Heating and reconnection of the emerging magnetic flux-tubes and the role of the interchange instability

Details Heating and reconnection of the emerging magnetic flux-tubes and the role of the interchange instability Heating and reconnection of the emerging magnetic flux-tubes and the role of the interchange instability

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...51..413u&link_type=abstract

Solar Physics, vol. 51, Mar. 1977, p. 413-429.

Astronomy and Astrophysics

Astronomy

31

Magnetic Flux, Solar Corona, Solar Magnetic Field, Solar X-Rays, Far Ultraviolet Radiation, Lines Of Force, Magnetohydrodynamic Stability, Spaceborne Astronomy

Scientific paper

It is shown that the basic behavior of the newly energed magnetic regions in the solar corona, as observed in EUV and soft X-rays from space, may be due to the fast dynamic relaxation of their field lines into the ambient field through intermingling by the interchange instability. The newly emerged magnetic flux region is thus made unstable and continually relaxes to lower energy states. These states are composed of thin sheets of plasma which penetrate into regions of opposite polarity.

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