Search Publications

Electric structure of dipolarization front at sub-proton scale
DOI: 10.1029/2012GL051274 Bibcode: 2012GeoRL..39.6105F

André, M.; Vaivads, A.; Huang, S. Y. +2 more

Using Cluster data, we investigate the electric structure of a dipolarization front (DF) - the ion inertial length (c/ωpi) scale boundary in the Earth's magnetotail formed at the front edge of an earthward propagating flow with reconnected magnetic flux. We estimate the current density and the electron pressure gradient throughout the D…

2012 Geophysical Research Letters
Cluster 179
Occurrence rate of earthward-propagating dipolarization fronts
DOI: 10.1029/2012GL051784 Bibcode: 2012GeoRL..3910101F

André, M.; Vaivads, A.; Huang, S. Y. +2 more

The occurrence rate of earthward-propagating dipolarization fronts (DFs) is investigated in this paper based on the 9 years (2001-2009) of Cluster 1 data. For the first time, we select the DF events by fitting the characteristic increase in Bz using a hyperbolic tangent function. 303 earthward-propagating DFs are found; they have on ave…

2012 Geophysical Research Letters
Cluster 153
Recent advances in understanding substorm dynamics
DOI: 10.1029/2012GL050859 Bibcode: 2012GeoRL..39.5101S

Nakamura, R.; Sergeev, V. A.; Angelopoulos, V.

Magnetospheric substorms are elemental processes of solar wind energy storage and explosive release in Earth's magnetosphere. They encompass fundamental plasma physics questions, are ubiquitous during all types of geomagnetic conditions, contribute significantly to magnetic storms, and are a key element of Space Weather applications. This paper re…

2012 Geophysical Research Letters
Cluster 134
Low-energy ions: A previously hidden solar system particle population
DOI: 10.1029/2011GL050242 Bibcode: 2012GeoRL..39.3101A

André, M.; Cully, C. M.

Ions with energies less than tens of eV originate from the Terrestrial ionosphere and from several planets and moons in the solar system. The low energy indicates the origin of the plasma but also severely complicates detection of the positive ions onboard sunlit spacecraft at higher altitudes, which often become positively charged to several tens…

2012 Geophysical Research Letters
Cluster 114
Electron acceleration in the reconnection diffusion region: Cluster observations
DOI: 10.1029/2012GL051946 Bibcode: 2012GeoRL..3911103H

André, M.; Vaivads, A.; Sahraoui, F. +10 more

We present one case study of magnetic islands and energetic electrons in the reconnection diffusion region observed by the Cluster spacecraft. The cores of the islands are characterized by strong core magnetic fields and density depletion. Intense currents, with the dominant component parallel to the ambient magnetic field, are detected inside the…

2012 Geophysical Research Letters
Cluster 113
Auroral evidence of Io's control over the magnetosphere of Jupiter
DOI: 10.1029/2011GL050253 Bibcode: 2012GeoRL..39.1105B

Bonfond, B.; Clarke, J. T.; Gérard, J. -C. +5 more

Contrary to the case of the Earth, the main auroral oval on Jupiter is related to the breakdown of plasma corotation in the middle magnetosphere. Even if the root causes for the main auroral emissions are Io's volcanism and Jupiter's fast rotation, changes in the aurora could be attributed either to these internal factors or to fluctuations of the…

2012 Geophysical Research Letters
eHST 108
Dielectric map of the Martian northern hemisphere and the nature of plain filling materials
DOI: 10.1029/2011GL050286 Bibcode: 2012GeoRL..39.2202M

Pommerol, Antoine; Kofman, Wlodek; Clifford, Stephen M. +2 more

A number of observations suggest that an extended ocean once covered a significant part of the Martian northern hemisphere. By probing the physical properties of the subsurface to unprecedented depth, the MARSIS/Mars Express provides new geophysical evidences for the former existence of a Late Hesperian ocean. The Vastitas Borealis formation, loca…

2012 Geophysical Research Letters
MEx 101
The importance of plasma β conditions for magnetic reconnection at Saturn's magnetopause
DOI: 10.1029/2012GL051372 Bibcode: 2012GeoRL..39.8103M

Coates, A. J.; Russell, C. T.; Dougherty, M. K. +7 more

Magnetic reconnection is an important process that occurs at the magnetopause boundary of Earth's magnetosphere because it leads to transport of solar wind energy into the system, driving magnetospheric dynamics. However, the nature of magnetopause reconnection in the case of Saturn's magnetosphere is unclear. Based on a combination of Cassini spa…

2012 Geophysical Research Letters
Cassini 98
Enceladus' extreme heat flux as revealed by its relaxed craters
DOI: 10.1029/2012GL052736 Bibcode: 2012GeoRL..3917204B

Singer, Kelsi N.; Schenk, Paul M.; McKinnon, William B. +1 more

Enceladus' cratered terrains contain large numbers of unusually shallow craters consistent with deformation by viscous relaxation of water ice under conditions of elevated heat flow. Here we use high-resolution topography to measure the relaxation fraction of craters on Enceladus far from the active South Pole. We find that many craters are shallo…

2012 Geophysical Research Letters
Cassini 89
Observations of turbulence within reconnection jet in the presence of guide field
DOI: 10.1029/2012GL052210 Bibcode: 2012GeoRL..3911104H

André, M.; Vaivads, A.; Sahraoui, F. +8 more

We present the first comprehensive observations of turbulence properties within high speed reconnection jet in the plasma sheet with moderate guide field. The power spectral density index is about -1.73 in the inertial range, and follows the value of -2.86 in the ion dissipation range. The turbulence is strongly anisotropic in the wave-vector spac…

2012 Geophysical Research Letters
Cluster 85