Small scale processes in solar and stellar plasmas

Details Small scale processes in solar and stellar plasmas Small scale processes in solar and stellar plasmas

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.344...97v&link_type=abstract

In ESA, Solar Physics and Astrophysics at Interferometric Resolution p 97-104 (SEE N93-10901 01-90)

Astronomy and Astrophysics

Astronomy

1

Chromosphere, High Resolution, Mathematical Models, Plasma Heating, Solar Flares, Solar Wind, Coronal Loops, Magnetic Disturbances, Solar Corona, Solar Physics, Spaceborne Astronomy

Scientific paper

Small scale processes which occur in the magnetically dominated outer layers of the Sun are reviewed. The transport coefficients for the thermal and the electrical conductivity in the classical limit and in the limit of anomalous processes are discussed. It is demonstrated that the corona and the chromosphere must have a filamentary structure. Various heating mechanisms which are based on small scale dissipation of magnetic energy are discussed. The observational requirements for improved modeling of the transition region and the chromosphere are formulated and the consequences of high resolution observations for flare models are pointed out.

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