Search Publications

Growth mechanisms and dune orientation on Titan
DOI: 10.1002/2014GL060971 Bibcode: 2014GeoRL..41.6093L

Lorenz, Ralph D.; Tokano, Tetsuya; Rodriguez, Sébastien +8 more

Dune fields on Titan cover more than 17% of the moon's surface, constituting the largest known surface reservoir of organics. Their confinement to the equatorial belt, shape, and eastward direction of propagation offer crucial information regarding both the wind regime and sediment supply. Herein, we present a comprehensive analysis of Titan's dun…

2014 Geophysical Research Letters
Cassini 51
Surface of Ligeia Mare, Titan, from Cassini altimeter and radiometer analysis
DOI: 10.1002/2013GL058877 Bibcode: 2014GeoRL..41..308Z

Le Gall, Alice; Hayes, Alex; Zebker, Howard +3 more

Cassini radar observations of the surface of Ligeia Mare collected during the 23 May 2013 (T91) Cassini flyby show that it is extremely smooth, likely to be mostly methane in composition, and exhibits no surface wave activity. The radar parameters were tuned for nadir-looking geometry of liquid surfaces, using experience from Cassini's only compar…

2014 Geophysical Research Letters
Cassini 47
Fast transport of resonant electrons in phase space due to nonlinear trapping by whistler waves
DOI: 10.1002/2014GL061380 Bibcode: 2014GeoRL..41.5727A

Krasnoselskikh, V.; Artemyev, A. V.; Agapitov, O. V. +4 more

We present an analytical, simplified formulation accounting for the fast transport of relativistic electrons in phase space due to wave-particle resonant interactions in the inhomogeneous magnetic field of Earth's radiation belts. We show that the usual description of the evolution of the particle velocity distribution based on the Fokker-Planck e…

2014 Geophysical Research Letters
Cluster 44
Dynamic auroral storms on Saturn as observed by the Hubble Space Telescope
DOI: 10.1002/2014GL060186 Bibcode: 2014GeoRL..41.3323N

Brown, R. H.; Baines, K. H.; Dougherty, M. K. +14 more

We present observations of significant dynamics within two UV auroral storms observed on Saturn using the Hubble Space Telescope in April/May 2013. Specifically, we discuss bursts of auroral emission observed at the poleward boundary of a solar wind-induced auroral storm, propagating at ∼330% rigid corotation from near ∼01 h LT toward ∼08 h LT. We…

2014 Geophysical Research Letters
eHST 40
The long-term steady motion of Saturn's hexagon and the stability of its enclosed jet stream under seasonal changes
DOI: 10.1002/2013GL059078 Bibcode: 2014GeoRL..41.1425S

Hueso, R.; Sánchez-Lavega, A.; Rojas, J. F. +14 more

We investigate the long-term motion of Saturn's north pole hexagon and the structure of its associated eastward jet, using Cassini imaging science system and ground-based images from 2008 to 2014. We show that both are persistent features that have survived the long polar night, the jet profile remaining essentially unchanged. During those years, …

2014 Geophysical Research Letters
Cassini eHST 40
The flushing of Ligeia: Composition variations across Titan's seas in a simple hydrological model
DOI: 10.1002/2014GL061133 Bibcode: 2014GeoRL..41.5764L

Lorenz, Ralph D.

We use a simple box model to explore possible differences in the liquid composition of Titan's seas. Major variations in the abundance of involatile ethane, somewhat analogous to salinity in terrestrial waters, arise from the hydrological cycle, which introduces more "fresh" methane rainfall at the highest latitudes in summer. The observed composi…

2014 Geophysical Research Letters
Cassini 38
Global model of low-frequency chorus (fLHR<f<0.1fce) from multiple satellite observations
DOI: 10.1002/2013GL059050 Bibcode: 2014GeoRL..41..280M

Meredith, Nigel P.; Horne, Richard B.; Thorne, Richard M. +2 more

Whistler mode chorus is an important magnetospheric emission, playing a dual role in the acceleration and loss of relativistic electrons in the Earth's outer radiation belt. Chorus is typically generated in the equatorial region in the frequency range 0.1-0.8 fce, where fce is the local electron gyrofrequency. However, as the…

2014 Geophysical Research Letters
Cluster 37
Cusp observation at Saturn's high-latitude magnetosphere by the Cassini spacecraft
DOI: 10.1002/2014GL059319 Bibcode: 2014GeoRL..41.1382J

Coates, A. J.; Krupp, N.; Dougherty, M. K. +11 more

We report on the first analysis of magnetospheric cusp observations at Saturn by multiple in situ instruments onboard the Cassini spacecraft. Using this we infer the process of reconnection was occurring at Saturn's magnetopause. This agrees with remote observations that showed the associated auroral signatures of reconnection. Cassini crossed the…

2014 Geophysical Research Letters
Cassini 35
Highly structured electron anisotropy in collisionless reconnection exhausts
DOI: 10.1002/2014GL060608 Bibcode: 2014GeoRL..41.5389S

Torbert, R. B.; Li, G.; Chen, L. -J. +6 more

Results from two-dimensional particle-in-cell simulations of collisionless magnetic reconnection with zero guide field discussed in this paper reveal that around the time when the reconnection rate peaks, electron velocity distributions become highly structured in magnetic islands and open exhausts. Rings, arcs, and counterstreaming beams are gene…

2014 Geophysical Research Letters
Cluster 33
Enhanced ionization of the Martian nightside ionosphere during solar energetic particle events
DOI: 10.1002/2013GL058895 Bibcode: 2014GeoRL..41..793N

Gurnett, D. A.; Futaana, Y.; Němec, F. +2 more

Electron densities in the Martian nightside ionosphere are more than 90% of time too low to be detected by the Mars Advanced Radar for Subsurface and Ionosphere Sounding radar sounder on board the Mars Express spacecraft. However, the relative number of ionograms with peak electron density high enough to be detected represents a good statistical p…

2014 Geophysical Research Letters
MEx 28