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Titlebook: Diffuse Radio Foregrounds; All-Sky Polarisation Matías Vidal Navarro Book 2016 Springer International Publishing Switzerland 2016 Cosmic mi

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发表于 2025-3-21 17:13:36 | 显示全部楼层 |阅读模式
书目名称Diffuse Radio Foregrounds
副标题All-Sky Polarisation
编辑Matías Vidal Navarro
视频video
概述Nominated as an outstanding Ph.D. thesis by the University of Manchester, UK.Offers a new polarization-bias reduction method.Provides a simple model to explain most of the large synchrotron polarizati
丛书名称Springer Theses
图书封面Titlebook: Diffuse Radio Foregrounds; All-Sky Polarisation Matías Vidal Navarro Book 2016 Springer International Publishing Switzerland 2016 Cosmic mi
描述.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 showsthat the spinning dust hypothesis can explain the radio properties observed..
出版日期Book 2016
关键词Cosmic microwave background; Polarisation of the cosmic microwave background radiation; Anomalous Micr
版次1
doihttps://doi.org/10.1007/978-3-319-26263-5
isbn_softcover978-3-319-79919-3
isbn_ebook978-3-319-26263-5Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightSpringer International Publishing Switzerland 2016
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发表于 2025-3-21 21:09:50 | 显示全部楼层
https://doi.org/10.1007/978-94-009-6726-7In this chapter we describe the processing of the .data and other full sky maps for the polarisation analysis.
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Red Cell Metabolism and FunctionIn this chapter we study the AME in the Lynds Dark Nebula (LDN) 1780. Here, we have detected AME using interferometric observations at 31 GHz with 6. angular resolution (Vidal et al. .).
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,, Polarised Filaments,At frequencies up to a few GHz, the total radio sky brightness is dominated by the diffuse Galactic synchrotron radiation, where cosmic rays (CR) electrons and positrons spiralling
发表于 2025-3-23 01:45:22 | 显示全部楼层
,AME in LDN 1780,In this chapter we study the AME in the Lynds Dark Nebula (LDN) 1780. Here, we have detected AME using interferometric observations at 31 GHz with 6. angular resolution (Vidal et al. .).
发表于 2025-3-23 08:49:57 | 显示全部楼层
Conclusions and Future Work,In this thesis we have studied the Galactic emission in the 23–43 GHz frequency range, focusing on the diffuse polarised emission and on the anomalous microwave emission.
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