Features of the Spectral Characteristics of Plasma Fluctuations in Different Large-Scale Streams of the Solar Wind

The turbulent characteristics of plasma fluctuations in the solar wind (SW) may substantially change depending on the SW conditions. Large-scale streams of different types, such as undisturbed slow solar wind, fast solar wind, interplanetary coronal mass ejection (EJECTA), magnetic cloud (MC), the c...

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Veröffentlicht in:	Geomagnetism and Aeronomy 2019-03, Vol.59 (2), p.127-135
Hauptverfasser:	Riazantseva, M. O., Rakhmanova, L. S., Zastenker, G. N., Yermolaev, Yu. I., Lodkina, I. G.
Format:	Artikel
Sprache:	eng
Schlagworte:	Computational fluid dynamics Coronal mass ejection Earth and Environmental Science Earth Sciences Ejecta Fluctuations Fluid flow Geophysics/Geodesy Ion flux Magnetic clouds Magnetohydrodynamic turbulence Magnetohydrodynamics Plasma Sheaths Solar corona Solar wind Spacecraft Spectra Streams
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