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...
Event Description:During an automobile accident, the body of ████ ██, a passenger in one involved vehicle, expanded to fill the entire interior of the vehicle. Because Mr. ██'s expanded body had taken on a consistency similar to stiff foam rubber, the other occupants of the vehicle...
Homework: The Polytechnic University of the Philippines Remote Workplace Arrangement Assessment With different views and perspectives in the effect of work-from-home arrangement on the productivity and efficiency of the delivery of work, this study ai... Dizon, Ricardo L.,Monsura, Melcah P.,Gapas...
Kopp, "Velocity measurements around low-profile, tilted, solar arrays mounted on large flat-roofs, for wall normal wind directions." Journal of Wind Engineering and Industrial Aerodynamics 123, 226-238, 2013.Pratt. R.N.. Kopp, G.A., 2013. Velocity measurements around low-profile, tilted, ...
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 ...