Identifying kinetic scale magnetic discontinuity structures in turbulent solar wind
Author:
Funder
Science and Engineering Research Board
Publisher
Springer Science and Business Media LLC
Link
https://link.springer.com/content/pdf/10.1007/s10509-024-04266-x.pdf
Reference37 articles.
1. Alexandrova, O., Lacombe, C., Mangeney, A., et al.: Solar wind turbulent spectrum at plasma kinetic scales. Astrophys. J. 760(2), 121 (2012). https://doi.org/10.1088/0004-637X/760/2/121
2. Bandyopadhyay, R., Matthaeus, W.H., Chasapis, A., et al.: Direct measurement of the solar-wind Taylor microscale using mms turbulence campaign data. Astrophys. J. 899(1), 63 (2020)
3. Biskamp, D.: Magnetohydrodynamic Turbulence. Cambridge (2003)
4. Borovsky, J.E.: Flux tube texture of the solar wind: strands of the magnetic carpet at 1 AU? J. Geophys. Res. Space Phys. 113(A8), A08110 (2008). https://doi.org/10.1029/2007JA012684
5. Bruno, R.: Intermittency in solar wind turbulence from fluid to kinetic scales. Earth Space Sci. 6(5), 656–672 (2019). https://doi.org/10.1029/2018EA000535
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