Solar limb darkening in the wings of the CaII H and K lines

Details Solar limb darkening in the wings of the CaII H and K lines Solar limb darkening in the wings of the CaII H and K lines

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ge%26ae..49..879o&link_type=abstract

Geomagnetism and Aeronomy, Volume 49, Issue 7, pp.879-883

Computer Science

1

Scientific paper

The method for measuring solar limb darkening has been proposed, and the formulas, describing the law of solar limb darkening in the wings of the CaII H (396.849 nm) and K (393.369 nm) lines, have been derived. To operate at arbitrary points on the Sun’s surface, it is necessary to know the law of solar limb darkening, which is specific in different spectral regions. The procedure of spectrum correction for a flat field, proposed in our previous works, is based on comparing line-free spectral regions with the solar center reference spectrum from the atlas by Brault and Neckel [1994].

Affiliated with

Also associated with

No associations

Rating

Solar limb darkening in the wings of the CaII H and K lines 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 Solar limb darkening in the wings of the CaII H and K lines, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar limb darkening in the wings of the CaII H and K lines will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1887386