Computer Science
Scientific paper
Apr 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999stin...9964428j&link_type=abstract
Technical Report, NASA/CR-1999-209246; NAS 1.26:209246
Computer Science
Zodiacal Dust, Temporal Distribution, Data Processing, Annual Variations, Near Infrared Radiation, Low Frequencies, High Frequencies, Extraction, Data Reduction, Cosmic Background Explorer Satellite, Asymmetry, Asteroids
Scientific paper
The report presents the results of the data analyses of the DIRBE-COBE data set to study the structure of the zodiacal cloud in the near-infrared wavebands at 1.2, 2.2, and 3.4 microns. The cloud has been divided into two components which have been analyzed and studied separately. The annual variation of the flux in the smooth or low frequency component has been measured in all three bands and the presence of any asymmetries due to the Earth's resonant ring have been studied. The high frequency component which primarily consisted of the asteroidal dust bands. Extensive and careful co-addition was done to extract the central bands in all three wavebands. The ten-degree bands are present in the 1.2 and 2.2 microns but not in the 3.4 micron waveband.
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