To the Problem of the Corona Heating

Details To the Problem of the Corona Heating To the Problem of the Corona Heating

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...3e..10b&link_type=abstract

Solar Active Regions and 3D Magnetic Structure, 26th meeting of the IAU, Joint Discussion 3, 16-17 August, 2006, Prague, Czech R

Physics

Scientific paper

The adequacy of different models of the corona heating is discussed. The correlation between the brightness of the coronal green line 530.5 nm Fe XIV and the calculated strength of the magnetic field in the corona is shown to be a very useful instrument to solve the problem. This correlation manifests a very strong dependence both on the solar cycle phase and heliolatitude. It seems reasonable that the effectiveness of the mechanisms depends strongly on the relative area of low and high (including open field) loops. The models based on slow field dissipation (DC) are more effective in the low-latitude zone and the wave models based on dissipation of Alfven waves (AC), in the high latitude zone.

Affiliated with

Also associated with

No associations

Rating

To the Problem of the Corona Heating 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 To the Problem of the Corona Heating, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and To the Problem of the Corona Heating will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1782085