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Planck-HFI focal plane concept

Maffei, Bruno, Ade, Peter A. R., Bock, James J., Brossard, J., Gleeson, Emily M., Lamarre, Jean-Michael, Lange, Andrew E., Longval, Yu-Ying, Murphy, John A., Pisano, Giampaolo, Puget, Jean-Loup, Ristorcelli, I., Sudiwala, Rashmikant V. and Yurchenko, Vladimir B. 2004. Planck-HFI focal plane concept. Presented at: Optical, Infrared, and Millimeter Space Telescopes, Glasgow, UK, 21-25 June 2004. Published in: Mather, John C. ed. Optical, Infrared, and Millimeter Space Telescopes (Proceedings). Proceedings of SPIE , vol. 5487. Bellingham, WA: SPIE, p. 523. 10.1117/12.552577

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Abstract

The future ESA space mission Planck Surveyor mission will measure the Cosmic Microwave Background temperature and polarisation anisotropies in a frequency domain comprised between 30GHz and 1THz. On board two instruments, LFI based on HEMT technology and HFI using bolometric detectors. We present the optical solutions adopted for this mission, in particular the focal plane design of HFI, concept which has been applied already to other instruments such as the balloon borne experiment Archeops.

Item Type: Conference or Workshop Item (Paper)
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Uncontrolled Keywords: Equipment and services; Field effect transistors; Polarization; Sensors
Publisher: SPIE
ISBN: 9780819454195
Related URLs:
Last Modified: 04 Jun 2017 04:38
URI: http://orca-mwe.cf.ac.uk/id/eprint/42032

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