Paper
29 August 2017 Microchannel plate life testing for UV spectroscopy instruments
N. T. Darling, O. H. W. Siegmund, T. Curtis, J. McPhate, J. Tedesco, S. Courtade, G. Holsclaw, A. Hoskins, S. Al Dhafri
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Abstract
The Emirates Mars Mission (EMM) UV Spectrograph (EMUS) is a far ultraviolet (102 nm to 170 nm) imaging spectrograph for characterization of the Martian exosphere and thermosphere. Imaging is accomplished by a photon counting open-face microchannel plate (MCP) detector using a cross delay line (XDL) readout. An MCP gain stabilization (“scrub”) followed by lifetime spectral line burn-in simulation has been completed on a bare MCP detector at SSL. Gain and sensitivity stability of better than 7% has been demonstrated for total dose of 2.5 × 1012 photons cm−2 (2 C · cm−2 ) at 5.5 kHz mm−2 counting rates, validating the efficacy of an initial low gain full-field scrub.
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N. T. Darling, O. H. W. Siegmund, T. Curtis, J. McPhate, J. Tedesco, S. Courtade, G. Holsclaw, A. Hoskins, and S. Al Dhafri "Microchannel plate life testing for UV spectroscopy instruments", Proc. SPIE 10397, UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XX, 1039712 (29 August 2017); https://doi.org/10.1117/12.2277343
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KEYWORDS
Microchannel plates

Spectrographs

Mars

Ultraviolet radiation

Exosphere

Far ultraviolet

Photon counting

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