[PDF] Top 20 Three dimensional density and compressible magnetic structure in solar wind turbulence
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Three dimensional density and compressible magnetic structure in solar wind turbulence
... The three-dimensional structure of both compress- ible and incompressible components of turbulence is investi- gated at proton characteristic scales in the solar ...the ... See full document
13
Solar wind control of plasma number density in the near-Earth plasma sheet: three-dimensional structure
... number density decreases. Subse- quently, the plasma number density in the nearer portion of the plasma sheet increases with a few hours ...number density suggests recon- figuration of plasma sheet ... See full document
19
Turbulence in the solar wind
... the solar wind The solar wind is thought to be a mixture of turbulence and structures, as suggested in Chapter ...of turbulence is the absence of a characteristic tempo- ... See full document
143
On the ion inertial range density power spectra in solar wind turbulence
... last three averaged nonlinear terms within the angu- lar brackets h ...the turbulence is bounded, in which case boundary effects must be taken into account at the large scales of the ...the solar ... See full document
17
Three-dimensional spatial structures of solar wind turbulence from 10 000-km to 100-km scales
... the three-dimensional wave-vector spectra of fluctuat- ing magnetic fields in the solar ...wind. Three different solar wind intervals of Cluster data are ... See full document
8
Finite size scaling in the solar wind magnetic field energy density as seen by WIND
... of turbulence [Frisch, 1995] and ideally one needs to construct a structure function from a range of spatial locations in the ...the solar wind is routinely single point and can yield strongly ... See full document
5
Multi scale analysis of compressible fluctuations in the solar wind
... the solar wind have revealed that the fluctuations at proton kinetic scales typi- cally have low intrinsic propagation speeds in the plasma ...KAW turbulence and coherent structures (Roberts et ...in ... See full document
6
Model for vortex turbulence with discontinuities in the solar wind
... for solar wind plasma as a turbulent medium which consists of a mixture of nonlinear Alfv´en waves and quasi-two dimensional MHD ...and magnetic field ...nonlinear structure formation ... See full document
9
Modeling of short scale turbulence in the solar wind
... Using dimensional arguments of the Kolmogorov type, we will first derive the fluctuation spectra associated with the velocity and magnetic ...entire magnetic spectrum with its three branches ... See full document
7
Proton kinetic effects in vlasov and solar wind turbulence
... five- dimensional (two-dimensional (2D) in space; three-dimensional (3D) in velocity space) Vlasov model (Valentini et ...fully three space dimensions would imply a reduction in the ... See full document
7
Modeling Solar Wind Turbulence: The Kolmogorov-like Way
... the solar wind tur- bulence are derived using the dimensional arguments a la Kolmogorov within the framework of the Hall mag- ...the magnetic field fluctuations are dynamically related, the ... See full document
8
Magnetic reconnection and intermittent turbulence in the solar wind
... on solar wind data acts to increase, within the selected population, the concentration of current sheets and reconnection ...upon magnetic field measurements, which are typically available at a ... See full document
6
The small amplitude of density turbulence in the inner solar wind
... 4.1 Density fluctuations as a proxy for magnetic fluctua- tions As mentioned in the Introduction, theories of magnetohydro- dynamic turbulence indicate that the energy density is pri- marily ... See full document
8
Measurements of the three-dimensional structure of flames at low turbulence
... Images were recorded by a Photron Fastcam digital CCD camera, which was used at 18,000 fps with a chip size of 255*256 pixels. A Sony TV zoom lens, with an aperture of f 1.8 and focal length between 12.5 and 75 mm, was ... See full document
36
Three dimensional topology of solar coronal magnetic fields
... The second problem is that, near to any of the fixed sources, an echo of the bifurcation line can appear or the line can disappear. This is because at these points the varied source is very close to one of the fixed ... See full document
142
On the fractal nature of the magnetic field energy density in the solar wind
... http://dx.doi.org/10.1029/2007GL029531 Publisher statement: An edited version of this paper was published by AGU. Copyright (2007) American Geophysical Union. B. Hnat, S. C. Chapman, K. Kiyani, G. Rowlands, and N. W. ... See full document
5
ANGEO - The structure and origin of magnetic clouds in the solar wind
... of solar wind data obtained near Earth's orbit during 1984±1991 showed a preference for ...The magnetic con®gurations of the ®laments, as inferred from the orientation of the prominence axis, the ... See full document
24
Power anisotropy in the magnetic field power spectral tensor of solar wind turbulence
... of magnetic field fluctuations in the fast solar wind for the first ...the magnetic field and velocity of the solar wind (θ B ) and the angle of the vector in the plane ... See full document
13
Solar Wind Heating by MHD Turbulence
... 2007, preprint], scatter plot of the Kolmogorov cascade rate (red diamonds - left), the IK cascade rate (red diamonds -right), and expected heating rate (blue crosses) as a function of..[r] ... See full document
18
Extreme ultraviolet imaging of three dimensional magnetic reconnection in a solar eruption
... 3D structure, observations made thus far of the reconnection are mostly restricted to 2D, in which the flux rope often appears as a hot plasma blob when viewed along the axis, and the reconnection site underneath ... See full document
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