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Effect of Uniform External Pressure and Oblique Incidence of the Solar Wind on the Terminal Shape of the Geomagnetic Field

John R. SpreiterAudrey L. SummersUnited States. National Aeronautics and Space Administration

出版	National Aeronautics and Space Administration, 1963
URL	http://books.google.com.hk/books?id=585Ap1ssQKAC&hl=&source=gbs_api
EBook	FULL_PUBLIC_DOMAIN

註釋Approximate solutions and numerical results are given for the coordinates of the boundary separating the geomagnetic field from the interplanetary plasma for a ±35° range of angles between the direction of the incident stream and the geomagnetic equatorial plane for a model that assumes the plasma pressure exerted on the boundary to be composed of a dynamic pressure, proportional to the normal component of the momentum of the plasma particles, and a static pressure considered constant over the entire boundary. Results are presented for a complete range of values for the ratio between the two pressure components.