The aluminum I autoionization doublet in the quiet solar spectrum

Details The aluminum I autoionization doublet in the quiet solar spectrum The aluminum I autoionization doublet in the quiet solar spectrum

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...248..352h&link_type=abstract

Astrophysical Journal, Part 1, vol. 248, Aug. 15, 1981, p. 352-357.

Astronomy and Astrophysics

Astrophysics

Aluminum, Autoionization, Line Spectra, Solar Atmosphere, Solar Spectra, Atmospheric Models, Skylab Program, Spectrum Analysis, Thermodynamic Equilibrium, Ultraviolet Spectra

Scientific paper

Observations are presented of the Al I autoionization doublet 1932 A and 1936 A in the quiet solar spectrum, obtained from the NRL slit spectrograph aboard Skylab and from the University of Hawaii Echelle Rocket Spectrograph. The observed profiles are compared with theoretical spectra computed for the Harvard Smithsonian Reference Atmosphere and the Vernazza, Avrett and Loeser (1976) solar models. It is found that nonlocal thermodynamic equilibrium effects are important in the line-formation problem and the synthetic spectra are in good agreeement with the data.

Affiliated with

Also associated with

No associations

Rating

The aluminum I autoionization doublet in the quiet solar spectrum 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 aluminum I autoionization doublet in the quiet solar spectrum, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The aluminum I autoionization doublet in the quiet solar spectrum will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1744817