2015 IEEE Aerospace Conference 2015
DOI: 10.1109/aero.2015.7119017
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The Mass Analyzer for Real-time Investigation of Neutrals at Europa (MARINE)

Abstract: Abstract-Presented herein is the progress on developing a new mass analyzer for analysis of the exospheres of planets, moons, and primitive bodies, such as found at Europa or Enceladus.

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Cited by 6 publications
(8 citation statements)
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“…Its major advantage over other existing solutions is its high performance, making it a viable tool for investigating a range of experimental operating modes that are to be achieved under spaceflight conditions, such as those found, for example, in flyby studies of Europa's exosphere [38]. For a specific set of voltage scan functions, the developed numeric model is used to identify the accessible secular frequencies and to predict the stability of the rf-driven micromotion with respect to the location within the trapping volume.…”
Section: Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…Its major advantage over other existing solutions is its high performance, making it a viable tool for investigating a range of experimental operating modes that are to be achieved under spaceflight conditions, such as those found, for example, in flyby studies of Europa's exosphere [38]. For a specific set of voltage scan functions, the developed numeric model is used to identify the accessible secular frequencies and to predict the stability of the rf-driven micromotion with respect to the location within the trapping volume.…”
Section: Resultsmentioning
confidence: 99%
“…The PFK test gas was introduced directly into the trap placed within the ultra-high vacuum (UHV) chamber with the base pressure below 1 × 10 −11 Torr [38]. The ring electrode is driven at the ω rf /2π = 752.243 kHz frequency using the scan rate of 6667 Th/s.…”
Section: Dipole Excitationmentioning
confidence: 99%
“…S11 to S17 in the Supplementary Data provide additional results). This is important in the context of designing optimized molecular collectors in MS instruments, as described in Darrach et al (2015), where concentric angled conical collectors enable gas molecules to specularly reflect in a single collision before exiting through the instrument's aperture.…”
Section: Factors That Influence V Fmentioning
confidence: 99%
“…HVI can also cause postimpact chemistry, potentially confounding interpretation of the collected data. Mitigation or avoidance of these problems imposes strict constraints on mission parameters, in particular flyby velocities, as well as on instrument design choices geared to reduce fragmentation and postimpact chemical reactions from HVI (Darrach et al, 2015).…”
mentioning
confidence: 99%
“…To monitor time-variable planetary atmospheric processes a complete inventory of relevant chemical species at high sampling rates is required. The QIT-MS instrument has the necessary analytical power: 50 full-range (10-150 u) mass spectra per second at high sensitivity (7.5 × 10 11 cps/Pa), supplemented with on-demand high resolution (4000 at 32 u and 5000 at 136 u) mode of operation [17]. These QIT-MS capabilities offer real-time altitude-resolved measurements of atmospheric chemical composition during probe descent below 60 km, including trace species detection and the ability to distinguish between most mass isobars.…”
Section: Introductionmentioning
confidence: 99%