Proton enhancement and decreased O6+/H at the heliospheric current sheet: 
implications for the origin of slow solar wind

Liu, Y. C.-M.; Galvin, A. B.; Popecki, M. A.; Simunac, K. D. C.; Kistler, L.; Farrugia, C.; Lee, M. A.; Klecker, B.; Bochsler, P.; Luhmann, J. L.; Jian, L. K.; Moebius, E.; Wimmer-Schweingruber, R.; Wurz, P.

doi:10.1063/1.3395875

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Proton enhancement and decreased O6+/H at the heliospheric current sheet: implications for the origin of slow solar wind

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Klecker, B.
Space Plasma Physics of Near-Earth Environment, MPI for Extraterrestrial Physics, Max Planck Society;

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Liu, Y.-C.-M., Galvin, A. B., Popecki, M. A., Simunac, K. D. C., Kistler, L., Farrugia, C., Lee, M. A., Klecker, B., Bochsler, P., Luhmann, J. L., Jian, L. K., Moebius, E., Wimmer-Schweingruber, R., & Wurz, P. (2010). Proton enhancement and decreased O6+/H at the heliospheric current sheet: implications for the origin of slow solar wind. In M., Maksimovic, K., Issautier, N., Meyer-Vernet, M., Moncuquet, & F., Pantellini (Eds.), Twelfth International Solar Wind Conference (pp. 363-366).

引用: https://hdl.handle.net/11858/00-001M-0000-0012-B9EE-A

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