[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
... 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, provides valu- able information about the ... See full document
9
Quantifying the latitudinal representivity of in situ solar wind observations
... of solar wind simulations from the magnetohydrodynamics algorithm outside a sphere (MAS) global coronal and heliosphere model (Linker et ...radial structures below ~10 6 km and time scales shorter ... See full document
16
Solar wind velocity at solar maximum: A search for latitudinal effects
... the solar activity maxi- mum the solar wind appears as a highly variable flow at all ...of latitudinal effects in the large-scale structure of the solar wind ...the ... See full document
7
Large-scale velocity fluctuations in polar solar wind
... same latitudinal range in the two ...the latitudinal excursions in the inner and outer intervals are not strongly different, thus variations, if any, should be mainly due to radial ... See full document
7
Large-scale velocity fluctuations in polar solar wind
... same latitudinal range in the two ...the latitudinal excursions in the inner and outer intervals are not strongly different, thus variations, if any, should be mainly due to radial ... See full document
8
Reconstruction of Helio-Latitudinal Structure of the Solar Wind Proton Speed and Density
... given latitudinal 3 ◦ -bin, then we set up the initial conditions for the neighboring maps using the W m coefficients retrieved from the nearest start ...◦ latitudinal bin using the information from all ... See full document
27
Wind Loading on Full-scale Solar Panels
... Introduction Solar energy is a renewable and clean energy which is a sustainable alternative to fossil fuels, from an environmental ...harness solar energy is to use solar cells attached on panels ... See full document
97
More about arc-polarized structures in the solar wind
... too large an angle to permit a meaningful determination, by triangulation, of the small nor- mal field components associated with most of the discontinu- ... See full document
17
Radial and latitudinal dependencies of discontinuities in the solar wind between 0.3 and 19 AU and 80 and 10
... However, we believe that the decrease in the rate of oc- currence is not obviously due to the non-identification. The DDs are perhaps unstable (maybe as a result of the annihi- lation due to the evolution in ω and r rg ... See full document
14
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 ...herent structures which are predominantly advected with ... See full document
6
Reconstruction of a large-scale reconnection exhaust structure in the solar wind
... Fig. 11. MHD reconstruction maps of the bifurcated current sheet seen by ACE on 2 February 2002, during the interval of 00:12:12– 02:57:32 UT. Format is the same as in Fig. 7 but scales are larger. The green line in the ... See full document
16
Large Scale Grid Integration of Wind and Solar Power with Storage
... include solar, wind, hydroelectric, bio-fuel and geothermal ...are solar power and wind power, since they can be scaled to replace the likes of coal and natural gas, which dominate our energy ... See full document
15
On arc-polarized structures in the solar wind
... The main focus is on intermediate-mode wave trains, which display double-branched magnetic hodogram signatures sim- ilar to those seen in the solar wind. The theoretically derived hodograms have field ... See full document
20
Large-scale solar wind flow around Saturn's non-axisymmetric magnetosphere
... “hinged” to the X-directed solar wind away from the magnetosheath. The resulting bending of the field lines generates a B Z component at latitudes above and below the equator. The key finding in Figure 4a is ... See full document
9
Statistical analysis of the dependence of large-scale Birkeland currents on solar wind parameters
... exhibit large-scale dynamics on time scales that are shorter than the one-hour accumulation times required to obtain Birkeland currents from the Iridium data used ...the solar wind ...and ... See full document
16
ANGEO - Latitudinal distribution of the solar wind properties in the low- and high-pressure regimes: Wind observations
... The solar wind properties depend on k, the heliomagnetic latitude with respect to the heliospheric current sheet (HCS), more than on the heliographic ...the wind properties observed by Wind at ... See full document
14
Large-scale solar systems
... - Heating of indoor swimming pools requires additional?. huge buffer tanks.[r] ... See full document
19
Large-scale solar heating plants
... sources, solar heating systems ensure fixed low energy costs for many years to ...new, large-scale solar heating installations, especially in connection with district heating ...have ... See full document
20
Perturbations of the solar wind flow by radial and latitudinal pick-up ion pressure gradients
... of solar wind modifications, ...but latitudinal pressure gradients also appear to be ...and latitudinal pick-up ion pressure gradients, occurring especially during solar minimum ... See full document
10
Modeling of short scale turbulence in the solar wind
... The large wavevec- tor limit of the dispersion relation of the nonlinear waves basically leads to the dispersive effects with the difference that now the relation between the velocity and the magnetic field ... See full document
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