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2. The lakes of Titan

Author

Stofan, E. R., Elachi, C., Lunine, J. I., Lorenz, R. D., Stiles, B., Mitchell, K. L., Ostro, S., Soderblom, L., Wood, C., Zebker, H., Wall, S., Janssen, M., Kirk, R., Lopes, R., Paganelli, F., Radebaugh, J., Wye, L., Anderson, Y., Allison, M., Boehmer, R., Callahan, P., Encrenaz, P., Flamini, E., Francescetti, G., Gim, Y., Hamilton, G., Hensley, S., Johnson, W. T. K., Kelleher, K., Muhleman, D., Paillou, P., Picardi, G., Posa, F., Roth, L., Seu, R., Shaffer, S., Vetrella, S., and West, R.

Subjects
Environmental issues, Science and technology, Zoology and wildlife conservation
Abstract

Author(s): E. R. Stofan (corresponding author) [1, 2]; C. Elachi [3]; J. I. Lunine [4]; R. D. Lorenz [5]; B. Stiles [3]; K. L. Mitchell [3]; S. Ostro [3]; L. [...]

Published
2007
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3. Titan Radar Mapper observations from Cassini's T3 fly-by

Author

Elachi, C., Wall, S., Janssen, M., Stofan, E., Lopes, R., Kirk, R., Lorenz, R., Lunine, J., Paganelli, F., Soderblom, L., Wood, C., Wye, L., Zebker, H., Anderson, Y., Ostro, S., Allison, M., Boehmer, R., Callahan, P., Encrenaz, P., Flamini, E., Francescetti, G., Gim, Y., Hamilton, G., Hensley, S., Johnson, W., Kelleher, K., Muhleman, D., Picardi, G., Posa, F., Roth, L., Seu, R., Shaffer, S., Stiles, B., Vetrella, S., and West, R.

Subjects
Environmental issues, Science and technology, Zoology and wildlife conservation
Abstract

Author(s): C. Elachi [1]; S. Wall (corresponding author) [1]; M. Janssen [1]; E. Stofan [2]; R. Lopes [1]; R. Kirk [3]; R. Lorenz [4]; J. Lunine [4, 5]; F. Paganelli [...]

Published
2006
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4. The sand seas of Titan: Cassini RADAR observations of longitudinal dunes

Author

Lorenz, R.D., Wall, S., Radebaugh, J., Boubin, G., Reffet, E., Janssen, M., Stofan, E., Lopes, R., Kirk, R., Elachi, C., Lunine, J., Mitchell, K., Paganelli, F., Soderblom, L., Wood, C., Wye, L., Zebker, H., Anderson, Y., Ostro, S., Allison, M., Boehmer, R., Callahan, P., Encrenaz, P., Ori, G.G., Francescetti, G., Gim, Y., Hamilton, G., Hensley, S., Johnson, W., Kelleher, K., Muhleman, D., Picardi, G., Posa, F., Roth, L., Seu, R., Shaffer, S., Stiles, B., Vetrella, S., Flamini, E., and West, R.

Subjects
Titan (Satellite) -- Observations, Titan (Satellite) -- Properties, Titan (Satellite) -- Research, Sand dunes -- Observations, Sand dunes -- Properties, Sand dunes -- Research
Published
2006

5. Cassini Radar views the surface of Titan

Author

Elachi, C., Wall, S., Allison, M., Anderson, Y., Boehmer, R., Callahan, P., Encrenaz, P., Flamini, E., Franceschetti, G., Gim, Y., Hamilton, G., Hensley, S., Janssen, M., Johnson, W., Kelleher, K., Kirk, R., Lopes, R., Lorenz, R., Lunine, J., Muhleman, D., Ostro, S., Paganelli, F., Picardi, G., Posa, F., Roth, L., Seu, R., Shaffer, S., Soderblom, L., Stiles, B., Stofan, E., Vetrella, S., West, R., Wood, C., Wye, L., and Zebker, H.

Subjects
Cassini (Space probe) -- Usage, Radar systems -- Usage, Titan (Satellite) -- Research -- Analysis -- Observations -- Usage, Science and technology
Abstract

The Cassini Titan Radar Mapper imaged about 1% of Titan's surface at a resolution of ~0.5 kilometer, and larger areas of the globe in lower resolution modes. The images reveal a complex surface, with areas of low relief and a variety of geologic features suggestive of dome-like volcanic constructs, flows, and sinuous channels. The surface appears to be young, with few impact craters. Scattering and dielectric properties are consistent with porous ice or organics. Dark patches in the radar images show high brightness temperatures and high emissivity and are consistent with frozen hydrocarbons., Saturn's largest satellite, Titan, is the only moon and one of only four solid bodies in the solar system to host a thick atmosphere, uniquely distinguished by nitrogen and methane [...]

Published
2005

11. Corrigendum: Titan Radar Mapper observations from Cassini's T3 fly-by

Author

Elachi, C., Wall, S., Janssen, M., Stofan, E., Lopes, R., Kirk, R., Lorenz, R., Lunine, J., Paganelli, F., Soderblom, L., Wood, C., Wye, L., Zebker, H., Anderson, Y., Ostro, S., Allison, M., Boehmer, R., Callahan, P., Encrenaz, P., Flamini, E., Francescetti, G., Gim, Y., Hamilton, G., Hensley, S., Johnson, W., Kelleher, K., Muhleman, D., Picardi, G., Posa, F., Roth, L., Seu, R., Shaffer, S., Stiles, B., Vetrella, S., and West, R.

Subjects
Environmental issues, Science and technology, Zoology and wildlife conservation
Abstract

Author(s): C. Elachi; S. Wall; M. Janssen; E. Stofan; R. Lopes; R. Kirk; R. Lorenz; J. Lunine; F. Paganelli; L. Soderblom; C. Wood; L. Wye; H. Zebker; Y. Anderson; S. [...]

Published
2006
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20. Titan Radar Mapper observations from Cassini's T3 fly-by.

Author

Elachi, C., Wall, S., Janssen, M., Stofan, E., Lopes, R., Kirk, R., Lorenz, R., Lunine, J., Paganelli, F., Soderblom, L., Wood, C., Wye, L., Zebker, H., Anderson, Y., Ostro, S., Allison, M., Boehmer, R., Callahan, P., Encrenaz, P., and Flamini, E.

Subjects
TITAN (Satellite), RADAR, SATELLITES of Saturn, LUNAR craters, LANDFORMS
Abstract

Cassini's Titan Radar Mapper imaged the surface of Saturn's moon Titan on its February 2005 fly-by (denoted T3), collecting high-resolution synthetic-aperture radar and larger-scale radiometry and scatterometry data. These data provide the first definitive identification of impact craters on the surface of Titan, networks of fluvial channels and surficial dark streaks that may be longitudinal dunes. Here we describe this great diversity of landforms. We conclude that much of the surface thus far imaged by radar of the haze-shrouded Titan is very young, with persistent geologic activity. [ABSTRACT FROM AUTHOR]

Published
2006
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24. Titan's surface from Cassini RADAR SAR and high resolution radiometry data of the first five flybys

Author

Paganelli, F., Janssen, M.A., Stiles, B., West, R., Lorenz, R.D., Lunine, J.I., Wall, S.D., Callahan, P., Lopes, R.M., Stofan, E., Kirk, R.L., Johnson, W.T.K., Roth, L., Elachi, C., and the Radar Team

Subjects
*TITAN (Satellite), *SOLAR system, *SATELLITES of Jupiter, *MOON
Abstract

Abstract: The first five Titan flybys with Cassini''s Synthetic Aperture RADAR (SAR) and radiometer are examined with emphasis on the calibration and interpretation of the high-resolution radiometry data acquired during the SAR mode (SAR-radiometry). Maps of the 2-cm wavelength brightness temperature are obtained coincident with the SAR swath imaging, with spatial resolution approaching 6 km. A preliminary calibration shows that brightness temperature in these maps varies from 64 to 89 K. Surface features and physical properties derived from the SAR-radiometry maps and SAR imaging are strongly correlated; in general, we find that surface features with high radar reflectivity are associated with radiometrically cold regions, while surface features with low radar reflectivity correlate with radiometrically warm regions. We examined scatterplots of the normalized radar cross-section versus brightness temperature, finding differing signatures that characterize various terrains and surface features. Implications for the physical and compositional properties of these features are discussed. The results indicate that volume scattering is important in many areas of Titan''s surface, particularly Xanadu, while other areas exhibit complex brightness temperature variations consistent with variable slopes or surface material and compositional properties. [Copyright &y& Elsevier]

Published
2007
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