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Solar control of radar wave absorption by the Martian ionosphere
DOI: 10.1029/2006GL026637 Bibcode: 2006GeoRL..3313202M

Gurnett, D. A.; Morgan, D. D.; Plaut, J. J. +6 more

The MARSIS active sounder aboard the Mars Express spacecraft, under certain conditions in the Martian ionosphere, fails to detect the planetary surface. We have generated a statistical measure of the surface reflection visibility, which we plot as a time series and compare with both in situ particle data taken at Mars and solar x-ray data taken at…

2006 Geophysical Research Letters
MEx 47
Hydrogen exosphere at Mars: Pickup protons and their acceleration at the bow shock
DOI: 10.1029/2006GL027799 Bibcode: 2006GeoRL..3322103D

Barabash, S.; Lundin, R.; Yamauchi, M. +3 more

Pickup protons (PIs) with a ring-beam distribution originating from the extended hydrogen exosphere of Mars are observed by the ASPERA-3 experiment onboard the Mars Express spacecraft at solar minimum conditions. PIs can contribute ~1% to the solar wind number density at close distances to the flank bow shock. The observed fluxes of PIs indicate t…

2006 Geophysical Research Letters
MEx 41
Substorm associated magnetotail energetic electrons pitch angle evolutions and flow reversals: Cluster observation
DOI: 10.1029/2006GL026595 Bibcode: 2006GeoRL..3317101W

Lucek, E.; Fritz, T. A.; Wu, P. +1 more

The Cluster satellites observed a distinct pattern in the evolution of energetic electron pitch angle distributions on November 13, 2003, in the mid-tail (radius >10RE) associated with intensifications of these electron fluxes that accompanied an observed local dipolarization of the magnetic field. The intensity of electrons (20-200 …

2006 Geophysical Research Letters
Cluster 39
Dust devils on Mars observed by the High Resolution Stereo Camera
DOI: 10.1029/2006GL025816 Bibcode: 2006GeoRL..3311202S

Greeley, Ronald; Pätzold, Martin; Neukum, Gerhard +2 more

Fourteen active dust devils were observed by the High Resolution Stereo Camera (HRSC) on Mars Express, which enable the first analysis of the forward speed of dust devils on Mars determined from orbit. Results show speeds on the order of 20 m/s, which compares favorably with values of the wind profiles estimated from the Martian Climate Database f…

2006 Geophysical Research Letters
MEx 39
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