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Nonlinear cosmic ray diffusion theories par Shalchi,, Andreas. Publication : [S.l.] Springer 2009 . 212 p. , This book deals with the physics of cosmic ray diffusion theory, focusing on the physics of nonlinear transport of cosmic rays through turbulent interplanetary or interstellar plasma. The author discusses fundamental processes such as cosmic ray propagation and acceleration in the solar system or in interstellar space, the properties of such plasmas, the standard quasilinear approach to describing plasma-particle interactions as well as several more accurate nonlinear theories. Within a nonlinear treatment he revisits the mechanism of diffusive shock acceleration, which is responsible for the high cosmic ray energies. Based on new results presented in this book the author proposes future numerical, theoretical and observational research that could advance the field of cosmic ray diffusion theory. 25 cm. Date : 2009 Disponibilité : Exemplaires disponibles: La bibliothèque des Sciences Exactes et Naturelles (1),

Solar neutrons and related phenomena par Dorman, Lev Publication : [S.l.] Springer 2010 . xlvi, 873 p. , This book presents the first comprehensive compilation and review of the extensive body of experimental and theoretical material on solar neutrons and related phenomena published in the scientific literature over the last sixty years. Phenomena related to solar neutrons are more specifically: - the decay products of solar neutrons - solar gamma rays generated in processes like nuclear reactions between solar energetic charged particles and matter of the solar atmosphere, as well as by the capture of solar neutrons by hydrogen atoms in the solar atmosphere - the propagation of solar neutrons, solar gamma rays and other secondary particles through the solar photosphere, chromosphere and corona, as well as through interplanetary space and through the Earth's atmosphere. Models and simulations of particle acceleration, interactions, and propagation processes show that observations of solar neutrons and gamma rays in space and in the Earth's atmosphere yield essential and unique information on the source function of energetic solar particles, as well as on the chemical composition and density distribution of plasma in the solar atmosphere. The results described in the book may also be useful for astrophysical studies of other stars and different astrophysical objects, as well as for space weather problems. The book will serve as a reference work for researchers and students in solar physics, plasma, neutron, and gamma ray physics, as well as in cosmic ray physics, space science, geophysics and those researching space weather problems. 24 cm. Date : 2010 Disponibilité : Exemplaires disponibles: La bibliothèque des Sciences Exactes et Naturelles (1),

Turbulence and Self-Organization Modeling Astrophysical Objects / par Marov, Mikhail Ya. Publication : . XXVIII, 657 p. Disponibilité :  http://dx.doi.org/10.1007/978-1-4614-5155-6,

Cosmic Electrodynamics Electrodynamics and Magnetic Hydrodynamics of Cosmic Plasmas / par Fleishman, Gregory D. Publication : . XXII, 712 p. 117 illus., 36 illus. in color. Disponibilité :  http://dx.doi.org/10.1007/978-1-4614-5782-4,

The Stars of Galileo Galilei and the Universal Knowledge of Athanasius Kircher par Buonanno, Roberto. Publication : . XIII, 178 p. 28 illus. Disponibilité :  http://dx.doi.org/10.1007/978-3-319-00300-9,

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