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The boundary conditions for the rarefaction wave are that the flow behind the wave must be accelerated toward the earth, the current density behind must be reduced, and the magnetic tension of the stretched tail field lines must be relaxed so that the field behind has a larger component normal to the neutral sheet. These boundary conditions can be satisfied by the slow hydromagnetic rarefaction wave 40 • Thus ionospheric breakup launches a slow rarefaction wave which propagates into the tail accelerating plasma and flux toward the nightside, relaxing the tail magnetic configuration, and producing an expansion of the plasma sheet.

Geophys. , 70, 1231. 15. , 1966, Planet. , 14,947. 16. , 1968, Dynamics of the Earth's Radiation Belts, Publishing House, Physical-Mathematical Literature, Moscow. 17. Y. A1ksne, 1969, Rev. of Geophysics, 7, 11. 18. F. Kennel, 1971, J. Geophys. , 76, 3055. 19. , 1968, J. Geophys. , 73, 7329. 20. F. Kennel, 1971, submitted to J. Geophys. Res. 21. T. G. Kive1son, 1970, J. Geophys. , 75, 7018. 22. , 1971, J. Geophys. , 76. 23. F. Kennel, 1971-,-submitted to J. Geophys. Res. 24. F. Ness, 1970, J. Geophys.

14,947. 16. , 1968, Dynamics of the Earth's Radiation Belts, Publishing House, Physical-Mathematical Literature, Moscow. 17. Y. A1ksne, 1969, Rev. of Geophysics, 7, 11. 18. F. Kennel, 1971, J. Geophys. , 76, 3055. 19. , 1968, J. Geophys. , 73, 7329. 20. F. Kennel, 1971, submitted to J. Geophys. Res. 21. T. G. Kive1son, 1970, J. Geophys. , 75, 7018. 22. , 1971, J. Geophys. , 76. 23. F. Kennel, 1971-,-submitted to J. Geophys. Res. 24. F. Ness, 1970, J. Geophys. , 75, 7032. 25. L. J. , 76, 1823.

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