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Observation of magnetic reconnection and current sheets in the solar wind

Published online by Cambridge University Press:  26 February 2010

Pablo R. Muñoz ,
Abraham C.-L. Chian ,
Rodrigo A. Miranda  and
Michio Yamada
Pablo R. Muñoz
Affiliation:
National Institute for Space Research (INPE), São José dos Campos-SP 12227-010, Brazil email: [email protected]
Abraham C.-L. Chian
Affiliation:
National Institute for Space Research (INPE), São José dos Campos-SP 12227-010, Brazil email: [email protected] Research Institute for Mathematical Sciences (RIMS), Kyoto University, Kyoto 606-8502, Japan
Rodrigo A. Miranda
Affiliation:
National Institute for Space Research (INPE), São José dos Campos-SP 12227-010, Brazil email: [email protected] Research Institute for Mathematical Sciences (RIMS), Kyoto University, Kyoto 606-8502, Japan
Michio Yamada
Affiliation:
Research Institute for Mathematical Sciences (RIMS), Kyoto University, Kyoto 606-8502, Japan
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Abstract

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We apply single- and multi-spacecraft techniques to search for currents sheets in the solar wind during the ICME event of 21 January 2005, using the Cluster magnetic field data. Two large-scale currents sheets are detected at the leading boundary of the ICME ejecta using the single-spacecraft technique, which exhibit physical characteristics typical of magnetic reconnection exhausts in the solar wind.

Keywords

Sun: solar windcoronal mass ejections (CMEs)magnetic fields
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. 369 - 372
Copyright
Copyright © International Astronomical Union 2010

References

Chian, A. C.-L., Kamide, Y., Rempel, E. L., & Santana, W. M. 2006, J. Geophys. Res. 111, A07S03, doi:10.1029/2005JA011396.Google Scholar
Chian, A. C.-L. & Miranda, R. A. 2009, Ann. Geophys. 27, 1789.CrossRefGoogle Scholar
Dunlop, M. W., Balogh, A., Glassmeier, K. H., & Robert, P. 2002, J. Geophys. Res-Space Phys. 107, A11, 1384.Google Scholar
Foullon, C., Owen, C. J., Dasso, S., et al. . 2007, Sol. Phys. 244, 139.CrossRefGoogle Scholar
Gosling, J. T., Skoug, R. M., McComas, D. J., & Smith, C. W. 2005, J. Geophys. Res.-Space Phys. 110, A01107.CrossRefGoogle Scholar
Li, G. 2008, ApJ (Letters) 672, L65.CrossRefGoogle Scholar
Li, G., Lee, E., & Parks, G. 2008, Ann. Geophys. 26, 1889.CrossRefGoogle Scholar
Nishida, A. 2007, in: Kamide, Y., & Chian, A. C.-L. (eds.) Handbook of the Solar-Terrestrial Environment (Berlin, Springer), p. 280.Google Scholar
Priest, E. R. 2007, in: Kamide, Y. & Chian, A. C.-L. (eds.) Handbook of the Solar-Terrestrial Environment (Berlin, Springer), p. 50.Google Scholar
Retinò, A., Sundkvist, D., & Vaivads, A., et al. 2007, Nature Phys. 3, 236.CrossRefGoogle Scholar
Sonnerup, B. U. O. & Cahill, L. J., 1967, J. Geophys. Res. 72 (1), 171.CrossRefGoogle Scholar
Sonnerup, B. U. O. et al. 1981, J. Geophys. Res. 86, 10049.CrossRefGoogle Scholar
Sundkvist, D.Retinò, A., Vaivads, A., & Bale, S. D. 2007, Phys. Rev Lett. 99, 025004.CrossRefGoogle Scholar