solar wind interactionIMFinterplanetary magnetic fieldsolar wind density[1] In this study we determine relationships between auroral brightness and each of the solar wind density and velocity under normal interplanetary magnetic field (IMF) conditions using Polar Lyman-Birge-Hopfield long band (170.0 nm...
The interaction of these large-scale features with the panels, in the form of locally oriented drag, results in the peak uplifting loads.R. Nicolas PrattGregory A. KoppJournal of Wind Engineering and Industrial AerodynamicsVelocity measurements around low-profile, tilted, solar arrays mounted on ...
The study focused on wall normal wind directions, which result in critical loads on panels within the separation bubble. The mean flow is not significantly altered above the array as compared to that for a bare roof. However, the array has a significant effect on the turbulence above and ...
A more mathematically rigorous approach to decomposing a given set of velocity and pressure fields into their corresponding eigenmodes is to project them onto the orthogonal basis set provided by the equatorial wave eigenfunctions. This procedure was carried out, for instance, in Gehne and Kleeman ...