http://www.cnr.it/ontology/cnr/individuo/prodotto/ID81185
Millimeterwave Tests on Passive Components of PLANCK-LFI (Contributo in atti di convegno)
- Type
- Label
- Millimeterwave Tests on Passive Components of PLANCK-LFI (Contributo in atti di convegno) (literal)
- Anno
- 2004-01-01T00:00:00+01:00 (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
- 10.1109/ICIMW.2004.1422150 (literal)
- Alternative label
Simonetto A., D'Arcangelo O., Figini L., Sozzi C., Guzzi P., Battaglia P., Villa F., Sandri M. and Bersanelli M. (2004)
Millimeterwave Tests on Passive Components of PLANCK-LFI
in Joint 29th International Conference on Infrared and Millimeter Waves/12th International Conference on Terahertz Electronics, Univ Karlsruhe, Karlsruhe, GERMANY, 17/9/2004-1/10/2004
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- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
- Simonetto A., D'Arcangelo O., Figini L., Sozzi C., Guzzi P., Battaglia P., Villa F., Sandri M. and Bersanelli M. (literal)
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- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#url
- http://ieeexplore.ieee.org/xpls/abs_all.jsp?arnumber=1422150 (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#titoloVolume
- CONFERENCE DIGEST OF THE 2004 JOINT 29TH INTERNATIONAL CONFERENCE ON INFRARED AND MILLIMETER WAVES AND 12TH INTERNATIONAL CONFERENCE ON TERAHERTZ ELECTRONICS (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#pagineTotali
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- ISI Web of Science (WOS) (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
- IFP-CNR Milano, Italy
Alenia Spazio Spa -LABEN, Vimodrone (MI) Italy
IASF-CNR/INAF, Bologna Italy
Universita' degli Studi di Milano, Milano Italy (literal)
- Titolo
- Millimeterwave Tests on Passive Components of PLANCK-LFI (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#isbn
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#curatoriVolume
- Thumm, M; Wiesbeck, W (literal)
- Abstract
- PLANCK [1] is the ESA mission devoted to Cosmic Microwave Background (CMB) to be launched in 2007. After COBE and WMAP pioneering work, PLANCK is designed to measure the anisotropy spectrum to the full extent of cosmological relevance and make quantitative measurements of CMB polarization. Its optical system will consist of a Gregorian telescope coupled with two instruments on the focal surface: the High Frequency Instrument (HFI) [2], an array of bolometers covering the spectral range from 84 GHz to 1THz; and the Low Frequency Instrument (LFI) [3,4], an array of pseudocorrelation radiometers spanning the range from 27 to 77 GHz in three 20% frequency bands. We measured vector patterns and return loss of feedhorns and S parameters of OMTs and waveguides, obtaining good agreement with the very demanding design specifications. (literal)
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