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A model of turbulence in magnetized plasmas: Implications for the dissipation range in the solar wind

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APA Style

Howes, G., Cowley, S., Dorland, W., Hammett, G., Quataert, E., & Schekochihin, A. (2008). A model of turbulence in magnetized plasmas: Implications for the dissipation range in the solar wind. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 113(A5).

MLA Style

Howes, G., et al. “A Model of Turbulence in Magnetized Plasmas: Implications for the Dissipation Range in the Solar Wind.” JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, vol. 113, no. A5, 2008.

Chicago Style

Howes, G, S Cowley, W Dorland, G Hammett, E Quataert, and A Schekochihin. 2008. “A Model of Turbulence in Magnetized Plasmas: Implications for the Dissipation Range in the Solar Wind.” JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 113 (A5).
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Publisher copy:: 10.1029/2007JA012665

Authors

+ Howes, G More by this author

Role:: Author

+ Cowley, S More by this author

Role:: Author

+ Dorland, W More by this author

Role:: Author

+ Hammett, G More by this author

Role:: Author

+ Quataert, E More by this author

Role:: Author

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Journal:: JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS More from this journal
Volume:: 113
Issue:: A5
Publication date:: 2008-05-23
DOI:: 10.1029/2007JA012665
ISSN:: 0148-0227

Pubs id:: pubs:196306
UUID:: uuid:eddc8131-2e18-4a2d-98d1-02140f44dd43
Local pid:: pubs:196306
Source identifiers:: 196306
Deposit date:: 2012-12-19

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Copyright date:: 2008

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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