找回密碼
 To register

QQ登錄

只需一步,快速開始

掃一掃,訪問微社區(qū)

打印 上一主題 下一主題

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

[復(fù)制鏈接]
查看: 33146|回復(fù): 35
樓主
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

書目名稱Diffuse Radio Foregrounds影響因子(影響力)




書目名稱Diffuse Radio Foregrounds影響因子(影響力)學(xué)科排名




書目名稱Diffuse Radio Foregrounds網(wǎng)絡(luò)公開度




書目名稱Diffuse Radio Foregrounds網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Diffuse Radio Foregrounds被引頻次




書目名稱Diffuse Radio Foregrounds被引頻次學(xué)科排名




書目名稱Diffuse Radio Foregrounds年度引用




書目名稱Diffuse Radio Foregrounds年度引用學(xué)科排名




書目名稱Diffuse Radio Foregrounds讀者反饋




書目名稱Diffuse Radio Foregrounds讀者反饋學(xué)科排名




單選投票, 共有 0 人參與投票
 

0票 0%

Perfect with Aesthetics

 

0票 0%

Better Implies Difficulty

 

0票 0%

Good and Satisfactory

 

0票 0%

Adverse Performance

 

0票 0%

Disdainful Garbage

您所在的用戶組沒有投票權(quán)限
沙發(fā)
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.
板凳
發(fā)表于 2025-3-22 02:43:27 | 只看該作者
地板
發(fā)表于 2025-3-22 07:45:08 | 只看該作者
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. .).
5#
發(fā)表于 2025-3-22 11:47:05 | 只看該作者
6#
發(fā)表于 2025-3-22 15:28:12 | 只看該作者
7#
發(fā)表于 2025-3-22 18:10:39 | 只看該作者
8#
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
9#
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. .).
10#
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.
 關(guān)于派博傳思  派博傳思旗下網(wǎng)站  友情鏈接
派博傳思介紹 公司地理位置 論文服務(wù)流程 影響因子官網(wǎng) 吾愛論文網(wǎng) 大講堂 北京大學(xué) Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點(diǎn)評 投稿經(jīng)驗總結(jié) SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學(xué) Yale Uni. Stanford Uni.
QQ|Archiver|手機(jī)版|小黑屋| 派博傳思國際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-5 15:24
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved
快速回復(fù) 返回頂部 返回列表
临海市| 富阳市| 垦利县| 阿城市| 洛宁县| 稷山县| 柘城县| 长乐市| 迁安市| 锦屏县| 馆陶县| 若尔盖县| 塔城市| 墨竹工卡县| 临武县| 永新县| 崇文区| 玉溪市| 平武县| 永泰县| 乐至县| 临颍县| 衡水市| 深圳市| 温泉县| 济阳县| 敦煌市| 忻州市| 海门市| 尼玛县| 泗洪县| 南江县| 金塔县| 华亭县| 温州市| 陈巴尔虎旗| 兴文县| 靖江市| 崇左市| 汾阳市| 广水市|