A perturbation solution of the radiative transfer equation in a differentially moving atmosphere

Details A perturbation solution of the radiative transfer equation in a differentially moving atmosphere A perturbation solution of the radiative transfer equation in a differentially moving atmosphere

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976jqsrt..16..347c&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer, vol. 16, Apr. 1976, p. 347-355.

Physics

Optics

1

Atmospheric Circulation, Perturbation Theory, Radiative Transfer, Atmospheric Optics, Convergence, Doppler Effect, Numerical Analysis, Spectral Line Width, Transfer Functions

Scientific paper

We present a new technique for solving the radiative transfer equation in a differentially moving atmosphere. The method is based on a perturbation of the solution of the transfer problem in a static atmosphere. The perturbation technique may be applied with any method for solving the static atmosphere problem and leads to significant reductions in computer time and storage requirements. The method is flexible and may be used to solve problems involving depth dependence in any of the parameters of the transfer equation.

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