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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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發(fā)表于 2025-3-21 17:13:36 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Diffuse Radio Foregrounds
副標(biāo)題All-Sky Polarisation
編輯Matías Vidal Navarro
視頻videohttp://file.papertrans.cn/279/278999/278999.mp4
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
叢書名稱Springer Theses
圖書封面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
關(guān)鍵詞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
The information of publication is updating

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發(fā)表于 2025-3-21 21:09:50 | 只看該作者
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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發(fā)表于 2025-3-22 02:43:27 | 只看該作者
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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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發(fā)表于 2025-3-23 00:36:01 | 只看該作者
,,?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
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發(fā)表于 2025-3-23 01:45:22 | 只看該作者
,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. .).
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發(fā)表于 2025-3-23 08:49:57 | 只看該作者
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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