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The interstellar environment of our galaxyTheory of extragalactic radio sourcesA magnetized jet from a massive protostar.Thermodynamic constraints on stochastic acceleration in compressional turbulence.Millisecond newly born pulsars as efficient accelerators of electrons.Electron Surfing and Drift Accelerations in a Weibel-Dominated High-Mach-Number Shock.Chemical Enhancements in Shock-Accelerated Particles: Ab initio Simulations.Nonlinear Waves in the Terrestrial Quasiparallel Foreshock.Transition from Collisional to Collisionless Regimes in Interpenetrating Plasma Flows on the National Ignition Facility.Scaling the yield of laser-driven electron-positron jets to laboratory astrophysical applications.Deciphering the Dipole Anisotropy of Galactic Cosmic Rays.Large-Eddy Simulations of Magnetohydrodynamic Turbulence in Heliophysics and AstrophysicsTurbulent amplification of magnetic field and diffusive shock acceleration of cosmic raysCosmic ray acceleration to very high energy through the non-linear amplification by cosmic rays of the seed magnetic fieldThe Anatomy of GalaxiesTowards Understanding the Physics of Collisionless Relativistic ShocksParticle acceleration in supernova-remnant shocksA cut-off in the TeV gamma-ray spectrum of the SNR Cassiopeia AARTEMIS Science ObjectivesLOFAR imaging of Cygnus A – direct detection of a turnover in the hotspot radio spectraEscaping the accelerator: how, when and in what numbers do cosmic rays get out of supernova remnants?X-ray haloes around supernova remnantsCollisionless electrostatic shock generation using high-energy laser systemsRecent Results in Cosmic Ray Physics and Their InterpretationThe origin of galactic cosmic raysTheoretical challenges in acceleration and transport of ultra high energy cosmic rays: A reviewA kinetic approach to cosmic-ray-induced streaming instability at supernova shocksDynamical feedback of self-generated magnetic fields in cosmic ray modified shocksOn the escape of particles from cosmic ray modified shocksNon-linear particle acceleration at non-relativistic shock waves in the presence of self-generated turbulenceSupernova remnants in the Local Group – I. A model for the radio luminosity function and visibility times of supernova remnantsLog-parabolic spectra and particle acceleration in blazars. III. SSC emission in the TeV band from Mkn 501H.E.S.S. detection of TeV emission from the interaction region between the supernova remnant G349.7+0.2 and a molecular cloudA brief review of “solar flare effects” on the ionosphereParticle Acceleration at Interplanetary ShocksStochastic particle acceleration and synchrotron self-Compton radiation in TeV blazarsOrigin of ultra-high-energy γ-rays from Cygnus X-3 and related sourcesCosmic γ-ray background from structure formation in the intergalactic mediumMultiple hotspots in extragalactic radio sourcesParticle acceleration in the hotspot of the jet of quasar 3C273
P2860
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P2860
description
im Februar 1978 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в лютому 1978
@uk
name
The acceleration of cosmic rays in shock fronts - I
@en
The acceleration of cosmic rays in shock fronts - I
@nl
type
label
The acceleration of cosmic rays in shock fronts - I
@en
The acceleration of cosmic rays in shock fronts - I
@nl
prefLabel
The acceleration of cosmic rays in shock fronts - I
@en
The acceleration of cosmic rays in shock fronts - I
@nl
P356
P1476
The acceleration of cosmic rays in shock fronts - I
@en
P2093
A. R. Bell
P304
P356
10.1093/MNRAS/182.2.147
P407
P577
1978-02-01T00:00:00Z
P819
1978MNRAS.182..147B