A Microwave Interferometric Study of the Subsurface of the Planet Mercury |
Contents
The Development of Microwave Observations | 2 |
C | 11 |
Model Calculations of Cuzzi | 18 |
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Common terms and phrases
addition angular antenna temperature Apollo 11 atmosphere baseline Chapter Clear Clear/Scattered coefficients correlation Creek Observatory Cuzzi decorrelation depth interval determined dielectric constant disk brightness temperature diurnal period emission employed epoch Epstein Figure flux density scale foot antenna frequency fringe amplitudes fringe visibility amplitude fringe visibility function g/cm g/cm³ Gary geocentric geocentric coordinates given ground level absolute group brightness temperatures heat conduction hour angle individual fringe integration interferometer Krotikov least squares level absolute humidity longitude mean disk brightness mean values measurements model calculations Morrison and Sagan observations of Mercury observing runs Olhoeft and Strangway Optical Depth phase angle phase fluctuations phase variation planet planetary pointing errors present procedure radiation radiative radio right ascension RMS Deviations rotation season signal signal-to-noise single dish antenna soil samples synodic period T₁ technique thermal conductivity thermophysical parameters Troitskii twenty foot telescope Ulich wavelengths zenith angle ΔΦ