東華大學圖書館 |

語系: 繁體中文

說明(常見問題)

回圖書館首頁

手機版館藏查詢

登入

回首頁

切換: 標籤 | MARC模式 | ISBD

Diffuse radio foregrounds = all-sky ...

Vidal Navarro, Matias.

FindBook

Google Book

Amazon

博客來

Diffuse radio foregrounds = all-sky polarisation, and anomalous microwave emission /

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Diffuse radio foregrounds/ by Matias Vidal Navarro.
其他題名:	all-sky polarisation, and anomalous microwave emission /
作者:	Vidal Navarro, Matias.
出版者:	Cham :Springer International Publishing : : 2016.,
面頁冊數:	xliv, 196 p. :ill., digital ;24 cm.
內容註:	Introduction -- Analysis Techniques for WMAP Polarisation data -- WMAP Polarised Filaments -- QUIET Galactic Observations -- AME in LDN1780 -- Conclusions and Future Work.
Contained By:	Springer eBooks
標題:	Cosmic background radiation. -
電子資源:	http://dx.doi.org/10.1007/978-3-319-26263-5
ISBN:	9783319262635$q(electronic bk.)

Diffuse radio foregrounds = 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$q(electronic bk.)

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

716083
Cosmic background radiation.

LC Class. No.: QB991.C64

Dewey Class. No.: 523.01

Diffuse radio foregrounds = all-sky polarisation, and anomalous microwave emission /
LDR:02258nmm a2200325 a 4500 001 2030081
003 DE-He213
005 20160810120759.0
006 m d
007 cr nn 008maaau
008 160908s2016 gw s 0 eng d
020 $a 9783319262635$q(electronic bk.)
020 $a 9783319262628$q(paper)
024 7 $a 10.1007/978-3-319-26263-5 $2 doi
035 $a 978-3-319-26263-5
040 $a GP $c GP
041 0 $a eng
050 4 $a QB991.C64
072 7 $a PHR $2 bicssc
072 7 $a SCI015000 $2 bisacsh
082 0 4 $a 523.01 $2 23
090 $a QB991.C64 $b V649 2016
100 1 $a Vidal Navarro, Matias. $3 2181492
245 1 0 $a Diffuse radio foregrounds $h [electronic resource] : $b all-sky polarisation, and anomalous microwave emission / $c by Matias Vidal Navarro.
260 $a Cham : $b Springer International Publishing : $b Imprint: Springer, $c 2016.
300 $a xliv, 196 p. : $b ill., digital ; $c 24 cm.
490 1 $a Springer theses, $x 2190-5053
505 0 $a Introduction -- Analysis Techniques for WMAP Polarisation data -- WMAP Polarised Filaments -- QUIET Galactic Observations -- AME in LDN1780 -- Conclusions and Future Work.
520 $a 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.
650 0 $a Cosmic background radiation. $3 716083
650 1 4 $a Physics. $3 516296
650 2 4 $a Cosmology. $3 531904
650 2 4 $a Astronomy, Observations and Techniques. $3 1066822
650 2 4 $a Astrophysics and Astroparticles. $3 1067087
710 2 $a SpringerLink (Online service) $3 836513
773 0 $t Springer eBooks
830 0 $a Springer theses. $3 1314442
856 4 0 $u http://dx.doi.org/10.1007/978-3-319-26263-5
950 $a Physics and Astronomy (Springer-11651)