Abstract
Observations of the 1.4 mm center to limb solar brightness distribution show that there is little, if any, limb brightening at this wavelength. Knowledge of the antenna radiation pattern is vital in interpreting the radio measurements.
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This work was supported by the U.S. Air Force under Contract No. F04701-70-C-0069.
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Shimabukuro, F.I. Observations of the 1.4mm brightness distribution of the sun. Sol Phys 18, 247–252 (1971). https://doi.org/10.1007/BF00145938
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DOI: https://doi.org/10.1007/BF00145938