On the Local Structure of Stochastic Parker Spirals in the Solar Wind

We present a Langevin model describing the local structure of the interplanetary magnetic field lines. It is established on the basis of the analysis of the Lagrangian properties of strong Alfvénic turbulence, which provides a new perspective on the critical balance condition. The model is consisten...

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Veröffentlicht in:	The Astrophysical journal 2022-12, Vol.941 (1), p.58
Hauptverfasser:	Bian, N. H., Li, Gang
Format:	Artikel
Sprache:	eng
Schlagworte:	Anisotropy Astrophysics In situ measurement Interplanetary magnetic field Interplanetary turbulence Magnetic fields Magnetic variations Magnetohydrodynamics Position measurement Solar magnetic field Solar wind Spacecraft Spirals Wavelet analysis
Online-Zugang:	Volltext
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