Sub-arcminute structure of the zodiacal emission

Details Sub-arcminute structure of the zodiacal emission Sub-arcminute structure of the zodiacal emission

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..819s&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.819

Computer Science

Scientific paper

In our study we used the data of the following Spitzer programs: (i) "First Look Survey - Ecliptic Plane Component" (FLS_ECLIPTIC_PLANE/98); (ii) "The production of zodiacal dust by asteroids and comets" (ZODY/2317); (iii) "High latitude dust bands in the main asteroid belt: Fingerprints of recent breakup events" (HILAT/20539); (iv) "A new source of interplanetary dust: Type II dust trails" (T2T/30545). Our main aims are to determine the structure of the zodiacal emission available by the Spitzer/MIPS 24 μm measurements. Based on these data we derive power spectra and correlation functions in the target fields, calculate confusion noise, and apply models to reveal the nature of dust evolution in the interplanetary dust cloud.

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