Identifier la Valeur de la Position, de Unités a Centaines De Millions (Format SI) (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

[“The nor- mal, thickness, and speed of the dusk magnetopause current layer from Cluster Electric Field and Wave experiment mea- surements of spacecraft potential”,

Neither the combined solar and auroral evidence for an individual intense (recurrent) geomagnetic storm during De- cember in AD 1128 (Sects. 2 and 3), nor the associated au-

(1981) solar flux model with the temperature depen- dent rate coefficient and a quantum yield of 0.36 for the re- action N 2 (A 3 P + u )+ O agree to within 8% of the observed

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

The tradi- tional K¨ohler theory that describes the equilibrium growth of a droplet as a function of supersaturation explains well the CCN activation of water soluble

An improved physical deterministic radiative transfer model along with long-term climatological data for various key physical surface and atmospheric parameters have been used