The Cassini RADAR altimeter has provided broad-scale surface topography data for Saturn's largest moon Titan. Herein, we adapt the delay/Doppler algorithm to take into account Cassini geometries and antenna mispointing usually occurring during hyperbolic Titan flybys. The proposed algorithm allows up to tenfold improvement in the along-track resolution. Preliminary results are provided that show how the improved topography presented herein can advance our understanding of Titan's surface characteristics.
High-resolution topography of Titan adapting the delay/doppler algorithm to the Cassini RADAR altimeter data / Poggiali, V.; Mastrogiuseppe, M.; Hayes, A. G.; Seu, R.; Mullen, J. P.; Birch, S. P. D.; Raguso, M. C.. - In: IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING. - ISSN 0196-2892. - 57:9(2019), pp. 7262-7268. [10.1109/TGRS.2019.2912575]
High-resolution topography of Titan adapting the delay/doppler algorithm to the Cassini RADAR altimeter data
Poggiali V.;Mastrogiuseppe M.;Seu R.;Raguso M. C.
2019
Abstract
The Cassini RADAR altimeter has provided broad-scale surface topography data for Saturn's largest moon Titan. Herein, we adapt the delay/Doppler algorithm to take into account Cassini geometries and antenna mispointing usually occurring during hyperbolic Titan flybys. The proposed algorithm allows up to tenfold improvement in the along-track resolution. Preliminary results are provided that show how the improved topography presented herein can advance our understanding of Titan's surface characteristics.File | Dimensione | Formato | |
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