Stability of the Lundquist Field and the Physical Nature of Eruptive Prominences with Helical Structure

Details Stability of the Lundquist Field and the Physical Nature of Eruptive Prominences with Helical Structure Stability of the Lundquist Field and the Physical Nature of Eruptive Prominences with Helical Structure

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..159..265x&link_type=abstract

Solar Physics, Volume 159, Issue 2, pp.265-273

Physics

2

Scientific paper

The stability of the Lundquist field is analysed in the light of the energy principle. The results show: (1) form = 0 disturbances, the Lundquist field is stable; (2) form = 1 disturbances, the Lundquist field will turn unstable in certain conditions. Whether the field will remain stable or not depends on parameters such as the helical pinch angle and radius and length of the prominence. Comparison between theory and observations reveals that a kink instability in the Lundquist field may be a critical physical reason for eruptive prominences with helical patterns.

Affiliated with

Also associated with

No associations

Rating

Stability of the Lundquist Field and the Physical Nature of Eruptive Prominences with Helical Structure 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 Stability of the Lundquist Field and the Physical Nature of Eruptive Prominences with Helical Structure, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stability of the Lundquist Field and the Physical Nature of Eruptive Prominences with Helical Structure will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1529936