Removing Artifacts in the Calibration of Cassini CIRS Spectra of Saturn and Titan

Details Removing Artifacts in the Calibration of Cassini CIRS Spectra of Saturn and Titan Removing Artifacts in the Calibration of Cassini CIRS Spectra of Saturn and Titan

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf...27c&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.27

Computer Science

Scientific paper

The Composite Infrared Spectrometer (CIRS) on the NASA Cassini spacecraft is a dual far- and mid-IR Fourier transform spectrometer (FTS) which covers the spectral range 10 - 1400 cm-1 with an adjustable spectral resolution of 7.8 - 0.27 cm-1 unapodized [1, 2]. The CIRS detectors comprise three separate focal planes totalling 21 individual pixels: A redundant pair of far-IR thermopiles (Focal Plane 1: 10 - 650 cm-1), a 1 x 10 mid-IR HgCdTe PC array (Focal Plane 3: 605 - 1119 cm-1), and a 1 x 10 mid-IR HgCdTe PV array (Focal Plane 4: 1114 - 1429 cm-1). CIRS is a dual-temperature FTS, since the FP3 and FP4 detector arrays are operated at ~ 76K, whereas the rest of CIRS, including the FP1 thermopiles, is maintained at ~170.0K to within ±0.1K.

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