Some closely spaced frequency Faraday rotation satellite observations

Details Some closely spaced frequency Faraday rotation satellite observations Some closely spaced frequency Faraday rotation satellite observations

Jul 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967jatp...29..871l&link_type=abstract

Journal of Atmospheric and Terrestrial Physics, vol. 29, no. 7, pp. 871-876

Physics

Scientific paper

Observations of the Faraday rotation of signals at two closely spaced frequencies (40 and 41 MHz) allows the unambiguous determination of total rotation angle along the ray path. For satellite borne transmitters this in turn allows the determination of electron content figures for several points along the sub-satellite track so that gradients and large scale irregularities in content can be detected. Some examples are shown of observations from two stations 1370 km apart along a N-S line (London and Great Whale River) and of simultaneous observations on two satellites (Explorer 22 and Explorer 27) one having a N-S and the other an E-W sub-satellite track.

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