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Measuring pickup ions to characterize the surfaces and exospheres of planetary bodies: Applications to the Moon

机译:测量拾取离子以表征行星体的表面和系外层:对月球的应用

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[1] The composition and structure of neutral exospheres imbedded in the solar wind can be determined by measurements of their pickup ion progeny. Using Earth's Moon as the parent body, we consider transport of pickup ions from their birthplaces to measurement sites on possible spacecraft orbits. An ion observed to have a specific mass and velocity at a spacecraft position can be mapped back to its point of birth on the surface or in the atmosphere. Ion measurements of this type are shown to be a sensitive way to map the composition of surfaces and atmospheres of bodies with surface bound exospheres.
机译:[1]埋在太阳风中的中性圈外层的组成和结构可以通过测量它们的吸收离子后代来确定。以地球的月球为母体,我们考虑了将拾取离子从其出生地传输到可能的航天器轨道上的测量位置。可以将观察到在航天器位置具有特定质量和速度的离子映射回其在表面或大气中的出生点。这种类型的离子测量显示出一种灵敏的方法,可以绘制带有表面束缚外球的物体的表面和大气成分。

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