| Literature DB >> 25613894 |
Hans Nilsson1, Gabriella Stenberg Wieser2, Etienne Behar3, Cyril Simon Wedlund4, Herbert Gunell5, Masatoshi Yamauchi2, Rickard Lundin2, Stas Barabash2, Martin Wieser2, Chris Carr6, Emanuele Cupido6, James L Burch7, Andrei Fedorov8, Jean-André Sauvaud8, Hannu Koskinen9, Esa Kallio10, Jean-Pierre Lebreton11, Anders Eriksson12, Niklas Edberg12, Raymond Goldstein5, Pierre Henri11, Christoph Koenders13, Prachet Mokashi7, Zoltan Nemeth14, Ingo Richter13, Karoly Szego14, Martin Volwerk15, Claire Vallat16, Martin Rubin17.
Abstract
The Rosetta mission shall accompany comet 67P/Churyumov-Gerasimenko from a heliocentric distance of >3.6 astronomical units through perihelion passage at 1.25 astronomical units, spanning low and maximum activity levels. Initially, the solar wind permeates the thin comet atmosphere formed from sublimation, until the size and plasma pressure of the ionized atmosphere define its boundaries: A magnetosphere is born. Using the Rosetta Plasma Consortium ion composition analyzer, we trace the evolution from the first detection of water ions to when the atmosphere begins repelling the solar wind (~3.3 astronomical units), and we report the spatial structure of this early interaction. The near-comet water population comprises accelerated ions (<800 electron volts), produced upstream of Rosetta, and lower energy locally produced ions; we estimate the fluxes of both ion species and energetic neutral atoms.Entities:
Year: 2015 PMID: 25613894 DOI: 10.1126/science.aaa0571
Source DB: PubMed Journal: Science ISSN: 0036-8075 Impact factor: 47.728