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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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ANGEO | Articles | Volume 36, issue 1
Ann. Geophys., 36, 47–52, 2018
https://doi.org/10.5194/angeo-36-47-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.
Ann. Geophys., 36, 47–52, 2018
https://doi.org/10.5194/angeo-36-47-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.

ANGEO Communicates 12 Jan 2018

ANGEO Communicates | 12 Jan 2018

Multi-scale analysis of compressible fluctuations in the solar wind

Owen W. Roberts et al.
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Latest update: 15 Sep 2019
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Short summary
To investigate compressible plasma turbulence in the solar wind on proton kinetic scales, a high time resolution measurement of the density is obtained from the spacecraft potential. Correlation between the magnetic field strength and the density is investigated as is the rotation sense of the magnetic field. The analysis reveals that compressible fluctuations are characteristic of kinetic Alfvén waves or a mixture of kinetic Alfvén and kinetic slow waves which counter-propagate.
To investigate compressible plasma turbulence in the solar wind on proton kinetic scales, a high...
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