2009
DOI: 10.2322/tstj.7.pk_1
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Development of the High-resolution FUV Detector for the BepiColombo Mission

Abstract: The PHEBUS (Probing of Hermean Exosphere By Ultraviolet Spectroscopy) instrument on Mercury Planetary Orbiter in the BepiColombo mission is a dual FUV-EUV spectrometer (EUV: 55-155 nm, FUV: 145-315 nm). We are now developing the compact detector system sensitive to FUV airglow emissions of the Mercury. The FUV detector is required to have high spatial resolution (512×512 pixels) so that the wavelength resolution of the PHEBUS instrument should be 2 nm at the FUV range. The FUV detector consists of a Cs2Te phot… Show more

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Cited by 2 publications
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“…The detector unit consists of five‐stage microchannel plates and a resistive anode. It is identical to the Far Ultraviolet (FUV) detector unit in the Probing of Hermean Exosphere by Ultraviolet Spectroscopy (PHEBUS) instrument on the Mercury Planetary Orbiter as part of the BepiColombo mission (Murakami et al, ), except for the photocathode material. The detector plane of LAICA includes a CsI photocathode whereas PHEBUS/FUV has a Cs 2 Te photocathode.…”
Section: Instrumentation and Observationsmentioning
confidence: 99%
“…The detector unit consists of five‐stage microchannel plates and a resistive anode. It is identical to the Far Ultraviolet (FUV) detector unit in the Probing of Hermean Exosphere by Ultraviolet Spectroscopy (PHEBUS) instrument on the Mercury Planetary Orbiter as part of the BepiColombo mission (Murakami et al, ), except for the photocathode material. The detector plane of LAICA includes a CsI photocathode whereas PHEBUS/FUV has a Cs 2 Te photocathode.…”
Section: Instrumentation and Observationsmentioning
confidence: 99%