Editing Rosetta (spacecraft) (section)

=== Gas and particles ===
* '''ROSINA''' (Rosetta Orbiter Spectrometer for Ion and Neutral Analysis). The instrument consisted of a double-focus [[Sector instrument|magnetic mass spectrometer]] (DFMS) and a [[reflectron]] type [[Time of flight|time of flight mass spectrometer]] (RTOF). The DFMS had a high resolution (could resolve [[nitrogen|N<sub>2</sub>]] from [[carbon monoxide|CO]]) for molecules up to 300 [[Atomic mass unit|amu]]. The RTOF was highly sensitive for neutral molecules and for ions. The Max Planck Institute for Solar System Research (MPS) has contributed to the development and construction of the instrument.<ref>{{cite journal |title=Rosetta Orbiter Spectrometer for Ion and Neutral Analysis—ROSINA |journal=Advances in Space Research |first1=H. |last1=Balsiger |first2=K. |last2=Altwegg|author2-link=Kathrin Altwegg |first3=E. |last3=Arijs |first4=J.-L. |last4=Bertaux |first5=J.-J. |last5=Berthelier |first6=P. |last6=Bochsler |first7=G. R. |last7=Carignan |first8=P. |last8=Eberhardt |first9=L. A. |last9=Fisk |first10=S. A. |last10=Fuselier |first11=A. G. |last11=Ghielmetti |first12=F. |last12=Gliem |first13=T. I. |last13=Gombosi |first14=E. |last14=Kopp |first15=A. |last15=Korth |first16=S. |last16=Livi |first17=C. |last17=Mazelle |first18=H. |last18=Rème |first19=J. A. |last19=Sauvaud |first20=E. G. |last20=Shelley |first21=J. H. |last21=Waite |first22=B. |last22=Wilken |first23=J. |last23=Woch |first24=H. |last24=Wollnik |first25=P. |last25=Wurz |first26=D. T. |last26=Young |display-authors=5 |volume=21 |issue=11 |pages=1527–1535 |year=1998 |doi=10.1016/S0273-1177(97)00945-9 |bibcode=1998AdSpR..21.1527B}}</ref> ROSINA was developed at the University of Bern in Switzerland.
* '''[[Micro-Imaging Dust Analysis System|MIDAS]]''' (Micro-Imaging Dust Analysis System). The high-resolution [[atomic force microscopy|atomic force microscope]] investigated several physical aspects of the dust particles which are deposited on a silicon plate.<ref>{{cite journal |title=The MIDAS experiment for the Rosetta mission |journal=Advances in Space Research |first1=W. |last1=Riedler |first2=K. |last2=Torkar |first3=F. |last3=Rüdenauer |first4=M. |last4=Fehringer |first5=R. |last5=Schmidt |first6=H. |last6=Arends |first7=R. J. L. |last7=Grard |first8=E. K. |last8=Jessberger |first9=R. |last9=Kassing |first10=H. St. C. |last10=Alleyne |first11=P. |last11=Ehrenfreund |first12=A. C. |last12=Levasseur-Regourd |first13=C. |last13=Koeberl |first14=O. |last14=Havnes |first15=W. |last15=Klöck |first16=E. |last16=Zinner |first17=M. |last17=Rott |display-authors=5 |volume=21 |issue=11 |pages=1547–1556 |year=1998 |doi=10.1016/S0273-1177(97)00947-2 |bibcode=1998AdSpR..21.1547R}}</ref>
* '''COSIMA''' (Cometary Secondary Ion Mass Analyser). COSIMA analysed the composition of dust particles by [[secondary ion mass spectrometry]], using [[indium]] ions. It could detect ions up to a mass of 6500&nbsp;amu. COSIMA was built by the Max Planck Institute for Extraterrestrial Physics (MPE, Germany) with international contributions. The COSIMA team is led by the Max Planck Institute for Solar System Research (MPS, Germany).<ref>{{cite journal |title=Chemometric evaluation of time-of-flight secondary ion mass spectrometry data of minerals in the frame of future ''in situ'' analyses of cometary material by COSIMA onboard ROSETTA |journal=Rapid Communications in Mass Spectrometry |first1=Cecile |last1=Engrand |first2=Jochen |last2=Kissel |first3=Franz R. |last3=Krueger |first4=Philippe |last4=Martin |first5=Johan |last5=Silén |first6=Laurent |last6=Thirkell |first7=Roger |last7=Thomas |first8=Kurt |last8=Varmuza |display-authors=5 |volume=20 |issue=8 |pages=1361–1368 |date=April 2006 |doi=10.1002/rcm.2448 |pmid=16555371|bibcode=2006RCMS...20.1361E }}</ref>
* '''GIADA''' (Grain Impact Analyser and Dust Accumulator). GIADA analysed the dust environment of the [[Coma (cometary)|comet coma]] by measuring the optical cross section, momentum, speed and mass of each grain entering inside the instrument.<ref>{{cite journal |title=The Grain Impact Analyser and Dust Accumulator (GIADA) experiment for the Rosetta mission: design, performances and first results |journal=Space Science Reviews |first1=L. |last1=Colangeli |first2=J. J. |last2=Lopez-Moreno |first3=P. |last3=Palumbo |first4=J. |last4=Rodriguez |first5=M. |last5=Cosi |first6=V. |last6=Della Corte |first7=F. |last7=Esposito |first8=M. |last8=Fulle |first9=M. |last9=Herranz |first10=J. M. |last10=Jeronimo |first11=A. |last11=Lopez-Jimenez |first12=E. |last12=Mazzotta Epifani |first13=R. |last13=Morales |first14=F. |last14=Moreno |first15=E. |last15=Palomba |first16=A. |last16=Rotundi |display-authors=5 |volume=128 |issue=1–4 |pages=803–821 |date=February 2007 |doi=10.1007/s11214-006-9038-5 |bibcode=2007SSRv..128..803C|s2cid=123232721 }}</ref><ref>{{cite journal |title=GIADA: its status after the Rosetta cruise phase and on-ground activity in support of the encounter with comet 67P/Churyumov-Gerasimenko |journal=[[Journal of Astronomical Instrumentation]] |first1=V. |last1=Della Corte |first2=A. |last2=Rotundi |first3=M. |last3=Accolla |first4=R. |last4=Sordini |first5=P. |last5=Palumbo |first6=L. |last6=Colangeli |first7=J. J. |last7=Lopez-Moreno |first8=J. |last8=Rodriguez |first9=F. J. M. |last9=Rietmeijer |first10=E. |last10=Mazzotta Epifani |first11=S. |last11=Ivanovski |first12=A. |last12=Aronica |first13=M. |last13=Cosi |first14=E. |last14=Bussoletti |first15=J. F. |last15=Crifo |first16=F. |last16=Esposito |first17=M. |last17=Fulle |first18=S. F. |last18=Green |first19=E. |last19=Gruen |first20=M. L. |last20=Herranz |first21=J. M. |last21=Jeronimo |first22=P. |last22=Lamy |first23=A. |last23=Lopez-Jimenez |first24=J. A. M.. |last24=McDonnell |first25=V. |last25=Mennella |first26=A. |last26=Molina |first27=R. |last27=Morales |first28=F. |last28=Moreno |first29=E. |last29=Palomba |first30=J. M. |last30=Perrin |first31=R. |last31=Rodrigo |first32=P. |last32=Weissman |first33=V. |last33=Zakharov |first34=J. C. |last34=Zarnecki |display-authors=5 |volume=3 |issue=1 |pages=1350011–110 |date=March 2014 |doi=10.1142/S2251171713500116 |bibcode=2014JAI.....350011D |url=http://oro.open.ac.uk/39545/1/2014_DellaCorte_et_al_JAI_1350011.pdf}}</ref>