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from Part IV - Environments and the Interstellar Medium
Published online by Cambridge University Press: 21 July 2022
The radiation from most pulsars has a high degree of linear polarisation, allowing measurements of Faraday rotation. Such radio observations of polarisation provide detailed measurements of the interstellar magnetic field along the line of sight to a pulsar, including the fields along the spiral arms and the large-scale field outside the plane of the Galaxy. Pulsars can probe the magnitude and direction of the galactic magnetic field.
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