The LFI radiometers use a pseudo-correlation design where the signal from the sky is continuously compared with a stable reference signal, provided by a cryogenic reference load system. The reference unit is composed by small pyramidal horns, one for each radiometer, 22 in total, facing small absorbing targets, made of a commercial resin ECCOSORB CRTM, cooled to ~ 4.5 K. Horns and targets are separated by a small gap to allow thermal decoupling. Target and horn design is optimized for each of the LFI bands, centered at 70, 44 and 30 GHz. Pyramidal horns are either machined inside the radiometer 20K module or connected via external electro-formed bended waveguides. The requirement of high stability of the reference signal imposed a careful design for the radiometric and thermal properties of the loads. Materials used for the manufacturing have been characterized for thermal, RF and mechanical properties. We describe in this paper the design and the performance of the reference system.

Planck-LFI : design and performance of the 4 Kelvin Reference Load Unit / L. Valenziano, F. Cuttaia, A. De Rosa, L. Terenzi, A. Brighenti, G. P. Cazzola, A. Garbesi, S. Mariotti, G. Orsi, L. Pagan, F. Cavaliere, M. Biggi, R. Lapini, E. Panagin, P. Battaglia, R. C. Butler, M. R. F. Bersanelli, O. D’Arcangelo, S. Levin, N. Mandolesi, A. Mennella, G. Morgante, G. Morigi, M. Sandri, A. Simonetto, M. Tomasi, F. Villa, M. Frailis, S. Galeotta, A. Gregorio, R. Leonardi, S. R. Lowe, M. Maris, P. Meinhold, L. Mendes, L. Stringhetti, A. Zonca, A. Zacchei. - In: JOURNAL OF INSTRUMENTATION. - ISSN 1748-0221. - 4:12(2009 Dec), pp. T12006.T12006.1-T12006.T12006.27. [10.1088/1748-0221/4/12/T12006]

Planck-LFI : design and performance of the 4 Kelvin Reference Load Unit

F. Cavaliere;M.R.F. Bersanelli;A. Mennella;M. Tomasi;A. Zonca
Penultimo
;
2009

Abstract

The LFI radiometers use a pseudo-correlation design where the signal from the sky is continuously compared with a stable reference signal, provided by a cryogenic reference load system. The reference unit is composed by small pyramidal horns, one for each radiometer, 22 in total, facing small absorbing targets, made of a commercial resin ECCOSORB CRTM, cooled to ~ 4.5 K. Horns and targets are separated by a small gap to allow thermal decoupling. Target and horn design is optimized for each of the LFI bands, centered at 70, 44 and 30 GHz. Pyramidal horns are either machined inside the radiometer 20K module or connected via external electro-formed bended waveguides. The requirement of high stability of the reference signal imposed a careful design for the radiometric and thermal properties of the loads. Materials used for the manufacturing have been characterized for thermal, RF and mechanical properties. We describe in this paper the design and the performance of the reference system.
space instrumentation ; microwave radiometers ; instruments for CMB observations ; microwave Calibrators
Settore FIS/05 - Astronomia e Astrofisica
Settore FIS/01 - Fisica Sperimentale
dic-2009
Article (author)
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2434/150611
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