Parker instability in the nonadiabatic ISM

Details Parker instability in the nonadiabatic ISM Parker instability in the nonadiabatic ISM

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005mpge.conf..253k&link_type=abstract

The Magnetized Plasma in Galaxy Evolution, Proceedings of the conference held in Kraków, Poland, Sept. 27th - Oct. 1st, 2004, Ed

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Scientific paper

We study Parker instability under the influence of heating and cooling
processes. We distinguish three models with respect to different heating
functions. We find that the properties of the Parker instability in such
a system are significantly different with respect to the adiabatic and
isothermal cases.

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