Spatial distribution of the interplanetary dust deduced by infrared observations

Details Spatial distribution of the interplanetary dust deduced by infrared observations Spatial distribution of the interplanetary dust deduced by infrared observations

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...370..396d&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 370, March 20, 1991, p. 396, 397. Research supported by ASI and Ministero d

Astronomy and Astrophysics

Astronomy

Infrared Astronomy, Interplanetary Dust, Interplanetary Medium, Spatial Distribution, Zodiacal Light, Brightness, Digital Simulation, Elongation, Homogeneity, Wavelengths, Interplanetary Dust, Distribution, Infrared, Wavelengths, Astronomy, Numerical Methods, Simulations, Density, Zodiacal Light, Idps, Experiments, Brightness, Thermal Properties, Emissions, Analysis

Scientific paper

IR observations of the interplanetary dust performed by the ZIP rocket experiment are analyzed, focusing on the effect of experimental errors on the inversion procedure previously used to obtain the spatial distribution of the dust. Numerical simulation shows that the experimental errors are too large to reveal deviations of the dust density from a simple power-law radial distribution. The accuracy which would be required in future experiments is estimated.

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