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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 27, issue 5
Ann. Geophys., 27, 2077–2085, 2009
https://doi.org/10.5194/angeo-27-2077-2009
© Author(s) 2009. This work is distributed under
the Creative Commons Attribution 3.0 License.
Ann. Geophys., 27, 2077–2085, 2009
https://doi.org/10.5194/angeo-27-2077-2009
© Author(s) 2009. This work is distributed under
the Creative Commons Attribution 3.0 License.

  06 May 2009

06 May 2009

STEREO/SEPT observations of upstream particle events: almost monoenergetic ion beams

A. Klassen1, R. Gómez-Herrero1, R. Müller-Mellin1, S. Böttcher1, B. Heber1, R. Wimmer-Schweingruber1, and G. M. Mason2 A. Klassen et al.
  • 1Institut für Experimentelle und Angewandte Physik, Universität Kiel, 24118 Kiel, Germany
  • 2Applied Physics Lab, Johns Hopkins University, Laurel, MD, USA

Abstract. We present observations of Almost Monoenergetic Ion (AMI) events in the energy range of 100–1200 keV detected with the Solar Electron and Proton Telescope (SEPT) onboard both STEREO spacecraft. The energy spectrum of AMI events contain 1, 2, or 3 narrow peaks with the relative width at half maximum of 0.1–0.7 and their energy maxima varies for different events from 120 to 1200 keV. These events were detected close to the bow-shock (STEREO-A&B) and to the magnetopause at STEREO-B as well as unexpectedly far upstream of the bow-shock and far away from the magnetotail at distances up to 1100 RE (STEREO-B) and 1900 RE (STEREO-A). We discuss the origin of AMI events, the connection to the Earth's bow-shock and to the magnetosphere, and the conditions of the interplanetary medium and magnetosphere under which these AMI bursts occur. Evidence that the detected spectral peaks were caused by quasi-monoenergetic beams of protons, helium, and heavier ions are given. Furthermore, we present the spatial distribution of all AMI events from December 2006 until August 2007.

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