Convective instability in a uniform magnetic field

Details Convective instability in a uniform magnetic field Convective instability in a uniform magnetic field

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981svjpp...7r.177g&link_type=abstract

(Fizika Plazmy, vol. 7, Jan.-Feb. 1981, p. 177-184.) Soviet Journal of Plasma Physics, vol. 7, Jan.-Feb. 1981, p. 99-102. Trans

Physics

Plasma Physics

Convective Flow, Magnetohydrodynamic Stability, Solar Magnetic Field, Sunspots, Flow Stability, Magnetic Flux, Plasma Temperature, Solar Activity

Scientific paper

A theoretical analysis is presented of the development of nonlinear axisymmetric convective instability in a homogeneous magnetic field directed along the gravity force. It is shown that the development of instability leads to the concentration of the magnetic field and a decrease of temperature in the vicinity of the axis of symmetry. This is suggested as a possible mechanism for the formation of sunspots.

Affiliated with

Also associated with

No associations

Rating

Convective instability in a uniform magnetic field 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 Convective instability in a uniform magnetic field, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Convective instability in a uniform magnetic field will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1409271