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Generalized Similarity in Finite Range Solar Wind Magnetohydrodynamic Turbulence

2009/11/18 by S. C. Chapman, R. M. Nicol · 14 citations
Computer Science · Engineering · Physics and Astronomy · #Aerospace engineering #Classical mechanics #Computer science #Fluid Dynamics and Turbulent Flows #Magnetohydrodynamic drive #Magnetohydrodynamic turbulence #Magnetohydrodynamics #Mechanics #Nuclear physics #Physics #Plasma #Range (aeronautics) #Similarity (geometry) #Solar Radiation and Photovoltaics #Solar and Space Plasma Dynamics #Solar wind #Statistical physics #Turbulence #physics.plasm-ph #physics.space-ph

paper · pdf · doi:10.1103/physrevlett.103.241101

published in Physical Review Letters 103(24), 241101 (American Physical Society) · Accepted for publication in PRL Nov 2009

arxiv created 2009/11/18 · openalex publication_date 2009/12/11 · arxiv updated 2015/05/14 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Extended or generalized similarity is a ubiquitous but not well understood feature of turbulence that is realized over a finite range of scales. The ULYSSES spacecraft solar polar passes at solar minimum provide in situ observations of evolving anisotropic magnetohydrodynamic turbulence in the solar wind under ideal conditions of fast quiet flow. We find a single generalized scaling function characterizes this finite range turbulence and is insensitive to plasma conditions. The recent unusually inactive solar minimum--with turbulent fluctuations down by a factor of approximately 2 in power--provides a test of this invariance.

Citations