Taylor Microscale and Effective Reynolds Number near the Sun from PSP

The Taylor microscale is a fundamental length scale in turbulent fluids, representing the end of fluid properties and onset of dissipative processes. The Taylor microscale can also be used to evaluate the Reynolds number in classical turbulence theory. Although the solar wind is weakly collisional,...

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Veröffentlicht in:	The Astrophysical journal 2022-07, Vol.933 (1), p.33
Hauptverfasser:	Phillips, C., Bandyopadhyay, R., McComas, D. J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Data collection Dissipation Fluid flow Interplanetary turbulence Magnetohydrodynamic turbulence Magnetohydrodynamics Reynolds number Solar probes Solar wind Space plasmas Spacecraft Sun Turbulence Turbulent flow
Online-Zugang:	Volltext
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