Lunar Photoemission Studies with a Xe Excimer UV Lamp

Physics – Plasma Physics

Scientific paper

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[6250] Planetary Sciences: Solar System Objects / Moon, [7831] Space Plasma Physics / Laboratory Studies And Experimental Techniques, [7849] Space Plasma Physics / Plasma Interactions With Dust And Aerosols

Scientific paper

The most populous species immediately above the lunar surface is the photoelectron gas. Measurements of a photoelectron sheath in the laboratory have been hindered by the lack of a sufficiently strong UV source to create an electron gas with large enough density to behave as plasma. We have evaluated the newly-developed Xe excimer lamp (Osram Xeradex) for creation of a photoelectron layer that is sufficiently dense to have a Debye shielding length that is of order 0.1 m. The measured photoemission from a Pt surface (quantum efficiency 1.0 x 10-3) is 0.01 A/m2 at a distance of 10 cm which corresponds to a UV photon flux (at 170 nm) of 6 x 1019 m-2s-1. The electron density above the illuminated metal surface is of order 1011 m-3 and the corresponding shielding length is 0.04 m. This photoelectron density is sufficient for studies of a photoelectron sheath. The quantum efficiency of lunar soil is about an order of magnitude smaller than that of Pt, which increases the shielding distance by about a factor of three. A new experimental configuration is under construction in which an array of nine lamps will illuminate a surface with simulated lunar soil and with prototype instruments for detecting and analyzing the lunar photoelectron gas and associated electric fields.

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