Decay of magnetohydrodynamic turbulence in the expanding solar wind: WIND observations Article Swipe
Andrea Verdini
,
Petr Hellinger
,
Simone Landi
,
Roland Grappin
,
Víctor Montagud-Camps
,
Emanuele Papini
·
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.1051/0004-6361/202450811
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.1051/0004-6361/202450811
We have studied the decay of turbulence in the solar wind. Fluctuations carried by the expanding wind are naturally damped because of flux conservation, slowing down the development of a turbulent cascade. The latter also damps fluctuations but results in plasma heating. We analyzed time series of the velocity and magnetic field ( v and B , respectively) obtained by the WIND spacecraft at 1 au. Fluctuations were recast in terms of the Elsasser variables, z ± = v ± B /√4 πρ , with ρ being the average density, and their second- and third-order structure functions were used to evaluate the Politano-Pouquet relation, modified to account for the effect of expansion. We find that expansion plays a major role in the Alfvénic stream, those for which z + ≫ z − . In such a stream, expansion damping and turbulence damping act, respectively, on large and small scales for z + , and also balance each other. Instead, z − is only subject to a weak turbulent damping because expansion is a negligible loss at large scales and a weak source at inertial range scales. These properties are in qualitative agreement with the observed evolution of energy spectra that is described by a double power law separated by a break that sweeps toward lower frequencies for increasing heliocentric distances. However, the data at 1 au indicate that injection by sweeping is not enough to sustain the turbulent cascade. We derived approximate decay laws of energy with distance that suggest possible solutions for the inconsistency: in our analysis, we either overestimated the cascade of z ± or missed an additional injection mechanism; for example, velocity shear among streams.
Related Topics
Concepts
Physics
Magnetohydrodynamic turbulence
Turbulence
Solar wind
Astrophysics
Magnetohydrodynamic drive
Magnetohydrodynamics
Astronomy
Solar physics
Coronal mass ejection
Meteorology
Plasma
Nuclear physics
Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1051/0004-6361/202450811
- OA Status
- hybrid
- Cited By
- 2
- References
- 70
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4402122878
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4402122878Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1051/0004-6361/202450811Digital Object Identifier
- Title
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Decay of magnetohydrodynamic turbulence in the expanding solar wind: WIND observationsWork title
- Type
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articleOpenAlex work type
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enPrimary language
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2024Year of publication
- Publication date
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2024-09-02Full publication date if available
- Authors
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Andrea Verdini, Petr Hellinger, Simone Landi, Roland Grappin, Víctor Montagud-Camps, Emanuele PapiniList of authors in order
- Landing page
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https://doi.org/10.1051/0004-6361/202450811Publisher landing page
- Open access
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YesWhether a free full text is available
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hybridOpen access status per OpenAlex
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https://doi.org/10.1051/0004-6361/202450811Direct OA link when available
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Physics, Magnetohydrodynamic turbulence, Turbulence, Solar wind, Astrophysics, Magnetohydrodynamic drive, Magnetohydrodynamics, Astronomy, Solar physics, Coronal mass ejection, Meteorology, Plasma, Nuclear physicsTop concepts (fields/topics) attached by OpenAlex
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2Total citation count in OpenAlex
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2025: 2Per-year citation counts (last 5 years)
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10Other works algorithmically related by OpenAlex
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