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Conclusions
New generation of Solar Wind Composition Spectrometer, with promise of high mass resolution > 1000 M/dM combined with high sensitivity that can make first measurements
- molecules in space, LISM, biomolecules, PAHs
- rare isotopes, e.g.17O/16O ratio of solar wind
- planetary atmospheres interaction w/plasma
- high time resolution of small structures: shocks, magnetic bubbles, boundary crossings