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Venus's winds and temperatures during the MESSENGER's flyby: An approximation to a three-dimensional instantaneous state of the atmosphere
DOI: 10.1002/2017GL072900 Bibcode: 2017GeoRL..44.3907P

Clancy, R. T.; Hueso, R.; Sánchez-Lavega, A. +14 more

Even though many missions have explored the Venus atmospheric circulation, its instantaneous state is poorly characterized. In situ measurements vertically sampling the atmosphere exist for limited locations and dates, while remote sensing observations provide only global averages of winds at altitudes of the clouds: 47, 60, and 70 km. We present …

2017 Geophysical Research Letters
VenusExpress 16
Radar sounder evidence of thick, porous sediments in Meridiani Planum and implications for ice-filled deposits on Mars
DOI: 10.1002/2017GL074431 Bibcode: 2017GeoRL..44.9208W

Grant, John A.; Plaut, Jeffrey J.; Phillips, Roger J. +5 more

Meridiani Planum is one of the most intensely studied regions on Mars, yet little is known about the physical properties of the deposits below those examined by the Opportunity rover. We report the detection of subsurface echoes within the Meridiani Planum deposits from data obtained by the Mars Advanced Radar for Subsurface and Ionospheric Soundi…

2017 Geophysical Research Letters
MEx 13
Growth rate measurement of ULF waves in the ion foreshock
DOI: 10.1002/2017GL072692 Bibcode: 2017GeoRL..44.2120D

Hietala, H.; Angelopoulos, V.; Dorfman, S. +1 more

We report the first satellite measurement of the ultralow frequency (ULF) wave growth rate in the upstream region of the Earth's bow shock. We employ the two identical ARTEMIS spacecraft orbiting the Moon to characterize crescent-shaped reflected ion beams and relatively monochromatic ULF waves. The event presented here features spacecraft separat…

2017 Geophysical Research Letters
Cluster 12
The interplanetary magnetic field observed by Juno enroute to Jupiter
DOI: 10.1002/2017GL073137 Bibcode: 2017GeoRL..44.5936G

Connerney, John E. P.; Gruesbeck, Jacob R.; Gershman, Daniel J. +1 more

The Juno spacecraft was launched on 5 August 2011 and spent nearly 5 years traveling through the inner heliosphere on its way to Jupiter. The Magnetic Field Investigation was powered on shortly after launch and obtained vector measurements of the interplanetary magnetic field (IMF) at sample rates from 1 to 64 samples/second. The evolution of the …

2017 Geophysical Research Letters
Ulysses 10
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