Abstract
The three-component model of magnetic field fluctuations is applied to the analysis of the wave number spectra to study fluctuations in the solar wind, the foreshock, and the magnetosheath. The analysis exhibits a transition of the dominant fluctuation component from the solar wind to the magnetosheath, from the two-dimensional to the Alfvénic in the foreshock, and to the compressible component in the magnetosheath.
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Acknowledgements
The work of YN and KHG in Braunschweig was supported by Bundesministerium für Wirtschaft und Technologie and Deutsches Zentrum für Luft- und Raumfahrt, Germany, under contract 50OC0103. We thank H. Rème and I. Dandouras for providing ion data of Cluster. The work of SPG was supported by the Los Alamos National Laboratory LDRD Program and by the NASA Solar and Heliospheric SR&T Program.
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Narita, Y., Glassmeier, KH., Gary, S.P., Goldstein, M.L., Treumann, R.A. (2010). Wave Number Spectra in the Solar Wind, the Foreshock, and the Magnetosheath. In: Laakso, H., Taylor, M., Escoubet, C. (eds) The Cluster Active Archive. Astrophysics and Space Science Proceedings. Springer, Dordrecht. https://doi.org/10.1007/978-90-481-3499-1_24
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DOI: https://doi.org/10.1007/978-90-481-3499-1_24
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