Galactic turbulence and magnetic fields through radiopolarimetry of the Galactic synchrotron background

Details Galactic turbulence and magnetic fields through radiopolarimetry of the Galactic synchrotron background Galactic turbulence and magnetic fields through radiopolarimetry of the Galactic synchrotron background

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..784..308h&link_type=abstract

MAGNETIC FIELDS IN THE UNIVERSE: From Laboratory and Stars to Primordial Structures. AIP Conference Proceedings, Volume 784, pp

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3

Galaxy, Turbulence, Interstellar Magnetic Fields, Astronomical Polarimetry, Synchrotron Radiation, Interstellar Matter, Physical Properties, Electric And Magnetic Fields, Polarimetry

Scientific paper

Multi-frequency radiopolarimetry of diffuse Galactic synchrotron emission and polarized extragalactic sources can yield estimates of Galactic magnetic field strength, of maximum scales of fluctuations in the magneto-ionized medium, or enable discovery of magnetic objects which are difficult or impossible to observe otherwise. I will discuss these methods and present the continuum part of the large, arcminute resolution Southern Galactic Plane Survey.

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