RESIDUAL ENERGY SPECTRUM OF SOLAR WIND TURBULENCE

It has long been known that the energy in velocity and magnetic field fluctuations in the solar wind is not in equipartition. In this paper, we present an analysis of 5 yr of Wind data at 1 AU to investigate the reason for this. The residual energy (difference between energy in velocity and magnetic...

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Veröffentlicht in:	The Astrophysical journal 2013-06, Vol.770 (2), p.1-10
Hauptverfasser:	Chen, C H K, Bale, S D, Salem, C S, Maruca, B A
Format:	Artikel
Sprache:	eng
Schlagworte:	ANISOTROPY ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Computational fluid dynamics COMPUTERIZED SIMULATION ENERGY SPECTRA Fluctuation FLUCTUATIONS Fluid flow FORECASTING HELICITY MAGNETIC FIELDS MAGNETOHYDRODYNAMICS NONLINEAR PROBLEMS PLASMA Residual energy SOLAR WIND TURBULENCE Turbulent flow VELOCITY
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