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Coronal Hole Flux Tubes and the Problem of Relating Interplanetary and Solar Features

Published online by Cambridge University Press:  12 April 2016

S. Bravo
S. Bravo*
Affiliation:
Instituto de Geofísica, UNAM Coyoacán, D.F., 04510México

Abstract

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Coronal flux tubes have in general very large divergence, and the properties of their flow vary greatly inside the flux tube. We present here a general description of the evolution and the characteristics of coronal holes and discuss how these characteristics may lead to erroneous associations between interplanetary and solar structures.

Keywords

Coronal holesSolar wind sources
Type
Quasi-Static Structures
Information
International Astronomical Union Colloquium , Volume 154: Solar and Interplanetary Transients , 1996 , pp. 113 - 121
Copyright
Copyright © Kluwer 1997

References

Altshuler, M.D. and Newkirk, G.: 1969, Solar Phys. 9, 131.CrossRefGoogle Scholar
Bravo, S. and Mendoza, B.: 1989, Astrophys. J. 338, 1171.CrossRefGoogle Scholar
Durney, B.R. and Pneuman, G.W.: 1975, Solar Phys. 40, 461 CrossRefGoogle Scholar
Hakamada, K.: 1987, J. Geophys. Res. 92, 4339.CrossRefGoogle Scholar
Hakamada, K., and Kojima, M.: 1994, Solar Phys. 153, 419.CrossRefGoogle Scholar
Hoeksema, J.T. and Scherrer, P.H.: 1986, The Solar Magnetic Field 1976 trhough 1985, World Data Center A for Solar Terrestrial Physics, Report UAG-94Google Scholar
Levine, R.C., Altschuier, M.D., Harvey, J.W., and Jackson, B.V.: 1977a, Astrophys. J. 215, 636.CrossRefGoogle Scholar
Levine, R.C., Altschuier, M.D., and Harvey, J.W.: 1977b, J. Geophys. Res 82, 1061.CrossRefGoogle Scholar
Pneuman, G.W.: 1973, Solar Phys. 28, 247.CrossRefGoogle Scholar
Pneuman, G.W.: 1976, J. Geophys. Res. 81, 5049.CrossRefGoogle Scholar
Pneuman, G.W. and Kopp, R.A.: 1971, Solar Phys. 18, 258.CrossRefGoogle Scholar
Shatten, K., Wilcox, J.W., and Ness, N.F.: 1969, Solar Phys. 6, 442.CrossRefGoogle Scholar
Sykora, J., Ambroz, P. and Badalyan, O.G.: 1994, Adv. Space. Res. 14(4), 69.CrossRefGoogle Scholar
Wang, Y.M. and Sheeley, N.R. Jr.: 1991, Astrophys. J. 372, 145.CrossRefGoogle Scholar
Wang, Y.M. and Sheeley, N.R. Jr.: 1992, Astrophys. J. 392, 310.CrossRefGoogle Scholar