4.9 Summary
The magnetosphere is a very complex system. Here we have presented some qualitative insight into the coupling of parts of the system with emphasis on those controlled by the solar wind. We still continue to improve our understanding of the magnetosphere with the study of existing databases, with the development of various types of numerical models, and with the development of new and more sophisticated instruments and missions. We have learned much about the magnetosphere in the last half century since the beginning of the International Geophysical Year in 1957. It has been important to do so because our increasingly technological society has moved critical systems into space for monitoring weather, for communnication, and for global monitoring of the health of the planet and the activities of one’s neighbours. It is clear that if we are to use space as much as our present plans foretell, we must continue to improve our understanding of this environment and how it works, and be able to predict its behaviour given knowledge of interplanetary conditions.
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4.11 References
Burton, R. K., R. L. McPherron, and C. T. Russell, An empirical relationship between interplanetary conditions and Dst., J. Geophys. Res., 80(31), 4204–4214, 1975.
Burton, R. K., R. L. McPherron, and C. T. Russell, The terrestrial magnetosphere: A half-wave rectifier of the interplanetary electric field, Science, 189(4204), 717–718, 1975.
Dessler, A. J., and E. N. Parker, Hydromagnetic theory of magnetic storms, J. Geophys. Res., 64, 2239–2259, 1959.
Dungey, J. W., Interplanetary magnetic field and the auroral zones, Phys. Rev. Lett., 6, 47–48, 1961.
Dungey, J. W., The structure of the exosphere or adventures in velocity space, Geophysics: The Earth’s Environment, C. Dewitt, J. Hieblot and A. Lebeau, editors, New York, Gordon and Breach: 505–550, 1963.
McPherron, R. L., C. T. Russell, and M. P. Aubry, Satellite studies of magnetospheric substorms on August 15, 1968. IX. Phenomenological model for substorms, J. Geophys. Res., 78, 3131–3149, 1973.
Petrinec, S. M. and C. T. Russell, Investigations of hydrodynamic and magneto-hydrodynamic equations across the bow shock and along the outer edge of planetary obstacles, Adv. Space Res., 20, 743–746, 1997.
Russell, C. T. and R. L. McPherron, The magnetotail and substorms, Space Sci. Rev., 15, 205–266, 1973.
Russell, C. T. and R. L. McPherron, Semiannual variation of geomagnetic activity, J. Geophys. Res., 78, 92–108, 1973.
Russell, C. T., Y. L. Wang, and J. Raeder, Possible dipole tilt dependence of dayside magnetopause reconnection, Geophys. Res. Lett., 30(18), 1937, doi:10.1029/2003GL017725, 2003.
Scholer, M., I. Sidorenko, C. H. Jaroschek, R. A. Treumann, and A. Zeiler, Onset of collisionless magnetic reconnection in thin current sheets: three-dimensional particle simulations, Physics of Plasmas, 10, 3521–3527, 2003.
Sckopke, N., A general relation between the energy of trapped particles and the disturbance field near the Earth, J. Geophys. Res., 71, 3125, 1966.
Spreiter, J. R., A. L. Summers, and A. Y. Alksne, Hydromagnetic flow around the magnetosphere, Planet. Space Sci., 14, 223–253, 1966.
Wang, Y. L., J. Raeder, and C. T. Russell, Plasma depletion layer: The role of the slow mode waves, Ann. Geophys., 22, 4259–4272, 2004.
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© 2007 Praxis Publishing Ltd, Chichester
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Russell, C.T. (2007). The coupling of the solar wind to the Earth’s magnetosphere. In: Space Weather- Physics and Effects. Springer Praxis Books. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-34578-7_4
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