Particle Acceleration in Mercury’s Magnetosphere |
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Authors: | L Zelenyi M Oka H Malova M Fujimoto D Delcourt W Baumjohann |
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Institution: | (1) Space Research Institute, Russian Academy of Sciences, Moscow, Russia;(2) Kwasan and Hida Observatory, Kyoto University, Kyoto, Japan;(3) Institute of Space and Astronautical Science, Sagamihara, Japan;(4) Centre d’études des Environnements Terrestres et Planétaires, CNRS, Saint-Maur des Faussés, France;(5) Space Research Institute, Austrian Academy of Sciences, Graz, Austria |
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Abstract: | This paper is devoted to the problem of particle acceleration in the closest to the Sun Hermean magnetosphere. We discuss
few available observations of energetic particles in Mercury environment made by Mariner-10 in 1974–1975 during Mercury flyby’s
and by Helios in 1979 upstream of the Hermean bow shock. Typically ions are non-adiabatic in a very dynamic and compact Mercury
magnetosphere, so one may expect that particle acceleration will be very effective. However, it works perfectly for electrons,
but for ions the scale of magnetosphere is so small that it allows their acceleration only up to 100 keV. We present comparative
analysis of the efficiency of various acceleration mechanisms (inductive acceleration, acceleration by the centrifugal impulse
force, stochastic acceleration in a turbulent magnetic fields, wave–particle interactions and bow shock energization) in the
magnetospheres of the Earth and Mercury. Finally we discuss several points which need to be addressed in a future Hermean
missions. |
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Keywords: | Hermean magnetosphere Particle acceleration |
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