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Global Distribution and Seasonality of Martian Atmospheric HCl Explained Through Heterogeneous Chemistry
DOI: 10.1029/2024GL111059 Bibcode: 2025GeoRL..5211059S

Trokhimovskiy, Alexander; Korablev, Oleg; Olsen, Kevin S. +4 more

Recent observations from the ExoMars Trace Gas Orbiter (TGO) have revealed the presence of hydrogen chloride (HCl) in the martian atmosphere. HCl shows strong seasonality, primarily appearing during Mars' perihelion period before decreasing faster than projected from photolysis and gas-phase chemistry. HCl profiles also display local anti-correlat…

2025 Geophysical Research Letters
ExoMars-16 1
Statistical Study of Electric Pc5 Pulsations in the Inner Magnetosphere Observed by Cluster
DOI: 10.1029/2024GL112358 Bibcode: 2025GeoRL..5212358Y

Li, Xinlin; Liu, Wenlong; Zhang, Dianjun +3 more

Ultra-low frequency (ULF) waves in the Pc5 band are essential for the transport of electrons in the radiation belt and the transport of energy from the solar wind into the magnetosphere. Based on ∼14-year of electric field data from Cluster satellite, the spatial distributions of power spectral densities (PSD) of electric field ULF waves in the in…

2025 Geophysical Research Letters
Cluster 0
A Case Study on the Impact of Interplanetary Coronal Mass Ejection on the Martian O(1S) 557.7 nm Dayglow Emission Using ExoMars TGO/NOMAD-UVIS Observations: First Results
DOI: 10.1029/2024GL111745 Bibcode: 2025GeoRL..5211745S

Vandaele, Ann Carine; Gérard, Jean-Claude; Thomas, Ian R. +6 more

We report, for the first time, the impact of interplanetary coronal mass ejections (ICME) on the recently discovered O(1S) 557.7 nm dayglow emission in the Martian atmosphere. While there are a few studies on the seasonal variation of 557.7 nm dayglow emission available in the literature, the impact of ICME has not been investigated so …

2025 Geophysical Research Letters
ExoMars-16 0
Evidence of Ice-Rich Layered Deposits in the Medusae Fossae Formation of Mars
DOI: 10.1029/2023GL105490 Bibcode: 2024GeoRL..5105490W

Orosei, Roberto; Plaut, Jeffrey J.; Campbell, Bruce A. +4 more

Subsurface reflectors in radar sounder data from the Mars Advanced Radar for Subsurface and Ionospheric Sounding instrument aboard the Mars Express spacecraft indicate significant dielectric contrasts between layers in the Martian Medusae Fossae Formation (MFF). Large density changes that create dielectric contrasts are less likely in deposits of …

2024 Geophysical Research Letters
MEx 6
Do Solar Energetic Particle (SEP) Events Influence the Formation of the V0 Layer in the Venusian Ionosphere?
DOI: 10.1029/2024GL109724 Bibcode: 2024GeoRL..5109724T

Choudhary, R. K.; Imamura, T.; Sánchez-Cano, Beatriz +2 more

This study investigates the potential impact of Solar Energetic Particles (SEPs) on the V0 layer of the Venus ionosphere. Electron density profiles obtained from radio occultation experiments conducted by the Venus Express (VEX) and Akatsuki missions were utilized for this purpose. Background data from the Analyzer of Space Plasma and E…

2024 Geophysical Research Letters
VenusExpress 1
Ion-Acoustic Waves Associated With Interplanetary Shocks
DOI: 10.1029/2024GL109956 Bibcode: 2024GeoRL..5109956B

Fedorov, A.; André, M.; Maksimovic, M. +10 more

Ion-acoustic waves (IAWs) commonly occur near interplanetary (IP) shocks. These waves are important because of their potential role in the dissipation required for collisionless shocks to exist. We study IAW occurrence statistically at different heliocentric distances using Solar Orbiter to identify the processes responsible for IAW generation nea…

2024 Geophysical Research Letters
SolarOrbiter 1
Frequency Chirping of Electromagnetic Ion Cyclotron Waves in Earth's Magnetosphere
DOI: 10.1029/2023GL106456 Bibcode: 2024GeoRL..5106456A

An, Zeyu; Tao, Xin; Zonca, Fulvio +1 more

Electromagnetic ion cyclotron (EMIC) waves are known to exhibit frequency chirping occasionally, contributing to the rapid acceleration and precipitation of energetic particles in the magnetosphere. However, the chirping mechanism of EMIC waves remains elusive. In this work, a phenomenological model of whistler mode chorus waves named the Trap-Rel…

2024 Geophysical Research Letters
Cluster 1
Revising the Basal Permittivity of the South Polar Layered Deposits of Mars With a Surficial Dust Cover
DOI: 10.1029/2024GL109085 Bibcode: 2024GeoRL..5109085G

Kofman, W.; Hérique, A.; Grima, C. +1 more

Bright basal reflections from the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) have been proposed to be consistent with permittivities characteristic of a wet material beneath the south polar layered deposits (SPLD). The characterization of a recently formed impact crater highlight the existence of a several meters thick ice…

2024 Geophysical Research Letters
MEx 1
Latitudinal Mapping of Chorus Waves Growth Rates Based on Multi-Spacecraft Wave and Plasma Measurements
DOI: 10.1029/2024GL110539 Bibcode: 2024GeoRL..5110539V

Agapitov, O. V.; Artemyev, A.; Mourenas, D. +3 more

Whistler mode chorus waves are one of the most intense and important electromagnetic emissions in the Earth's radiation belt, where these waves are responsible for electron acceleration to relativistic energies and for energetic electron precipitation into the Earth's atmosphere. This study reports a unique multi-spacecraft observation event that …

2024 Geophysical Research Letters
Cluster 1
Strong Localized Pumping of Water Vapor to High Altitudes on Mars During the Perihelion Season
DOI: 10.1029/2023GL107224 Bibcode: 2024GeoRL..5107224B

Aoki, S.; Vandaele, A. C.; Daerden, F. +18 more

Here we present water vapor vertical profiles observed with the ExoMars Trace Gas Orbiter/Nadir and Occultation for MArs Discovery instrument during the perihelion and Southern summer solstice season (LS = 240°-300°) in three consecutive Martian Years 34, 35, and 36. We show the detailed latitudinal distribution of H2O at tan…

2024 Geophysical Research Letters
ExoMars-16 0