Preliminary observations of solar radio sources with the Culgoora radioheliograph operating at four frequencies

Solar Physics(1983)

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摘要
The Culgoora radioheliograph has been modified for observing at 327.4 MHz, which is in addition to the three frequencies (43.25, 80, and 160 MHz) previously available. At the new frequency the array beamwidth is 56?, which represents the highest resolution yet available for metre-wavelength solar mapping.
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关键词
High Resolution,Lower Layer,Radio Emission,Radio Source,Preliminary Observation
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