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

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

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.133..177s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 133, no. 1, May 1987, p. 177-182.

Statistics

Computation

Computational Astrophysics, Larmor Radius, Magnetohydrodynamic Stability, Stellar Atmospheres, Thermal Instability, Hall Effect, Perturbation Theory, Specific Heat, Stellar Magnetic Fields, Temperature Gradients, Thermal Expansion

Scientific paper

Thermal-convective instability of a hydromagnetic-composite 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 finite Larmor radius.

Affiliated with

Also associated with

No associations

Rating

Thermal-convective instability of a composite plasma in a stellar atmosphere with finite Larmor radius does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Thermal-convective instability of a composite plasma in a stellar atmosphere with finite Larmor radius, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Thermal-convective instability of a composite plasma in a stellar atmosphere with finite Larmor radius will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-856686