By Bruce T. Tsurutani, Robert G. Stone
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Published by means of the yankee Geophysical Union as a part of the Geophysical Monograph Series.
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Extra resources for Collisionless Shocks in the Heliosphere: Reviews of Current Research
A. Dulk, L. L. House, R. Illing, C. Sawyer, W. J. Wagner, D. J. McLean, and E. Hildner, Type II bursts, shock waves, and coronal transients: The event of 1980 June 29, 0233 UT, Astron. , 134, 222, 1984. Gergely, T. , Mass ejections from the solar corona into interplanetary space, in Studies of Travelling Interplanetary Phenomena/1977, edited by M. A. , p. 3, D. , 1977. , J. T. Gosling, R. M. MacQueen, R. H. Munro, A. I. Poland, and C. L. Ross, The large coronal transient of 10 June 1973, I, Observational description, Sol.
Helios observations of the earthwarddirected mass ejection of 27 November, 1979, Sol. , 95, 363, 1985. Jackson, B. , and E. Hildner, Forerunners: Outer rims of solar coronal transients, Sol. , 60, 155, 1978. Jackson, B. , and K. V. Sheridan, Evidence for a peak in the number of isolated type III bursts prior to large solar flares, Proc. Astron. Soc. , 3, 383, 1979. Jackson, B. , K. V. Sheridan, G. A. Dulk, and D. J. McLean, A possible association of solar type III bursts and white light transients, Proc.
35 BOUGERET is still unclear. Coordinated observations are essential to an analysis of the many-faceted aspects of shock formation and evolution in the corona; but despite all the observers' efforts they may sometimes be deceptive. For instance, no single Moreton wave phenomenon has been observed during the SMM operations as yet, and there are very few associations in position and time of type II bursts with CME's. A frequently cited example is the correlation between Moreton waves with type II bursts [Smith and Harvey, 1971], which jumped from 25% before 1963 to 52% after 1963 and is presently up to 70%.