The progresses on the magnetodynamic phenomena in the solar and stellar atmosphere.

Details The progresses on the magnetodynamic phenomena in the solar and stellar atmosphere. The progresses on the magnetodynamic phenomena in the solar and stellar atmosphere.

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ppmto..14..323g&link_type=abstract

Publ. Purple Mt. Obs., Vol. 14, No. 4, p. 323 - 327

Physics

Solar Atmosphere: Magnetohydrodynamics, Stellar Atmospheres: Magnetohydrodynamics

Scientific paper

The IAU Colloquium No. 153 was held in Makuhari near Tokyo (Japan), from May 22 to 26, 1995. The topic of the meeting, concentrating on the advances of magnetodynamic phenomena in the solar and stellar atmosphere, consists of four parts: magnetic atmospheres of the Sun and stars; wind and mass-loss from the Sun and stars; production of superhot plasma and high-energy particles in the Sun and stars; magnetic behavior of the Sun and stars and their activity cycles. This paper gives a short review on this colloquium.

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