TAILIEUCHUNG - Plasma Physics of the Local Cosmos

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. An additional objective was to relate basic scientific studies of plasmas to studies of the Sun’s influence. | Plasma Physics of the Local Cosmos Committee on Solar and Space Physics Space Studies Board The National Academies Press Plasma Physics of the Local Cosmos Committee on Solar and Space Physics Space Studies Board Division on Engineering and Physical Sciences NATIONAL RESEARCH COUNCIL OF THE NATIONAL ACADEMIES THE NATIONAL ACADEMIES PRESS Washington . THE NATIONAL ACADEMIES PRESS 500 Fifth Street . Washington DC 20001 NOTICE The project that is the subject of this report was approved by the Governing Board of the National Research Council whose members are drawn from the councils of the National Academy of Sciences the National Academy of Engineering and the Institute of Medicine. The members of the committee responsible for the report were chosen for their special competences and with regard for appropriate balance. This study was supported by Contracts NASW-96013 and NASW-01001 between the National Academy of Sciences and the National Aeronautics and Space Administration. Any opinions findings conclusions or recommendations expressed in this publication are those of the author s and do not necessarily reflect the views of the agency that provided support for the project. International Standard Book Number 0-309-09215-9 POD International Standard Book Number 0-309-53215-9 PDF Cover Top The aurora australis southern lights photographed from the International Space Station on April 18 2003. Courtesy of Earth Sciences and Image Analysis Laboratory NASA Johnson Space Center. Bottom Conceptual representation of the heliosphere and the solar system s immediate galactic environment. Distances in astronomical units AU are indicated on a logarithmic scale. 1 AU is the mean distance between the Sun and the Earth or roughly 150 000 000 kilometers. Courtesy of P. Liewer Jet Propulsion Laboratory and R. Mewaldt California Institute of Technology . Copies of this report are available free of charge from Space Studies Board National Research Council 500 Fifth .

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