Search Publications

Tangential deflection and formation of counterstreaming flows at the impact of a plasma jet on a tangential discontinuity
DOI: 10.1002/2017GL073763 Bibcode: 2017GeoRL..44.5920V

Echim, M.; Voitcu, G.

In this letter we report three-dimensional particle-in-cell simulations of the interaction between a nonpenetrable magnetosheath jet and the magnetopause, for northward interplanetary magnetic field. The magnetopause is modeled as a tangential discontinuity with no magnetic shear. We investigate the deflection of the plasma jet in the direction ta…

2017 Geophysical Research Letters
Cluster 10
The vertical transport of methane from different potential emission types on Mars
DOI: 10.1002/2017GL074613 Bibcode: 2017GeoRL..44.8611H

Patel, M. R.; Lewis, S. R.; Holmes, J. A.

The contrasting evolutionary behavior of the vertical profile of methane from three potential release scenarios is analyzed using a global circulation model with assimilated temperature profiles. Understanding the evolving methane distribution is essential for interpretation of future retrievals of the methane vertical profile taken by instruments…

2017 Geophysical Research Letters
ExoMars-16 9
Schumann resonances at Mars: Effects of the day-night asymmetry and the dust-loaded ionosphere
DOI: 10.1002/2016GL071635 Bibcode: 2017GeoRL..44..648T

Montmessin, F.; Toledo-Redondo, S.; Molina-Cuberos, G. J. +6 more

Schumann resonances are standing waves that oscillate in the electromagnetic cavity formed between the conducting lower ionosphere and the surface of the planet. They have been measured in situ only on Earth and Titan, although they are believed to exist on other planets like Mars. We report numerical simulations of the Martian electromagnetic cav…

2017 Geophysical Research Letters
ExoMars-16 7
Observations of multiharmonic ion cyclotron waves due to inverse ion cyclotron damping in the northern magnetospheric cusp
DOI: 10.1002/2016GL071680 Bibcode: 2017GeoRL..44...22S

Gunell, H.; Slapak, R.; Hamrin, M.

We present a case study of inverse ion cyclotron damping taking place in the northern terrestrial magnetospheric cusp, exciting waves at the ion cyclotron frequency and its harmonics. The ion cyclotron waves are primarily seen as peaks in the magnetic-field spectral densities. The corresponding peaks in the electric-field spectral densities are no…

2017 Geophysical Research Letters
Cluster 6
Dual E × B flow responses in the dayside ionosphere to a sudden IMF By rotation
DOI: 10.1002/2017GL073374 Bibcode: 2017GeoRL..44.6525E

Trattner, K. J.; Eriksson, S.; Baker, J. B. H. +3 more

We report for the first time a dual transition state in the dayside ionosphere following a sudden rotation of the interplanetary magnetic field (IMF) in the upstream magnetosheath from IMF <fi>B</fi><fi>y</fi> < 0 to <fi>B</fi><fi>y</fi> > 0 during <fi>B</fi>

2017 Geophysical Research Letters
Cluster 3
New suprathermal proton population around the Moon: Observation by SARA on Chandrayaan-1
DOI: 10.1002/2017GL072605 Bibcode: 2017GeoRL..44.4540D

Barabash, Stas; Holmström, Mats; Futaana, Yoshifumi +4 more

We report a new population of suprathermal H+ (∼1.5-3 times the solar wind energy) around the Moon observed by Solar Wind Monitor (SWIM)/Sub-keV Atom Reflecting Analyzer (SARA) on Chandrayaan-1. These ions have large initial velocity (>100 km s-1) and are observed on the dayside, near the terminator, and in the near-wake r…

2017 Geophysical Research Letters
Chandrayaan-1 2
Cassini UVIS observations of Titan ultraviolet airglow intensity dependence with solar zenith angle
DOI: 10.1002/2016GL071756 Bibcode: 2017GeoRL..44...88R

West, R. A.; Esposito, L. W.; Royer, E. M. +3 more

The Cassini Ultraviolet Imaging Spectrometer (UVIS) observed the airglow (dayglow and nightglow) of Titan over a range of solar zenith angles (SZA) from 14 to 150° on five separate observations obtained between 2008 and 2012. The modeling of the solar cycle normalized UVIS observations indicates that a Chapman layer function provides a satisfactor…

2017 Geophysical Research Letters
Cassini 1
Enceladus's internal ocean and ice shell constrained from Cassini gravity, shape, and libration data
DOI: 10.1002/2016GL068634 Bibcode: 2016GeoRL..43.5653C

Bourgeois, Olivier; Massé, Marion; Čadek, Ondřej +8 more

The intense plume activity at the South Pole of Enceladus together with the recent detection of libration hints at an internal water ocean underneath the outer ice shell. However, the interpretation of gravity, shape, and libration data leads to contradicting results regarding the depth of ocean/ice interface and the total volume of the ocean. Her…

2016 Geophysical Research Letters
Cassini 130
Mass loading at 67P/Churyumov-Gerasimenko: A case study
DOI: 10.1002/2015GL067436 Bibcode: 2016GeoRL..43.1411B

Behar, E.; Nilsson, H.; Richter, I. +3 more

We study the dynamics of the interaction between the solar wind ions and a partially ionized atmosphere around a comet, at a distance of 2.88 AU from the Sun during a period of low nucleus activity. Comparing particle data and magnetic field data for a case study, we highlight the prime role of the solar wind electric field in the cometary ion dyn…

2016 Geophysical Research Letters
Rosetta 63
Flux transfer event observation at Saturn's dayside magnetopause by the Cassini spacecraft
DOI: 10.1002/2016GL069260 Bibcode: 2016GeoRL..43.6713J

Coates, Andrew J.; Arridge, Christopher S.; Waite, J. Hunter +6 more

We present the first observation of a flux rope at Saturn's dayside magnetopause. This is an important result because it shows that the Saturnian magnetopause is conducive to multiple X-line reconnection and flux rope generation. Minimum variance analysis shows that the magnetic signature is consistent with a flux rope. The magnetic observations w…

2016 Geophysical Research Letters
Cassini 40