Ambipolar diffusion in the solar atmosphere

Details Ambipolar diffusion in the solar atmosphere Ambipolar diffusion in the solar atmosphere

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001mnras.323l..23c&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 323, Issue 2, pp. L23-L25.

Astronomy and Astrophysics

Astronomy

8

Diffusion, Sun: Atmosphere, Sun: Magnetic Fields

Scientific paper

The process of non-linear ambipolar diffusion in the region overlying the solar surface can be an effective mechanism for producing sharp magnetic structures and current sheets. These may be the sites responsible for the occurrence of connectivity of magnetic field lines, and the subsequent explosive input of energy for heating of some of the features in the atmosphere of the Sun..

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