9,235 research outputs found

    Solar-cycle variation of the sound-speed asphericity from GONG and MDI data 1995-2000

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    We study the variation of the frequency splitting coefficients describing the solar asphericity in both GONG and MDI data, and use these data to investigate temporal sound-speed variations as a function of both depth and latitude during the period from 1995-2000 and a little beyond. The temporal variations in even splitting coefficients are found to be correlated to the corresponding component of magnetic flux at the solar surface. We confirm that the sound-speed variations associated with the surface magnetic field are superficial. Temporally averaged results show a significant excess in sound speed around 0.92 solar radii and latitude of 60 degrees.Comment: To be published in MNRAS, accepted July 200

    Antiferromagnetic Alignment and Relaxation Rate of Gd Spins in the High Temperature Superconductor GdBa_2Cu_3O_(7-delta)

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    The complex surface impedance of a number of GdBa2_2Cu3_3O7δ_{7-\delta} single crystals has been measured at 10, 15 and 21 GHz using a cavity perturbation technique. At low temperatures a marked increase in the effective penetration depth and surface resistance is observed associated with the paramagnetic and antiferromagnetic alignment of the Gd spins. The effective penetration depth has a sharp change in slope at the N\'eel temperature, TNT_N, and the surface resistance peaks at a frequency dependent temperature below 3K. The observed temperature and frequency dependence can be described by a model which assumes a negligibly small interaction between the Gd spins and the electrons in the superconducting state, with a frequency dependent magnetic susceptibility and a Gd spin relaxation time τs\tau_s being a strong function of temperature. Above TNT_N, τs\tau_s has a component varying as 1/(TTN)1 / (T - T_N), while below TNT_N it increases T5\sim T^{-5}.Comment: 4 Pages, 4 Figures. Submitted to Phys. Rev.

    Saving for retirement: a review of ethnic minorities in the UK

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    This article examines the saving behaviour of ethnic minorities in the UK. Within the context of pension planning, we investigate saving for retirement patterns in relation to ethnicity, gender and age. We use data from the Family Resources Survey (FRS) to analyse employment status, income, saving types and levels. Although we find profound heterogeneity, ethnic minorities show higher levels of unemployment, lower income and consistently lower levels of saving for retirement compared to our white control group. Disadvantages of ethnic minorities during their working life persist, especially for women, although to a lesser extent than in the past, and continue to affect private savings and prospective retirement income. Indian and Chinese men have experienced the greatest improvements in terms of employment status and income and this is reflected in higher levels of saving for retirement since the mid 1990s

    Global shallow water magnetohydrodynamic waves in the solar tachocline

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    We derive analytical solutions and dispersion relations of global magnetic Poincar\'e (magneto-gravity) and magnetic Rossby waves in the approximation of shallow water magnetohydrodynamics. The solutions are obtained in a rotating spherical coordinate system for strongly and weakly stable stratification separately in the presence of toroidal magnetic field. In both cases magnetic Rossby waves split into fast and slow magnetic Rossby modes. In the case of strongly stable stratification (valid in the radiative part of the tachocline) all waves are slightly affected by the layer thickness and the toroidal magnetic field, while in the case of weakly stable stratification (valid in the upper overshoot layer of the tachocline) magnetic Poincar\'e and fast magnetic Rossby waves are found to be concentrated near the solar equator, leading to equatorially trapped waves. However, slow magnetic Rossby waves tend to concentrate near the poles, leading to polar trapped waves. The frequencies of all waves are smaller in the upper weakly stable stratification region than in the lower strongly stable stratification one
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