ACCELERATION OF COSMIC RAYS AT LARGE SCALE COSMIC SHOCKS IN THE UNIVERSE |
KANG HYESUNG
(Department of Earth Sciences, Pusan National University)
JONES T. W. (Department of Astronomy, University of Minnesota) |
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Cosmic-Ray Electrons in Groups and Clusters of Galaxies: Primary and Secondary Populations from a Numerical Cosmological Simulation
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DOI ScienceOn |
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One-dimensional front-tracking based on high resolution wave propagation methods
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DOI ScienceOn |
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Particle Acceleration at Astrophysical Shocks - a Theory of Cosmic-Ray Origin
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DOI ScienceOn |
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cosmic-Ray Protons Accelerated at Cosmological Shocks and Their Impact on Groups and Clusters of Galaxies
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Nonthermal origin of the EUV and HEX excess emission of the Coma cluster - the nature of the energetic electrons
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6 |
Properties of Cosmic Shock Waves in Large-Scale Structure Formation
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8 |
Acceleration of Solar Wind Ions by Nearby Interplanetary Shocks: Comparison of Monte Carlo Simulations with ULYSSES Observations
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Contributions to the Cosmic Ray Flux above the Ankle: Clusters of Galaxies
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10 |
Numerical Studies of Costmic-Ray Injection and Acceleration
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11 |
Nonthermal Origin of the EUV and Soft X-Rays from the Coma Cluster: Cosmic Rays in Equipartition with the Thermal Medium
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A statistical detection of gamma-ray emission from galaxy clusters: implications for the gamma-ray background and structure formation
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Time Evolution of Cosmic-Ray Modified Plane Shocks
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Inter-galactic Shock Acceleration and the Cosmic Gamma-ray Background
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15 |
cosmic ray streaming. Ⅰ - Effect of Alfv<TEX>$\'{e}$</TEX>n waves on particles
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Ion leakage from quasiparallel collisionless shocks: Implications for injection and shock dissipation
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Cluster magnetic fields
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The acceleratin of cosmic rays in shock fronts. Ⅰ
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Nonlinear theory of diffusive acceleration of particles by shock waves
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Theory and simulation of collisionless parallel shocks
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21 |
Cosmic .-ray background from structure formation in the intergalactic medium
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22 |
Detection of excess rotation measure due to intracluster magnetic fields in clusters of galaxies
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23 |
Numerical studies of diffusive particle acceleration in supernova remnants
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24 |
Time dependent cosmic-ray shock acceleration with self-consistent injection
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25 |
Hard X-Ray Radiation in the Coma Cluster Spectrum
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Particle injection and acceleration at earth's bow shock - Com - parison of upstream and downstream events
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27 |
Diffusive ion acceleration at shocks: the problem of injection
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28 |
The magnetic field in the Coma cluster
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29 |
Time-dependent evolution of cosmic-ray-mediated shocks in the two-fluid model
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30 |
Cosmic magnetic fields in large scale filaments and sheets
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31 |
Radio halo and relic candidates from the NRAO VLA Sky Survey
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32 |
An Introduction to the Theory of Shock Acceleration of Energetic Particles in Tenuous Plasmas
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33 |
Clusters of Galaxies as Storage Room for Cosmic Rays
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34 |
The Origin of Cosmic Rays above 10 18.5 eV
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35 |
Extreme-Ultraviolet Emission from Clusters of Galaxies: Inverse Compton Radiation from & Relic Population of Cosmic Ray Electrons?
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36 |
Diffusive shock Acceleration Simulations: Comparison with Particle Methods and Bow Shock Measurements
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37 |
The Energy Spectrum of Primary Cosmic-Ray Electrons in Clusters of Galaxies and Inverse Compton Emission
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38 |
Searching for cluster magnetic fields in the cooling flows of 0745-191, A2029, and A4059
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39 |
Adaptive Mesh Refinement using Wave-Propagation Algorithms for Hyperbolic Systems
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40 |
Contributions to the Cosmic Ray Flux above the Ankle: Clusters of Galaxies
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DOI ScienceOn |
41 |
The structure of cosmic ray shocks
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42 |
Efficiency of CR acceleration in supernova remnants
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43 |
Non-linear amplification of a magnetic field driven by cosmic ray streaming
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44 |
Hot gas in the cold dark matter scenario: X-ray clusters from a high-resolution numerical simulation
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45 |
The Protogalactic Origin for Cosmic Magnetic Fields
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46 |
A New Radio-X-Ray Probe of Galaxy Cluster Magnetic Fields
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47 |
Hard X-Ray Emission from the Galaxy Cluster A225
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