Anisotropic Plasma-resulted High Coronal Temperature

Details Anisotropic Plasma-resulted High Coronal Temperature Anisotropic Plasma-resulted High Coronal Temperature

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.9503h&link_type=abstract

American Astronomical Society Meeting 210, #95.03; Bulletin of the American Astronomical Society, Vol. 39, p.224

Astronomy and Astrophysics

Astronomy

Scientific paper

In order to examine the assumption that the high temperature of the coronal results from the development of an anisotropic plasma with a perpendicular temperature slightly higher than its parallel temperature at the coronal loop foot as the magnetic field decreases significantly from the foot of the loop to its vertex, the formation of higher perpendicular temperature at the coronal loop foot and the process of energetic particles being confined through particle’s pitch angle diffusion at the loop vertex are studied. An example for the detailed processes is given.

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