Differentiation of three dimensional models of the zodiacal interplanetary dust cloud for experiments with micrometeoroids decay detectors on the space station

Details Differentiation of three dimensional models of the zodiacal interplanetary dust cloud for experiments with micrometeoroids decay detectors on the space station Differentiation of three dimensional models of the zodiacal interplanetary dust cloud for experiments with micrometeoroids decay detectors on the space station

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phdt........10k&link_type=abstract

Ph.D. Thesis Ruhr Univ., Bochum (Germany, F.R.). Fakultaet für Physik und Astronomie.

Astronomy and Astrophysics

Astronomy

1

Explorer Satellites, Micrometeoroids, Zodiacal Dust, Infrared Spectra, Mathematical Models, Particle Flux Density, Poynting-Robertson Effect, Ulysses Mission, Visible Spectrum

Scientific paper

The spatial distribution of the zodiacal dust is presented as a result of inversion of the radiation or light integrales, and described by models from observations in visible and infrared spectra. The particle concentration and the flux densities are measured and the inclination is infrared, since the micrometeoroid detector Cosmic Dust Facility on the satellite platform space station does not take into account the vectors of the relative velocity. It is shown that all zodiacal particles cut across the ecliptic plane in its trajectory node so that the inclination distribution density can be estimated with consideration of the observation choice effects.

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