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Do oblique Alfven/ion-cyclotron or fast-mode/whistler waves dominate the dissipation of solar wind turbulence near the proton inertial length?

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Marsch,  Eckart
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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He, J., Tu, C., Marsch, E., & Yao, S. (2012). Do oblique Alfven/ion-cyclotron or fast-mode/whistler waves dominate the dissipation of solar wind turbulence near the proton inertial length? Astrophysical Journal, 745: L8. doi:10.1088/2041-8205/745/1/L8.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0015-074D-B
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