Abstract. The time domain sampler (TDS) experiment on WIND measures electric and magnetic wave forms with a sampling rate which reaches 120 000 points per second. We analyse here observations made in the solar wind near the Lagrange point v1. In the range of frequencies above the proton plasma frequency f pi and smaller than or of the order of the electron plasma frequency f pe , TDS observed three kinds of electrostatic (e.s.) waves: coherent wave packets of Langmuir waves with frequencies f 9 f pe , coherent wave packets with frequencies in the ion acoustic range f pi f`f pe , and more or less isolated non-sinusoidal spikes lasting less than 1 ms. We con®rm that the observed frequency of the low frequency (LF) ion acoustic wave packets is dominated by the Doppler eect: the wavelengths are short, 10 to 50 electron Debye lengths k h . The electric ®eld in the isolated electrostatic structures (IES) and in the LF wave packets is more or less aligned with the solar wind magnetic ®eld. Across the IES, which have a spatial width of the order of 925k h , there is a small but ®nite electric potential drop, implying an average electric ®eld generally directed away from the Sun. The IES wave forms, which have not been previously reported in the solar wind, are similar, although with a smaller amplitude, to the weak double layers observed in the auroral regions, and to the electrostatic solitary waves observed in other regions in the magnetosphere. We have also studied the solar wind conditions which favour the occurrence of the three kinds of waves: all these e.s. waves are observed more or less continuously in the whole solar wind (except in the densest regions where a parasite prevents the TDS observations). The type (wave packet or IES) of the observed LF waves is mainly determined by the proton temperature and by the direction of the magnetic ®eld, which themselves depend on the latitude of WIND with respect to the heliospheric current sheet.
L'estimation des stocks de poissons que peut abriter un secteur de cours d'eau non pollué nécessite le calcul de sa capacité d'accueil en terme d'espace et de nourriture. Le premier volet a donné lieu aux Etats-Unis à la mise en place de modèles de comportement de différentes espèces de poissons en fonction de variables physiques et de modèles hydrauliques décrivant l'évolution temporelle de ces variables.
Les hypothèses sous-jacentes sont discutées. Une modification du calcul de la perte de charge linéaire est préconisée pour le modèle hydraulique dans le cas des rivières à truites, et l'utilisation de méthodes multivariées est proposée pour décrire avec une meilleure fiabilité les relations entre densités de poissons et variables physiques des cours d'eau.
Quelques cas d'application illustrent l'intérêt de cette démarche pour répondre à des questions posées par les gestionnaires, tant en matière de prévision des impacts piscicoles des aménagements que d'optimisation des repeuplements.
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