Cross-scale turbulence in space plasmas: old concepts, recent findings, and future challenges Article Swipe
Tommaso Alberti
,
Simone Benella
,
Mirko Stumpo
,
L. Sorriso‐Valvo
,
V. Carbone
·
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.1088/1361-6587/ada6ff
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.1088/1361-6587/ada6ff
Turbulence, a fascinating and intricate phenomenon, has captivated scientists over different domains, mainly for its complex cross-scale nature spanning a wide range of temporal and spatial scales. Despite significant advances in theories and observations in the last decades, some aspects of turbulence still remain unsolved, motivating new efforts to understand its underlying physical mechanisms and refine mathematical theories along with numerical models. This topical review explores recent findings from the Parker Solar Probe mission, providing a distinctive opportunity to characterize solar wind features at varying heliocentric distances. Analyzing the radial evolution of magnetic and velocity field fluctuations across the inertial range, a transition has been evidenced from local to global self-similarity as proximity to the Sun increases. This behavior has been reconciled with magnetohydrodynamic theory revising an old concept by emphasizing the evolving nature of the coupling between fields. This offers inspiration for novel modeling approaches to understand open challenges in interplanetary plasma physics as the heating and acceleration of the solar wind, as well as, its evolution within the inner Heliosphere.
Related Topics
Concepts
Heliosphere
Physics
Solar wind
Turbulence
Magnetohydrodynamic drive
Plasma
Magnetohydrodynamics
Magnetohydrodynamic turbulence
Scale (ratio)
Interplanetary spaceflight
Space physics
Interplanetary magnetic field
Aerospace engineering
Geophysics
Mechanics
Engineering
Quantum mechanics
Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1088/1361-6587/ada6ff
- OA Status
- hybrid
- References
- 119
- Related Works
- 10
- OpenAlex ID
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All OpenAlex metadata
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https://openalex.org/W4406136105Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1088/1361-6587/ada6ffDigital Object Identifier
- Title
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Cross-scale turbulence in space plasmas: old concepts, recent findings, and future challengesWork title
- Type
-
articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2025Year of publication
- Publication date
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2025-01-07Full publication date if available
- Authors
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Tommaso Alberti, Simone Benella, Mirko Stumpo, L. Sorriso‐Valvo, V. CarboneList of authors in order
- Landing page
-
https://doi.org/10.1088/1361-6587/ada6ffPublisher landing page
- Open access
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YesWhether a free full text is available
- OA status
-
hybridOpen access status per OpenAlex
- OA URL
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https://doi.org/10.1088/1361-6587/ada6ffDirect OA link when available
- Concepts
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Heliosphere, Physics, Solar wind, Turbulence, Magnetohydrodynamic drive, Plasma, Magnetohydrodynamics, Magnetohydrodynamic turbulence, Scale (ratio), Interplanetary spaceflight, Space physics, Interplanetary magnetic field, Aerospace engineering, Geophysics, Mechanics, Engineering, Quantum mechanicsTop concepts (fields/topics) attached by OpenAlex
- Cited by
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0Total citation count in OpenAlex
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119Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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