Nonlinear theory of diffusive acceleration of particles by shock waves
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PAMELA Measurements of Cosmic-Ray Proton and Helium SpectraAcceleration of petaelectronvolt protons in the Galactic Centre.Mechanism for spectral break in cosmic ray proton spectrum of supernova remnant W44.Proton-helium spectral anomaly as a signature of cosmic ray accelerator.Relativistic Electrons Produced by Foreshock Disturbances Observed Upstream of Earth's Bow Shock.Particle acceleration in turbulence and weakly stochastic reconnection.Magnetic Fields in Cosmic Particle Acceleration SourcesParticle spectra and efficiency in nonlinear relativistic shock acceleration – survey of scattering modelsSupernova Remnants Interacting with Molecular Clouds: X-Ray and Gamma-Ray SignaturesCosmic ray acceleration in supernova remnants and the FERMI/PAMELA dataTesting Astrophysical Models for the PAMELA Positron Excess with Cosmic Ray NucleiCosmic ray acceleration and Balmer emission from RCW 86 (G315.4 – 2.3)Cosmic ray acceleration and Balmer emission from SNR 0509-67.5Possible causes of a rise with energy of the cosmic ray positron fractionDiscovery of very high energyγ-ray emission from the BL Lacertae object PKS 0301−243 with H.E.S.SA low level of extragalactic background light as revealed by γ-rays from blazarsSupernova remnant W44: a case of cosmic-ray reaccelerationGalactic 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 reviewOrigin of the Positron Excess in Cosmic RaysGAMMA RAYS FROM CLUSTERS OF GALAXIESKinetic approaches to non-linear particle acceleration at shock frontsON 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 remnantsMorphological and spectral properties of the W51 region measured with the MAGIC telescopesMeasuring the Broad-Band X-Ray Spectrum from 400eV to 40keV in the Southwest Part of the Supernova Remnant RXJ1713.7$-$3946Constraints on cosmic-ray efficiency in the supernova remnant RCW 86 using multi-wavelength observationsUpper limit on the cosmological gamma-ray background
P2860
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P2860
Nonlinear theory of diffusive acceleration of particles by shock waves
description
im März 2001 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в березні 2001
@uk
name
Nonlinear theory of diffusive acceleration of particles by shock waves
@en
Nonlinear theory of diffusive acceleration of particles by shock waves
@nl
type
label
Nonlinear theory of diffusive acceleration of particles by shock waves
@en
Nonlinear theory of diffusive acceleration of particles by shock waves
@nl
prefLabel
Nonlinear theory of diffusive acceleration of particles by shock waves
@en
Nonlinear theory of diffusive acceleration of particles by shock waves
@nl
P356
P1476
Nonlinear theory of diffusive acceleration of particles by shock waves
@en
P2093
L O'C Drury
M A Malkov
P304
P356
10.1088/0034-4885/64/4/201
P407
P577
2001-03-15T00:00:00Z