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Future magnetic fields studies using the Planck Surveyor experiment

Abstract:
The Planck mission will permit measurements of the polarization of the cosmic microwave background and of polarized foregrounds such as our own Galaxy with an unprecedented combination of accuracy and completeness. This will provide information on cosmological and galactic magnetic fields. The latter can be studied in detail via nearly Faraday-rotation free synchrotron and polarized dust emission. Methods are discussed to extract physically relevant information on the magnetic turbulence from Planck data and other measurements.
Publication status:
Published

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Publisher copy:
10.1002/asna.200610607

Authors


Ensslin, TA More by this author
Waelkens, A More by this author
Schekochihin, AA More by this author
Journal:
ASTRONOMISCHE NACHRICHTEN
Volume:
327
Issue:
5-6
Pages:
626-631
Publication date:
2005-11-16
DOI:
EISSN:
1521-3994
ISSN:
0004-6337
URN:
uuid:3ab6ab61-86da-4434-9f8d-f45598694b5b
Source identifiers:
160210
Local pid:
pubs:160210
Language:
English
Keywords:

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