• ВХОД

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    Полное описание

    Aschwanden, M. Self-Organized Criticality in Astrophysics : the Statistics of Nonlinear Processes in the Universe / by Markus Aschwanden. - Berlin ; Heidelberg : Imprint: Springer,, 2011. - on-line. - (Springer Praxis Books). - URL: http://dx.doi.org/10.1007/978-3-642-15001-2. - Загл. с экрана. - ISBN 978-3-642-15001-2. - Текст : электронный.
    Содержание:
    1 Self-Organized Criticality in the Universe -- 2 Numerical SOC Models -- 3 Statistics of Random Processes -- 4 Time Series Analysis -- 5 Time Scale Distributions -- 6 Waiting Time Distributions -- 7 Occurrence Frequency Distributions -- 8 Fractal Geometry -- 9 Scaling Laws -- 10 Physical SOC Models in Astrophysics.

    ГРНТИ УДК
    41.17524

    Рубрики:
    physics
    geophysics
    astronomy
    astrophysics
    cosmology
    space sciences
    statistical physics
    dynamical systems
    statistics
    physics
    astronomy, Astrophysics and Cosmology
    statistical Physics, Dynamical Systems and Complexity
    geophysics/Geodesy
    extraterrestrial Physics, Space Sciences
    statistics for Engineering, Physics, Computer Science, Chemistry and Earth Sciences

    Аннотация: The concept of ‘self-organized criticality’ (SOC) has been applied to a variety of problems, ranging from population growth and traffic jams to earthquakes, landslides and forest fires. The technique is now being applied to a wide range of phenomena in astrophysics, such as planetary magnetospheres, solar flares, cataclysmic variable stars, accretion disks, black holes and gamma-ray bursts, and also to phenomena in galactic physics and cosmology. Self-organized Criticality in Astrophysics introduces the concept of SOC and shows that, due to its universality and ubiquity, it is a law of nature. The theoretical framework and specific physical models are described, together with a range of applications in various aspects of astrophyics. The mathematical techniques, including the statistics of random processes, time series analysis, time scale and waiting time distributions, are presented and the results are applied to specific observations of astrophysical phenomena.

    http://dx.doi.org/10.1007/978-3-642-15001-2


    Держатели документа:
    Государственная публичная научно-техническая библиотека России : 123298, г. Москва, ул. 3-я Хорошевская, д. 17 (Шифр в БД-источнике (KATBW): -594057879)

    Шифр в сводном ЭК: 3351b25eb3a395832e7c18af754c9123



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