[PDF] Top 20 Latitudinal extent of large-scale structures in the solar wind
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Latitudinal extent of large-scale structures in the solar wind
... Comparison of solar wind observations from the ACE spacecraft, in the ecliptic plane at ∼1 AU, and the Ulys- ses spacecraft as it orbits over the Sun’s poles, ... Voir le document complet
10
Radial and latitudinal dependencies of discontinuities in the solar wind between 0.3 and 19 AU and ?80° and +10°
... ◦ in the 3D heliosphere are investigated during mini- mum solar ...activity. The data are surveyed using the identifi- cation criteria of Burlaga (1969) (B) and Tsurutani and ... Voir le document complet
15
Solar cycle changes in the geo-effectiveness of small-scale solar wind turbulence measured by Wind and ACE at 1 AU
... regimes of inertial range turbulence reasonably well described by a single ex- ponent power law over a fixed range of τ ...lesser extent, depending on the particular parameter and chosen range ... Voir le document complet
16
Solar wind velocity at solar maximum: A search for latitudinal effects
... variations of larger amplitude. This is similar to the findings of Burlaga et ...(2003). The occurrence frequency F of the Ulysses velocity differ- ences dV 0, dV 1, dV 2, dV 3, ... Voir le document complet
8
K-mouflage Cosmology: Formation of Large-Scale Structures
... the one of Λ-CDM. At the perturbative level, and first in the linear theories, deviations from GR occur on scales lower than the Compton wavelength of the scalar ... Voir le document complet
25
K-mouflage Cosmology: Formation of Large-Scale Structures
... the one of Λ-CDM. At the perturbative level, and first in the linear theories, deviations from GR occur on scales lower than the Compton wavelength of the scalar ... Voir le document complet
25
Combining global and multi-scale features in a description of the solar wind-magnetosphere coupling
... Conclusions The solar wind-magnetosphere coupling during substorms exhibits dynamical features in a wide range of spatial and temporal ...scales. The large-scale ... Voir le document complet
18
A study of the large-scale structure of the wind of WR 134
... form in the winds of hot stars because of a perturbation at the base of the wind, which causes more or less line driving and therefore different velocity flows that ... Voir le document complet
113
Latitudinal distribution of the solar wind properties in the low- and high-pressure regimes: Wind observations
... crossing the sign of azB changes while Q remains antisunward so that, if azQ azB is counted between 90 and 450 , azB and azQ azB jump in the same direction: this occurs on days ...days, ... Voir le document complet
15
Large-scale velocity fluctuations in polar solar wind
... leg, the same time length does not cor- respond to the same latitudinal range in the two ...hemispheres. In fact, in the Northern (Southern) Hemisphere 13 rotations ... Voir le document complet
8
Magnetically dominated structures as an important component of the solar wind turbulence
... transfer of energy to smaller and smaller scales while, these structures, being advected, have a much longer ...As the expansion goes on, the relative weight of these fluctu- ations ... Voir le document complet
16
Alignments of quasar axes with large-scale structures
... Analysis of polarization measurements – In order to compare the quasar polarization angles to the direction of the local structures, we consider four sub-structures ... Voir le document complet
1
Nonlinear optimal large-scale structures in turbulent channel flow
... means of a linear transient-growth analysis [ 10 ]. In fact, optimally-growing perturbations can be employed to understand the features of the coherent motion in transitional and ... Voir le document complet
14
EISCAT measurements of the solar wind
... waves in the solar wind, with the observed scintillation being produced by the interactions of Alfve´n waves with the anisotropic ...medium. In this case ... Voir le document complet
12
Alignments of quasar axes with large-scale structures
... polarization in LQGs The distribution of the acute angle Δθ between quasar polarizations and the orientation of their host large-scale ...structure. The ... Voir le document complet
23
Solar cycle dependence of scaling in solar wind fluctuations
... purpose of this review is to bring together two quan- titative features of solar wind fluctuations seen on timescales that are within the observed inertial range of ... Voir le document complet
12
Rapid density fluctuations in the solar wind
... Hz) in the solar wind have been studied, using the EFW experiment on the Cluster spacecraft, which measures density through measurements of the biased probe ... Voir le document complet
10
The large scale structures. A window on the dark components of the Universe
... the estimation of the significance: each random patch is first subjected to the same rescaling as the one done on the identified void ...have the effect of mixing ... Voir le document complet
223
Multifractality and intermittency in the solar wind
... for the generalized two-scale Cantor set as a func- tion of α with the same parameters are shown by dashed line in ...that the multifractal spectrum of the ... Voir le document complet
7
The origin of slow Alfvénic solar wind at solar minimum
... ). In contrast, the solar sources of wind with slow and intermediate speeds are varied and still not entirely clear ...see the review of Abbo et ...lines of ... Voir le document complet
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