Using ARTEMIS pickup ion observations to place constraints on the lunar atmosphere

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Using ARTEMIS pickup ion observations to place constraints on the lunar atmosphere

[1] We present a method for deriving constraints on the structure and composition of the lunar atmosphere by using pickup ion measurements from ARTEMIS, mapping observed fluxes from the spacecraft location to derive production rates at the source region, and fitting to a parameterized neutral atmosphere model. We apply this technique to ~12min of high-resolution burst data collected by ARTEMIS ...

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ARTEMIS observations of lunar pickup ions: Mass constraints on ion species

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Model-based constraints on the lunar exosphere derived from ARTEMIS pickup ion observations in the terrestrial magnetotail

[1] We use Acceleration, Reconnection, Turbulence and Electrodynamics of the Moon’s Interaction with the Sun (ARTEMIS) measurements of lunar exospheric pickup ions in the terrestrial magnetotail lobes combined with a particle-tracing model to constrain the source species and distributions of the lunar neutral exosphere. These pickup ions, generated by photoionization of neutral species while th...

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Lunar pickup ions observed by ARTEMIS: Spatial and temporal distribution and constraints on species and source locations

[1] ARTEMIS observes pickup ions around the Moon, at distances of up to 20,000 km from the surface. The observed ions form a plume with a narrow spatial and angular extent, generally seen in a single energy/angle bin of the ESA instrument. Though ARTEMIS has no mass resolution capability, we can utilize the analytically describable characteristics of pickup ion trajectories to constrain the pos...

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ژورنال

عنوان ژورنال: Journal of Geophysical Research: Planets

سال: 2013

ISSN: 2169-9097

DOI: 10.1029/2012je004292