Interstellar magnetic fields: from Galactic scales to the edge of the heliosphere

被引：12
作者：
Ferriere, Katia [1 ]
机构：
[1] Univ Toulouse, CNRS, IRAP, F-31028 Toulouse 4, France
来源：
13TH ANNUAL INTERNATIONAL ASTROPHYSICS CONFERENCE: VOYAGER, IBEX, AND THE INTERSTELLAR MEDIUM | 2015年 / 577卷
关键词：
PULSAR ROTATION MEASURES; MILKY-WAY; VOYAGER; RADIATIVE TORQUES; FARADAY-ROTATION; GALAXY; POLARIZATION; GAS; HELIOSHEATH; CONSTRAINTS;
D O I：
10.1088/1742-6596/577/1/012008
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
I review the observational properties of interstellar magnetic fields in our Galaxy, starting from the large Galactic scales and gradually zooming in toward the heliosphere. It emerges that the large-scale magnetic field is predominantly azimuthal in the Galactic disk, but that this global field orientation is severely perturbed in the small-scale surroundings of the heliosphere.
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页数：12
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