Magnetohydrodynamic Processes in Solar Plasmas 1st Edition

Grab the forefront of solar physics with Magnetohydrodynamic Processes in Solar Plasmas, 1st Edition by Abhishek Kumar Srivastava, Marcel Goossens, and Iñigo Arregui. This authoritative volume delivers a rigorous, accessible treatment of magnetohydrodynamic (MHD) phenomena that shape the Sun’s dynamic atmosphere — an essential read for anyone working on solar plasmas, coronal seismology, or space weather.

Begin a deep dive into the fundamental theory and modern applications: wave propagation and damping, instabilities, nonlinear MHD behavior, and the latest approaches to modeling and observation. Rich with clear derivations, illustrative figures, and real-case solar examples, the book bridges analytical insight and observational diagnostics to explain how MHD processes govern the corona, chromosphere, and solar wind.

Designed for graduate students, researchers, and professional solar physicists, this volume helps translate complex MHD concepts into practical tools for data interpretation and prediction. Whether you’re advancing coronal heating theories, analyzing oscillations from spaceborne telescopes, or developing models for forecasting space weather, you’ll find focused chapters that accelerate understanding and inspire new research directions.

Beloved by the global solar physics community — from university classrooms to research centers and observatories across Europe, Asia, and the Americas — this 1st Edition is both a primary textbook and a long-term reference. Add Magnetohydrodynamic Processes in Solar Plasmas to your library to stay at the cutting edge of MHD research and solar exploration. Order now to enrich your work with a definitive, practice-oriented guide to the physics powering our star.

Note: eBooks do not include supplementary materials such as CDs, access codes, etc.