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Dive into the research topics where A. Le Gall is active.

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Featured researches published by A. Le Gall.


Geophysical Research Letters | 2010

Active shoreline of Ontario Lacus, Titan: A morphological study of the lake and its surroundings

S. D. Wall; Alexander G. Hayes; Charlie S. Bristow; Ralph D. Lorenz; Ellen R. Stofan; Jonathan I. Lunine; A. Le Gall; Michael A. Janssen; Rosaly M. C. Lopes; Lauren C. Wye; L. A. Soderblom; Philippe Paillou; Oded Aharonson; Howard A. Zebker; T. Farr; Giuseppe Mitri; R. L. Kirk; K. L. Mitchell; Claudia Notarnicola; Domenico Casarano; B. Ventura

Of more than 400 filled lakes now identified on Titan, the first and largest reported in the southern latitudes is Ontario Lacus, which is dark in both infrared and microwave. Here we describe recent observations including synthetic aperture radar (SAR) images by Cassinis radar instrument (λ = 2 cm) and show morphological evidence for active material transport and erosion. Ontario Lacus lies in a shallow depression, with greater relief on the southwestern shore and a gently sloping, possibly wave-generated beach to the northeast. The lake has a closed internal drainage system fed by Earth-like rivers, deltas and alluvial fans. Evidence for active shoreline processes, including the wave-modified lakefront and deltaic deposition, indicates that Ontario is a dynamic feature undergoing typical terrestrial forms of littoral modification.


Geophysical Research Letters | 2015

Spectral properties of Titan's impact craters imply chemical weathering of its surface

Catherine Dorothy Neish; Jason W. Barnes; Christophe Sotin; Shannon M. MacKenzie; Jason M. Soderblom; S. Le Mouélic; R. L. Kirk; Bryan W. Stiles; Michael Malaska; A. Le Gall; Robert H. Brown; Kevin H. Baines; Bonnie J. Buratti; Roger N. Clark; P. D. Nicholson

Abstract We examined the spectral properties of a selection of Titans impact craters that represent a range of degradation states. The most degraded craters have rims and ejecta blankets with spectral characteristics that suggest that they are more enriched in water ice than the rims and ejecta blankets of the freshest craters on Titan. The progression is consistent with the chemical weathering of Titans surface. We propose an evolutionary sequence such that Titans craters expose an intimate mixture of water ice and organic materials, and chemical weathering by methane rainfall removes the soluble organic materials, leaving the insoluble organics and water ice behind. These observations support the idea that fluvial processes are active in Titans equatorial regions.


Journal of Geophysical Research | 2006

An estimation of the electrical characteristics of planetary shallow subsurfaces with TAPIR antennas

A. Le Gall; Alain Reineix; V. Ciarletti; J. J. Berthelier; Richard Ney; F. Dolon; Charlotte Corbel

In the frame of the NETLANDER program, we have developed the Terrestrial And Planetary Investigation by Radar (TAPIR) imaging ground-penetrating radar to explore the Martian subsurface at kilometric depths and search for potential water reservoirs. This instrument which is to operate from a fixed lander is based on a new concept which allows one to image the various underground reflectors by determining the direction of propagation of the reflected waves. The electrical parameters of the shallow subsurface (permittivity and conductivity) need to be known to correctly determine the propagation vector. In addition, these electrical parameters can bring valuable information on the nature of the materials close to the surface. The electric antennas of the radar are 35 m long resistively loaded monopoles that are laid on the ground. Their impedance, measured during a dedicated mode of operation of the radar, depends on the electrical parameters of soil and is used to infer the permittivity and conductivity of the upper layer of the subsurface. This paper presents an experimental and theoretical study of the antenna impedance and shows that the frequency profile of the antenna complex impedance can be used to retrieve the geoelectrical characteristics of the soil. Comparisons between a numerical modeling and in situ measurements have been successfully carried over various soils, showing a very good agreement.


Geophysical Research Letters | 2005

Initial results of the Netlander imaging ground‐penetrating radar operated on the Antarctic Ice Shelf

J. J. Berthelier; S. Bonaimé; V. Ciarletti; R. Clairquin; F. Dolon; A. Le Gall; D. Nevejans; Richard Ney; Alain Reineix

The objective of the Netlander mission was to land 4 small geophysical stations on the surface of Mars to study the deep interior, subsurface, surface and atmosphere of the planet. Included in the payload was a ground penetrating radar (GPR) designed to retrieve not only the distance but also the direction of the reflectors, thus providing a simplified 3D imaging of the subsurface. In this paper we report initial results obtained during the RANETA campaign on the Antarctic ice shelf. Data from two soundings of the ice-bed rock interface are analyzed, demonstrating the capability of the radar to disentangle echoes from different reflecting facets of the bed rock.


Icarus | 2009

Titan's surface at 2.2-cm wavelength imaged by the Cassini RADAR radiometer: Calibration and first results

Michael A. Janssen; Ralph D. Lorenz; Robert West; F. Paganelli; Rosaly M. C. Lopes; R. Kirk; Charles Elachi; S. D. Wall; William T. K. Johnson; Y. Z. Anderson; R. A. Boehmer; Philip S. Callahan; Yonggyu Gim; G. Hamilton; K. D. Kelleher; Luz Roth; Bryan W. Stiles; A. Le Gall


Icarus | 2011

Cassini SAR, radiometry, scatterometry and altimetry observations of Titan's dune fields

A. Le Gall; Michael A. Janssen; Lauren C. Wye; Alexander G. Hayes; Jani Radebaugh; C. Savage; Howard A. Zebker; Ralph D. Lorenz; Jonathan I. Lunine; R. L. Kirk; Rosaly M. C. Lopes; S. D. Wall; Philip S. Callahan; Ellen R. Stofan; T. Farr


Icarus | 2014

Global mapping and characterization of Titan's dune fields with Cassini: correlation between RADAR and VIMS observations

Sebastien Rodriguez; A. Garcia; Antoine Lucas; T. Appéré; A. Le Gall; E. Reffet; Lucille Le Corre; S. Le Mouélic; Thomas Cornet; S. Courrech du Pont; Clément Narteau; O. Bourgeois; Jani Radebaugh; K. Arnold; Jason W. Barnes; K. Stephan; R. Jaumann; C. Sotin; Robert H. Brown; Ralph D. Lorenz; Elizabeth P. Turtle


Icarus | 2010

Radar-bright channels on Titan

A. Le Gall; Michael A. Janssen; Philippe Paillou; Ralph D. Lorenz; S. D. Wall


Icarus | 2012

Latitudinal and altitudinal controls of Titan’s dune field morphometry

A. Le Gall; Alexander G. Hayes; Ryan C. Ewing; Michael A. Janssen; Jani Radebaugh; C. Savage; P. Encrenaz


Icarus | 2016

Titan’s surface at 2.18-cm wavelength imaged by the Cassini RADAR radiometer: Results and interpretations through the first ten years of observation

Michael A. Janssen; A. Le Gall; Rosaly M. C. Lopes; Ralph D. Lorenz; Michael Malaska; Alexander G. Hayes; Catherine Dorothy Neish; Anezina Solomonidou; K. L. Mitchell; Jani Radebaugh; Stephen J. Keihm; Mathieu Choukroun; Cedric Leyrat; P. Encrenaz; Marco Mastrogiuseppe

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Michael A. Janssen

California Institute of Technology

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Ralph D. Lorenz

Johns Hopkins University Applied Physics Laboratory

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Rosaly M. C. Lopes

California Institute of Technology

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Stephen D. Wall

Jet Propulsion Laboratory

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J. Radebaugh

United States Geological Survey

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Michael Malaska

California Institute of Technology

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Bryan W. Stiles

Jet Propulsion Laboratory

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