Out of ecliptic zodiacal cloud profile

Details Out of ecliptic zodiacal cloud profile Out of ecliptic zodiacal cloud profile

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983p%26ss...31..871m&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 31, Aug. 1983, p. 871-873.

Physics

Brightness Distribution, Light Scattering, Zodiacal Dust, Particle Density (Concentration), Zodiacal Light

Scientific paper

An attempt is made to find the zodiacal cloud shape out of the ecliptic, on the basis of the Mujica et al (1980) establishment of the optical homogeneity of the medium in the ecliptic plane by means of ecliptic density and scattering functions. The consistency of the profile obtained is checked through the calculation of the brightness curves obtainable by a hypothetical observer placed in the ecliptic at distances of 1.5, 2.0, and 2.5 AU.

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