| The Start of Cosmic Ray Research |
| The Scope of Cosmic Ray Research |
| Cosmic Rays as Part of the Universe |
| Direct Observations of Cosmic Rays |
| Interactions of Cosmic Ray Electrons |
| Interactions of Cosmic Ray Nuclei |
| Acceleration of Cosmic Ray Particles at Shock Waves |
| Indirect Observations of Cosmic Rays |
| Immediate Consequences of Galactic Cosmic Ray Observations |
| Global Cosmic Ray Source Energetics |
| Cosmic Ray Scattering, Confinement and Isotropy |
| Statistical Mechanics of Charged Particles |
| Waves in Cold Magnetized Plasmas |
| Waves in Hot Magnetized Isotropic Plasmas |
| Generation of Plasma Waves |
| Acceleration and Transport Processes of Cosmic Rays |
| Interplanetary Transport of Cosmic Ray Particles |
| Comparison with Quasilinear Theory |
| Solar Modulation of Galactic Cosmic Rays |
| Formation of Cosmic Ray Momentum Spectra |
| Conductivity Tensor in a Hot Magnetized Plasma |
| Isotropic Distribution Functions |
| Calculation of the Integral |
| The Integral J for Imaginary Values of y |
| The Integral J for Non-imaginary Values of y |
| A Second Form of the Integral J |
| The Integral J for Non-relativistic Temperatures |
| Galactic Cosmic Ray Diffusion |
| Cosmic Ray Propagation in the Leaky-Box Approximation |
| Secondary Cosmic Ray Clocks |
| Cosmic Ray Propagation Including Interstellar Acceleration |
| Sources of Cosmic Ray Primaries |
| Steady-State Primary Particle Spectrum Below Rmax |
| Influence of Source Spectral Index Dispersion on the Steady-State Primary Particle Spectrum Below Rmax |
| Steady-State Primary Particle Spectrum Above Rmax |
| Time-Dependent Calculation |
| Secondary/Primary Ratio Including Interstellar Acceleration |
| Test Wave Approach 2. Waves in Hot Magnetized Isotropic Plasmas |
| Conductivity Tensor for Isotropic Distribution Functions |
| Illustrative Example: Longitudinal Waves in an Equilibrium Electron Plasma |
| Non-relativistic Plasma Temperatures |
| Infinitely Large Speed of Light, c ® ? |
| Solution of the Non-relativistic Dispersion Relation |
| Landau Damping of Subluminal Solutions |
| Weak Damping Approximation |
| Collisionless Damping of Transverse Oscillations |
| Interactions of Cosmic Ray Electrons |
| Emission and Transfer of Synchrotron Radiation |
| Synchrotron Radiation from Cosmic Ray Electrons in the Interstellar Medium |
| Synchrotron Energy Loss of Relativistic Electrons |
| Inverse Compton Scattering |
| Inverse Compton Scattering of Target Photons in the Interstellar Medium by Cosmic Ray Electrons |
| Inverse Compton Energy Loss of Relativistic Electrons |
| Nonthermal Relativistic Electron Bremsstrahlung |
| Nonthermal Bremsstrahlung Power |
| Nonthermal Bremsstrahlung of Cosmic Ray Electrons in the Interstellar Medium |
| Bremsstrahlung Energy Loss of Relativistic Electrons |
| Ionization and Coulomb Interactions |
| Continuum Radiation Processes of Relativistic Electrons |
| Interactions of Cosmic Ray Nuclei |
| Relativistic Kinematics of Inelastic Collisions |
| The Energy of One Particle Seen from the Rest System of Another |
| Interactions Between Cosmic Ray Nuclei and Cosmic Photons |
| Interactions Betw een Cosmic Ray Nuclei and Matter |
| Gamma-Ray, Electron, Positron and Neutrino Source Functions |
| Secondary Electrons and Positrons |
| Energy Loss by Pion Production |
| Coulomb and Ionization Interactions |
| Catastrophic Losses from Fragmentation and Radioactive Decay |
| Total Energy Loss Rate from Interactions w ith Matter |
| Ionization and Heating Rate of Interstellar Matter by Cosmic Rays |
| Continuum Radiation Processes of Relativistic Nuclei |
| Acceleration of Cosmic Ray Particles at Shock Waves |
| Magnetohydrodynamic Shock Discontinuities |
| Stationary Discontinuities |
| Alfv.en Wave Transmission Through a Parallel Fast Shock |
| Reflection and Transmission Coefficients |
| Only Forw ard Moving Waves Upstream |
| Only Backw ard Moving Waves Downstream |
| Shock Effect on Wavenumbers |
| Precursor Streaming Instability |
| Astrophysical Shock Waves |
| Cosmic Ray Transport and Acceleration Parameters |
| Upstream Cosmic Ray Transport Equation |
| Dow nstream Cosmic Ray Transport Equation |
| Scattering Center Compression Ratio |
| Importance of Dow nstream Momentum Diffusion |
| Solution of the Transport Equations |
| Finite Momentum Diffusion |
| Acceleration and Transport Processes of Cosmic Rays |
| Structure of the Cosmic Ray Transport Equation |
| Inclusion of Momentum Losses |
| Continuous and Catastrophic Momentum Losses |
| Steady-State and Time-Dependent Transport Equations |
| Scattering Time Method: Separation of Spatial and Momentum Problem |
| Formal Mathematical Solution |
| Illustrative Example: Galactic Cosmic Ray Diffusion |
| Solutions Without Momentum Diffusion |
| Statistical Mechanics of Charged Particles |
| Kinetic Description of Plasmas |
| Magnetohydrodynamics of Plasmas |
| The Relativistic Vlasov Equation and Maxwell Equations |
| Kinetic Theory of Plasma Waves |
| Linearization of Kinetic Plasma Equations |
| Solution of the Linearized Vlasov Equation |
| Conductivity Tensor in a Homogeneous Hot Magnetized Plasma |
| Energy Transfer in Dispersive Media |
| Indirect Observations of Cosmic Rays |
| Clues from Radio Astronomy |
| Clues from g-Ray Astronomy |
| g-Ray Emission Above 10 MeV |
| Continuum g-Ray Emission Below10 MeV |
| g-Ray Line Emission Below10 MeV from the Orion Region |
| g-Ray Observations of Active Galactic Nuclei |
| Nonthermal g-Ray Emission Processes in the Jets of Active Galactic Nuclei |
| Direct Observations of Cosmic Rays |
| Solar and Heliospheric Cosmic Rays |
| Solar Flare Cosmic Ray Particles |
| The Anomalous Cosmic Ray Component |
| Time History from Cosmogenic Nuclei |
| Ultrahigh Energy Cosmic Rays |
| Test Wave Approach 1. Waves in Cold Magnetized Plasmas |
| Plasma Waves in a Cold Moving Magnetized Plasma |
| Plasma Waves in a Cold Magnetized Plasma at Rest |
| Cold Unmagnetized Plasma at Rest |
| Cold Electron-Proton Plasma |
| Propagation Along the Static Magnetic Field |
| Propagation Across the Static Magnetic Field |
| Oblique Propagation of Low-Frequency Waves |
| Oblique Propagation of High-Frequency Waves |
| More Rigorous Treatment of Dispersion Relation and Polarization of Low -Frequency Waves |
| Test Wave Approach 3. Generation of Plasma Waves |
| Cosmic-Ray-Induced Instabilities |
| Parallel Propagating Waves |
| Growth Rates at Arbitrary Angles of Propagation |
| Cosmic Ray Self-Confinement in Galaxies |
| Competition of Wave Grow th and Damping |
| Damping by Ion-Neutral Collisions |
| Super-Alfv.enic Cosmic Ray Propagation? |
| Formation of Cosmic Ray Momentum Spectra |
| Fundamental Physical Picture |
| Some Exact Solutions for q =2 |
| Shock Acceleration of Relativistic Electrons Undergoing Radiation Losses |
| Shock Acceleration of Relativistic Electrons Undergoing Ionization and Coulomb Losses |
| Bessel Function Solutions |
| Cosmic Rays as Part of the Universe |
| Our Present Viewof the Structure of the Universe |
| Cosmic Ray Isotopic and Elemental Composition |
| Formation of Particle Momentum Spectra |
| Hierarchy of Transport Equations |
| >>Note: Test Particle Approach 1 |
| The Diffusion Approximation |
| The Diffusion-Convection Transport Equation |
| Quasilinear Fokker-Planck Coefficients |
| Unperturbed Particle Orbits |
| Fokker-Planck Coefficients for Plasma Wave Turbulence |
| Calculation of Transport Parameters |
| >>Note: Test Particle Approach 2 |
| Cosmic Transport Parameters from Fast Mode Waves and Slab Alfven Waves |
| Modifications Due to Slab Alfven Waves |
| Transport Parameters in the Case of Admixture of Slab Alfven Waves to Fast Mode Waves |
| Fast Mode Wave Fokker-Planck Coefficients |
| Isotropic Fast Mode Waves |
| Cosmic Ray Mean Free Path from Fast Mode Waves |
| Cosmic Ray Momentum Diffusion Coefficient from Fast Mode Waves |
| Fast Mode Time Scale Relation |
| Parallel Propagating Magnetohydrodynamic Waves |
| Undamped Non-dispersive Alfven Waves |
| Influence of Damping and Dissipation |
| Numerical Test of Quasilinear Theory |
| Linearly Polarized Alfven Waves |
| Alfv.en Wave Fokker-Planck Coefficients |
| Magnetic Turbulence Tensors |
| Slab Linearly Polarized Alfven Turbulence |
| Isotropic Linearly Polarized Alfven Waves |
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