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Interferometer Confusion and Some
The VectorAverage Approach and
0bservation of Saturn and Uranus by
4 other sections not shown
0bservations 1900 m baseline 21 cm wavelength 8085 MHz fringe ammonia amplitude antenna aperture synthesis assumed atmosphere average background sources Berge and Read brightness distribution brightness spectrum brightness temperature calibration Ceres Chapter confusing sources correlation coverage curve diameter dielectric constant effects Ephemeris equation estimate ferometer flux density Fourier transform frequencies fringe phase fringe visibility function function of hour Gulkis and Poynter hour angle Icarus infrared integration interferometer baseline limb darkening long wavelength Mars Martian measured Mercury MHz fringe visibility motion noise temperature NRA0 obtained opacity optical optical depth parameter particles percent planet point source polar position angle projected baseline region response right ascension rms confusion level Sagan Saturn scattering signal single dish sky plane subtracted surface synthesized beam synthesized scan system noise level technique tion Titan u-v plane uncertainty uniform disk upper limit Uranus variation vector vector-average water ice Yerbury zero