Contextual Predictions for Parker Solar Probe. II. Turbulence Properties and Taylor Hypothesis

The Parker Solar Probe (PSP) primary mission extends seven years and consists of 24 orbits of the Sun with descending perihelia culminating in a closest approach of ∼9.8 R . In the course of these orbits PSP will pass through widely varying conditions, including anticipated large variations of turbu...

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Veröffentlicht in:	The Astrophysical journal. Supplement series 2019-05, Vol.242 (1), p.12
Hauptverfasser:	Chhiber, Rohit, Usmanov, Arcadi V., Matthaeus, William H., Parashar, Tulasi N., Goldstein, Melvyn L.
Format:	Artikel
Sprache:	eng
Schlagworte:	Boundary conditions Computational fluid dynamics Computer simulation Correlation Fluid flow Flux density Helicity Hypotheses Magnetic fields Magnetohydrodynamic simulation Magnetohydrodynamic turbulence magnetohydrodynamics (MHD) Orbits Parameters Solar probes solar wind Sun: corona Turbulence Turbulent energy
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