Coordinated MAVEN/IUVS and EMM/EMUS observations show the May 2024 ICME produced a planet-wide enhancement of Martian UV dayglow via simultaneous proton and electron precipitation.
and Stevens, M.H., 2018
3 Pith papers cite this work, alongside 543 external citations. Polarity classification is still indexing.
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Statistical multipoint observations indicate ICME shock acceleration efficiency increases with heliocentric distance up to 0.7 AU before decreasing.
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Impact of May 2024 ICME Event on Martian UV Dayglow Emissions using MAVEN/IUVS and EMM/EMUS Observations
Coordinated MAVEN/IUVS and EMM/EMUS observations show the May 2024 ICME produced a planet-wide enhancement of Martian UV dayglow via simultaneous proton and electron precipitation.
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Radial Dependency of ICME-associated Particle Acceleration Processes: Statistical Multipoint Observations from 2016-2023
Statistical multipoint observations indicate ICME shock acceleration efficiency increases with heliocentric distance up to 0.7 AU before decreasing.
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Automated Classification of Plasma Regions at Mars Using Machine Learning
A convolutional neural network trained on MAVEN SWIA ion spectra reliably classifies solar wind, magnetosheath, and induced magnetosphere regions at Mars, outperforming a multilayer perceptron.