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Markus Aschwanden

    Self-organized criticality in astrophysics
    Particle Acceleration and Kinematics in Solar Flares
    Physics of the solar corona
    • A thorough introduction to solar physics based on recent spacecraft observations. The author introduces the solar corona and sets it in the context of basic plasma physics before moving on to discuss plasma instabilities and plasma heating processes. The latest results on coronal heating and radiation are presented. Spectacular phenomena such as solar flares and coronal mass ejections are described in detail, together with their potential effects on the Earth.

      Physics of the solar corona
    • Particle Acceleration and Kinematics in Solar Flares

      A Synthesis of Recent Observations and Theoretical Concepts

      • 236bladzijden
      • 9 uur lezen

      Recent advancements in solar flare physics are explored through high-resolution imaging from spacecraft like Yohkoh, SoHO, and TRACE, alongside high-energy photon data from the Compton GRO. This review addresses the historical divide between traditional astronomical observations and modern astrophysical analysis, emphasizing the importance of quantifying physical parameters and applying theoretical models. By focusing on key physical processes such as particle acceleration and radiation signatures, it aims to enhance understanding of the underlying physics of solar flares.

      Particle Acceleration and Kinematics in Solar Flares
    • Self-organized criticality in astrophysics

      The Statistics of Nonlinear Processes in the Universe

      Markus Aschwanden introduces the concept of self-organized criticality (SOC) and shows that due to its universality and ubiquity it is a law of nature for which he derives the theoretical framework and specific physical models in this book. He begins by providing an overview of the many diverse phenomena in nature which may be attributed to SOC behaviour. The author then introduces the classic lattice-based SOC models that may be explored using numerical computer simulations. These simulations require an in-depth knowledge of a wide range of mathematical techniques which the author introduces and describes in subsequent chapters. These include the statistics of random processes, time series analysis, time scale distributions, and waiting time distributions. Such mathematical techniques are needed to model and understand the power-law-like occurrence frequency distributions of SOC phenomena. Finally, the author discusses fractal geometry and scaling laws before looking at a range of physical SOC models which may be applicable in various aspects of astrophysics. Problems, solutions and a glossary will enhance the pedagogical usefulness of the book. SOC has been receiving growing attention in the astrophysical and solar physics community. This book will be welcomed by students and researchers studying complex critical phenomena.

      Self-organized criticality in astrophysics