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Correlations between neutral and ionized solar wind
Advances in Space Research, 2005Abstract We report results of a statistical study correlating ionized solar wind (ISW) fluxes observed by ACE during late 2000 and throughout 2001 with neutral solar wind (NSW) fluxes observed by IMAGE/LENA over the same period. The average correlation coefficient between the neutral and ionized solar wind is 0.66 with correlations greater than 0.80 ...
B.M. Pilkerton, M.R. Collier, T.E. Moore
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Journal of Geophysical Research: Space Physics, 2004
The classical polar wind is an ambipolar outflow of ions from high latitudes along open geomagnetic field lines. The polar wind consists of light thermal ions (H+, He+) and energetic light and heavy ions (H+, He+, O+). The characteristics of these ions have been studied quite extensively since the 1960s.
Larry C. Gardner, Robert W. Schunk
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The classical polar wind is an ambipolar outflow of ions from high latitudes along open geomagnetic field lines. The polar wind consists of light thermal ions (H+, He+) and energetic light and heavy ions (H+, He+, O+). The characteristics of these ions have been studied quite extensively since the 1960s.
Larry C. Gardner, Robert W. Schunk
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Ionospheric warming by neutral winds
Planetary and Space Science, 1971Undisturbed ionospheric ion and electron temperature warming, investigating frictional heating effect by neutral ...
Stubbe, P., Chandra, S.
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Planetary and Space Science, 1975
Abstract The Navier-Stokes equations are solved by introducing a statistical model of density and a distinct temperature model. The non-linear terms of inertia and the viscous term are not included. The computations have been made for equinoctial conditions at a height of 300 km and at different latitudes.
M. Ill, J. Clairemidi, J.-L. Falin
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Abstract The Navier-Stokes equations are solved by introducing a statistical model of density and a distinct temperature model. The non-linear terms of inertia and the viscous term are not included. The computations have been made for equinoctial conditions at a height of 300 km and at different latitudes.
M. Ill, J. Clairemidi, J.-L. Falin
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Neutral earthing in off-shore wind farm grids [PDF]
2009 IEEE Bucharest PowerTech, 2009 The maintenance of offshore wind farms is more complicated than those onshore. The effort associated with cable repairs in terms of time and cost is much larger compared to I similar tasks in conventional distribution grids. Current and voltage stress of the grid following the most common single phase to ground fault primarily affected by the type of ...
van de Sandt, Robert C. P. +3 more
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Non-neutral or Diabatic Wind Profile
2021In non-neutral stability conditions, adjustment—termed Monin-Obukhov Similarity Theory—must be made to the logarithmic wind profile to account for the increased or decreased tendency for rising motion, because the turbulent eddies are anisotropic rather than isotropic.
Robert V. Rohli, Chunyan Li
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Neutral Wind Measurement during Daytime in the Thermosphere
Nature, 1972A SKYLARK rocket (SL 1023) was launched in the British National Space Research Programme at Woomera Range, S. Australia, at 1130 local time on March 14, 1972. The objective was to make a detailed analysis of the structure of the local daytime ionospheric current system.
Rees, D. +5 more
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Global neutral polar wind model
Journal of Geophysical Research: Space Physics, 2005The neutral polar wind shows a highly dynamic structure that depends on the characteristics of convection and precipitation. The ions in the polar wind are highly dependent on convection electric fields at high latitudes, and their outflow dynamics are modified by the heat input of precipitating electrons in the auroral zone.
Larry C. Gardner, Robert W. Schunk
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On neutral sheets in the solar wind
Solar Physics, 1972The structure and dynamics of neutral sheets in the solar wind is examined. The internal magnetic topology of the sheet is argued to be that of thin magnetic tongues greatly distended outward by the expansion inside the sheet. Due to finite conductivity effects, outward flow takes place across field lines but is retarded relative to the ambient solar ...
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