[PDF] Top 20 Modeling of short scale turbulence in the solar wind
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Modeling of short scale turbulence in the solar wind
... The nonlinear solution is an exact solution for waves prop- agating in one direction. For the superposition of the right and the left propagating waves the nonlinearity remains and this is what could give rise to the ... See full document
7
Modeling Momentum-Diffusion in the Solar Wind
... Spiral solar wind. They occur when there is a fast solar wind next to a slower wind such that as the solar wind propagates out through heliosphere the faster wind ... See full document
15
Modeling Momentum-Diffusion in the Solar Wind
... of solar, wind, fossil fuel, and even food ...as solar flares and coronal mass ejec- tions (CMEs), are when the Sun ejects large amounts of energy, magnetic field, and plasma from its ...them ... See full document
15
Modeling Solar Wind Turbulence: The Kolmogorov-like Way
... the various spectral branches. This spectra is shown in Fig. 8 where the low k end (k −1 ) and (k −5/3 ) are derived in the ideal MHD regime and the high k end (k −5/3 ) and (k −7/3 ) for the kinetic energy and (k −11/3 ... See full document
8
Asymmetric multifractal model for solar wind intermittent turbulence
... intermittent turbulence (Man- delbrot, ...energy turbulence cascade and the degree of multifractality in the solar wind plasma (Meneveau and Sreenivasan, ...of solar wind has ... See full document
6
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
Statistical analysis of transfer of fluctuations in solar wind turbulence
... MHD turbulence are studied in details (see, ...for modeling MHD flows and nu- merical ...of turbulence by shell models or numer- ical simulations (see, ...of turbulence directly using ... See full document
7
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 ...each ... See full document
14
Design of Mini Wind Tunnel Based on Coanda Effect
... RNG turbulence model and experimental measurements are implemented to design an unconventional small–scale laboratory wind tunnel (mini–wind tunnel) based on Coanda effect suitable for ... See full document
7
Limitations of Hall MHD as a model for turbulence in weakly collisional plasmas
... that turbulence in the dissipation range of the solar wind must be one, or a mixture, of three electromag- netic wave modes: the parallel whistler, oblique whistler, or kinetic Alfv´en ...in ... See full document
14
Three dimensional density and compressible magnetic structure in solar wind turbulence
... Given modern computer processing power, an alternative to using Taylor’s hypothesis is to investigate the spatial struc- ture of plasma through direct numerical simulations. Several different schemes have been employed ... See full document
13
Proton kinetic effects in vlasov and solar wind turbulence
... small scale gradients; Haynes et ...the solar wind (Bruno & Carbone 2005; Sahraoui et ...with solar wind datasets from the Wind spacecraft, and we investigate the structures ... See full document
7
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
A nonextensive entropy path to probability distributions in solar wind turbulence
... plasma turbulence by comparing observed PDFs of fluctua- tions of the velocity field magnitude in the solar wind with the global theoretical core-halo representation (6) account- ing for nonlocality ... See full document
10
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 ...Large scale coherent structures of solar origin, such as CMEs, can be directly identified in the ... See full document
5
Wind Loading on Full-scale Solar Panels
... of solar panels and constitutes approximately fifty percent of the total ...test scale related issues while testing solar panels (small structures) in boundary layer wind tunnel laboratories ... See full document
97
Experimental Investigation into the Influence of Turbulence Intensity on Aerodynamic Performance of a Small Scale Vertical Axis Wind Turbine
... hydropower, solar and wind energy provide the best alternative to the finite fossil fuels ...[5] Wind energy source has increasingly been utilized since it is free, clean and readily ...ambient ... See full document
9
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 ... See full document
17
Parallel and perpendicular cascades in solar wind turbulence
... should scale with the Mach number in a specific ...of solar wind observations also yields an 80–20 2D/slab ...of solar wind fluc- tuations as they are transported outwards by the ... See full document
12
Turbulence in the solar wind
... the solar wind the instrument cadence and accuracy has improved, such that now a full range of temporal scales from the solar rotation period to 1/450 seconds may be recorded using a combination of ... See full document
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