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Correlation lengths, the Ultrascale, and the spatial structure of interplanetary turbulence
AIP Conference Proceedings, 1999Characteristic length scales can be employed to describe the large scale structural and statistical features of solar wind plasma turbulence. At least two outer scales of interplanetary turbulence, the correlation scale and an independent quantity that has been called the “Ultra scale,” have application in the theory of field line random walk and ...
W. H. Matthaeus +2 more
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Hydromagnetic Waves, Turbulence, and Collisionless Processes in the Interplanetary Medium
1983The solar wind does not flow quietly. It seethes and undulates, fluctuating on time scales that range from the solar rotation period down to fractions of milliseconds. Most of the power in interplanetary waves and turbulence lies at hydromagnetic scales.
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Premixed flames subjected to extreme turbulence: Some questions and recent answers
Progress in Energy and Combustion Science, 2020Aaron W Skiba +2 more
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Spray–turbulence–chemistry interactions under engine-like conditions
Progress in Energy and Combustion Science, 2021Lei Zhou, Ming Jia
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Turbulence Modeling in the Age of Data
Annual Review of Fluid Mechanics, 2019Karthik Duraisamy +2 more
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Particles and fields in fluid turbulence
Reviews of Modern Physics, 2001Gregory Falkovich, Massimo Vergassola
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The Solar Wind as a Turbulence Laboratory
Living Reviews in Solar Physics, 2013Roberto Bruno, Vincenzo Carbone
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Onsager and the theory of hydrodynamic turbulence
Reviews of Modern Physics, 2006Gregory L Eyink
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High–Reynolds Number Wall Turbulence
Annual Review of Fluid Mechanics, 2011Alexander J Smits +2 more
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