Automated system for resolving the position of solar radio bursts

Details Automated system for resolving the position of solar radio bursts Automated system for resolving the position of solar radio bursts

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985aifo.reptq....g&link_type=abstract

Interim Scientific Report Air Force Geophysics Lab., Hanscom AFB, MA.

Physics

Geophysics

Interferometers, Position (Location), Radio Interferometers, Solar Radio Bursts, Solar Radio Emission, Sweep Frequency, Maps, Precision, Resolution

Scientific paper

A swept freqency interferometer system such as the one in operation at Sagamore Hill observatory, described in AFGL Tech report 76-0194 1976, contains in its output data, precise information which can determine, in a plane resolution, the position of a radio source on the solar disk within 1.3 min arc. This information is the frequency separation between the interference fringes within the spectrum observed. A system which could, automatically, convert this information to degrees and minutes of arc is described.

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