The fibril structure of prominences

Details The fibril structure of prominences The fibril structure of prominences

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..138..331h&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 138, no. 2, April 1992, p. 331-351. Research supported by SERC.

Physics

8

Solar Corona, Solar Prominences, Solar Temperature, Thermal Instability, Boundary Conditions, Solar Magnetic Field, Temperature Profiles

Scientific paper

This paper presents several magnetohydrostatic equilibrium models for prominences with fibril-like fine structure. For all the models ad hoc temperature profiles are used without discussing the energetics. For the models fine structure is assumed to occur either across the prominence axis or along it. This approach is intended as a first step toward more realistic models based upon a series of vertical fibril structures.

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