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- W3100839434 abstract "Multi-frequency radio polarimetry of the diffuse Galactic synchrotron background gives new viewpoints on the Galactic magnetic field. Rotation measure maps reveal magnetic structures on arcminute to degree scales, such as a ring in polarization that we interpret as a magnetic tunnel. A complication using this technique is depolarization across the beam and along the line of sight. The influence of beam depolarization has been estimated using numerical models of the magneto-ionic ISM, through which polarized radiation propagates. The models show that depolarization canals similar to those observed can be caused by beam depolarization, and that the one-dimensional gradients in RM needed to produce these canals are ubiquitous in the medium." @default.
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- W3100839434 date "2004-01-01" @default.
- W3100839434 modified "2023-09-23" @default.
- W3100839434 title "Galactic Magnetic Fields, from Radio Polarimetry of the WIM" @default.
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- W3100839434 doi "https://doi.org/10.1007/1-4020-2620-x_62" @default.
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