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

Tu, C.-Y.; Marsch, E.

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

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.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-D8B9-6 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-D8BA-4

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Creators:
Tu, C.-Y.¹, Author
Marsch, E.^{2, 3}, Author

Affiliations:
1MPS General, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832292
2MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291
3Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289

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MPIS_GROUPS: Sun and Heliosphere

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Dates: Date issued: 1997

Publication Status: Issued

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Rev. Type: Peer

Identifiers: BibTex Citekey: Tu:1997-215

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Title: Solar Physics

Source Genre: Journal

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Pages: - Volume / Issue: 171 Sequence Number: - Start / End Page: 363 - 391 Identifier: -