Thermal architecture design tests for the Planck/HFI instrument

Details Thermal architecture design tests for the Planck/HFI instrument Thermal architecture design tests for the Planck/HFI instrument

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000nimpa.444..413p&link_type=abstract

Nuclear Instruments and Methods in Physics Research Section A, Volume 444, Issue 1-2, p. 413-418.

Physics

5

Scientific paper

The ESA satellite project Planck is designed to survey the sky at sub-millimetre and millimetre wavelengths in a drift scan mode. The High-Frequency Instrument (HFI) will use 48 bolometers cooled to 100mK by a dilution cooler. In this paper, we describe how the scan strategy leads to requirements on the 0.1K stage temperature stability and how a combination of a passive and an active system can be used to approach this specification.

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