Opacity ratios for Doppler-broadened lines from common upper levels
- 31 August 1990
- journal article
- Published by Elsevier in Journal of Quantitative Spectroscopy and Radiative Transfer
- Vol. 44 (2) , 275-288
- https://doi.org/10.1016/0022-4073(90)90033-3
Abstract
No abstract availableThis publication has 15 references indexed in Scilit:
- Expressions for the computer-evaluation of the four kernel functions for line formation with Doppler and Lorentz profilesJournal of Quantitative Spectroscopy and Radiative Transfer, 1981
- An approximate calculation of the effect of opacity in the solar spectral lines of C IIIMonthly Notices of the Royal Astronomical Society, 1980
- The escape factor in plasma spectroscopy—I. The escape factor defined and evaluatedJournal of Quantitative Spectroscopy and Radiative Transfer, 1979
- Probability distributions for photon exitJournal of Quantitative Spectroscopy and Radiative Transfer, 1972
- Asymptotic Expansions of the Integrated Absorptance for Simple Spectral Lines and Lines with Hyperfine Structure and Isotope ShiftsJournal of the Optical Society of America, 1968
- The relative intensities of CI lines in the solar EUV spectrumSolar Physics, 1967
- Non-Coherent Scattering II: Line Formation with A Frequency Independent Source FunctionMonthly Notices of the Royal Astronomical Society, 1965
- Tables of functions encountered in the theory of resonance radiation transfer. I.Astrophysics, 1965
- über Linienemission aus inhomogener Schicht. II. TeilThe European Physical Journal A, 1949
- Imprisonment of Resonance Radiation in GasesPhysical Review B, 1947