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The effect of plume/interplume lanes on ion-cyclotron resonance heating

Published online by Cambridge University Press:  08 June 2011

Suzan Doğan  and
E. Rennan Pekünlü
Suzan Doğan
Affiliation:
Department of Astronomy and Space Sciences, Faculty of Science, University of Ege, Bornova, 35100, İzmir, Turkey email: [email protected], [email protected]
E. Rennan Pekünlü
Affiliation:
Department of Astronomy and Space Sciences, Faculty of Science, University of Ege, Bornova, 35100, İzmir, Turkey email: [email protected], [email protected]
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Abstract

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The effect of the Plume/Interplume Lane (PIPL) structure of the solar North Polar Coronal Hole (NPCH) on the ion-cyclotron resonance (ICR) process is investigated. The ICR process in the interplume lanes is much more effective than in the plumes, agreeing with the observations which show the source of fast solar wind is interplume lanes.

Keywords

Sun: coronasolar windacceleration of particlesplasmaswaves
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S274: Advances in Plasma Astrophysics , September 2010 , pp. 137 - 139
Copyright
Copyright © International Astronomical Union 2011

References

Cranmer, S. R., Panasyuk, A. V., & Kohl, J. L. 2008, ApJ, 678, 1480CrossRefGoogle Scholar
Hollweg, J. V. 1999a, JGR, 104, 24781CrossRefGoogle Scholar
Hollweg, J. V. 1999b, JGR, 104, 24793CrossRefGoogle Scholar
Hollweg, J. V. 1999c, JGR, 104, 505CrossRefGoogle Scholar
Kohl, J. L., Noci, G., Antonucci, E. et al. . 1997, SoPh, 175, 613Google Scholar
Wilhelm, K., Marsch, E., Dwivedi, B. N. et al. . 1998, ApJ, 500, 1023CrossRefGoogle Scholar