Astrophysical plasmas

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  • This book provides readers with a clear progress to theoretical and observational astrophysics. It is not surprising that astrophysics is continually growing because very sophisticated telescopes are being developed and they bring the universe closer and make it accessible. Astrophysics Book presents a unique opportunity for readers to demonstrate processes do occur in Nature.

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  • The inner magnetosphere is an important region of space plasma because it is one of the “kitchens” for space weather effects. The scientific understanding of this region is important for predicting the interaction between space environmental conditions and human activities. The inner magnetospheric plasma is a unique composition of different plasma particles and waves. It covers a huge plasma energy range with spatial and time variations of many orders of magnitude.

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  • This textbook is intended as an introduction to the physics of solar and stellar coronae, emphasizing kinetic plasma processes. It is addressed to observational astronomers, graduate students, and advanced undergraduates without a background in plasma physics. Coronal physics is today a vast field with many different aims and goals. Sorting out the really important aspects of an observed phenomenon and using the physics best suited for the case is a formidable problem.

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  • In recent years many efforts have been devoted to the search for the Quark Gluon Plasma, a new, deconfined phase of hadronic matter, through ultrarelativistic heavy ion collisions. In 1986 the Alternate Gradient Synchrotron in Brookhaven started accelerating nuclei, thus beginning the Era of high energy nucleus-nucleus collisions. Since then, many experiments developed, with increasing luminosity and energy of the ion beams: the Large Hadron Collider, expected to be completed by 2007 at CERN will allow to study Pb-Pb collisions at y/s ~ 5.5 TeV/nucleon....

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  • We present the proceedings from the workshop entitled Scientific Detectors for Astronomy 2005, a weeklong meeting held in Taormina, Sicily during 19-25 June 2005. This was the sixth workshop of this series, and the fourth with hardcover proceedings. By all measures, this workshop surpassed the previous meetings. The primary purpose of any technical meeting is the exchange of scientific and engineering information.

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  • This report originated in 1999 as a result of discussions between the Committee on Solar and Space Physics (CSSP) and officials within NASA’s Office of Space Science Sun- Earth Connections program. As noted in the statement of task (Appendix A), the objective of the study was to provide a scientific assessment and strategy for the study of magnetized plasmas in the solar system. By emphasizing the connections between locally occurring (solar system) structures and processes and their astrophysical counterparts, the study would contribute to a unified view of cosmic plasma behavior.

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  • The Committee on High Energy Density Plasma Physics was established in April 2001 by the National Research Council’s (NRC’s) Board on Physics and Astronomy to identify scientific opportunities and develop a unifying theme for research on matter under extreme high energy density conditions.

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