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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?

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.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0015-074D-B Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0015-074E-9
Genre: Journal Article

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 Creators:
He, Jiansen, Author
Tu, Chuanyi, Author
Marsch, Eckart1, 2, Author           
Yao, Shuo, Author
Affiliations:
1MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              
2Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              

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Free keywords: -
 MPIS_GROUPS: Sun and Heliosphere
 MPIS_PROJECTS: STEREO: IMPACT
 MPIS_PROJECTS: WIND
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 Dates: 2012
 Publication Status: Issued
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1088/2041-8205/745/1/L8
BibTex Citekey: He:2012-004
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Title: Astrophysical Journal
Source Genre: Journal
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Pages: - Volume / Issue: 745 Sequence Number: L8 Start / End Page: - Identifier: -