Diffuse Radio Foregrounds - All-Sky Polarisation, and Anomalous Microwave Emission (Hardcover, 1st ed. 2016)

This extensive thesis work covers several topics, including intensity and polarization, focusing on a new polarization bias reduction method. Vidal studied data from the WMAP satellite, which is low signal-to-noise and as such has to be corrected for polarization bias. He presents a new method for correcting the data, based on knowledge of the underlying angle of polarization. Using this novel method, he sets upper limits for the polarization fraction of regions known to emit significant amounts of spinning dust emissions. He also studies the large-scale loops and filaments that dominate the synchrotron sky. The dominant features are investigated, including identification of several new features. For the North Polar Spur, a model of an expanding shell in the vicinity of the Sun is tested, which appears to fit the data. Implications for CMB polarization surveys are also discussed. In addition, Vidal presents interferometric observations of the dark cloud LDN 1780 at 31 GHz and shows that the spinning dust hypothesis can explain the radio properties observed.

General

Imprint:	Springer International Publishing AG
Country of origin:	Switzerland
Series:	Springer Theses
Release date:	December 2015
First published:	2016
Authors:	Matias Vidal Navarro
Dimensions:	235 x 155 x 14mm (L x W x T)
Format:	Hardcover
Pages:	196
Edition:	1st ed. 2016
ISBN-13:	978-3-319-26262-8
Categories:	Books > Science & Mathematics > Astronomy, space & time > Cosmology & the universe Promotions
LSN:	3-319-26262-9
Barcode:	9783319262628

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