Ion composition at comet 67P near perihelion: Rosetta observations and model-based interpretation
K. L. Héritier(Imperial College London), V. Vuitton(Centre National de la Recherche Scientifique), N. Fougere(University of Michigan), J. J. Berthelier(Centre National de la Recherche Scientifique), M. Rubı́n(Planetary Science Institute), Ursina Calmonte(University of Bern), N. Biver(Centre National de la Recherche Scientifique), H. Balsiger(University of Bern), Johan De Keyser(AZ Delta), E. Kopp(University of Bern), Arnaud Beth(Imperial College London), T. I. Gombosi(University of Michigan), K. Altwegg(University of Bern), A. I. Eriksson(Swedish Institute of Space Physics), Elias Odelstad(Swedish Institute of Space Physics), S. A. Fuselier(Southwest Research Institute), M. Hässig(University of Bern), Chia-Yu Tzou(University of Bern), S. Gasc(University of Bern), K. C. Hansen(University of Michigan), M. Galand(Imperial College London), A. Bieler(University of Bern), E. Vigren(Swedish Institute of Space Physics), B. Fiethe(Technische Universität Braunschweig), M. R. Combi(Department of Space)
Cited by 39
Related Papers
The Mars Atmosphere and Volatile Evolution (MAVEN) Mission
|Space Science Reviews|2015|814
Electron-scale measurements of magnetic reconnection in space
|Science|2016|724
Cassini Ion and Neutral Mass Spectrometer: Enceladus Plume Composition and Structure
|Science|2006|689
Prebiotic chemicals—amino acid and phosphorus—in the coma of comet 67P/Churyumov-Gerasimenko
|Science Advances|2016|560
Cassini Plasma Spectrometer Investigation
|Space Science Reviews|2004|514