Semiempirical LTE Modelling of Solar Photospheric Layers I. Theoretical background

Details Semiempirical LTE Modelling of Solar Photospheric Layers I. Theoretical background Semiempirical LTE Modelling of Solar Photospheric Layers I. Theoretical background

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993coska..23..107b&link_type=abstract

Contributions of the Astronomical Observatory Skalnate Pleso, vol. 23, p. 107-117.

Statistics

Computation

4

Solar Atmosphere, Lte Modelling, Spectral Lines Calculations

Scientific paper

The calculation of the physical parameters of photospheric layers using the LTE approximation is described. The main algorithm for calculating photospheric lines is given.The corrections of the Saha and Boltzman equations for the upper layers are discused and the effect of the magnetic field is taken into account. The actual computational code and detailed description of how to use it will be published in Part II of this paper.

Affiliated with

Also associated with

No associations

Rating

Semiempirical LTE Modelling of Solar Photospheric Layers I. Theoretical background 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 Semiempirical LTE Modelling of Solar Photospheric Layers I. Theoretical background, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Semiempirical LTE Modelling of Solar Photospheric Layers I. Theoretical background will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1070570