Abstract
Energization at a quasi‐perpendicular shock is described for ions which approach the shock with a speed much less than that of the incoming plasma. These ions may be trapped between the shock electrostatic potential and the upstream Lorentz force and accelerated by “surfing” along the shock surface, before eventually escaping the shock into the upstream or downstream plasma. The process is described in detail, extending previous work on the mechanism, and energy gains are calculated. It is pointed out that pickup ions in the solar wind are ideally configured, so that a reasonable fraction of the ions can be accelerated by this mechanism at cometary bow shocks, the solar wind termination shock, and interplanetary traveling shocks. The mechanism may provide the required “injection” or preacceleration at quasi‐perpendicular shocks for subsequent diffusive shock acceleration.
Topics

No keywords indexed for this article. Browse by subject →

References
79
[1]
Axford W. I. "The acceleration of cosmic rays by shock waves" Proc. Int. Conf. Cosmic Rays 15th (1977)
[3]
The acceleration of cosmic rays in shock fronts - I

A. R. Bell

Monthly Notices of the Royal Astronomical Society 10.1093/mnras/182.2.147
[4]
Particle acceleration by astrophysical shocks

R. D. Blandford, J. P. Ostriker

The Astrophysical Journal 10.1086/182658
[6]
Chandrasekhar S. (1989)
[13]
Galeev A. A. "Alfvén waves in a space plasma and its role in the solar wind interaction with comets" Astrophys. Space Sci. (1988) 10.1007/bf00793196
[14]
Galeev A. A. (1987)
[15]
Galeev A. A. "MHD turbulence caused by a comet in the solar wind" Sov. Phys. JETP (1987)
[18]
Goldstein H. (1980)
[19]
Gombosi T. I. "Combined first‐ and second‐order Fermi acceleration in cometary environments" J. Geophys. Res. (1989)
[23]
Gribov B. E. "Stochastic Fermi acceleration of ions in the pre‐shock region of comet Halley" Astron. Astrophys. (1987)
[24]
Huddleston D. E. "Quasi‐linear pitch angle and energy diffusion of pickup ions near Comet Halley" J. Geophys. Res. (1991)
[25]
Huddleston D. E. "Quasi‐linear velocity space diffusion of heavy cometary pickup ions on bispherical diffusion characteristics" J. Geophys. Res. (1992)
[31]
Particle acceleration at a termination shock: 1. Application to the solar wind and the anomalous component

J. R. Jokipii

Journal of Geophysical Research: Oceans 10.1029/ja091ia03p02929
[34]
Jones F. C. "Noncoplanar magnetic fields, shock potentials, and ion deflection" J. Geophys. Res. (1987)
[37]
Kennel C. F. "Alfvén shock wave trains with a dispersion" JETP Lett. (1988)
[38]
Krymsky G. F. "A regular mechanism for the acceleration of charged particles on the front of a shock wave" Dokl. Akad. Nauk SSSR (1977)
[39]
Lee M. A. "Hydromagnetic wave excitation by ionized interstellar hydrogen and helium in the solar wind" J. Geophys. Res. (1987)
[44]
Möbius E. "Interaction of interstellar pickup ions with the solar wind" Astrophys. Space Sci. (1988) 10.1007/bf00793200

Showing 50 of 79 references

Cited By
243
Journal of Geophysical Research: Sp...
Journal of Geophysical Research: Oc...
The Astrophysical Journal
Journal of Geophysical Research: Oc...
Physical Review Letters
Journal of Geophysical Research: Oc...
Metrics
243
Citations
79
References
Details
Published
Mar 01, 1996
Vol/Issue
101(A3)
Pages
4777-4789
License
View
Cite This Article
Martin A. Lee, Vitali D. Shapiro, Roald Z. Sagdeev (1996). Pickup ion energization by shock surfing. Journal of Geophysical Research: Oceans, 101(A3), 4777-4789. https://doi.org/10.1029/95ja03570