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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
Current Sheet Thinning in the Wake of a Bubble Injection
DOI: 10.1029/2022GL100737 Bibcode: 2022GeoRL..4900737W

Nakamura, Rumi; Yang, Jian; Cui, Jun +3 more

A crucial property of the substorm growth phase is the current sheet thinning, which is often attributed to adiabatic convection. Injecting low-entropy bubbles reduce pressure-balance inconsistencies and restore current sheet thickness to its initial value. Recent observations from Cluster and MMS showed additional thinning of the current sheet in…

2022 Geophysical Research Letters
Cluster 0
Evidence of Small Scale Plasma Irregularity Effects on Whistler Mode Chorus Propagation
DOI: 10.1029/2021GL092850 Bibcode: 2021GeoRL..4892850H

Agapitov, Oleksiy; Hosseini, Poorya; Harid, Vijay +1 more

The impact of randomly distributed field aligned density irregularities on whistler mode wave propagation is investigated using full wave simulations and multipoint spacecraft observations. The irregularities are modeled as randomized density perturbations between 1% and 10% of the nominal background density value with scales of ∼10-60 km transver…

2021 Geophysical Research Letters
Cluster 32
Revealing a High Water Abundance in the Upper Mesosphere of Mars With ACS Onboard TGO
DOI: 10.1029/2021GL093411 Bibcode: 2021GeoRL..4893411B

Montmessin, Franck; Belyaev, Denis A.; Fedorova, Anna A. +7 more

We present the first water vapor profiles encompassing the upper mesosphere of Mars, 100-120 km, far exceeding the maximum altitudes where remote sensing has been able to observe water to date. Our results are based on solar occultation measurements by Atmospheric Chemistry Suite (ACS) onboard the ExoMars Trace Gas Orbiter (TGO). The observed wave…

2021 Geophysical Research Letters
ExoMars-16 31
Strong MARSIS Radar Reflections From the Base of Martian South Polar Cap May Be Due to Conductive Ice or Minerals
DOI: 10.1029/2021GL093880 Bibcode: 2021GeoRL..4893880B

Putzig, N. E.; Bierson, C. J.; Tulaczyk, S. +1 more

Recent results from the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) instrument have been interpreted as evidence of subsurface brine pooled beneath 1.3 km-thick South Polar Layered Deposit (SPLD). This interpretation is based on the assumption that the regionally high strength of MARSIS radar reflections from the base of th…

2021 Geophysical Research Letters
MEx 30
A Solid Interpretation of Bright Radar Reflectors Under the Mars South Polar Ice
DOI: 10.1029/2021GL093618 Bibcode: 2021GeoRL..4893618S

Smith, I. B.; Horgan, B. H. N.; Whitten, J. L. +4 more

Bright radar reflections observed beneath the south polar layered deposits (SPLD) by the Mars Advanced Radar for Subsurface and Ionosphere Sounding instrument were interpreted to represent liquid water, but the required amounts of salt and heat to form and maintain liquids in this location are implausible given what is known about Mars. Here, we p…

2021 Geophysical Research Letters
MEx 29
A Stable H2O Atmosphere on Europa's Trailing Hemisphere From HST Images
DOI: 10.1029/2021GL094289 Bibcode: 2021GeoRL..4894289R

Roth, Lorenz

Previous studies of the global intensities of the oxygen emissions at 1,356 Å and 1,304 Å revealed molecular oxygen (O2) in Europa's atmosphere. Here we investigate the relative changes of the two oxygen emissions when Europa emerges from eclipse as well as the radial profiles of the relative emissions across the sunlit disk in Hubble S…

2021 Geophysical Research Letters
eHST 27