Collisionless Shocks in the Heliosphere: Reviews of Current by Bruce T. Tsurutani, Robert G. Stone

By Bruce T. Tsurutani, Robert G. Stone

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Published via the yankee Geophysical Union as a part of the Geophysical Monograph Series.


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Fig. 9. Schematic diagram showing the location of the dominant scattering zones along the line of sight and two examples of interplanetary disturbances inferred by Gapper et al. [1982]: corotating (left) and transient (right) disturbances, the latter being sketched for several consecutive days. S, E denote the sun, earth. tinuously over a wider range of solar elongations (Figure 9). Both a corotating stream and a transient shell were observed in the form of long-lived enhancements of scintillations which were identified with regions of compressed plasma moving outward in front of high-speed regions later observed at I AU.

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NASA SPo342, 577, 1973. D. Altschuler, and G. , Flareproduced coronal MHDofast mode wavefronts and Moo reton's wave phenomenon, Sol. , 28, 495, 1973. Vlasov, V. , Radio imagery of the turbulent interplanetary plasma, Sov. , Engl. , 23, 55, 1979. Wagner, W. , SERF studies of mass motions arising in flares, Adv. , 2, 203, 1983. Wagner, W. , and R. M. MacQueen, The excitation of type II radio bursts in the corona, Astron. , 120, 136, 1983. Ward, B. , Interplanetary scintillation and flareproduced disturbances, Proc.

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