Fine structure of solar magnetic fields

Details Fine structure of solar magnetic fields Fine structure of solar magnetic fields

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010bcrao.106...49b&link_type=abstract

Bulletin of the Crimean Astrophysical Observatory, Volume 106, Issue 1, pp.49-53

Astronomy and Astrophysics

Astrophysics

Fine Structure, Magnetic Field, The Sun

Scientific paper

The problem of inequality of results of longitudinal magnetic fields measured in the magnotosensetive lines FeI 5250 and FeI 5247 is investigated. The observed ratio of longitudinal components of magnetic field H 11(5250)/ H 11(5247) is compared to the calculated for different combinations of magnetic field elements. The calculations have been made with standard model photosphere for quiet regions. It was concluded that the underestimated value of magnetic field obtained with the FeI 5250 line is explained by the presence of unresolved elements with kilogauss magnetic fields.

Affiliated with

Also associated with

No associations

Rating

Fine structure of solar magnetic fields 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 Fine structure of solar magnetic fields, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fine structure of solar magnetic fields will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-836311