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Cassini radio occultations of Saturn's ionosphere: Model comparisons using a constant water flux
DOI: 10.1029/2006GL027375 Bibcode: 2006GeoRL..3322202M

Moore, Luke; Kliore, Arvydas J.; Mendillo, Michael +3 more

Recent radio occultations of Saturn's equatorial ionosphere by the Cassini spacecraft provide important insight into this poorly constrained region. Twelve new electron density profiles identify a clear dawn/dusk asymmetry as well as two apparently separate electron density peaks. This study uses a 3D general circulation model along with 1D water …

2006 Geophysical Research Letters
Cassini 39
Geologically recent tectonic, volcanic and fluvial activity on the eastern flank of the Olympus Mons volcano, Mars
DOI: 10.1029/2006GL026396 Bibcode: 2006GeoRL..3313201B

Head, J. W.; Neukum, G.; van Gasselt, S. +4 more

We show evidence of very recent (<=25-40 Myr) geologic activity on the eastern flank of Olympus Mons volcano that includes a suite of fluvial (channel networks), volcanic (emplacement of lava flows and dikes), and tectonic (wrinkle ridges and troughs) processes. The combination and youth of these features confirms the importance of geological a…

2006 Geophysical Research Letters
MEx 38
Cluster PEACE observations of electron pressure tensor divergence in the magnetotail
DOI: 10.1029/2006GL027868 Bibcode: 2006GeoRL..3322106H

Lucek, E.; Fazakerley, A. N.; Owen, C. J. +4 more

Cluster crossed the magnetotail neutral sheet on four occasions between 16:38 and 16:43 UT on 08/17/2003. The four-spacecraft capabilities of Cluster are used to determine spatial gradients from the magnetic field vectors and, for the first time, full electron pressure tensors. We find that the contribution to the electric field from the Hall term…

2006 Geophysical Research Letters
Cluster 38
A global magnetic model of Saturn's magnetosphere and a comparison with Cassini SOI data
DOI: 10.1029/2006GL025896 Bibcode: 2006GeoRL..33.8101A

Alexeev, I. I.; Belenkaya, E. S.; Nichols, J. D. +4 more

A re-scaling of a recent model of Jupiter's magnetosphere incorporating ring current, magnetopause, and tail current systems is used as a starting-point for modeling Saturn's magnetospheric field. The model is compared with observations obtained by Cassini during its Saturn orbit insertion fly-through of Saturn's magnetosphere, and is shown to giv…

2006 Geophysical Research Letters
Cassini 38
Electrostatic solitary structures observed at Saturn
DOI: 10.1029/2005GL024532 Bibcode: 2006GeoRL..33.6103W

Gurnett, D. A.; Dougherty, M. K.; Kurth, W. S. +2 more

We report observations of electric field solitary structures, measured by the Cassini Radio and Plasma Wave Science (RPWS) instrument in the vicinity of Saturn's magnetosphere with ambient magnetic fields that range from ~0.1 nT to 8000 nT. The peak-to-peak electric field amplitudes of the observed solitary structures range from a few µV/m t…

2006 Geophysical Research Letters
Cassini 30
Europa's FUV auroral tail on Jupiter
DOI: 10.1029/2005GL025487 Bibcode: 2006GeoRL..33.6201G

Clarke, J. T.; Mauk, B. H.; Gérard, J. -C. +3 more

Ultraviolet images of Jupiter's northern aurora obtained in 2005 confirm the existence of an electromagnetic interaction between Europa and the Jovian ionosphere. The auroral signature shows a two-component structure: a quasi-circular Europa spot, followed by a previously undetected faint tail emission trailing in the direction of corotation flow.…

2006 Geophysical Research Letters
eHST 28
Kinetic properties of heavy solar wind ions from Ulysses-SWICS
DOI: 10.1029/2005GL024998 Bibcode: 2006GeoRL..33.9103V

Zurbuchen, T. H.; von Steiger, R.

The kinetic properties of heavy ions in the solar wind reflect the plasma processes governing the solar wind in the heliosphere. We use Ulysses-SWICS data that resolve heavy ions in a wide range of mass-per-charge values, 2 <= m/q <= 9.33, to investigate the heavy ions and their dynamic evolution throughout the heliosphere. While at 1 AU the…

2006 Geophysical Research Letters
Ulysses 28
A steep fan at Coprates Catena, Valles Marineris, Mars, as seen by HRSC data
DOI: 10.1029/2005GL025435 Bibcode: 2006GeoRL..33.7204D

Neukum, G.; Hauber, E.; Reiss, D. +4 more

We investigate a steep fan-like deposit in the Coprates Catena region, using the new High Resolution Stereo Camera (HRSC) data and other Martian data sets. Water flowing in a 45-km-long sapping valley entered a deep trough and formed a stepped fan 1100-m-high above the trough floor with a mean slope of 7.4°. The origin of the fan is uncertain. How…

2006 Geophysical Research Letters
MEx 27
Kinetic aspects of foreshock cavities
DOI: 10.1029/2005GL025612 Bibcode: 2006GeoRL..3312103S

Schwartz, Steven J.; Meziane, Karim; Horbury, Timothy S. +2 more

We have investigated the kinetic signatures within, and at the edges of, a foreshock cavity. Such cavities are believed to be formed when an isolated collection of interplanetary magnetic field lines connect to quasi-parallel regions of the Earth's bow shock, allowing energetic ions to flow upstream and excavate a local cavity. Observations by the…

2006 Geophysical Research Letters
Cluster 26
Formation of Saturn's ring spokes by lightning-induced electron beams
DOI: 10.1029/2006GL028146 Bibcode: 2006GeoRL..3321202J

Krupp, N.; Woch, J.; Fränz, M. +10 more

Spokes are near-linear markings sometimes visible on Saturn's rings. They are widely accepted as being electrostatically-levitated sheets of ~0.6 micron-radius charged grains. Previously-suggested causes of the grains' charging do not agree with all spoke characteristics, which include their rapid generation, localized formation primarily in Satur…

2006 Geophysical Research Letters
Cassini 25