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Models of synthetic aperture radar backscattering for bright flows and dark spots on Titan

Paillou, Philippe and Crapeau, Marc and Elachi, Charles and Wall, Stephen and Encrenaz, Pierre (2006) Models of synthetic aperture radar backscattering for bright flows and dark spots on Titan. Journal of Geophysical Research E, 111 (E11). Art. No. E11011. ISSN 0148-0227. https://resolver.caltech.edu/CaltechAUTHORS:20121119-100632030

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Abstract

The synthetic aperture radar (SAR) imaging mode of the Cassini RADAR instrument enables us to map the surface of Titan through its thick atmosphere. The first Cassini close flyby, acquired on 26 October 2004, revealed a complex surface, with areas of low relief and dome-like volcanic constructs, flows, and sinuous channels. In particular, fan-like features with strong radar backscattering were observed. Such structures, extending from tens of kilometers to more than 200 km in length, could be the result of cryovolcanism. Several radar dark spots, up to 30 km across, were also observed; they may correspond to smooth hydrocarbon deposits. We present here a first modeling of these radar-bright and radar-dark features on the basis of classical radar backscattering models. We considered two main materials which could constitute the surface of Titan, tholins and water-ammonia ice, and modeled both single- and two-layer cases, taking into account volume and subsurface scattering. Our results show that SAR-bright regions could better be explained by the effect of a thin layer of water-ammonia ice covering a tholin substratum. Radar-dark spots can be modeled in two ways: a rough tholin surface or a smooth one with some volume scattering. We show that multi-incidence SAR data could help discriminate between the various scenarios proposed.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1029/2006JE002724DOIUNSPECIFIED
http://www.agu.org/pubs/crossref/2006/2006JE002724.shtmlPublisherUNSPECIFIED
Additional Information:© 2006 American Geophysical Union. Received 29 March 2006; accepted 12 July 2006; published 25 November 2006. The authors are grateful to two anonymous reviewers for their critical and valuable comments on earlier versions of this manuscript.
Subject Keywords:SAR; scattering; Titan
Issue or Number:E11
Record Number:CaltechAUTHORS:20121119-100632030
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20121119-100632030
Official Citation:Paillou, P., M. Crapeau, C. Elachi, S. Wall, and P. Encrenaz (2006), Models of synthetic aperture radar backscattering for bright flows and dark spots on Titan, J. Geophys. Res., 111, E11011, doi:10.1029/2006JE002724.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:35533
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:19 Nov 2012 19:28
Last Modified:03 Oct 2019 04:29

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