Advanced pseudo-correlation radiometers for the Planck-LFI instrument
| dc.creator | Mennella, A. | |
| dc.creator | Bersanelli, M. | |
| dc.creator | Butler, R. C. | |
| dc.creator | Maino, D. | |
| dc.creator | Mandolesi, N. | |
| dc.creator | Morgante, G. | |
| dc.creator | Valenziano, L. | |
| dc.creator | Villa, F. | |
| dc.creator | Gaier, T. | |
| dc.creator | Seiffert, M. | |
| dc.creator | Levin, S. | |
| dc.creator | Lawrence, C. | |
| dc.creator | Meinhold, P. | |
| dc.creator | Lubin, P. | |
| dc.creator | Tuovinen, J. | |
| dc.creator | Varis, J. | |
| dc.creator | Karttaavi, T. | |
| dc.creator | Hughes, N. | |
| dc.creator | Jukkala, P. | |
| dc.creator | Sjman, P. | |
| dc.creator | Kangaslahti, P. | |
| dc.creator | Roddis, N. | |
| dc.creator | Kettle, D. | |
| dc.creator | Winder, F. | |
| dc.creator | Blackhurst, E. | |
| dc.creator | Davis, R. | |
| dc.creator | Wilkinson, A. | |
| dc.creator | Castelli, C. | |
| dc.creator | Aja, B. | |
| dc.creator | Artal, E. | |
| dc.creator | de la Fuente, L. | |
| dc.creator | Mediavilla, A. | |
| dc.creator | Pascual, J. P. | |
| dc.creator | Gallegos, J. | |
| dc.creator | Martinez-Gonzalez, E. | |
| dc.creator | de Paco, P. | |
| dc.creator | Pradell, L. | |
| dc.date | 2003-07-07 | |
| dc.date.accessioned | 2026-07-07T02:08:55Z | |
| dc.date.available | 2026-07-07T02:08:55Z | |
| dc.description | The LFI (Low Frequency Instrument) on board the ESA Planck satellite is constituted by an array of radiometric detectors actively cooled at 20 K in the 30-70 GHz frequency range in the focal plane of the Planck telescope. In this paper we present an overview of the LFI instrument, with a particular focus on the radiometer design. The adopted pseudo-correlation scheme uses a software balancing technique (with a tunable parameter called gain modulation factor) which is effective in reducing the radiometer susceptibility to amplifier instabilities also in presence of small non-idealities in the radiometric chain components, provided that the gain modulation factor is estimated with an accuracy of the order of 0.2%. These results have been recently confirmed by experimental laboratory measurements conducted on the LFI prototype radiometers at 30, 70 and 100 GHz. | |
| dc.description | 6 pages, 3 figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0307116 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0307116 | |
| dc.identifier | Proc 3rd ESA Workshop on millimetre wave technology and applications (ESPOO, 21-23 May 2003), Page 69 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6247 | |
| dc.subject | Astrophysics | |
| dc.title | Advanced pseudo-correlation radiometers for the Planck-LFI instrument | |
| dc.type | text |