Energetic pickup proton population downstream of the termination shock as revealed by the IBEX-Hi data
I. I. Baliukin,
V. V. Izmodenov,
D. B. Alexashov
Abstract:The pickup protons originate as a result of the ionization of hydrogen atoms in the supersonic solar wind, forming the suprathermal component of protons in the heliosphere. While picked by the heliospheric magnetic field and convected into the heliosheath, the pickup protons may suffer the stochastic acceleration by the solar wind turbulence in the region from the Sun up to the heliospheric termination shock, where they can also experience the shock-drift acceleration or the reflection from the cross-shock pot… Show more
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