AbstractThere is much evidence to show that lunar “horizon glow” and “streamers” observed at the terminator are caused by sunlight scattered by dust grains originating from the surface. The dust grains and lunar surface are electrostatically charged by the Moon’s interaction with the local plasma environment and the photoemission of electrons due to solar UV and X-rays. This effect causes the like-charged surface and dust particles to repel each other, and creates a near-surface electric field. Previous models have explained micron-sized dust observed at ∼10cm above the surface, by suggesting that charged grains “levitate” in the local electric field; however this cannot account for observations of 0.1μm-scale grains at ∼100 km altitude. In order to explain the high-altitude dust observations, we propose a dynamic “fountain” model in which charged dust grains follow ballistic trajectories, subsequent to being accelerated upward through a narrow sheath region by the surface electric field. These dust grains could affect the optical quality of the lunar environment for astronomical observations and interfere with exploration activities.


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    Titel :

    A dynamic fountain model for lunar dust


    Beteiligte:

    Erschienen in:

    Erscheinungsdatum :

    2005-04-14


    Format / Umfang :

    8 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




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