The Theory of Cosmic Ray Modulation - Edition 1 - By Du Toit Strauss and Nicolas Eugene Engelbrecht Elsevier Educate

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The Theory of Cosmic Ray Modulation,

Edition 1

By Du Toit Strauss and Nicolas Eugene Engelbrecht

Publication Date: 01 Jun 2026

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The Theory of Cosmic Ray Modulation concretely lays out the current understanding of cosmic ray particle interactions, offering a comprehensive introduction to the underlying theory, observational data, and practical applications that have implications for various fields, including high-energy astrophysics, space weather, and cosmogenic isotope studies. The book provides a solid theoretical foundation, explaining the physical processes involved in cosmic ray modulation. It delves into mathematical details with meticulous explanations and applies them to topics ranging from the implications of cosmic rays in space-based anti-matter research to their role in studying solar variability over timescales, and even in planetary habitability.

This book not only provides a solid foundation for research but also offers wider perspectives on the impact of cosmic rays in our understanding of the universe. With its strong underlying theory and up-to-date coverage, it is a must-read for anyone actively working in the field of cosmic rays or on fields influenced by charged particle physics.

Key Features

Provides an essential starting point in the field of cosmic ray transport, including detailed explanations of underlying physical processes
Includes observational data and current understandings on specific topics such as cosmic ray diffusion, drift, and turbulence.
Covers mathematical expressions, derivations, and equations that describe the behavior of cosmic rays and their modulation processes
Bridges the gap between plasma physics and space weather, making it an indispensable resource for space scientists seeking to understand the complexities of cosmic ray dynamics

About the author

By Du Toit Strauss, Professor of physics, North-West University, South Africa and Nicolas Eugene Engelbrecht, Professor in Physics, North-West University, South Africa

Introduction
The Turbulent Heliosphere
1. The active Sun
2. The Solar Wind
3. The Heliospheric Magnetic Field
4. The Heliospheric Current Sheet
5. The Global Heliosphere
  1. The Supersonic Solar Wind
  2. The Termination Shock and Inner Heliosheath
  3. The Heliopause and Outer Heliosheath
6. Turbulence
  1. Some useful concepts from hydrodynamic turbulence
  2. Solar wind turbulence
  3. Selected turbulence observations in the solar wind
7. Closing remarks
8. References
Cosmic Rays
1. Time-dependent variations
  1. Neutron monitors
  2. 11 and 22 year variations
  3. 27 day recurrent variations
  4. Forbush decreases
  5. Daily variations
2. Galactic Cosmic Rays
  1. Modulation through the heliosphere
  2. Modulation and spectral changes
  3. Latitudinal gradients and other features
  4. Drift effect and anti-particles
3. Anomalous Cosmic Rays
4. Jovian electrons
5. Solar Energetic Particles and Other Species
6. References
Cosmic ray transport equations
1. Introduction
2. The distribution function in phase space
3. Transforming Between Different Coordinate Systems
  1. The Forman Transformations
  2. The Compton-Getting Transformation
4. Towards Observational Quantities
  1. A note on the relativistic energy calculations
5. The Parker Transport Equation
  1. The Continuity Equation
  2. The Webb & Gleeson Approach
  3. A note on Liouville’s theorem
6. The Parker Transport Equation in Spherical Coordinates
7. Hierarchy and Validity of Different Approximations
  1. Diffusion-convection Approximation
  2. Force-field Approximation
8. Limitations of the Parker Equation
9. Closing remarks
10. References
Diffusion
1. The basics of diffusion
2. Ascertaining diffusion coefficients
  1. Deriving Diffusion Coefficients from Cosmic Ray Measurements
  2. Simulating Diffusion Coefficients
3. Pitch angle diffusion
  1. Quasi-linear theory
  2. Wave-particle scattering
  3. A note on gyro-resonances
  4. The relationship to parallel transport
4. Parallel diffusion
5. Perpendicular diffusion
  1. Fieldline random walk
  2. Non-linear guiding center theory
6. Discussion
7. References
Drift Effects
1. Basic drift theory
  1. Current Sheet Drift
  2. Electric Field Drift
2. The Combined Drift and Diffusion Tensor
3. Drift Reduction Due to Turbulence
  1. Numerical Test Particle Simulations
  2. Modelling the influence of turbulence
4. Modelling drift effects
5. Drifts in a Parker field
6. Drifts in Cosmic Ray Observations
7. Discussion
8. References
Adiabatic Energy Changes
1. Introduction
2. Thermodynamic Approach: Particles in a Box
3. From First Principles: Charged particle propagation in a plasma
  1. Betatron effect
  2. Inverse Fermi effect
  3. Adiabatic energy loss rate
  4. The adiabatic limit
4. Diffusive Shock Acceleration
  1. Solutions from the Parker equation
5. Discussion
6. References
Concluding Remarks