Dés 10 ! – Le blog du Cancre
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Models describing the evolution of long internal waves are proposed that are based on different polynomial approximations of the exact expression for the phase speed of
board the FAST spacecraft when it was located in the night- side magnetosphere at an invariant latitude of 68 ◦. In this figure we see a large number of negative sloped traces in
L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des
From a modelling point of view, the conclusion is that a uni-modal approach is not well suited for describing the evo- lution (i.e. generation and propagation) of internal
(7), (21)–(23) with corre- sponding boundary conditions, the self-consistent profiles of partial and total current densities, plasma density, electric and magnetic fields as well
Figure 4a shows 30 ms of the parallel electric wave form measured at three locations with respect to the acceleration layer, in the upper part of the layer (indicated as above layer)
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