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THE SIZES OF THE SOURCES OF SOLAR RADIO BURSTS AT 40 AND 60 Mc/s
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1962
Year
Terrestrial Gamma-ray FlashesEngineeringSwept-phase InterferometerInterferometryAnd 60Angular SizesSpace PhysicSolar PhysicSolar-terrestrial InteractionRadiometrySynchrotron RadiationSwept-frequency InterferometerSpace WeatherHigh-energy AstrophysicsSolar ActivityRadio TelescopeAstrophysics
A swept-phase interferometer has been used in conjunction with the radio spectrograph and the swept-frequency interferometer to study the angular sizes of the sources of the bursts of radio emission from the sun. Measurements were made at either 40 or 60 Mc/s and with aerial spacings of 1 km or 1/4 km, A preliminary discussion on the data is presented. (W.D.M.)