Synchrotron Polarization at High Galactic Latitude

dc.creatorAbidin, Z. Zainal
dc.creatorLeahy, J. P.
dc.creatorWilkinson, A.
dc.creatorReich, P.
dc.creatorReich, W.
dc.creatorWielebinski, R.
dc.date2003-07-03
dc.date.accessioned2026-07-25T19:01:37Z
dc.descriptionWe present preliminary results from mapping the high-latitude Galactic polarization with the Effelsberg Telescope at $λ$21 cm. Structures on the resulting maps are mostly on the scale of several degrees. The results show detection of polarization over most of the field, at the level of tens of percent of the synchrotron emission. The evidence of more structure in Stokes Q and U rather than in $\sqrt{Q^2+U^2}$ suggests the existence of Faraday rotation.
dc.descriptionTo be published in the proceedings of "The Cosmic Microwave Background and its Polarization", New Astronomy Reviews, (eds. S. Hanany and K.A. Olive)
dc.identifierhttps://arxiv.org/abs/astro-ph/0307078
dc.identifierhttp://arxiv.org/abs/astro-ph/0307078
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/60738
dc.subjectAstrophysics
dc.titleSynchrotron Polarization at High Galactic Latitude
dc.typetext

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