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Transport of open magnetic flux between solar polar regions

  • Alexei A. Pevtsov (a1) and Valentyna I. Abramenko (a2)
Abstract

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.

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Copyright
References
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Durrant, C. J. & Wilson, P. R. 2003, Solar Phys., 214, 23
Harvey, K. L. & Recely, F. 2002, Solar Phys., 211, 31
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, 229
Karachik, N., Pevtsov, A. A., & Sattarov, I. 2006, ApJ, 642, 562
Pevtsov, A. A., Balasubramaniam, K. S., & Rogers, J. W. 2003, ApJ, 595, 500
Wang, Y.-M. & Sheeley, N. R. 2004, ApJ, 612, 1196
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Proceedings of the International Astronomical Union
  • ISSN: 1743-9213
  • EISSN: 1743-9221
  • URL: /core/journals/proceedings-of-the-international-astronomical-union
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