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 through the yank Geophysical Union as a part of the Geophysical Monograph Series.

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By Bruce T. Tsurutani, Robert G. Stone

About The Product

Published through the yank Geophysical Union as a part of the Geophysical Monograph Series.

Content:

Show description

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And R. R. Fisher, The kinetmatics of solar inner coronal transients, Sol. , 89, 89, 1983. Malitson, H. , J. Fainberg, and R. G. Stone, Observation of a type II solar radio burst to 37 R o, Astrophys. , 14, 111, 1973a. Malitson, H. , J. Fainberg, and R. G. Stone, A density scale for the interplanetary medium from observations of a type II solar radio burst out to 1 AU, Astrophys. , 183, L35, 1973b. Martin, S. , A moving emission front with the flare of 4 Sept. 1973, 1826 UT, (abstract), Bull. Am.

T) Fig. 8. The intensity of solar radio bursts observed at a number of frequencies by the ISEE 3 radio experiment. The bottom panel shows groups of ordinary type III bursts. The horizontal bars along the time axis represent the duration of associated water wavelength type III groups. , 1981]. Since its discovery by Hewish et al. [1964], interplanetary scintillation (hereinafter IPS) of celestial radio sources due to turbulence along the line of sight has been recognized as a powerful method for investigating the solar wind and the small-scale structure of the interplanetary medium.

Webb, Soft X-ray observations of large-scale coronal active region brightenings, Sol. , 54, 403, 1977. Rust, D. , Mass ejections, in Solar Flares, A Monograph From Skylab Workshop II, edited by P. Sturrock, pp. , 1980. Sawant, H. , T. E. Gergely, and M. R. Kundu, Positions of type II fundamental and harmonic sources in the 30-100 MHz range, Sol. , 77, 249, 1982. , R. Howard, N. R. , M. Koomen, and D. Michels, Major mass ejection rate from three space coronographs, Bull. Am. Astron. , 15, 706, 1983.

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