Future magnetic field studies using the Planck surveyor experiment

被引：7
|
作者：
Ensslin, T. A.
Waelkens, A.
Vogt, C.
Schekochihin, A. A.
机构：
[1] Max Planck Inst Astrophys, D-85741 Garching, Germany
[2] Stichting ASTRON, NL-7990 AA Dwingeloo, Netherlands
[3] Univ Cambridge, CMS, DAMTP, Cambridge CB3 OWA, England
来源：
ASTRONOMISCHE NACHRICHTEN | 2006年 / 327卷 / 5-6期
基金：
英国科学技术设施理事会;
关键词：
space vehicles : instruments; cosmic microwave background; polarization; ISM : magnetic fields; Galaxy : structure;
D O I：
10.1002/asna.200610607
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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. (c) 2006 WILEY-VCH Verlag GmbH& Co. KGaA, Weinheim.
引用
收藏
页码：626 / 631
页数：6
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