[PDF] Top 20 Turbulence in the solar wind
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Turbulence in the solar wind
... of turbulence it is important to determine the probability and joint probability distribution of ...hydrodynamic turbulence vortex tubes are created and ... See full document
143
Magnetic reconnection and intermittent turbulence in the solar wind
... — Turbulence is ubiquitous in space plasmas and leads to the emergence of coherent structures (see ...The solar wind is an ideal laboratory for the in situ study of coherent structures, which have ... See full document
6
The effect of upstream turbulence and its anisotropy on the efficiency of solar wind – magnetosphere coupling
... the solar wind changes over ...of turbulence in the solar wind is typi- cally less than a ...magnetohydrodynamic turbulence is of the order of some ... See full document
7
Modeling of short scale turbulence in the solar wind
... Solar wind is a turbulent supersonic outflow of plasma from the solar ...with Solar flare caused blast waves propagate out in the form of various linear and nonlinear plasma ...the ... See full document
7
The small amplitude of density turbulence in the inner solar wind
... to turbulence in the solar wind has been discussed previously by Spangler and Sakurai (1995) and numerous reports ex- ist on the general phenomenon of interplanetary scintilla- tions ...plasma ... 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 non- ... See full document
10
Solar wind vs magnetosheath turbulence and Alfv´en vortices
... fluid turbulence, the dissipative range is described by an exponential function and not by a power-law, as dis- cussed ...the solar wind turbulence we observe a completely different ... See full document
14
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
On the ion inertial range density power spectra in solar wind turbulence
... the solar wind at 1 AU is pre- ...in solar wind velocity turbulence and referring to observations of density- power spectra suggest that the occasionally observed scale- limited bumps ... See full document
17
Statistical analysis of transfer of fluctuations in solar wind turbulence
... km/s) solar wind (see, ...fast wind is more homogeneous and incompressible in comparison with the slow wind, but both types of the solar wind are quite variable in space and ... See full document
7
Solar wind plasma parameter variability across solar cycles 23 and 24 : from turbulence to extremes
... The solar wind in the ecliptic exhibits two states: fast wind, which originates from the edges of long-lived, extended polar coronal holes (Hassler et ...slow wind, thought to be generated in ... See full document
18
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
Self similar signature of the active solar corona within the inertial range of solar wind turbulence
... The solar wind is also studied in-situ to infer informa- tion pertaining to coronal ...of solar origin, such as CMEs, can be directly identified in the solar ...the solar wind ... See full document
5
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
Multifractal two-scale Cantor set model for slow solar wind turbulence in the outer heliosphere during solar maximum
... of solar wind turbulence, we have developed a generalized weighted two-scale Cantor set model using the partition technique (Macek and Szczepa- niak, ...of solar wind turbulence ... See full document
8
Model for vortex turbulence with discontinuities in the solar wind
... high-speed solar wind flow (63 : 37 and 57 : 44) (Neugebauer et ...Alfv´enic turbulence, our result shows less coincidence with measurements made for slow- speed solar wind regions, ... See full document
9
Wavevector anisotropy of plasma turbulence at ion kinetic scales: solar wind observations and hybrid simulations
... Abstract. Wavevector anisotropy of ion-scale plasma turbu- lence is studied at various values of ion beta. Two comple- mentary methods are used. One is multi-point measurements of magnetic field in the near-Earth ... See full document
9
Observations of the solar wind turbulence near the sun
... An important study of the solar-wind turbulence was done by Belcher and Davis 1971 with data frm Mariner 5 1967, enu us They found t h a t 30 t o 50 percent of the time the turbulence wa[r] ... See full document
159
Parallel and perpendicular cascades in solar wind turbulence
... schematic solar wind spectrum. In the classical view of turbulence, energy is transferred from the energy-containing scales to the dissipa- tion range scales not directly, but rather via passage ... 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
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