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- W2005080650 abstract "Measurements at 3.5 mm of the disk-average brightness temperature of Mars during the 1978 opposition can be represented by TB(Mars, 3 5 mm, Jan/Feb 1978) = (The errors cited are from the internal scatter; the estimated absolute calibration uncertainty is 3%.) This longitudinal variation must be taken into account if Mars is to be used as a calibration source at millimeter wavelengths. The total range of the 3.5-mm variation is three to four times larger than both the 2.8-cm and 20-μm variations. This unexpected result can possibly be explained by subsurface scattering from rocks ≲1.5-cm radius." @default.
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- W2005080650 date "1983-12-01" @default.
- W2005080650 modified "2023-10-16" @default.
- W2005080650 title "Mars: Subsurface properties from observed longitudinal variation of the 3.5-mm brightness temperature" @default.
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- W2005080650 doi "https://doi.org/10.1016/0019-1035(83)90167-7" @default.
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