Spectral lines in hot dense matter

Details Spectral lines in hot dense matter Spectral lines in hot dense matter

Jan 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977jqsrt..17...77r&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer, vol. 17, Jan. 1977, p. 77-88.

Statistics

Computation

15

Absorption Cross Sections, High Temperature Plasmas, Photoabsorption, Plasma Density, Plasma Spectra, Beryllium, Dense Plasmas, Elastic Scattering, Electron Impact, Germanium, Inelastic Scattering, Line Spectra, Metallic Plasmas, Stark Effect, Temperature Effects

Scientific paper

An algorithm is presented for the computation of photoabsorption cross sections at arbitrary temperature and matter density. The 'average atom' model is refined to give an approximate account for the different ionization stages. The broadening of spectral lines is accounted for in a simple approximation. Calculations are presented for the beryllium and germanium plasmas in the frequency region of spectral lines.

Affiliated with

Also associated with

No associations

Rating

Spectral lines in hot dense matter 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 Spectral lines in hot dense matter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectral lines in hot dense matter will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-952716