Tangential Discontinuities in the Solar Wind: Correlated Field and Velocity 
Changes and the Kelvin-Helmholtz Instability

Neugebauer, M.; Alexander, C. J.; Schwenn, R.; Richter, A. K.

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Tangential Discontinuities in the Solar Wind: Correlated Field and Velocity Changes and the Kelvin-Helmholtz Instability

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Schwenn, R.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Richter, A. K.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Neugebauer, M., Alexander, C. J., Schwenn, R., & Richter, A. K. (1986). Tangential Discontinuities in the Solar Wind: Correlated Field and Velocity Changes and the Kelvin-Helmholtz Instability. Journal Geophysical Research, 91, 13694-13698.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0014-E86D-C

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