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Particle acceleration and Alfvén wave generation by an interplanetary shock
Astronomy Letters, 2016Based on the event observed by ISEE 3 near the Earth’s orbit at 01:21 UT on April 5, 1979, we investigate the diffusive shock acceleration of ions and the generation of Alfven waves by accelerated particles near the quasi-parallel parts of interplanetary shock fronts within a quasi-linear approach.
S N Taneev, E G Berezhko, Taneev S N
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The structure and evolution of interplanetary shocks and the relevance for particle acceleration
Nuclear Physics, Section B, Proceedings Supplements, 1995It is now widely accepted that interplanetary shocks initiated by coronal mass ejections play a dominant role in the generation of the vast majority of large solar energetic particle events. However, our understanding of the details of the acceleration process is far from complete.
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The acceleration of charged particles in interplanetary shock waves
Space Science Reviews, 1982Consideration of the theoretical and observational literature on energetic ion acceleration in interplanetary shock waves is the basis for the present discussion of the shock acceleration of the solar wind plasma and particle transport effects. It is suggested that ISEE data be used to construct data sets for shock events that extend continuously from ...
M.E. Pesses, R.B. Decker, T.P. Armstrong
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Acceleration in solar flares: Interacting particles versus interplanetary particles
Advances in Space Research, 1993Abstract We study the properties of flare accelerated particles using gamma ray observations. We derive ion and electron energy spectra, electron to proton ratios, and numbers of interacting particles. We investigate the effects of the abundance variations implied by the gamma ray data on these parameters.
R. Ramaty +3 more
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Solar and interplanetary particle acceleration
Advances in Space Research, 2003Abstract The nature and location of energetic particle acceleration (excluding planetary magnetospheres) in the inner heliosphere ( 1000 km/sec) coronal mass ejections is examined, but we find that they are not normally associated with relativistic energetic particle acceleration, although they may enhance the energy of particles already present in ...
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Fe/O Ratios in Interplanetary Shock Accelerated Particles
Space Science Reviews, 2007It is widely accepted that diffusive shock acceleration is an important process in the heliosphere, in particular in producing the energetic particles associated with interplanetary shocks driven by coronal mass ejections. In its simplest formulation shock acceleration is expected to accelerate ions with higher mass to charge ratios less efficiently ...
H. V. Cane +2 more
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Interplanetary particle acceleration, modulation and drift
Reviews of Geophysics, 1979This report is concerned mainly with the contribution of U. S. scientists, during the period 1975–1978, to the general area of particle acceleration and transport in the solar wind, excluding particles of solar origin. Other work is cited only when it bears directly on the subject being discussed.
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Particle acceleration by coronal and interplanetary shock waves
Advances in Space Research, 1982Utilizing many years of observation from deep space and near-earth spacecraft a theoretical understanding has evolved on how ions and electrons are accelerated in interplanetary shock waves. This understanding is now being applied to solar flare-induced shock waves propagating through the solar atmosphere.
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Charged particle acceleration processes in the interplanetary medium
Advances in Space Research, 1989Abstract Selected aspects of energetic (>35 keV) ion acceleration processes in three regions of the heliosphere are reviewed: at interplanetary travelling shocks near 1 AU, in the outer heliosphere and in cometary environments. Clear examples of diffusive acceleration events at quasi-parallel shocks as well as of shock drift acceleration events at ...
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Particle Acceleration Processes in Interplanetary Space
1985The preceeding chapters have been concerned mainly with multiple scattering, diffusion, and convective transport of particles. In passing, some processes of particle energy variations have been considered, such as adiabatic deceleration in expanding streams of magnetic inhomogeneities (§8,1, 12, 13) and in large-scale magnetic fields frozen into the ...
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