Efficient Surface Conversion for Neutral Atom Detection*

Astronomy and Astrophysics – Astrophysics

Scientific paper

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7594 Instruments And Techniques

Scientific paper

Neutral atom detection is a useful way of studying astrophysical plasma structures. When plasma ions undergo charge exchange with the neutral background gas, energetic neutral atoms (ENAs) are generated. These neutral atoms travel in straight lines from the point of charge exchange because they are not subject to deflection by the electric and magnetic fields in space and as a result ENAs can be used to image the plasma structures from which they originate. ENAs in the energy range from .01 to 1.5 keV are particularly worth studying and are best detected by their conversion to negative ions at a surface, a method that is being used in the IMAGE** spacecraft's low energy neutral atom (LENA) imager. While the results from LENA are contributing to knowledge of the Earth's magnetosphere, the low efficiency (<1%) limits temporal and spatial resolution. In order to improve the efficiency of conversion, we have begun detailed studies of the properties of a variety of surfaces and have correlated surface properties with conversion efficiencies. The surfaces studied so far are tungsten, highly oriented pyrolytic graphite (HOPG), diamond-like carbon and secondary electron emitting glasses. XPS spectra and work function for clean samples and samples exposed to the atmosphere have been taken. The results have been compared with measured conversion efficiencies. For the tungsten surfaces, it appears that adsorbates play an important role in conversion efficiency. This has implications for the sensitivity and stability of neutral atom imagers. *T.E. Moore, et. al., Space Sci. Rev. 91, 155 (2000). ** Work supported in part by NASA grant ACT-05-0040

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