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- W2161224749 abstract "It has been argued that the introduction of an ensemble average in calculations of lunar backscatter may not be justified because of the limited sample of the lunar surface illuminated during a backscatter measurement. By taking explicit account of the relative motion of the moon and earth and by assuming that the effective area illuminated remains the same during the observation period, we have been able to derive an expression for the rms error caused by replacing time averages with ensemble averages in the autocorrelation of the scatter amplitude. This error is found to depend on the total averaging time as well as on the libration rate. For lunar backscatter it is shown that the error is less than 10% for a radar that averages 600 sec during lunar transit." @default.
- W2161224749 created "2016-06-24" @default.
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- W2161224749 date "1967-08-15" @default.
- W2161224749 modified "2023-09-25" @default.
- W2161224749 title "On the time averaged radar cross section of the Moon" @default.
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- W2161224749 doi "https://doi.org/10.1029/jz072i016p04069" @default.
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