By Alan Watt, M. Watt
Facing state of the art suggestions in rendering and animation, this article offers a special synthesis of complicated suggestions now not formerly on hand in a single coherent resource.
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Astrophys. : Astron. Astrophys. 537, A5 (2012) Part II Techniques for Observing Cosmic Magnetic Fields Chapter 3 Synchrotron Radiation and Faraday Rotation George Heald Abstract Synchrotron radiation and its degree of linear polarization are powerful tracers of magnetic fields that are illuminated by cosmic ray electrons. Faraday rotation of the linearly polarized radiation is induced by intervening line-ofsight magnetic fields that are embedded in ionized plasmas. For decades these observational tools have been workhorses for utilizing radio telescopes to study magnetic fields inside and outside the Milky Way.
The contours indicate the 330 GHz continuum emission in steps of 6 , from 6 to 96 , where D 20 mJy beam 1 . The greyscale is the polarized emission (up to 38:3 mJy beam 1 and the line segments indicate the derived magnetic field direction. The panel on the right is a synthetic dust polarization map generated with the ARTIST module DustPol (Padovani et al. 2012; Sect. 4) produced with the same contour and intensity levels observations in Frau et al. (2011). The resulting map, made from 8 h SMA tracks in the sub-compact, compact and extended configuration is shown in Fig.
Powerful optical and infrared techniques have been developed for studying magnetic fields, but these are mostly applicable in the very nearby Universe, typically within the Milky Way (see contributions in this volume by Jones and Anderson). Zeeman splitting is a very important radio tracer of magnetic field strengths (see Troland, this volume) but is also used primarily within the Milky Way. For the study of cosmic magnetism, it is the illumination of magnetic fields by relativistic positrons and electrons (henceforth referred to collectively as electrons) that provides the most powerful and far-reaching information.