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IPS Observations of Flare-Generated Disturbances

Published online by Cambridge University Press:  14 August 2015

Takashi Watanabe
Takashi Watanabe*
Affiliation:
Space Environment Laboratory, NOAA/ERL Boulder, Colorado 80303, U.S.A.

Abstract

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Dynamical behaviour of a flare-generated disturbance can be followed by IPS observations through a comparison between the IPS observations and a model of the disturbance. The highly turbulent post-shock plasma can be attributed to the contact surface of the disturbance. Two examples of IPS observations of flare-generated disturbances will be discussed.

Type
Part V. Coronal and Interplanetary Responses to Short Time Scale Phenomena: - Observations
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 409 - 412
Copyright
Copyright © Reidel 1980 

References

Dryer, M.: 1972, in Sonett, C.P., Coleman, P.J. Jr., and Wilcox, J.M. (eds.) Solar Wind, NASA SP-308, pp. 453–465.Google Scholar
Kakinuma, T., and Watanabe, T.: 1976, Space Sci. Rev., 19, pp. 611–627.Google Scholar
Mihalov, J.D.: 1979, Communicated.Google Scholar
Smith, E.J.: 1976, Space Sci. Rev., 19, pp. 661–686.Google Scholar
Watanabe, T.: 1977, in Shea, M.A., Smart, D.F., and Wu, S.T. (eds.) Contributed Papers to the Study of Travelling Interplanetary Phenomena/1977 (Proceedings of COSPAR Symposium B, Tel Aviv, Israel, June 1977), AFGL-TR-77-0309, pp. 139–149.Google Scholar
Wolfe, J., Intriligator, D.S., Mihalov, J., Collard, H., McKibbin, D., and Whitten, R.: 1979, Science, 203, pp. 750–752.Google Scholar