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Extremely high reflection of solar wind protons as neutral hydrogen atoms from regolith in space

机译:太阳风质子的极高反射是太空中再凝结的中性氢原子

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We report on measurements of extremely high reflection rates of solar wind particles from regolith-covered lunar surfaces. Measurements by the Sub-keV Atom Reflecting Analyzer (SARA) instrument on the Indian Chandrayaan-1 spacecraft in orbit around the Moon show that up to 20% of the impinging solar wind protons are reflected from the lunar surface back to space as neutral hydrogen atoms. This finding, generally applicable to regolith-covered atmosphereless bodies, invalidates the widely accepted assumption that regolith almost completely absorbs the impinging solar wind.
机译:我们报告了来自被白云石覆盖的月球表面的太阳风粒子的极高反射率的测量结果。用Sub-keV原子反射分析仪(SARA)在印度绕月轨道的Chandrayaan-1航天器上进行的测量表明,撞击的太阳风质子中有多达20%作为中性氢原子从月球表面反射回太空。 。这一发现通常适用于覆盖有粉煤灰的无气天体,这使广为接受的关于粉煤灰几乎完全吸收了撞击的太阳风的假设无效。

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