Texture and Composition of Titan's Equatorial Sand Seas Inferred From Cassini SAR Data: Implications for Aeolian Transport and Dune Morphodynamics-Reference-Cited by-同舟云学术

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Texture and Composition of Titan's Equatorial Sand Seas Inferred From Cassini SAR Data: Implications for Aeolian Transport and Dune Morphodynamics

Published:2019-11 Issue:11 Volume:124 Page:3140-3163
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res. Planets

Author:

Lucas A.¹^ORCID,Rodriguez S.¹^ORCID,Lemonnier F.²^ORCID,Le Gall A.³^ORCID,MacKenzie S.⁴^ORCID,Ferrari C.¹^ORCID,Paillou P.⁵,Narteau C.¹^ORCID

Affiliation:

1. Université de Paris, Institut de physique du globe de Paris, CNRS Paris France

2. LMD,UPMC, CNRS Paris France

3. LATMOS/IPSL, UVSQ Université Paris‐Saclay, CNRS Guyancourt France

4. Department of PhysicsUniversity of Idaho Moscow ID USA

5. Observatoire de Bordeaux, Université de Bordeaux, CNRS Bordeaux France

Funder

Nvidia

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2019JE005965

Reference66 articles.

1. Relationship between profile length and roughness variables for natural surfaces

2. Spectroscopy, morphometry, and photoclinometry of Titan's dunefields from Cassini/VIMS

3. Production and global transport of Titan’s sand particles

4. Compositional and spatial variations in Titan dune and interdune regions from Cassini VIMS and RADAR

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3. Composition, Roughness, and Topography from Radar Backscatter at Selk Crater, the Dragonfly Landing Site;The Planetary Science Journal;2022-08-01

4. Modeling transmission windows in Titan’s lower troposphere: Implications for infrared spectrometers aboard future aerial and surface missions;Icarus;2021-03

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