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Jupiter's X-Ray and UV Dark Polar Region
DOI: 10.1029/2021GL097390 Bibcode: 2022GeoRL..4997390D

Jackman, C. M.; Johnson, R. E.; Branduardi-Raymont, G. +16 more

We present 14 simultaneous Chandra X-ray Observatory (CXO)-Hubble Space Telescope (HST) observations of Jupiter's Northern X-ray and ultraviolet (UV) aurorae from 2016 to 2019. Despite the variety of dynamic UV and X-ray auroral structures, one region is conspicuous by its persistent absence of emission: the dark polar region (DPR). Previous HST o…

2022 Geophysical Research Letters
eHST 6
Evidence of Alfvén Waves Generated by Mode Coupling in the Magnetotail Lobe
DOI: 10.1029/2021GL096359 Bibcode: 2022GeoRL..4996359S

Zhang, Tielong; Sun, Jicheng; Wang, Guoqiang +2 more

Mode coupling is an important mechanism to excite Alfvén waves and has been extensively investigated based on numerical simulations. However, no direct observational evidence has been found regarding to this mechanism in the magnetotail lobe. Here, we report an in-situ observation that an Alfvén wave with a period of several minutes is clearly rel…

2022 Geophysical Research Letters
Cluster 6
Tracking the Evolution of an Ocean Within Mimas Using the Herschel Impact Basin
DOI: 10.1029/2022GL100516 Bibcode: 2022GeoRL..4900516D

Rhoden, A. R.; Denton, C. A.

Mimas' small size, lack of geologic activity, and high eccentricity suggest a frozen, inactive history. However, Cassini libration measurements are best explained by a present-day liquid ocean under an ice shell 24-31 km thick, a configuration that tidal heating can support. These unexpected findings have motivated further study of Mimas' surface …

2022 Geophysical Research Letters
Cassini 6
BepiColombo Mio Observations of Low-Energy Ions During the First Mercury Flyby: Initial Results
DOI: 10.1029/2022GL100279 Bibcode: 2022GeoRL..4900279H

Persson, Moa; Saito, Yoshifumi; Delcourt, Dominique +14 more

We present initial results of low-energy ion observations from BepiColombo's first Mercury flyby. Unprecedentedly high time resolution measurements of low energy ions at Mercury by BepiColombo Mio reveal rapid (a few seconds) and large (1-2 orders of magnitude) fluctuations of ion flux around the magnetopause and within the magnetosphere. Around t…

2022 Geophysical Research Letters
BepiColombo 5
Paleolake Inlet Valley Formation: Factors Controlling Which Craters Breached on Early Mars
DOI: 10.1029/2022GL101097 Bibcode: 2022GeoRL..4901097B

Fassett, C. I.; Bamber, Emily R.; Goudge, T. A. +2 more

The ancient surface of Mars is dominated by degraded impact craters with reduced or eliminated rim relief. Some degraded craters have an inlet valley, while many remain fluvially isolated. Despite controlling Martian fluvial connectivity, few constraints exist on why some—but not all—degraded craters possess inlets. We compared a suite of properti…

2022 Geophysical Research Letters
MEx 5
Saturn Anomalous Myriametric Radiation, a New Type of Saturn Radio Emission Revealed by Cassini
DOI: 10.1029/2022GL099237 Bibcode: 2022GeoRL..4999237W

Jackman, C. M.; Kurth, W. S.; Cecconi, B. +10 more

A new radio component namely Saturn Anomalous Myriametric Radiation (SAM) is reported. A total of 193 SAM events have been identified by using all the Cassini Saturn orbital data. SAM emissions are L-O mode radio emission and occasionally accompanied by a first harmonic in R-X mode. SAM's intensities decrease with increasing distance from Saturn, …

2022 Geophysical Research Letters
Cassini 4
In Situ Observation of a Magnetopause Indentation that Is Correspondent to Throat Aurora and Is Caused by Magnetopause Reconnection
DOI: 10.1029/2022GL099408 Bibcode: 2022GeoRL..4999408Q

Shi, Run; Li, Bin; Zhou, Su +6 more

Throat auroras have been suggested to correspond to magnetopause indentations, but how such indentations can be generated is an open question. Using coordinated magnetopause in situ and two-dimensional auroral imaging observations, we showed that a transient magnetopause crossing observed by Time History of Events and Macroscale Interactions durin…

2022 Geophysical Research Letters
Cluster 4
Geologic Context of the Bright MARSIS Reflectors in Ultimi Scopuli, South Polar Layered Deposits, Mars
DOI: 10.1029/2022GL098724 Bibcode: 2022GeoRL..4998724L

Landis, M. E.; Whitten, J. L.

Radar-bright basal reflectors have been detected below the South Polar Layered Deposits (SPLD), using Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) data and have an exciting but controversial interpretation: liquid water from subglacial lakes. We mapped the surface of the SPLD immediately above and surrounding the putative la…

2022 Geophysical Research Letters
MEx 3
MAVEN Proton Observations Near the Martian Moon Phobos: Does Phobos Backscatter Solar Wind Protons?
DOI: 10.1029/2022GL101014 Bibcode: 2022GeoRL..4901014D

André, N.; Halekas, J. S.; Fowler, C. M. +7 more

ESA's Mars Express (MEX) may have observed twice solar wind protons backscattered by Phobos. However, these detections remain uncertain and call for an independent confirmation. Here, we analyze the proton measurements collected by the Suprathermal And Thermal Ion Composition experiment onboard NASA's Mars Atmosphere and Volatile EvolutioN mission…

2022 Geophysical Research Letters
MEx 1
Observations of Modulation of Ion Flux in the Coma of Comet 67P/Churyumov-Gerasimenko
DOI: 10.1029/2022GL098042 Bibcode: 2022GeoRL..4998042G

Altwegg, K.; Nilsson, H.; Goldstein, R. +4 more

On 6-8 June 2015, the Ion and Electron Sensor on board Rosetta observed keV-range water-group pickup ions arriving from the solar direction. Based on magnetic field intensification and variations, the appearance of the ions was likely to have been caused by a coronal mass ejection. During the 3-day period when Rosetta was 200 km from the comet, pe…

2022 Geophysical Research Letters
Rosetta 0