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Radar Sounding of Subsurface Structure in Eastern Coprates and Capri Chasmata, Mars
DOI: 10.1029/2020GL088556 Bibcode: 2020GeoRL..4788556N

Kasaba, Yasumasa; Kumamoto, Atsushi; Oura, Aina +5 more

We surveyed the subsurface structure in eastern Coprates and Capri Chasmata in the equatorial region using high-resolution visible images, digital terrain models, and radar sounding data. We identified subsurface reflectors in four areas of the chasmata. At the stratigraphic exposure on the chasmata walls, the corresponding depth of the reflector …

2020 Geophysical Research Letters
MEx 2
High-Spatiotemporal Resolution Observations of Jupiter Lightning-Induced Radio Pulses Associated With Sferics and Thunderstorms
DOI: 10.1029/2020GL088397 Bibcode: 2020GeoRL..4788397I

Wong, Michael H.; Bolton, Scott J.; Levin, Steven M. +6 more

Jupiter lightning discharges produce various kinds of phenomena including radio wave pulses at different frequencies. On 6 April 2019, the Juno Waves instrument captured an extraordinary series of radio pulses at frequencies below 150 kHz on timescales of submilliseconds. Quasi-simultaneous multi-instrument data show that the locations of their ma…

2020 Geophysical Research Letters
eHST 2
Saturn's Deep Atmospheric Flows Revealed by the Cassini Grand Finale Gravity Measurements
DOI: 10.1029/2018GL078087 Bibcode: 2019GeoRL..46..616G

Iess, L.; Guillot, T.; Miguel, Y. +4 more

How deep do Saturn's zonal winds penetrate below the cloud level has been a decades-long question, with important implications not only for the atmospheric dynamics but also for the interior density structure, composition, magnetic field, and core mass. The Cassini Grand Finale gravity experiment enables answering this question for the first time,…

2019 Geophysical Research Letters
Cassini 72
Energy Range of Electron Rolling Pin Distribution Behind Dipolarization Front
DOI: 10.1029/2019GL082100 Bibcode: 2019GeoRL..46.2390Z

Xu, Y.; Fu, H. S.; Burch, J. L. +4 more

The electron rolling pin distribution, showing electron pitch angles primarily at 0°, 90°, and 180°, has recently been observed behind dipolarization fronts (DFs) and explained using an analytical model. However, the energy range of such distribution has been unknown so far, owing to the low-resolution data in previous spacecraft missions. Here us…

2019 Geophysical Research Letters
Cluster 54
The Onset and Growth of the 2018 Martian Global Dust Storm
DOI: 10.1029/2019GL083207 Bibcode: 2019GeoRL..46.6101S

Sánchez-Lavega, A.; Delcroix, M.; Hernández-Bernal, J. +1 more

We analyze the onset and initial expansion of the 2018 Martian Global Dust Storm (GDS 2018) using ground-based images in the visual range. This is the first case of a confirmed GDS initiating in the Northern Hemisphere. A dusty area extending about 1.4×105 km2 and centered at latitude +31.7°±1.8° and west longitude 18°±5°W in…

2019 Geophysical Research Letters
MEx 52
Effects of Ducting on Whistler Mode Chorus or Exohiss in the Outer Radiation Belt
DOI: 10.1029/2019GL083115 Bibcode: 2019GeoRL..46.5735H

Hanzelka, Miroslav; Santolík, Ondřej

Previously published statistics based on Cluster spacecraft measurements surprisingly show that in the outer radiation belt, lower band whistler mode waves predominantly propagate unattenuated parallel to the magnetic field lines up to midlatitudes, where ray tracing simulations indicated highly attenuated waves with oblique wave vectors. We expla…

2019 Geophysical Research Letters
Cluster 42
Detection of Rotational Acceleration of Bennu Using HST Light Curve Observations
DOI: 10.1029/2018GL080658 Bibcode: 2019GeoRL..46.1956N

Emery, J. P.; Chesley, S. R.; Noll, K. S. +7 more

We observed the near-Earth asteroid (101955) Bennu from the ground in 1999 and 2005, and with the Hubble Space Telescope (HST) in 2012, to constrain its rotation rate. The data reveal an acceleration of 2.64 ± 1.05 × 10-6 deg/day2, which could be due to a change in the moment of inertia of Bennu or to spin up from the Yarkovs…

2019 Geophysical Research Letters
eHST 37
Plasma Pressures in the Heliosheath From Cassini ENA and Voyager 2 Measurements: Validation by the Voyager 2 Heliopause Crossing
DOI: 10.1029/2019GL083924 Bibcode: 2019GeoRL..46.7911D

Krimigis, Stamatios M.; Mitchell, Donald G.; Dialynas, Konstantinos +1 more

We report "ground truth," 28- to 3,500-keV in situ ion and 5.2- to 55-keV remotely sensed ENA measurements from Voyager 2/Low Energy Charged Particle detector and Cassini/Ion and Neutral Camera, respectively, that assess the components of the ion pressure in the heliosheath. In this process, we predict an interstellar neutral hydrogen density of ∼…

2019 Geophysical Research Letters
Cassini 35
Multispacecraft Analysis of Electron Holes
DOI: 10.1029/2018GL080757 Bibcode: 2019GeoRL..46...55S

Russell, C. T.; Vaivads, A.; Khotyaintsev, Yu. V. +4 more

Electron holes (EHs) are nonlinear electrostatic structures in plasmas. Most previous in situ studies of EHs have been limited to single- and two-spacecraft methods. We present statistics of EHs observed by Magnetospheric Multiscale on the magnetospheric side of the magnetopause during October 2016 when the spacecraft separation was around 6 km. E…

2019 Geophysical Research Letters
Cluster 33
Combined Scattering of Radiation Belt Electrons Caused by Landau and Bounce Resonant Interactions With Magnetosonic Waves
DOI: 10.1029/2019GL084438 Bibcode: 2019GeoRL..4610313F

Fu, Song; Ni, Binbin; Gu, Xudong +2 more

We develop a full relativistic test particle code to model the combined electron scattering effect of Landau and bounce resonances with magnetosonic waves. Test particle simulations of magnetosonic wave-electron interactions indicate that the two resonances coexist to affect radiation belt electrons at different energies and pitch angles, and the …

2019 Geophysical Research Letters
Cluster 32