Problems in constructing a genetic model of the interplanetary dust cloud

Details Problems in constructing a genetic model of the interplanetary dust cloud Problems in constructing a genetic model of the interplanetary dust cloud

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980avest..13..160l&link_type=abstract

(Astronomicheskii Vestnik, vol. 13, July-Sept. 1979, p. 160-168.) Solar System Research, vol. 13, no. 3, Jan. 1980, p. 122-128.

Astronomy and Astrophysics

Astronomy

1

Astronomical Models, Interplanetary Dust, Meteoroids, Genetics, Illuminance, Mass Distribution, Orbital Elements, Radio Meteors

Scientific paper

It is shown that a revised theory of photographic meteor noticeability taking the laboratory simulation of meteoric phenomena into account allows us to approximate the orbital distribution of radio and photographic meteors. A more correct calculation of the effect of light pressure and the Poynting-Robertson effect on the motion of interplanetary dust particles leads to an explanation of the observed ultraviolet brightness excess in the zodiacal light and the relative deficit of the orbits with retrograde motion for these particles in comparison with larger meteoroids.

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