Tableau de Valeur de Position (de Centaines de Milliers à des Unités)

(2005) observed an early/fast type VLF perturbation in association with an optical elve captured during the EuroSprite2003 campaign, which constitutes indirect evidence for

2, 3, 4 and 5 that the time series data of the 3-point running average of zonal, meridional and vertical velocities are in- creasing with increasing height in the troposphere and

(i) we establish a more comprehensive description of day- side auroral morphology applicable to southeast/west IMF which contains as three basic elements the PMAFs/prenoon, midday

We concluded from these simulation studies that, if QP echoes were the result of the projection movement of gravity wave packets along the radar beam, then we can identify the slope

for unperturbed Central European summer conditions: lines and symbols refer to 10-percentile, 90-percentile, and median values from ECHAM/MADE for Central Europe in July/August

IRIS keeps the full ISSA resolution, it includes well-calibrated point sources, and the diffuse emission calibration at scales smaller than 1  was corrected for the variation of

A key element when modeling dust in any astrophysical environment is a self-consistent treatment of the evolution of the dust material properties (size distribution,

Our models a4 and a4he match the SN 1987A light curve better at early times but less well around the time of maximum (model a4he peaks about 10 d later than SN 1987A).. As argued