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- W3034134489 abstract "While intensity of electromagnetic radiation (radio, infrared, light, or X-ray) gives us primary information about the distribution of the baryonic matter in the Universe, polarisation is a parameter that enables us to investigate many additional details. Polarisation at radio frequencies gives us details of emission processes since the non-thermal synchrotron process dominates at low radio frequencies in emission regions. In addition, polarised radio sources can be used as probes of the intervening interstellar medium through which the radio waves are propagated. Faraday rotation effects are observed and in conjunction with known thermal emission can be used to determine magnetic fields. The Zeeman effect, a direct method of determining magnetic fields, depends on the observation of the circular polarisation components of a spectral line. In this paper I describe the early polarisation observations of radio sources, but in addition I follow the developments through to the present day." @default.
- W3034134489 created "2020-06-12" @default.
- W3034134489 creator A5044007329 @default.
- W3034134489 date "2012-07-01" @default.
- W3034134489 modified "2023-10-03" @default.
- W3034134489 title "A HISTORY OF RADIO ASTRONOMY POLARISATION MEASUREMENTS" @default.
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- W3034134489 doi "https://doi.org/10.3724/sp.j.1440-2807.2012.02.01" @default.
- W3034134489 hasPublicationYear "2012" @default.
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