Search Publications

Energetic neutral atoms from the Earth's subsolar magnetopause
DOI: 10.1029/2010GL044140 Bibcode: 2010GeoRL..3713101F

Wurz, P.; Reisenfeld, D. B.; McComas, D. J. +10 more

The shocked solar wind in the Earth's magnetosheath becomes nearly stationary at the subsolar magnetopause. At this location, solar wind protons are neutralized by charge exchange with neutral hydrogen atoms at the extreme limits of the Earth's tenuous exosphere. The resulting Energetic Neutral Atoms (ENAs) propagate away from the subsolar region …

2010 Geophysical Research Letters
Cluster 66
Specular reflection on Titan: Liquids in Kraken Mare
DOI: 10.1029/2009GL042312 Bibcode: 2010GeoRL..37.7104S

Sotin, Christophe; Barnes, Jason W.; Soderblom, Jason M. +12 more

After more than 50 close flybys of Titan by the Cassini spacecraft, it has become evident that features similar in morphology to terrestrial lakes and seas exist in Titan's polar regions. As Titan progresses into northern spring, the much more numerous and larger lakes and seas in the north-polar region suggested by Cassini RADAR data, are becomin…

2010 Geophysical Research Letters
Cassini 66
The reversal of the rotational modulation rates of the north and south components of Saturn kilometric radiation near equinox
DOI: 10.1029/2010GL045796 Bibcode: 2010GeoRL..3724101G

Gurnett, D. A.; Persoon, A. M.; Kurth, W. S. +5 more

It has been known for many years that Saturn emits intense radio emissions at kilometer wavelengths and that this radiation is modulated by the rotation of the planet at a rate that varies slowly on time scales of years. Recently it has been shown that the radio emission consists of two components that have different rotational modulation rates, o…

2010 Geophysical Research Letters
Cassini Ulysses 66
Active shoreline of Ontario Lacus, Titan: A morphological study of the lake and its surroundings
DOI: 10.1029/2009GL041821 Bibcode: 2010GeoRL..37.5202W

Stofan, E.; Le Gall, A.; Mitchell, K. +18 more

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 Cassini's radar instrument (λ = 2 cm) and show morphological evidence for active mate…

2010 Geophysical Research Letters
Cassini 65
Link between EMIC waves in a plasmaspheric plume and a detached sub-auroral proton arc with observations of Cluster and IMAGE satellites
DOI: 10.1029/2010GL042711 Bibcode: 2010GeoRL..37.7108Y

Lucek, E.; Frey, H. U.; Décréau, P. M. E. +7 more

In this paper, we report observations from a Cluster satellite showing that ULF wave occurred in the outer boundary of a plasmaspheric plume on September 4, 2005. The band of observed ULF waves is between the He+ ion gyrofrequency and O+ ion gyrofrequency at the equatorial plane, implying that those ULF waves can be identifie…

2010 Geophysical Research Letters
Cluster 61
Variation of Saturn's UV aurora with SKR phase
DOI: 10.1029/2010GL044057 Bibcode: 2010GeoRL..3715102N

Cecconi, B.; Lamy, L.; Nichols, J. D. +6 more

It is well known that a wide range of kronian magnetospheric phenomena, including the Saturn kilometric radiation (SKR), exhibit oscillations near the planetary rotation period. However, although the SKR is believed to be generated by unstable auroral electrons, no connection has been established to date between diurnal SKR modulations and UV auro…

2010 Geophysical Research Letters
Cassini eHST 57
Dawn-dusk oscillation of Saturn's conjugate auroral ovals
DOI: 10.1029/2010GL045818 Bibcode: 2010GeoRL..3724102N

Lamy, L.; Nichols, J. D.; Cowley, S. W. H.

We present observations of the oscillation of the dawn-dusk locations of Saturn's northern and southern UV auroral ovals obtained using the Hubble Space Telescope during the 2009 equinoctial campaign. We determine the dawn-dusk locations of the centers of the southern and northern auroral ovals from the mean of the dawnward and duskward extents of…

2010 Geophysical Research Letters
Cassini eHST 53
Oxygen flux in the solar wind: Ulysses observations
DOI: 10.1029/2010GL045389 Bibcode: 2010GeoRL..3722101V

Zurbuchen, Thomas H.; von Steiger, Rudolf; McComas, David J.

We use the complete set of Ulysses solar wind data to conduct a comprehensive determination of the oxygen flux in relation to the proton flux in the solar wind during a wide range of solar activity levels. The data cover the heliosphere between 1.3 and 5.4 AU and, due to the unique orbit of Ulysses, all of the heliographic latitudes within ±80°. W…

2010 Geophysical Research Letters
Ulysses 53
Particle pressure, inertial force, and ring current density profiles in the magnetosphere of Saturn, based on Cassini measurements
DOI: 10.1029/2009GL041920 Bibcode: 2010GeoRL..37.2102S

Coates, A. J.; Krupp, N.; Dougherty, M. K. +9 more

We report initial results on the particle pressure distribution and its contribution to ring current density in the equatorial magnetosphere of Saturn, as measured by the Magnetospheric Imaging Instrument (MIMI) and the Cassini Plasma Spectrometer (CAPS) onboard the Cassini spacecraft. Data were obtained from September 2005 to May 2006, within ±0.…

2010 Geophysical Research Letters
Cassini 49
First results from the Venetia Burney Student Dust Counter on the New Horizons mission
DOI: 10.1029/2010GL043300 Bibcode: 2010GeoRL..3711101P

James, David; Horányi, Mihály; Poppe, Andrew +1 more

The Venetia Burney Student Dust Counter (SDC) onboard the New Horizons mission is an impact-based dust detector designed to map the size and spatial variability of the interplanetary dust population throughout the solar system. SDC consists of fourteen permanently polarized polyvinylidene fluoride detectors that register a charge upon impact by hy…

2010 Geophysical Research Letters
Ulysses 45