Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays
about
Sharp knee phenomenon of primary cosmic ray energy spectrumUltrahigh energy cosmic raysAcceleration of petaelectronvolt protons in the Galactic Centre.The basis for cosmic ray feedback: Written on the wind.Nonlinear Monte Carlo model of superdiffusive shock acceleration with magnetic field amplification.Generalized Ohm's law for a background plasma in the presence of relativistic charged particles.Towards Understanding the Physics of Collisionless Relativistic ShocksHigh energy neutrinos and gamma-ray emission from supernovae in compact star clustersMagnetic Fields in Cosmic Particle Acceleration SourcesMagnetic Fields in Supernova Remnants and Pulsar-Wind NebulaeParticle acceleration in supernova-remnant shocksUltrahard spectra of PeV neutrinos from supernovae in compact star clustersElectron and ion acceleration in relativistic shocks with applications to GRB afterglowsRadio confirmation of Galactic supernova remnant G308.3−1.4A cut-off in the TeV gamma-ray spectrum of the SNR Cassiopeia ATurbulent magnetic field amplification driven by cosmic ray pressure gradientsEscaping the accelerator: how, when and in what numbers do cosmic rays get out of supernova remnants?Spectra of accelerated particles at supernova shocks in the presence of neutral hydrogen: the case of TychoGalactic cosmic raysRecent 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 reviewUltrahigh energy neutrinos from population III stars: Concept and constraintsON THE ORIGIN OF VERY HIGH ENERGY COSMIC RAYSULTRA HIGH ENERGY COSMIC RAYSSupernova remnants in the Local Group – I. A model for the radio luminosity function and visibility times of supernova remnantsVisualizing electromagnetic fields in laser-produced counter-streaming plasma experiments for collisionless shock laboratory astrophysicsMeasuring the Broad-Band X-Ray Spectrum from 400eV to 40keV in the Southwest Part of the Supernova Remnant RXJ1713.7$-$3946Structures and Components in Galaxy Clusters: Observations and ModelsEvidence of nonthermal particles in coronal loops heated impulsively by nanoflaresEnergetic particle transport in the presence of magnetic turbulence: influence of spectral extension and intermittency
P2860
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P2860
Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays
description
im September 2004 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована у вересні 2004
@uk
name
Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays
@en
Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays
@nl
type
label
Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays
@en
Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays
@nl
prefLabel
Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays
@en
Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays
@nl
P1476
Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays
@en
P2093
A. R. Bell
P304
P356
10.1111/J.1365-2966.2004.08097.X
P407
P577
2004-09-01T00:00:00Z
P819
2004MNRAS.353..550B