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

(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

Wadhams (2015), Relating wave attenuation to pancake ice thickness, using field measurements and model results, Geophys.. American

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

Comparison of critical supersaturation as a function of particle size for initial dry (solid lines) and wet (dashed lines) particles of ternary mixtures of adipic acid, succinic

The absence of a clear enhance- ment of the HONO-formation under UV-A light, as expected from the UV-A experiments on the humic acid coatings (i.e. by a factor of ≈3 under