Synchrotron angular spectra at various Galactic latitudes and frequencies

Details Synchrotron angular spectra at various Galactic latitudes and frequencies Synchrotron angular spectra at various Galactic latitudes and frequencies

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..609..261b&link_type=abstract

ASTROPHYSICAL POLARIZED BACKGROUNDS: Workshop on Astrophysical Polarized Backgrounds, held 9-12 October, 2001 in Bologna Italy.

Physics

Radiation Mechanisms, Polarization, Electric And Magnetic Fields, Radio, Microwave

Scientific paper

We study the angular power spectra of the polarized Galactic synchrotron emission in the range 10<~l<=800, at several frequencies between 0.4 and 2.7 GHz and at several Galactic latitudes up to near the North Galactic Pole. We properly distinguish between the various polarization spectra that can be defined and measured, including the CPI spectrum which is insensitive to the polarization direction. .

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