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Isolated magnetic field structures in Mercury's magnetosheath as possible analogues for terrestrial magnetosheath plasmoids and jets
DOI: 10.1016/j.pss.2016.06.002 Bibcode: 2016P&SS..129...61K

Karlsson, Tomas; Raines, Jim M.; Liljeblad, Elisabet +3 more

We have investigated MESSENGER magnetic field data from the Mercury magnetosheath and near solar wind, to identify isolated magnetic field structures (defined as clear, isolated changes in the field magnitude). Their properties are studied in order to determine if they may be considered as analogues to plasmoids and jets known to exist in Earth's …

2016 Planetary and Space Science
Cluster 27
Access of energetic particles to Titan's exobase: A study of Cassini's T9 flyby
DOI: 10.1016/j.pss.2015.11.013 Bibcode: 2016P&SS..130...40R

Coates, A. J.; Krupp, N.; Dougherty, M. K. +6 more

We study how the local electromagnetic disturbances introduced by Titan affect the ionization rates of the atmosphere. For this, we model the precipitation of energetic particles, specifically hydrogen and oxygen ions with energies between 1 keV and 1 MeV, into Titan's exobase for the specific magnetospheric configuration of the T9 flyby. For the …

2016 Planetary and Space Science
Cassini 24
A classification of martian gullies from HiRISE imagery
DOI: 10.1016/j.pss.2016.08.002 Bibcode: 2016P&SS..131...88A

Auld, Katherine S.; Dixon, John C.

Due to the large and varied population of gullies observed in Mars High Resolution Imaging Science Experiment (HiRISE) imagery that exhibit diverse characteristics, this paper develops a classification of martian gullies based on their morphological characteristics. This provides a firmer foundation for future investigation of the genesis of diffe…

2016 Planetary and Space Science
MEx 23
Dynamics of planetary ions in the induced magnetospheres of Venus and Mars
DOI: 10.1016/j.pss.2015.08.012 Bibcode: 2016P&SS..127....1J

Luhmann, J. G.; Brain, D. A.; Jarvinen, R.

We compare dynamics of planetary ions in the induced magnetospheres of Venus and Mars in a global hybrid simulation to study factors controlling the ion escape at unmagnetized planets. In the simulation we find that the finite Larmor radius (FLR) effects of escaping heavy ions are stronger at Mars than Venus under nominal solar wind conditions. Bu…

2016 Planetary and Space Science
VenusExpress 23
Martian surface microtexture from orbital CRISM multi-angular observations: A new perspective for the characterization of the geological processes
DOI: 10.1016/j.pss.2016.05.005 Bibcode: 2016P&SS..128...30F

Schmidt, F.; Douté, S.; Fernando, J.

The surface of Mars has a high morphological and mineralogical diversity due to the intricacy of external, internal processes, and exchanges with the atmosphere, the hydrosphere and the cryosphere. In particular, liquid water played an important role in surface evolution. However, the origin, duration and intensity of those wet events have been hi…

2016 Planetary and Space Science
MEx 18
The daily processing of asteroid observations by Gaia
DOI: 10.1016/j.pss.2015.11.009 Bibcode: 2016P&SS..123...87T

Muinonen, Karri; Fedorets, Grigori; Pentikäinen, Hanna +15 more

The Gaia mission started its regular observing program in the summer of 2014, and since then it is regularly obtaining observations of asteroids. This paper draws the outline of the data processing for Solar System objects, and in particular on the daily ;short-term; processing, from the on-board data acquisition to the ground-based processing. We…

2016 Planetary and Space Science
Gaia 18
Separation of dynamic and isostatic components of the Venusian gravity and topography and determination of the crustal thickness of Venus
DOI: 10.1016/j.pss.2016.06.001 Bibcode: 2016P&SS..129...24Y

Yang, An; Huang, Jinshui; Wei, Daiyun

Assuming that the long-wavelength geoid and topography of Venus are supported by both mantle convection and Airy isostasy, we propose a method to separate the dynamic and isostatic components of the Venusian gravity and topography with the aid of the dynamic admittance from numerical models of mantle convection and the isostatic admittance from an…

2016 Planetary and Space Science
VenusExpress 17
A comprehensive analysis of ion cyclotron waves in the equatorial magnetosphere of Saturn
DOI: 10.1016/j.pss.2016.06.003 Bibcode: 2016P&SS..129...47M

Simon, Sven; Kabanovic, Slawa; Meeks, Zachary

We present a comprehensive analysis of ion cyclotron waves in the equatorial magnetosphere of Saturn, considering all magnetic field data collected during the Cassini era (totaling to over 4 years of data from the equatorial plane). This dataset includes eight targeted flybys of Enceladus, three targeted flybys of Dione, and three targeted flybys …

2016 Planetary and Space Science
Cassini 16
Systematic processing of Mars Express HRSC panchromatic and colour image mosaics: Image equalisation using an external brightness reference
DOI: 10.1016/j.pss.2015.12.002 Bibcode: 2016P&SS..121...18M

Jaumann, R.; van Gasselt, S.; Dumke, A. +8 more

After more than ten years in orbit at Mars, the coverage from the High Resolution Stereo Camera (HRSC) on the European Space Agency's Mars Express is sufficient to begin constructing mosaic products on a global scale. We describe our systematic processing procedure and, in particular, the technique used to bring images affected by atmospheric dust…

2016 Planetary and Space Science
MEx 15
Polarimetry observations of comets: Status, questions, future pathways
DOI: 10.1016/j.pss.2015.11.016 Bibcode: 2016P&SS..123...41H

Hines, Dean C.; Levasseur-Regourd, Anny-Chantal

Polarimetric observations of comets have provided crucial insight into the composition and evolution of cometary dust particles. Herein, we present a brief overview of the polarization properties observed in comets, and some possible interpretations. We also discuss recent imaging polarimetry observations of C/2012 S1 (ISON) and 67P/Churyumov-Gera…

2016 Planetary and Space Science
Rosetta eHST 15