Henyey–Greenstein and Mie phase functions in Monte Carlo radiative transfer computations

Applied Optics

Volumn 35, Issue 18, 1996, Pages 3270-3274

  Toublanc, Dominique ^a  

^a CNRS   (France)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001102490     PISSN: 1559128X     EISSN: 21553165     Source Type: Journal    
DOI: 10.1364/AO.35.003270     Document Type: Article

References (11)

1. L. C. Henyey and J. L. Greenstein, “Diffuse radiation in the galaxy,”Astrophys. J. 93, 70-83 (1941).
2. W. M. Irvine, “Multiple scattering by large particles,”Astro-phys. J. 4, 1563-1575 (1965).
3. W. M. Cornette and J. G. Shanks, “Physically reasonable analytic expression for the single-scattering phase function,” Appl. Opt. 31, 3152-3160 (1992).
4. C. M. Chu and S. W. Churchill, “Representation of the angular distribution of radiation scattered by a spherical particle,” J. Opt. Soc. Am. 45, 958-962 (1955).
5. J. E. Hansen and L. D. Travis, “Light scattering in planetary atmospheres,” Space Science Rev. 16, 527-610 (1974).
6. W. J. Lentz, “Generating Bessel functions in Mie scattering calculations using continued fractions,” Appl. Opt. 15, 668-671 (1976).
7. W. J. Wiscombe, “Improved Mie scattering algorithms,” Appl. Opt. 19, 1505-1509 (1980).
8. H. C. van de Hulst, Light Scattering by Small Particles (Wiley, New York, 1957).
9. G. W. Kattawar, “A three-parameter analytic phase function for multiple scattering calculations,” J. Quant. Spectrosc. Radiat. Transfer 15, 839-849 (1975).
10. C. P. McKay, J. B. Pollack, and R. Courtin, “The thermal structure of Titan’s atmosphere,”Icarus 80, 23-53 (1989).
11. D. Toublanc, J. P. Parisot, J. Brillet, D. Gautier, F. Raulin, and C. P. McKay, “Photochemical modeling of Titan’s atmosphere,” Icarus 113, 2-26 (1995)