The Helios Faraday Rotation Data Archive

The Helios Faraday Rotation (FR) Experiment, a passive radio science investigation requiring no on‐board hardware other than the existing spacecraft radio subsystem, was designed to study the dynamic and quiescent structure of the magnetic fields and electron density in the solar corona. Measurements of coronal Faraday rotation were derived from the linearly polarized S‐band downlink carrier signal, which probed otherwise inaccessible regions of the corona in the radial range from 2 to 15 solar radii during the regularly recurring solar conjunctions. More than 1250 hours of Helios FR data were recorded over the duration of the Helios 1 (1974–84) and Helios 2 (1976–80) missions. The time scales of FR variations provide information on various physical phenomena: (a) slowly‐varying rise and fall associated with the changing ray path offset, combined with the rotation of the quasi‐static corona; (b) ubiquitous random oscillations with higher fluctuation amplitude at smaller solar offset distances, probably ca...

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