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Jovian Auroral Radio Sources Detected In Situ by Juno/Waves: Comparisons With Model Auroral Ovals and Simultaneous HST FUV Images
DOI: 10.1029/2019GL084799 Bibcode: 2019GeoRL..4611606L

Kurth, W. S.; Lamy, L.; Zarka, P. +4 more

Since the discovery of Jovian auroral radio emissions, the question arises of the source positions of the different components (broadband kilometric, hectometric, and decametric) and their association with far ultraviolet (FUV) auroral emissions. We surveyed Juno's first 15 perijoves to track local radio sources from in situ Juno/Waves measurement…

2019 Geophysical Research Letters
eHST 20
Raised Rims Around Titan's Sharp-Edged Depressions
DOI: 10.1029/2018GL078099 Bibcode: 2019GeoRL..46.5846B

Lunine, J. I.; Hayes, A. G.; Lopes, R. M. C. +6 more

We perform a systematic survey of Titan's sharp-edged depressions (SEDs) using a combination of Cassini synthetic aperture radar images and delay-Doppler processed altimetry. We identify a characteristic bright-dark pattern around 172 SEDs that correlates with elevated features only resolved with the highest resolution topographic data. We find th…

2019 Geophysical Research Letters
Cassini 18
Formation of a New Great Dark Spot on Neptune in 2018
DOI: 10.1029/2019GL081961 Bibcode: 2019GeoRL..46.3108S

Simon, A. A.; Wong, M. H.; Hsu, A. I.

For the first time, Hubble Space Telescope visible-wavelength imaging shows the formation history of a dark vortex on Neptune. A new northern Great Dark Spot (NDS-2018) was discovered in September and November 2018 images, spanning roughly 12° of latitude and 27° in longitude (11,000 × 5,000 km) at 23°N planetographic latitude. NDS-2018 is similar…

2019 Geophysical Research Letters
eHST 18
High-Frequency Wave Generation in Magnetotail Reconnection: Nonlinear Harmonics of Upper Hybrid Waves
DOI: 10.1029/2019GL083361 Bibcode: 2019GeoRL..46.7873D

Graham, Daniel B.; Yoon, Peter H.; Sibeck, David G. +4 more

MMS3 spacecraft passed the vicinity of the electron diffusion region of magnetotail reconnection on 3 July 2017, observing discrepancies between perpendicular electron bulk velocities and E>→×B>→ drift, and agyrotropic electron crescent distributions. Analyzing linear wave dispersions, Burch et al. (2019,

Cluster 18
The Effects of Crustal Magnetic Fields and Solar EUV Flux on Ionopause Formation at Mars
DOI: 10.1029/2019GL083499 Bibcode: 2019GeoRL..4610257C

Gurnett, D. A.; Morgan, D. D.; Kopf, A. J. +5 more

We study the ionopause of Mars using a database of 6,893 ionopause detections obtained over 11 years by the MARSIS (Mars Advanced Radar for Subsurface and Ionosphere Sounding) experiment. The ionopause, in this work, is defined as a steep density gradient that appears in MARSIS remote sounding ionograms as a horizontal line at frequencies below 0.…

2019 Geophysical Research Letters
MEx 18
Observational Evidence for Summer Rainfall at Titan's North Pole
DOI: 10.1029/2018GL080943 Bibcode: 2019GeoRL..46.1205D

Sotin, Christophe; Barnes, Jason W.; Soderblom, Jason M. +13 more

Methane rain on Saturn's moon Titan makes it the only place, other than Earth, where rain interacts with the surface. When and where that rain wets the surface changes seasonally in ways that remain poorly understood. Here we report the discovery of a bright ephemeral feature covering an area of 120,000 km2 near Titan's north pole in ob…

2019 Geophysical Research Letters
Cassini 16
The 2018 Martian Global Dust Storm Over the South Polar Region Studied With MEx/VMC
DOI: 10.1029/2019GL084266 Bibcode: 2019GeoRL..4610330H

Hueso, R.; Sánchez-Lavega, A.; Titov, D. +6 more

We study the 2018 Martian global dust storm (GDS 2018) over the Southern Polar Region using images obtained by the Visual Monitoring Camera (VMC) on board Mars Express (MEx) during June and July 2018. Dust penetrated into the polar cap region but never covered the cap completely, and its spatial distribution was nonhomogeneous and rapidly changing…

2019 Geophysical Research Letters
MEx 16
Jovian High-Latitude Ionospheric Ions: Juno In Situ Observations
DOI: 10.1029/2019GL084146 Bibcode: 2019GeoRL..46.8663V

Thomsen, M. F.; Wilson, R. J.; Louarn, P. +10 more

The low-altitude, high-velocity trajectory of the Juno spacecraft enables the Jovian Auroral Distributions Experiment to make the first in situ observations of the high-latitude ionospheric plasma. Ions are observed to energies below 1 eV. The high-latitude ionospheric ions are observed simultaneously with a loss cone in the magnetospheric ions, s…

2019 Geophysical Research Letters
eHST 15
First Observations of the Disruption of the Earth's Foreshock Wave Field During Magnetic Clouds
DOI: 10.1029/2019GL084437 Bibcode: 2019GeoRL..4612644T

Escoubet, C. P.; Dandouras, I.; Palmroth, M. +8 more

The foreshock, extending upstream of Earth's bow shock, is a region of intense electromagnetic wave activity and nonlinear phenomena, which can have global effects on geospace. It is also the first geophysical region encountered by solar wind disturbances journeying toward Earth. Here, we present the first observations of considerable modification…

2019 Geophysical Research Letters
Cluster 14
Energetic Oxygen and Sulfur Charge States in the Outer Jovian Magnetosphere: Insights From the Cassini Jupiter Flyby
DOI: 10.1029/2019GL085185 Bibcode: 2019GeoRL..4611709A

Wilson, R. J.; Krimigis, S. M.; Mitchell, D. G. +10 more

On 10 January 2001, Cassini briefly entered into the magnetosphere of Jupiter, en route to Saturn. During this excursion into the Jovian magnetosphere, the Cassini Magnetosphere Imaging Instrument/Charge-Energy-Mass Spectrometer detected oxygen and sulfur ions. While Charge-Energy-Mass Spectrometer can distinguish between oxygen and sulfur charge …

2019 Geophysical Research Letters
Cassini 13