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Oxygen airglow emission on Venus and Mars as seen by VIRTIS/VEX and OMEGA/MEX imaging spectrometers
DOI: 10.1016/j.pss.2010.05.019 Bibcode: 2011P&SS...59..981M

Bibring, J. -P.; Gondet, B.; Bellucci, G. +8 more

Imaging spectrometers are highly effective instruments for investigation of planetary atmospheres. They present the advantage of coupling the compositional information to the spatial distribution, allowing simultaneous study of chemistry and dynamics in the atmospheres of Venus and Mars. In this work, we summarize recent results about the O 2…

2011 Planetary and Space Science
MEx VenusExpress 7
ROY—A multiscale magnetospheric mission
DOI: 10.1016/j.pss.2010.05.001 Bibcode: 2011P&SS...59..606S

Novikov, D.; Kozak, L.; Amata, E. +21 more

The scientific rationale of the ROY multi-satellite mission addresses multiscale investigations of plasma processes in the key magnetospheric regions with strong plasma gradients, turbulence and magnetic field annihilation in the range from electron inertial length to MHD scales. The main scientific aims of ROY mission include explorations of:

2011 Planetary and Space Science
Cluster 7
MHD-instability of the magnetotail: Global modes
DOI: 10.1016/j.pss.2011.01.006 Bibcode: 2011P&SS...59..402L

Leonovich, A. S.

A hydromagnetic stability problem is solved for the magnetospheric tail inside the solar wind plasma flow. A model magnetotail is used in the form of a plasma cylinder which is inhomogeneous over the radius. For a qualitative analysis of the problem the solution is obtained analytically, in the WKB approximation. The plasma cylinder boundary is as…

2011 Planetary and Space Science
Cluster 7
Hydroxyl airglow on Venus in comparison with Earth
DOI: 10.1016/j.pss.2010.05.004 Bibcode: 2011P&SS...59..974M

Drossart, P.; Piccioni, G.; Migliorini, A. +1 more

Hydroxyl nightglow is intensively studied in the Earth atmosphere, due to its coupling to the ozone cycle. Recently, it was detected for the first time also in the Venus atmosphere, thanks to the VIRTIS-Venus Express observations. The main Δ ν=1, 2 emissions in the infrared spectral range, centred, respectively, at 2.81 and 1.46 µm (which co…

2011 Planetary and Space Science
VenusExpress 7
Scaling law of the reduced magnetic helicity in fast streams
DOI: 10.1016/j.pss.2010.04.017 Bibcode: 2011P&SS...59..575P

Perri, S.; Balogh, A.; Bruno, R. +2 more

The reduced magnetic helicity is a quantity related to the handedness of the magnetic field fluctuations. In the present paper we study the scaling law of the reduced magnetic helicity in fast streams in the solar wind by using high-resolution magnetic field data by the Ulysses spacecraft. We show that at high frequencies both the left-hand and th…

2011 Planetary and Space Science
Ulysses 6
On turbulence in the quasi-perpendicular bow shock
DOI: 10.1016/j.pss.2010.03.013 Bibcode: 2011P&SS...59..475H

Meziane, K.; Hamza, A. M.

In this paper we propose to review the fundamental aspects of turbulence theories and their relevance to particle distribution functions observed by the cluster satellites in the quasi-perpendicular shock. The paper focusses on the hierarchical model describing the different levels of plasma turbulence; from the linear theory, through the quasi-li…

2011 Planetary and Space Science
Cluster 6
Comparative investigation of the terrestrial and Venusian magnetopause: Kinetic modeling and experimental observations by Cluster and Venus Express
DOI: 10.1016/j.pss.2010.04.019 Bibcode: 2011P&SS...59.1028E

Barabash, S.; Lundin, R.; Zhang, T. L. +4 more

In June 2006 Venus Express crossed several times the outer boundary of Venus induced magnetosphere, its magnetosheath and its bow shock. During the same interval the Cluster spacecraft surveyed the dawn flank of the terrestrial magnetosphere, intersected the Earth's magnetopause and spent long time intervals in the magnetosheath. This configuratio…

2011 Planetary and Space Science
Cluster VenusExpress 5
Dispersive MHD turbulence in one dimension
DOI: 10.1016/j.pss.2010.02.003 Bibcode: 2011P&SS...59..556L

Passot, T.; Sulem, P. L.; Laveder, D. +1 more

Numerical simulations of dispersive turbulence in magnetized plasmas based on the Hall-MHD description are presented, assuming spatial variations along a unique direction making a prescribed angle with the ambient magnetic field. Main observations concern the energy transfers among the different scales and the various types of MHD waves, together …

2011 Planetary and Space Science
Cluster 5
Comparative planetology, climatology and biology of Venus, Earth and Mars
DOI: 10.1016/j.pss.2010.11.009 Bibcode: 2011P&SS...59..889T

Taylor, F. W.

Spacecraft studies of the three terrestrial planets with atmospheres have made it possible to make meaningful comparisons that shed light on their common origin and divergent evolutionary paths. Early in their histories, all three apparently had oceans and extensive volcanism; Mars and Earth, at least, had magnetic fields, and Earth, at least, had…

2011 Planetary and Space Science
VenusExpress 4
Integrating advanced visualization technology into the planetary Geoscience workflow
DOI: 10.1016/j.pss.2010.07.015 Bibcode: 2011P&SS...59.1273H

Dickson, James; Huffman, John; Forsberg, Andrew +3 more

Recent advances in computer visualization have allowed us to develop new tools for analyzing the data gathered during planetary missions, which is important, since these data sets have grown exponentially in recent years to tens of terabytes in size. As part of the Advanced Visualization in Solar System Exploration and Research (ADVISER) project, …

2011 Planetary and Space Science
MEx 4