[PDF] Top 20 Model for vortex turbulence with discontinuities in the solar wind
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Model for vortex turbulence with discontinuities in the solar wind
... the solar wind. This model can be considered as develop- ment of one-dimensional nonlinear model proposed in Buti et ...the model will be ... See full document
9
Voyager 2 observation of the multifractal spectrum in the heliosphere and the heliosheath
... plasma turbulence (Sahraoui, 2008). It is also known that the solar wind is characterized by nonlin- ear Alfvén waves ...directional discontinuities and magnetic de- creases (Tsurutani et ... See full document
10
Modeling Solar Wind Turbulence: The Kolmogorov-like Way
... along with other values of p. Key observations of the solar wind turbulence are: 1. velocity, density, magnetic field and temperature vary in time; 2. magnetohydrodynam- ics accounted for ... See full document
8
Multifractal two-scale Cantor set model for slow solar wind turbulence in the outer heliosphere during solar maximum
... In Fig. 3 we also show the calculated universal multifractal singularity spectra. We can take the degree of multifractal- ity 1 and measure of asymmetry A defined in Eqs. (8) and (9), respectively. Both values of 1 and A ... See full document
8
Investigation of the strong turbulence in the geospace environment
... The isolated magnetospheric substorm starts with a growth phase when a southward interplanetary magnetic field (IMF) merges with the Earth’s dayside magnetic field and transfers energy from the solar wind ... See full document
8
Solar wind vs magnetosheath turbulence and Alfv´en vortices
... phenomenological model allows to explain the vari- ations of the spectral index of the high frequency part of the solar wind spectrum from − 4 to − 2 by different degree of plasma compression, γ ∈[− ... See full document
14
Proton kinetic effects in vlasov and solar wind turbulence
... of solar wind plasma (Kasper et ...of solar wind parcels in a plane described by the parallel plasma beta and the proton temperature anisotropy have attracted intensive ...with wind ... See full document
7
The small amplitude of density turbulence in the inner solar wind
... theoretical model allows for the retrieval of C N0 2 ...the solar wind at different heliocentric distances, an extensive observational program with observations of many sources can establish C 2 N ... See full document
8
A nonextensive entropy path to probability distributions in solar wind turbulence
... intermittent turbulence model for the solar wind and for the Earth’s magnetotail, which comprises neither cascades nor requires local interactions in Fourier ...the solar wind ... See full document
10
Self similar signature of the active solar corona within the inertial range of solar wind turbulence
... at solar maximum, the magnetic energy density is self-affine; we can clearly identify a plateau with a H = ζ(2)/2 value of H ≃ ...for WIND and H ≃ 0.45 ± 0.01 for ACE. At solar minimum, there is no ... See full document
5
Solar wind plasma parameter variability across solar cycles 23 and 24 : from turbulence to extremes
... a model-independent method for comparing two empirically sam- pled statistical distributions (Braun & Murdoch, ...same model but with time-dependent ... See full document
18
Limitations of Hall MHD as a model for turbulence in weakly collisional plasmas
... fluid model of MHD is not sufficient to de- scribe this new regime of kinetic turbulence in the weakly collisional solar wind ...MHD model – an extension of MHD that main- tains a fluid ... See full document
14
Statistical analysis of transfer of fluctuations in solar wind turbulence
... MHD turbulence are studied in details (see, ...of turbulence by shell models or numer- ical simulations (see, ...of turbulence directly using experimental ... See full document
7
Three dimensional density and compressible magnetic structure in solar wind turbulence
... the solar wind are provided from the Cluster mission (Escoubet et ...statistical model of the spacecraft charging as a function of the spacecraft spin phase ... See full document
13
On the ion inertial range density power spectra in solar wind turbulence
... different model- independent point of view, avoiding reference to any super- imposed plasma instabilities or intermittency ...the solar wind (Woo, 1981; Coles and Fil- ice, 1985; Bourgeois et ... See full document
17
Parallel and perpendicular cascades in solar wind turbulence
... A paper of particular interest is Cho and Lazarian (2002). They performed isothermal simulations, with the plasma beta ≈ 0.2, and analyzed the data by projecting the fluctuations onto the linear mode polarizations, ... See full document
12
The influence of solar wind turbulence on geomagnetic activity
... The solar wind is an inhomogeneous, anisotropic and compress- ible magnetized plasma, in which the bulk plasma parameters and the magnetic field fluctuate over a broad range of spatial and temporal scales ... See full document
7
Asymmetric multifractal model for solar wind intermittent turbulence
... for solar wind turbulence depending on the solar cycle activ- ...the solar wind measured in situ by Advanced Composi- tion Explorer spacecraft during solar maximum (2001) ... See full document
6
Modeling of short scale turbulence in the solar wind
... the solar wind are trans- formed into the wave vector spectra Doppler shifted by the Super Alfv´enic Solar wind ...MHD turbulence is now being highly emphasized (Matthaeus et ...we ... See full document
7
Magnetic reconnection and intermittent turbulence in the solar wind
... the solar wind only one case of multiple island reconnection has been reported [65] and magnetic reconnection often does not lead directly to dissipation or plasma heating, particularly for asymmetric ... See full document
6
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