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• W3104304815 abstract "Context. Linear polarization of diffuse Galactic emission is a signature of magnetic fields in the interstellar medium of our Galaxy. Observations at high frequencies are less affected by Faraday depolarization than those at lower frequencies and are able to detect polarized emission from more distant Galactic regions." @default.
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• W3104304815 date "2011-03-22" @default.
• W3104304815 modified "2023-10-16" @default.
• W3104304815 title "A Sino-German<i>λ</i>6 cm polarization survey of the Galactic plane" @default.
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• W3104304815 doi "https://doi.org/10.1051/0004-6361/201016226" @default.
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