's atmosphere as singular Alfven waves

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990esasp.311...33p&link_type=abstract

In ESA, Plasma Astrophysics p 33-34 (SEE N91-15046 06-90)

Astronomy and Astrophysics

Astrophysics

Chromosphere, Magnetohydrodynamic Waves, Solar Atmosphere, Solar Prominences, Differential Equations, Electrons, Energetic Particles, Integral Equations, Mathematical Models, Wave Equations

Scientific paper

A model is proposed which treats filamentary structures observed in the Sun's chromosphere as thin beams of energetic electrons. The structures are corresponded to Alfven waves with filamentary singularity. The set of integro-differential equations describing dynamics of the beams are derived from the ordinary magnetohydrodynamic equations. Some solutions of this set are obtained.

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