The problem of the depth of spectral line formation in the solar atmosphere

Details The problem of the depth of spectral line formation in the solar atmosphere The problem of the depth of spectral line formation in the solar atmosphere

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978poast..26..233s&link_type=abstract

Postepy Astronomii, vol. 26, Oct.-Dec. 1978, p. 233-243. In Polish.

Mathematics

Line Spectra, Solar Atmosphere, Solar Spectra, Spectral Line Width, Atmospheric Stratification, Functions (Mathematics), Integral Equations

Scientific paper

In the present paper, two methods of determining the depth of spectral line formation in the solar atmosphere are examined. One method is based on the concept of a contribution function (CF) (in the sense of contribution to the observed intensity or absorption). The other method is based on the use of a response function (RF) which illustrates the action of small disturbances in solar atmospheric layers on the observed line profile.

Affiliated with

Also associated with

No associations

Rating

The problem of the depth of spectral line formation in the solar atmosphere 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 problem of the depth of spectral line formation in the solar atmosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The problem of the depth of spectral line formation in the solar atmosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-889774