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Radiative transfer in the surfaces of atmosphereless bodies. I - Theory. II - Interpretation of phase curves

Lumme, K., Bowell, E.·1981·The Astronomical Journal

Abstract

A generalized theory of radiative transfer is presented which includes single and multiple scattering of light in particulate surfaces, and is applicable to both the surfaces of atmosphereless bodies and to laboratory samples. Single scattering is described in terms of the effects of porosity and roughness, and is formulated by means of a probabilistic method. It is shown that, for low-albedo surfaces, the effects of porosity and roughness are separable, the opposition effect is caused by the former, and the slope of the linear part of the phase curve is mainly controlled by the latter. The theory, which is applicable to all albedos and phase angles, may be used in both surface brightness and integrated brightness studies. The limiting case of roughness and volume density tending to zero yields the results of classical radiative transfer theory.

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Metadata

Authors
Lumme, K., & Bowell, E.
Venue
The Astronomical Journal
Published
1981-11
Volume
86
Pages
1694
ISSN
0004-6256 (ISSN-L)
OpenAlex
W2068141725
Cited by
265
References
0
FWCI
9.56
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Radiative transfer in the surfaces of atmosphereless bodies. I - Theory. II - Interpretation of phase curves. https://app.cochat.ai/papers/10.1086/113054
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Lumme, K., & Bowell, E. (1981). Radiative transfer in the surfaces of atmosphereless bodies. I - Theory. II - Interpretation of phase curves. The Astronomical Journal. https://doi.org/10.1086/113054

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