Annales Geophysicae
Annales Geophysicae
ANGEO
Articles | Volume 33, issue 11
Articles | Volume 33, issue 11
https://doi.org/10.5194/angeo-33-1413-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/angeo-33-1413-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
Articles | Volume 33, issue 11
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: 13 Dec 2024
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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.
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