A decametric wavelength radio telescope for interplanetary scintillation observations

Details A decametric wavelength radio telescope for interplanetary scintillation observations A decametric wavelength radio telescope for interplanetary scintillation observations

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stin...7527981c&link_type=abstract

Unknown

Computer Science

Performance

Interplanetary Space, Radio Telescopes, Scintillation Counters, Wavelengths, Antenna Arrays, Electron Density Profiles, Ionospherics, Project Planning, Research Facilities, Solar Wind

Scientific paper

A phased array, electrically steerable radio telescope (with a total collecting area of 18 acres), constructed for the purpose of remotely sensing electron density irregularity structure in the solar wind, is presented. The radio telescope is able to locate, map, and track large scale features of the solar wind, such as streams and blast waves, by monitoring a large grid of natural radio sources subject to rapid intensity fluctuation (interplanetary scintillation) caused by the irregularity structure. Observations verify the performance of the array, the receiver, and the scintillation signal processing circuitry of the telescope.

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