Properties of interplanetary dust from infrared and optical observations. I - Temperature, global volume intensity, albedo and their heliocentric gradients

Details Properties of interplanetary dust from infrared and optical observations. I - Temperature, global volume intensity, albedo and their heliocentric gradients Properties of interplanetary dust from infrared and optical observations. I - Temperature, global volume intensity, albedo and their heliocentric gradients

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...191..154d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 191, no. 1, Feb. 1988, p. 154-160. CNRS-supported research.

Computer Science

Sound

37

Albedo, Infrared Astronomy Satellite, Interplanetary Dust, Rocket Sounding, Zodiacal Dust, Line Of Sight, Mathematical Models, Interplanetary Dust, Optical Properties, Infrared, Wavelengths, Intensity, Temperature, Physical Properties, Volume, Albedo, Photometry, Brightness, Scattering, Calculations, Procedure, Iras Satellite, Gradients, Radiation, Satellite Observations, Thermal Properties, Emissions, Astronomy

Scientific paper

The method of the 'nodes of lesser uncertainty' developed by Dumont and Levasseur-Regourd (1985) for retrieval of local information on the properties of interplanetary dust medium was used for determinations on thermal emission of interplanetary dust. The techniques applicable for the thermal case are presented, and results on temperature, global volume intensity, and albedo are derived from the available observations of optical scattering and thermal emission. The method allowed the retrieval of various parameters of the interplanetary dust cloud at 1 AU heliocentric distance, as well as their gradients in a 0.5-1.5 AU range.

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