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Volume 31, issue 12
Ann. Geophys., 31, 2201–2206, 2013
https://doi.org/10.5194/angeo-31-2201-2013
© Author(s) 2013. This work is distributed under
the Creative Commons Attribution 3.0 License.
Ann. Geophys., 31, 2201–2206, 2013
https://doi.org/10.5194/angeo-31-2201-2013
© Author(s) 2013. This work is distributed under
the Creative Commons Attribution 3.0 License.

ANGEO Communicates 17 Dec 2013

ANGEO Communicates | 17 Dec 2013

Ion cyclotron waves during the Rosetta approach phase: a magnetic estimate of cometary outgassing

M. Volwerk1, C. Koenders2, M. Delva1, I. Richter2, K. Schwingenschuh1, M. S. Bentley1, and K.-H. Glassmeier2 M. Volwerk et al.
  • 1Space Research Institute, Austrian Academy of Sciences, 8042 Graz, Austria
  • 2Institute for Geophysics and Extraterrestrial Physics, TU Braunschweig, Germany

Abstract. A theoretical model for the ion cyclotron wave generation during the approach phase of Rosetta to 67P/Churyumov–Gerasimenko is presented. For various activity levels of the comet, the crossing of the observational threshold is determined, whose level is derived from the wave power in the undisturbed solar wind near the comet's location during the approach phase at the appropriate frequency. The Giotto flyby at 27P/Grigg–Skjellerup is used to obtain an estimate of how often water-group ion cyclotron waves are observed, and to get insight into the wave forms. At 67P/Churyumov–Gerasimenko one can expect to observe water-group ion cyclotron waves already at a distance of 600 000 km from the nucleus for a nominal outgassing rate of Q = 350 × 1023 molecules per second. The observed first location of cyclotron waves during the Rosetta approach phase will give an indication of the actual outgassing rate of the comet.

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