50 research outputs found

    Analysis of Strong-Coupling Parameters for Superfluid 3He

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    Superfluid 3^{3}He experiments show strong deviation from the weak-coupling limit of the Ginzburg-Landau theory, and this discrepancy grows with increasing pressure. Strong-coupling contributions to the quasiparticle interactions are known to account for this effect and they are manifest in the five β\beta-coefficients of the fourth order Ginzburg-Landau free energy terms. The Ginzburg-Landau free energy also has a coefficient gzg_{z} to include magnetic field coupling to the order parameter. From NMR susceptibility experiments, we find the deviation of gzg_{z} from its weak-coupling value to be negligible at all pressures. New results for the pressure dependence of four different combinations of β\beta-coefficients, β\beta_{345}, β\beta_{12}, β\beta_{245}, and β\beta_{5} are calculated and comparison is made with theory.Comment: 6 pages, 2 figures, 1 table. Manuscript prepared for QFS200

    The G-O Rule and Waldmeier Effect in the Variations of the Numbers of Large and Small Sunspot Groups

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    We have analysed the combined Greenwich and Solar Optical Observing Network (SOON) sunspot group data during the period of 1874-2011 and determined variations in the annual numbers (counts) of the small, large and big sunspot groups (these classifications are made on the basis of the maximum areas of the sunspot groups). We found that the amplitude of an even-numbered cycle of the number of large groups is smaller than that of its immediately following odd-numbered cycle. This is consistent with the well known Gnevyshev and Ohl rule or G-O rule of solar cycles, generally described by using the Zurich sunspot number (Rz). During cycles 12-21 the G-O rule holds good for the variation in the number of small groups also, but it is violated by cycle pair (22, 23) as in the case of Rz. This behaviour of the variations in the small groups is largely responsible for the anomalous behaviour of Rz in cycle pair (22, 23). It is also found that the amplitude of an odd-numbered cycle of the number of small groups is larger than that of its immediately following even-numbered cycle. This can be called as `reverse G-O rule'. In the case of the number of the big groups, both cycle pairs (12, 13) and (22, 23) violated the G-O rule. In many cycles the positions of the peaks of the small, large, and big groups are different and considerably differ with respect to the corresponding positions of the Rz peaks. In the case of cycle 23, the corresponding cycles of the small and large groups are largely symmetric/less asymmetric (Waldmeier effect is weak/absent) with their maxima taking place two years later than that of Rz. The corresponding cycle of the big groups is more asymmetric (strong Waldmeier effect) with its maximum epoch taking place at the same time as that of Rz.Comment: 13 pages, 5 figures, 1 table, accepted by Solar Physic

    Propriedades químicas de uma Terra Roxa Estruturada influenciadas pela cobertura vegetal de inverno e pela adubação orgânica e mineral

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    O presente trabalho teve por objetivo avaliar a influência da cobertura vegetal de inverno, constituída de uma associação de aveia preta (Avena strigosa Schreb) com nabo forrageiro (Raphanus sativus L.), da adubação orgânica com esterco de aves e da adubação mineral sobre propriedades químicas de uma Terra Roxa Estruturada do estado de Santa Catarina. As análises foram realizadas em amostras de solo coletadas em agosto de 1994 e janeiro de 1995, nas profundidades de 0-10, 10-20 e 20-30 cm, em um experimento iniciado em 1990. Observou-se que a cobertura vegetal de inverno mostrou-se eficiente na manutenção de nutrientes, especialmente o potássio, e dos níveis de carbono orgânico, dentro dos limites da camada arável. O uso de adubo orgânico proporcionou acúmulo de nutrientes no solo, enquanto os adubos organomineral e mineral mostraram tendência de redução, principalmente dos níveis de potássio do solo

    Solar Surface Magnetism and Irradiance on Time Scales from Days to the 11-Year Cycle

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    ULTRALOW INTERACTION TEMPERATURES AND CRYSTAL FIELD EFFECTS FOR Gd IMPURITIES IN YPd3 AND CePd3

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    La susceptibilité magnétique des impuretés de Gd montre que le comportement des ions est indépendant jusqu'à 10 mK si la concentration est inférieure 0.15 % dans YPd3 et inférieure à 0,5% dans CePd3. On peut expliquer ces résultats dans un modèle de champ cristallin.The magnetic susceptibility of Gd impurities shows single ion behaviour down to 10 mK at concentrations below 0.15 a/o in YPd3 and below 0.5 a/o in CePd3. The data can be fitted with crystal field theory

    Lost in Transit — A Forgotten Rodent Welfare Issue?

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