Theoretical Network Structure of the Transition Region Chromosphere / Corona - Part Two - the Coronal Holes

Details Theoretical Network Structure of the Transition Region Chromosphere / Corona - Part Two - the Coronal Holes Theoretical Network Structure of the Transition Region Chromosphere / Corona - Part Two - the Coronal Holes

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....86..188e&link_type=abstract

Astronomy and Astrophysics, Vol. 86, P. 188, 1980

Astronomy and Astrophysics

Astrophysics

Scientific paper

A detailed model for the solar transition zone for hole regions is constructed. It shows the correct network width, reproduces the observed UV-line intensities above a temperature range of 100,000 K, is a critical solution of the solar wind equation, and shows a shift of the Ne VII-layer (temperature range between 650,000 and 700,000 K) of several thousand kilometers upwards as observed by Huber et al. (1974). The last two features of the model can be achieved only if the magnetic field line divergence in the outer corona is greater than radial, and if, in addition to the coronal, there is a second peak in the heating function at lower layers.

Affiliated with

Also associated with

No associations

Rating

Theoretical Network Structure of the Transition Region Chromosphere / Corona - Part Two - the Coronal Holes 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 Theoretical Network Structure of the Transition Region Chromosphere / Corona - Part Two - the Coronal Holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Theoretical Network Structure of the Transition Region Chromosphere / Corona - Part Two - the Coronal Holes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1214273