Wind energy potential in the site of Borj-Cedria in Tunisia

Two examples of snapshots of absolute momentum fluxes (colors, logarithmic scale) and wind speed (thick gray lines for isotachs 20 and 40 m s −1 , thick black line for 60 m s −1 ) at

The median momentum flux in- creases linearly with background wind speed: for winds larger than 50 m s −1 , the median gravity wave momentum fluxes are about 4 times larger than

In the high-time-resolution data from Explorer 43 (Imp I) we found that the lowest magnetic field intensities (< 1 'y) in the solar wind at 1 A U nearly always occur

2 Observed probability distribution (bins) and Weibull probability distribution (lines) of the wind speed in the pre-monsoon period during day, night and both day and night at

L’accès à ce site Web et l’utilisation de son contenu sont assujettis aux conditions présentées dans le site LISEZ CES CONDITIONS ATTENTIVEMENT AVANT D’UTILISER CE SITE

Cette étude nous permettra de caractériser et hiérarchiser les paramètres à prendre en compte pour appréhender le transfert sol-nappe-rivière des pesticides, de cibler ceux

Noisy labels are contained in the Dataset: images selected through AMEDA contours and labeled as AE or CE might not contain eddy signature or, mutatis mutandis, images la- beled as N

In this article we re- port eddy covariance flux measurements obtained during a field test of a newly developed and improved tunable quan- tum cascade laser absorption