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Extra resources for Cross-Scale Coupling in Space Plasmas
AndB. , 8, 1253, 1981. FluidsB, 5, 2646, 1993. mechanismandthe relationshipof the mechanisms to each other.
1988; Seyler, 1990]. Another feature of the evolution is to generate steep density gradients and associatedlocal velocity shear due to nonlinear convective effects. As shownin the simulationsof the KH instability[seeFig. , 1994b], the initial density gradient is convected by the waves and locally steepened. These steepeneddensitystructuresremain quasisteadyover the time scalesassociated with the low frequencywave. As the scalesize of the densitystructuresbecomecomparableto or smallerthan an ion gyrodiameter,an ambipolarelectric field is self-consistentlydeveloped.
99, 121, 1994. Reasoner,D. , P. D. Craven, and C. R. Chappell, Characteristics of low-energy plasma in the plasmasphere and plasma trough, J. , 88, 7913, 1983. Retterer, J. , T. Chang, and J. R. Jasperse,Transversely accelerated ions in the topside ionosphere, J. , 99, 13,189, 1994. , S. Perraut, J. L. Rauch, C. de Villedary, G. Kremser, A. Korth,andD. ;r. Young, Wave-particle interactions near •He+ observedon board G EOS I and 2; 2. Generationof ion cyclotronwavesand heatingof He+ ions,J. Geophys.