Abstract
Radiometeric CMB measurements need to be highly stable and this stability is best obtained with differential receivers. The residual 1/f noise in the differential output is strongly dependent on the radiometer input offset which can be cancelled using various balancing strategies. In this paper we discuss a software method implemented in the PLANCK-LFI pseudo-correlation receivers which uses a tunable gain modulation factor, r, in the sky-load difference. Numerical simulations and experimental data show how proper tuning of the parameter r ensures a very stable differential output with knee frequencies of the order of few mHz, Various approaches to calculate r using the radiometer total power data are discussed with some examples relevant to PLANCK-LFI. Although the paper focuses on pseudo-correlation receivers and the examples are relative to PLANCK-LFI, the proposed method and its analysis is general and can be applied to a large class of differential radiometric receivers.
Original language | English |
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Pages (from-to) | 1089-1100 |
Number of pages | 11 |
Journal | Astronomy and Astrophysics |
Volume | 410 |
Issue number | 3 |
DOIs | |
Publication status | Published - Nov 2003 |
Keywords
- Cosmology: cosmic microwave background, observations
- Instrumentation: detectors
- Methods: analytical