The Solar X-Ray Corona

Details The Solar X-Ray Corona The Solar X-Ray Corona

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.237...33g&link_type=abstract

Astrophysics and Space Science, Volume 237, Issue 1-2, pp. 33-48

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

The solar corona, and the coronae of solar-type stars, consist of a low-density magnetized plasma at temperatures exceeding 106 K. The primary coronal emission is therefore in the UV and soft x-ray range. The observed close connection between solar magnetic fields and the physical parameters of the corona implies a fundamental role for the magnetic field in coronal structuring and dynamics. Variability of the corona occurs on all temporal and spatial scales—at one extreme, as the result of plasma instabilities, and at the other extreme driven by the global magnetic flux emergence patterns of the solar cycle.

Affiliated with

Also associated with

No associations

Rating

The Solar X-Ray Corona 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 The Solar X-Ray Corona, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Solar X-Ray Corona will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1643561