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Interplanetary Response to Solar Long Time-Scale Phenomena

Published online by Cambridge University Press:  14 August 2015

C. D'Uston  and
J. M. Bosqued
C. D'Uston
Affiliation:
Centre d'Etude Spatiale des Rayonnements 9, avenue Colonel Roche - B.P. 4346 31029 TOULOUSE CEDEX - France
J. M. Bosqued
Affiliation:
Centre d'Etude Spatiale des Rayonnements 9, avenue Colonel Roche - B.P. 4346 31029 TOULOUSE CEDEX - France

Extract

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In this paper, we briefly review the experimental knowledge gained in the recent years on the interplanetary response to solar long-time scale phenomena such as the coronal magnetic structure and its evolution. Observational evidence that solar wind flow in the outer corona comes from the unipolar diverging magnetic regions of the photosphere is discussed along with relations to coronal holes. High-speed solar wind streams observed within the boundary of interplanetary magnetic sectors are associated with these structures. Their boundaries appear as very narrow velocity shears.

Type
Part II. Coronal and Interplanetary Responses to Long Time Scale Phenomena
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 105 - 125
Copyright
Copyright © Reidel 1980 

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