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Diffuse radio foregrounds[electronic resource] :all-sky polarisation, and anomalous microwave emission /

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
杜威分類號:	523.01
書名/作者:	Diffuse radio foregrounds : all-sky polarisation, and anomalous microwave emission // by Matias Vidal Navarro.
作者:	Vidal Navarro, Matias.
出版者:	Cham : : Springer International Publishing :, 2016.
面頁冊數:	xliv, 196 p. : : ill., digital ;; 24 cm.
Contained By:	Springer eBooks
標題:	Cosmic background radiation.
標題:	Physics.
標題:	Cosmology.
標題:	Astronomy, Observations and Techniques.
標題:	Astrophysics and Astroparticles.
ISBN:	9783319262635
ISBN:	9783319262628
內容註:	Introduction -- Analysis Techniques for WMAP Polarisation data -- WMAP Polarised Filaments -- QUIET Galactic Observations -- AME in LDN1780 -- Conclusions and Future Work.
摘要、提要註:	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.
電子資源:	http://dx.doi.org/10.1007/978-3-319-26263-5

Diffuse radio foregrounds[electronic resource] :all-sky polarisation, and anomalous microwave emission /
Vidal Navarro, Matias.

Diffuse radio foregroundsall-sky polarisation, and anomalous microwave emission /[electronic resource] :by Matias Vidal Navarro. - Cham :Springer International Publishing :2016. - xliv, 196 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

Introduction -- Analysis Techniques for WMAP Polarisation data -- WMAP Polarised Filaments -- QUIET Galactic Observations -- AME in LDN1780 -- Conclusions and Future Work.

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.

ISBN: 9783319262635

Standard No.: 10.1007/978-3-319-26263-5doiSubjects--Topical Terms:

605783
Cosmic background radiation.

LC Class. No.: QB991.C64

Dewey Class. No.: 523.01

Diffuse radio foregrounds[electronic resource] :all-sky polarisation, and anomalous microwave emission /
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