Magnetic instabilities

Details Magnetic instabilities Magnetic instabilities

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.220..147e&link_type=abstract

In ESA The Hydromagnetics of the Sun p 147-153 (SEE N85-25091 14-92)

Physics

Magnetohydrodynamic Stability, Solar Magnetic Field, Solar Physics, Magnetic Dispersion, Solar Corona, Tearing Modes (Plasmas)

Scientific paper

Theoretical aspects of ideal and resistive instabilities related to solar phenomena are reviewed. The interest in the stability of solar coronal structures derives from their observed lifetime (much longer than the relevant hydromagnetic timescale) coupled with their active behavior. This means that they must be generally stable with respect to fast, destructive instabilities, typically those governed by the ideal MHD equations, and, at the same time, they must allow slow, non-disrupting, dissipative processes to take place.

Affiliated with

Also associated with

No associations

Rating

Magnetic instabilities 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 Magnetic instabilities, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetic instabilities will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1753304