JPL Technical Report Server

Bolometric detectors for the high frequency instrument on the Planck surveyor

Show simple item record

dc.contributor.author Koch, T. C. en_US
dc.contributor.author Paine, C. en_US
dc.contributor.author Husted, L. en_US
dc.contributor.author Yun, M. en_US
dc.contributor.author Lange, A. en_US
dc.contributor.author Bock, J. en_US
dc.contributor.author Jones, B. en_US
dc.contributor.author Ade, P. en_US
dc.contributor.author Sudiwala, R. en_US
dc.date.accessioned 2004-09-17
dc.date.available 2004-09-17
dc.date.issued 2002-03 en_US
dc.identifier.citation 2002 IEEE Aerospace Conference en_US
dc.identifier.citation Big Sky, MT, USA en_US
dc.identifier.clearanceno 02-0032 en_US
dc.identifier.uri http://hdl.handle.net/2014/8080
dc.description.abstract The High Frequency Instrument (HFI) on Planck will obtain all-sky images of the Cosmic Microwave Background (CMB) and other astrophysical sources of emission with resolution of 9 arcniin at 100 GHz, 7 arcmin at 143 GHz and 5 arcniin at 217, 353, 545 and 857 GHz. The HFI focal plane will contain 48 silicon nitride micromesh bolometric detectors operating from a 100 mK heat sink. Four detectors in each of the 6 bands will detect the sum of the power in both linear polarizations. An additional 4 pair of detectors will provide sensitivity to linear polarization of emission at 143, 217 and 353 GHz. We report on the development of these detectors, which are being produced at the JPL Micro Devices Laboratory, packaged at JPL Electronics Packaging, characterized at 100 mK before delivery to our HFI consortium partners at the UWCC, UK. en_US
dc.format.extent 4294208 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Planck CMB bolometer en_US
dc.title Bolometric detectors for the high frequency instrument on the Planck surveyor en_US


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search


Browse

My Account