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The acceleration of energetic charged particles by interplanetary and supernova shock waves
AIP Conference Proceedings, 1979Pioneer 11 observations of energetic proton acceleration in interplanetary shock are in good agreement with predictions of the V↘×B↘ electric field model of shock acceleration. The V↘×B↘ model predicts that relativistic particles are accelerated by a factor of 2–15 in kinetic energy during a single encounter with a quasi‐perpendicular (ψ≳75 ...
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Comparison of Particle Acceleration at Planetary Bow Shocks and Interplanetary Shocks
The spatial size of collisionless shock waves is suggested to play an important role in determining the maximum energy gain of particles accelerated at heliospheric and astrophysical shocks. In addition, shocks energize particles with different starting/upstream energies differently.Martin Lindberg +3 more
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Advances in Space Research, 2005
Abstract Observations of hard X-ray (HXR)/γ-ray continuum and γ-ray lines produced by energetic electrons and ions, respectively, colliding with the solar atmosphere, have shown that large solar flares can accelerate ions up to many GeV and electrons up to hundreds of MeV.
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Abstract Observations of hard X-ray (HXR)/γ-ray continuum and γ-ray lines produced by energetic electrons and ions, respectively, colliding with the solar atmosphere, have shown that large solar flares can accelerate ions up to many GeV and electrons up to hundreds of MeV.
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Diffusive Acceleration of Ions at Interplanetary Shocks
AIP Conference Proceedings, 2005Matthew Baring, Baring Matthew G
exaly
A model of quiet time particle acceleration in interplanetary space
2005LEPRETI, Fabio +3 more
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Particle acceleration at interplanetary shocks—Observations at a few tens of keV vs some tens of MeV
Advances in Space Research, 1995exaly