The impact of atmospheric fluctuations on degree-scale imaging of the cosmic microwave background

There is currently an active effort to map the spatial variations in the intensity of the cosmic microwave background (CMB), with different experiments utilizing chopped beam, swept beam, and interferometric approaches to minimize systematic errors. Fluctuations in the brightness of the Earth’s atmo...

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Main Authors: Oliver P. Lay, Nils W. Halverson
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Published: 2000
Subjects:
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.336.9177
http://arxiv.org/pdf/astro-ph/9905369v1.pdf
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spelling ftciteseerx:oai:CiteSeerX.psu:10.1.1.336.9177 2023-05-15T13:36:25+02:00 The impact of atmospheric fluctuations on degree-scale imaging of the cosmic microwave background Oliver P. Lay Nils W. Halverson The Pennsylvania State University CiteSeerX Archives 2000 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.336.9177 http://arxiv.org/pdf/astro-ph/9905369v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.336.9177 http://arxiv.org/pdf/astro-ph/9905369v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/astro-ph/9905369v1.pdf text 2000 ftciteseerx 2016-01-07T23:42:32Z There is currently an active effort to map the spatial variations in the intensity of the cosmic microwave background (CMB), with different experiments utilizing chopped beam, swept beam, and interferometric approaches to minimize systematic errors. Fluctuations in the brightness of the Earth’s atmosphere originating from water vapor are an important source of noise for ground-based instruments. This paper presents a model for the fluctuations and derives simple expressions to predict the contribution of the atmosphere to experimental measurements. Data from the South Pole and from the Atacama Desert in Chile, two of the driest places on Earth, are used to assess the level of fluctuations at each site. The model consists of a layer of turbulence in which the fluctuations follow a modified Kolmogorov power law, with both three- and two-dimensional regimes. The isotropic, three-dimensional case, which applies on small scales, is dominant in most applications. The analysis treats the instruments as window functions that act on the power spectrum of the fluctuations, resulting in a simple pictorial approach analogous to the instrumental window functions that are applied to theoretical models of the CMB angular power spectrum. The South Pole data are from the Python V experiment, and are used to estimate the level of atmospheric fluctuations over 2 months of the summer. The distribution is bimodal, with long periods of very stable conditions (∆Trms < 1 mK in a 6 ◦ strip) broken by occasional periods of much stronger fluctuations (∆Trms> 10 mK), which appear to be associated with clouds. These periods are correlated with a change in wind direction that brings moist air from West Antarctica. 1 Text Antarc* Antarctica South pole South pole West Antarctica Unknown South Pole West Antarctica
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description There is currently an active effort to map the spatial variations in the intensity of the cosmic microwave background (CMB), with different experiments utilizing chopped beam, swept beam, and interferometric approaches to minimize systematic errors. Fluctuations in the brightness of the Earth’s atmosphere originating from water vapor are an important source of noise for ground-based instruments. This paper presents a model for the fluctuations and derives simple expressions to predict the contribution of the atmosphere to experimental measurements. Data from the South Pole and from the Atacama Desert in Chile, two of the driest places on Earth, are used to assess the level of fluctuations at each site. The model consists of a layer of turbulence in which the fluctuations follow a modified Kolmogorov power law, with both three- and two-dimensional regimes. The isotropic, three-dimensional case, which applies on small scales, is dominant in most applications. The analysis treats the instruments as window functions that act on the power spectrum of the fluctuations, resulting in a simple pictorial approach analogous to the instrumental window functions that are applied to theoretical models of the CMB angular power spectrum. The South Pole data are from the Python V experiment, and are used to estimate the level of atmospheric fluctuations over 2 months of the summer. The distribution is bimodal, with long periods of very stable conditions (∆Trms < 1 mK in a 6 ◦ strip) broken by occasional periods of much stronger fluctuations (∆Trms> 10 mK), which appear to be associated with clouds. These periods are correlated with a change in wind direction that brings moist air from West Antarctica. 1
author2 The Pennsylvania State University CiteSeerX Archives
format Text
author Oliver P. Lay
Nils W. Halverson
spellingShingle Oliver P. Lay
Nils W. Halverson
The impact of atmospheric fluctuations on degree-scale imaging of the cosmic microwave background
author_facet Oliver P. Lay
Nils W. Halverson
author_sort Oliver P. Lay
title The impact of atmospheric fluctuations on degree-scale imaging of the cosmic microwave background
title_short The impact of atmospheric fluctuations on degree-scale imaging of the cosmic microwave background
title_full The impact of atmospheric fluctuations on degree-scale imaging of the cosmic microwave background
title_fullStr The impact of atmospheric fluctuations on degree-scale imaging of the cosmic microwave background
title_full_unstemmed The impact of atmospheric fluctuations on degree-scale imaging of the cosmic microwave background
title_sort impact of atmospheric fluctuations on degree-scale imaging of the cosmic microwave background
publishDate 2000
url http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.336.9177
http://arxiv.org/pdf/astro-ph/9905369v1.pdf
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http://arxiv.org/pdf/astro-ph/9905369v1.pdf
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