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0142108971
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note
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The uniform spacing of the sixteen 2001 spectra allows the diffuse component to be partially deconvolved so that each resultant spectrum more closely represents the diffuse scattering from a limited range of longitudes. There is no change in the amplitude or shape of the specular echoes. When estimating the diffuse cross section of the bright region, this process compensates for its limited extent in longitude. Its limited extent in latitude was compensated for by assuming that the surface south of the bright region has the same scattering properties as the trailing hemisphere. The deconvolution has the effect of symmetrizing the diffuse spectra, making the detection of a weak specular echo in the fits much easier.
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15
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0142077400
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note
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2, a good estimate of ε can be obtained from a measurement of the specular cross section.
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16
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0142045513
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note
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-1/2 is the (undulating) surface RMS slope (21).
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17
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0033759851
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22
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0142108962
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note
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We thank A. Hine, A. Crespo, R. French, J-L. Margot, M. Nolan, P. Nicholson, P. Perillat, and the staffs of the Arecibo and Green Bank telescopes. J. Chandler and J. Giorgini provided the Titan observing ephemeredes. Extensive comments by C. Griffith, one of which is paraphrased in the last paragraph, are appreciated. D.B.C., L.M.C., and S.J.O. acknowledge support by the Planetary Astronomy and Planetary Geology and Geophysics Programs of the National Aeronautics and Space Administration (NASA). Part of this research was conducted at the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA. The Arecibo Observatory is part of the National Astronomy and Ionosphere Center, which is operated by Cornell University under a cooperative agreement with the National Science Foundation (NSF) and with support from NASA. The Green Bank Telescope is part of the National Radio Astronomy Observatory, a facility of the NSF operated under cooperative agreement by Associated Universities, Inc.
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