Magnetic Reconnection as a Driver of Chromospheric Surges

Details Magnetic Reconnection as a Driver of Chromospheric Surges Magnetic Reconnection as a Driver of Chromospheric Surges

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996soph..169..357g&link_type=abstract

Solar Physics, Volume 169, Issue 2, pp.357-366

Physics

6

Scientific paper

The basal structure of a surge precisely on the limb has been photographed with 1″-resolution in the core and wings of Hα. The dynamics observed in the fine structures are consistent in general with reconnection theory, but they also display flows more complicated than those predicted by 2D-reconnection models. The magnetic topology of the surrounding long-lived plage indicates that flux cancellation rather than its emergence is the key factor in promoting recurrent surges at this site.

Affiliated with

Also associated with

No associations

Rating

Magnetic Reconnection as a Driver of Chromospheric Surges 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 Reconnection as a Driver of Chromospheric Surges, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetic Reconnection as a Driver of Chromospheric Surges will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1173172