Thermal-convective instability of a composite rotating plasma in a stellar atmosphere with finite Larmor radius

Details Thermal-convective instability of a composite rotating plasma in a stellar atmosphere with finite Larmor radius Thermal-convective instability of a composite rotating plasma in a stellar atmosphere with finite Larmor radius

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988japa....9....1s&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 9, March 1988, p. 1-5.

Astronomy and Astrophysics

Astrophysics

1

Convective Heat Transfer, Rotating Plasmas, Stellar Atmospheres, Thermal Instability, Collision Parameters, Inviscid Flow, Larmor Radius, Neutral Gases, Perturbation Theory

Scientific paper

Thermal-convective instability of a hydromagnetic, composite, rotating,
inviscid and infinitely conducting plasma in a stellar atmosphere has
been studied in the presence of finite Larmor radius. It is found that
the criterion for monotonic instability holds good in the presence of
the effects due to rotation and finite Larmor radius.

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