Rosina – Rosetta Orbiter Spectrometer for Ion and Neutral Analysis

By H. Balsiger, K. Altwegg, P. Bochsler, P. Eberhardt, J. Fischer, S. Graf, A. Jäckel, E. Kopp, U. Langer, M. Mildner and 40 more. 2007

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Elemental and molecular abundances in comet 67P/Churyumov-Gerasimenko (2019, background): “The resulting mass resolution was m/ m = 3000 for a mass/charge ratio of 28 u/e at 1 per cent of the peak height (Balsiger et al. 2007).”
Sulphur-bearing species in the coma of comet 67P/Churyumov–Gerasimenko (2016, methodology): “Besides this, DFMS is designed in such a way that it covers a mass range from m/z = 12–140 u/e, has good energy focusing properties in order that E/E is up to 1 per cent and a high mass dispersion in the focal plane making it possible to use a position-sensitive detector (Balsiger et al. 2007).”
Inventory of the volatiles on comet 67P/Churyumov-Gerasimenko from Rosetta/ROSINA (2015, methodology): “The results presented in this paper come mainly from the DFMS instrument (see Balsiger et al. 2007 for a detailed description).”
Organics in comet 67P – a first comparative analysis of mass spectra from ROSINA–DFMS, COSAC and Ptolemy (2017, methodology): “About 5h earlier, Rosetta was most probably hit by a chunk of ice and dust, showing high-density peaks for more than 3 h in the vicinity of the ROSINA–COPS nude gauge with its FOV of 340◦ (Fig.”