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Coronal Holes and Flare Related Phenomena

Published online by Cambridge University Press:  30 March 2016

Rajendra N. Shelke  and
M. C. Pande
Rajendra N. Shelke
Affiliation:
College of Engineering, Badnera 444 701, India
M. C. Pande
Affiliation:
U.P.State Observatory, Naini Tal 263 129, India

Abstract

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We conclude that coronal holes exhibit differential rotation and they do not follow a specific polarity rule. Further, proximity of holes to type II burst rich active regions (ARs) indicates that shock waves propagate almost along the magenetic field of the holes.

Type
Joint Commission Meetings
Information
Highlights of Astronomy , Volume 7: Highlights of Astronomy. As presented at the XIXth General Assembly of the IAU, 1985 , 1986 , pp. 759 - 760
Copyright
Copyright © Reidel 1986

References

Bohlin, J.D. and Sheeley, N.R. Jr.: 1978, Solar Phys. 56, 125.Google Scholar
Newton, H.W. and Nunn, M.L.:1951, Monthly Notices Roy. Astron. Soc. 111, 413.Google Scholar
Timothy, A.F., Krieger, A.S., And Vaiana, G.A. 1975, Solar Phys. 42, 135.Google Scholar
Uchida, Y.: 1974, Solar Phys. 39, 431.Google Scholar
Wagner, W.J. :1975, Astrophyg. 3. Letters 198, L141.Google Scholar