The ionosphere of Mars after 20 years of Mars Express contributions
K Peter, B Sánchez-Cano, F Němec… - Space Science …, 2024 - Springer
The Martian ionosphere originates from the ionization of the planetary neutral atmosphere
by solar radiation. This conductive layer is embedded within the thermosphere and …
by solar radiation. This conductive layer is embedded within the thermosphere and …
The twisted configuration of the Martian magnetotail: MAVEN observations
Measurements provided by the Mars Atmosphere and Volatile EvolutioN (MAVEN)
spacecraft are analyzed to investigate the Martian magnetotail configuration as a function of …
spacecraft are analyzed to investigate the Martian magnetotail configuration as a function of …
Discrete aurora on Mars: Insights into their distribution and activity from MAVEN/IUVS observations
NM Schneider, Z Milby, SK Jain… - Journal of …, 2021 - Wiley Online Library
Abstract Mars Atmosphere and Volatile Evolution (MAVEN)'s Imaging Ultraviolet
Spectrograph has identified 278 occurrences of discrete aurora events on Mars, which are …
Spectrograph has identified 278 occurrences of discrete aurora events on Mars, which are …
A technique to infer magnetic topology at Mars and its application to the terminator region
Magnetic topology is important for understanding the Martian plasma environment, including
particle precipitation, energy transport, cold ion escape, and wave‐particle interaction. In this …
particle precipitation, energy transport, cold ion escape, and wave‐particle interaction. In this …
A statistical investigation of factors influencing the magnetotail twist at Mars
The Martian magnetotail exhibits a highly twisted configuration, shifting in response to
changes in polarity of the interplanetary magnetic field's (IMF) dawn‐dusk (BY) component …
changes in polarity of the interplanetary magnetic field's (IMF) dawn‐dusk (BY) component …
MAVEN observations of magnetic reconnection at Martian induced magnetopause
The Martian‐induced magnetopause (IMP), characterized by the sudden changes of
magnetic fields and ion compositions, is the transition boundary separating the …
magnetic fields and ion compositions, is the transition boundary separating the …
Evidence for magnetic reconnection as the precursor to discrete aurora at mars
Discrete aurora at Mars are characterized as localized, short‐lasting ultraviolet emissions on
the nightside. They are caused by the precipitation of accelerated electron along open …
the nightside. They are caused by the precipitation of accelerated electron along open …
The effect of solar wind variations on the escape of oxygen ions from Mars through different channels: MAVEN observations
E Dubinin, M Fraenz, M Pätzold… - Journal of …, 2017 - Wiley Online Library
We present multi‐instrument observations of the effects of solar wind on ion escape fluxes
on Mars based on the Mars Atmosphere and Volatile EvolutioN (MAVEN) data from 1 …
on Mars based on the Mars Atmosphere and Volatile EvolutioN (MAVEN) data from 1 …
MAVEN observations of periodic low-altitude plasma clouds at Mars
Ion escape to space through the interaction of solar wind and Mars is an important factor
influencing the evolution of the Martian atmosphere. The plasma clouds (explosive bulk …
influencing the evolution of the Martian atmosphere. The plasma clouds (explosive bulk …
The morphology of the topside Martian ionosphere: Implications on bulk ion flow
Abstract Prior to the Mars Atmosphere and Volatile Evolution mission, the only information
on the composition of the Martian ionosphere came from the Viking Retarding Potential …
on the composition of the Martian ionosphere came from the Viking Retarding Potential …