Rapid changes in the fine structure of a coronal 'bright point' and a small coronal 'active region'

Details Rapid changes in the fine structure of a coronal 'bright point' and a small coronal 'active region' Rapid changes in the fine structure of a coronal 'bright point' and a small coronal 'active region'

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...63..119s&link_type=abstract

Solar Physics, vol. 63, Aug. 1979, p. 119-126.

Physics

63

Fine Structure, Solar Activity, Solar Corona, Solar X-Rays, Spectroheliographs, Photosphere, X Ray Imagery

Scientific paper

A coronal bright point is resolved into a pattern of emission which, at any given time, consists of 2 or 3 miniature loops (each approximately 2500 km in diameter and approximately 2000 km long). During the half-day lifetime of the 'bright point' individual loops evolved on a time scale approximately 7 min. A small 'active region' seemed to evolve in this way, but the occasional blurring together of several loops made it difficult to follow individual changes.

Affiliated with

Also associated with

No associations

Rating

Rapid changes in the fine structure of a coronal 'bright point' and a small coronal 'active region' 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 Rapid changes in the fine structure of a coronal 'bright point' and a small coronal 'active region', we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rapid changes in the fine structure of a coronal 'bright point' and a small coronal 'active region' will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1487366