Polarization of the atmosphere as a foreground for cosmic microwave background polarization experiments
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Shaul Hanany | Cambridge | Philip Rosenkranz University of Minnesota | Twin Cities | Minneapolis Massachusetts Institute of Technology | Massachusetts
[1] Iaga Division,et al. Revision of International Geomagnetic Reference Field released , 1996 .
[2] Bruce G. Terrell,et al. National Oceanic and Atmospheric Administration , 2020, Federal Regulatory Guide.
[3] D. H. Staelin,et al. Polarized thermal microwave emission from oxygen in the mesosphere , 1988 .
[4] William B. Lenoir,et al. Microwave spectrum of molecular oxygen in the mesosphere. , 1968 .
[5] Brian Keating,et al. LARGE ANGULAR SCALE POLARIZATION OF THE COSMIC MICROWAVE BACKGROUND RADIATION AND THE FEASIBILITY OF ITS DETECTION , 1997 .
[6] M. Tinkham. Theory of the fine structure of the molecular oxygen ground state with an experimental study of its microwave paramagnetic spectrum , 1955 .
[7] G. Giardino,et al. Towards a model of full-sky Galactic synchrotron intensity and linear polarisation: A re-analysis of the Parkes data , 2002, astro-ph/0202520.
[8] David J. Schlegel,et al. Extrapolation of Galactic Dust Emission at 100 Microns to Cosmic Microwave Background Radiation Frequencies Using FIRAS , 1999, astro-ph/9905128.
[9] Philip W. Rosenkranz,et al. Atmospheric 60-GHz oxygen spectrum : new laboratory measurements and line parameters , 1992 .
[10] M. Strandberg,et al. Interaction of Molecular Oxygen with a Magnetic Field , 1955 .