Principles of modeling planetary thermal radiation intensity fields

Details Principles of modeling planetary thermal radiation intensity fields Principles of modeling planetary thermal radiation intensity fields

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979kosis..17..146k&link_type=abstract

Kosmicheskie Issledovaniia, vol. 17, Jan.-Feb. 1979, p. 146-150. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Planetary Radiation, Radiant Flux Density, Thermal Radiation, Thermal Simulation, Approximation, Conical Bodies, Diffuse Radiation, Error Analysis, Flat Surfaces, Heat Transfer, Radiation Spectra

Scientific paper

Some aspects of the problem of reproducing, under terrestrial conditions, a planetary thermal radiation field are discussed. Requirements are formulated for the orientation and the emission law of the radiating elements of an ideally diffuse planetary model. Approaches to the approximate solution to the problem of reproducing the thermal radiation field of a planet with a uniform flux density distribution are examined.

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