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Two-fluid model for heating of the solar corona and acceleration of the solar wind by high-frequency Alfvén waves

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons104260

Tu,  C.-Y.
MPS General, Max Planck Institute for Solar System Research, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons104072

Marsch,  E.
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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Tu, C.-Y., & Marsch, E. (1997). Two-fluid model for heating of the solar corona and acceleration of the solar wind by high-frequency Alfvén waves. Solar Physics, 171, 363-391.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-D8B9-6
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