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Transport of open magnetic flux between solar polar regions

Published online by Cambridge University Press:  26 February 2010

Alexei A. Pevtsov  and
Valentyna I. Abramenko
Alexei A. Pevtsov
Affiliation:
National Solar Observatory, Sunspot, NM 88349, U.S.A. email: [email protected]
Valentyna I. Abramenko
Affiliation:
Big Bear Solar Observatory, New Jersey Institute of Technology, Big Bear City, CA 92314-9672, U.S.A. email: [email protected]
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Abstract

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We present the observations of coronal hole that has originated at the polar hole in one hemisphere, extended to equatorial region, got disconnected and transported across the equator to polar region of opposite hemisphere.

Keywords

Sun: magnetic fieldsSun: activitySun: coronaSun: photosphere
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S264: Solar and Stellar Variability: Impact on Earth and Planets , August 2009 , pp. 210 - 212
Copyright
Copyright © International Astronomical Union 2010

References

Durrant, C. J. & Wilson, P. R. 2003, Solar Phys., 214, 23Google Scholar
Harvey, K. L. & Recely, F. 2002, Solar Phys., 211, 31Google Scholar
Jones, H. P. 2005, in: Sankarasubramanian, K., Penn, M., & Pevtsov, A. (eds.) Large-scale Structures and their Role in Solar Activity, Astron. Soc. Pac. CS-346, 229Google Scholar
Karachik, N., Pevtsov, A. A., & Sattarov, I. 2006, ApJ, 642, 562Google Scholar
Pevtsov, A. A., Balasubramaniam, K. S., & Rogers, J. W. 2003, ApJ, 595, 500Google Scholar
Wang, Y.-M. & Sheeley, N. R. 2004, ApJ, 612, 1196Google Scholar