Observing CMB polarisation through ice

Ice crystal clouds in the upper troposphere can generate polarization signals at the μK level. This signal can seriously affect very sensitive ground-based searches for E and B modes of cosmic microwave background polarization. In this paper, we estimate this effect within the CLOVER experiment obse...

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Bibliographic Details
Published in:Monthly Notices of the Royal Astronomical Society
Main Authors: Pietranera, Luca, Buehler, Stefan A., Calisse, Paolo G., Emde, Claudia, Hayton, Darren, John, Viju O., Maffei, Bruno, Piccirillo, Lucio, Pisano, Giampaolo, Savini, Giorgio, Sreerekha, T. R.
Format: Article in Journal/Newspaper
Language:unknown
Published: Oxford University Press 2007
Subjects:
Fernerkundung der Atmosphäre
Antarc*
Antarctica
Online Access:https://elib.dlr.de/47834/
http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2007.11464.x/full
Description
Summary:Ice crystal clouds in the upper troposphere can generate polarization signals at the μK level. This signal can seriously affect very sensitive ground-based searches for E and B modes of cosmic microwave background polarization. In this paper, we estimate this effect within the CLOVER experiment observing bands (97, 150 and 220 GHz) for the selected observing site (Llano de Chajnantor, Atacama desert, Chile). The results show that the polarization signal from the clouds can be of the order of or even bigger than the cosmic microwave background expected polarization. Climatological data suggest that this signal is fairly constant over the whole year in Antarctica. On the other hand, the stronger seasonal variability in Atacama allows for a 50 per cent of clean observations during the dry season.

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