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The Mars Atmosphere and Volatile Evolution (MAVEN) Mission
The MAVEN spacecraft launched in November 2013, arrived at Mars in September 2014,
and completed commissioning and began its one-Earth-year primary science mission in …
and completed commissioning and began its one-Earth-year primary science mission in …
The MAVEN magnetic field investigation
The MAVEN magnetic field investigation is part of a comprehensive particles and fields
subsystem that will measure the magnetic and electric fields and plasma environment of …
subsystem that will measure the magnetic and electric fields and plasma environment of …
The MAVEN solar wind electron analyzer
Abstract The MAVEN Solar Wind Electron Analyzer (SWEA) is a symmetric hemispheric
electrostatic analyzer with deflectors that is designed to measure the energy and angular …
electrostatic analyzer with deflectors that is designed to measure the energy and angular …
MAVEN suprathermal and thermal ion compostion (STATIC) instrument
Abstract The MAVEN SupraThermal And Thermal Ion Compostion (STATIC) instrument is
designed to measure the ion composition and distribution function of the cold Martian …
designed to measure the ion composition and distribution function of the cold Martian …
The solar wind ion analyzer for MAVEN
JS Halekas, ER Taylor, G Dalton, G Johnson… - Space Science …, 2015 - Springer
Abstract The Solar Wind Ion Analyzer (SWIA) on the MAVEN mission will measure the solar
wind ion flows around Mars, both in the upstream solar wind and in the magneto-sheath and …
wind ion flows around Mars, both in the upstream solar wind and in the magneto-sheath and …
The Langmuir probe and waves (LPW) instrument for MAVEN
We describe the sensors, the sensor biasing and control, the signal-processing unit, and the
operation of the Langmuir Probe and Waves (LPW) instrument on the Mars Atmosphere and …
operation of the Langmuir Probe and Waves (LPW) instrument on the Mars Atmosphere and …
Martian low‐altitude magnetic topology deduced from MAVEN/SWEA observations
Abstract The Mars Atmosphere and Volatile Evolution mission has obtained comprehensive
particle and magnetic field measurements. The Solar Wind Electron Analyzer provides …
particle and magnetic field measurements. The Solar Wind Electron Analyzer provides …
Ion energization and escape on Mars and Venus
Mars and Venus do not have a global magnetic field and as a result solar wind interacts
directly with their ionospheres and upper atmospheres. Neutral atoms ionized by solar UV …
directly with their ionospheres and upper atmospheres. Neutral atoms ionized by solar UV …
Electron pitch angle distributions as indicators of magnetic field topology near Mars
We have analyzed electron angular distributions recorded near Mars over a period of 7
years in order to constrain the topology of magnetic field lines near Mars. We used 63 million …
years in order to constrain the topology of magnetic field lines near Mars. We used 63 million …
Discovery of diffuse aurora on Mars
Planetary auroras reveal the complex interplay between an atmosphere and the
surrounding plasma environment. We report the discovery of low-altitude, diffuse auroras …
surrounding plasma environment. We report the discovery of low-altitude, diffuse auroras …