Identifier la Valeur de la Position, de Unités a Milliers (Format Européen) (A)

using both methods with such a relatively large maximum allowed shift (17 grid points) yields to an unphysical comparison between forecast an observed fields.. A larger do- main over

Dst and Dst*, characteristic of the equatorial magnetic ®eld, responded to the 1314 (‹5) UT southward turning prior to the ®rst observed substorm expansion phase onset, suggesting

Whereas the 13:00–15:00 MLT sector is characterized by classical poleward moving auroral forms (PMAFs) asso- ciated with merging cell transients, the aurora in the 15:00– 17:00

Though the conceptual forced Lorenz model is too simple to be used directly for the study of monsoon predictability, the bifurcation analysis of the forced Lorenz model presented

The annual contours of the EW (zonal) and NS (meridional) components of the mean winds, as functions of height versus time, are shown in Fig.. The height co-ordinates are dif- ferent

The auroral features which the combination of two meridian scanning photometers and an all-sky imager made us able to illuminate are the following: (1) a three- phase evolution of

Phys. W.: The structure of the exosphere, or adventures in ve- locity space, in: Geophysics, The Earth’s Environment, edited by: De-Witt, C., Hiebolt, J., and Lebeau, A., pp. D.:

The direct effect of aerosols on solar radiation based on satellite observations, reanalysis datasets, and spectral aerosol optical properties from Global Aerosol Data Set