2014
DOI: 10.1007/s11214-014-0043-9
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The Neutral Mass Spectrometer on the Lunar Atmosphere and Dust Environment Explorer Mission

Abstract: The Neutral Mass Spectrometer (NMS) of the Lunar Atmosphere and Dust Environment Explorer (LADEE) Mission is designed to measure the composition and variability of the tenuous lunar atmosphere. The NMS complements two other instruments on the LADEE spacecraft designed to secure spectroscopic measurements of lunar composition and in situ measurement of lunar dust over the course of a 100-day mission in order to sample multiple lunation periods. The NMS utilizes a dual ion source designed to measure both surface… Show more

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Cited by 55 publications
(33 citation statements)
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“…Mahaffy et al, 2014]. The ordinate is the average data count from 15 sequential, 247 ms, integration periods, each corrected for the effect of the steady rise of ion source temperature on inviscid gas equilibrium in the instrument [cf.…”
Section: Evidence Of Exospheric Methanementioning
confidence: 99%
See 1 more Smart Citation
“…Mahaffy et al, 2014]. The ordinate is the average data count from 15 sequential, 247 ms, integration periods, each corrected for the effect of the steady rise of ion source temperature on inviscid gas equilibrium in the instrument [cf.…”
Section: Evidence Of Exospheric Methanementioning
confidence: 99%
“…The possibility of exospheric escape of solar carbon from the Moon was explored by Hodges [1976]. Elphic et al, 2014;Mahaffy et al, 2014]. Elphic et al, 2014;Mahaffy et al, 2014].…”
Section: Introductionmentioning
confidence: 99%
“…The NMS was also to be operated in an "Ion Scan Mode" where the aperture was directed towards the Moon's North or South Pole and held there for the duration of a portion of an orbit. More details on NMS can be found at [11].…”
Section: Neutral Mass Spectrometer (Nms) -The Ladee Neutralmentioning
confidence: 99%
“…In addition to UVS and the species it can measure (Table 1), the LADEE Neutral Mass Spectrometer (NMS) measured a number of neutral gases and ions which UVS could not detect, including a number of noble gases (e.g., He, Ne, and Ar), as well as measuring some gases and ions UVS could measure (e.g., Na, K, and OH) (Mahaffey et al 2014). Thus the UVS and NMS instruments were very complimentary.…”
Section: Lunar Exosphere: Theory and Observationsmentioning
confidence: 99%