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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 33, issue 11
Ann. Geophys., 33, 1413–1419, 2015
https://doi.org/10.5194/angeo-33-1413-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
Ann. Geophys., 33, 1413–1419, 2015
https://doi.org/10.5194/angeo-33-1413-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.

ANGEO Communicates 13 Nov 2015

ANGEO Communicates | 13 Nov 2015

Non-elliptic wavevector anisotropy for magnetohydrodynamic turbulence

Y. Narita

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Latest update: 28 Oct 2020
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Short summary
A lot of efforts have been put into understanding the turbulence structure in space and astrophysical plasmas, in particular how the filamentary structure develops as the length scale of the turbulent fluctuations changes from large to smaller ones. Motivated by the recent spacecraft observations in the solar wind, an analytic model is proposed to explain the nature of filament-formation processes in space plasma turbulence with a successful test against the spacecraft observations.
A lot of efforts have been put into understanding the turbulence structure in space and...
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