115 research outputs found

    Observations of the brightness temperature distribution of the quiet solar corona at decametric wavelengths

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    The brightness temperature distribution of the quiet solar corona at a wavelength of 8.9 meters is measured by two types of radio telescope: (1) a 'T' type array with a resolution of 26'X38', and (2) a fan beam interferometer with an E-W resolution of 3'. It is found that the persistent bright regions do not have any angular structure on scales of 6' or less. The daily variations of the brightness temperature of different regions are studied and the possible interpretation discussed

    The pressure-amorphized state in zirconium tungstate: a precursor to decomposition

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    In contrast to widely accepted view that pressure-induced amorphization arises due to kinetic hindrance of equilibrium phase transitions, here we provide evidence that the metastable pressure-amorphized state in zirconium tungstate is a precursor to decomposition of the compound into a mixture of simple oxides. This is from the volume collapse ΔV across amorphization, which is obtained for the first time by measuring linear dimensions of irreversibly amorphized samples during their recovery to the original cubic phase upon isochronal annealing up to 1000 K. The anomalously large ΔV of 25.7 ± 1.2% being the same as that expected for the decomposition indicates that this amorphous state is probably a precursor to kinetically hindered decomposition. A P–T diagram of the compound is also proposed

    A Wideband Annular Ring Radiator with Polygonal Ground Plane

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    Vivaldi radiators and its variants have been extensively used for wideband single antenna and array applications. The Vivaldi radiator and other radiators such as spirals, log periodic, ridged gap wave guides are predominantly 3D antennas. There has been a need for a truly planar antenna for antenna array applications in the Communications, EW and Radar band of 6-18 GHz. In this paper a wideband radiator covering 6-22GHz is designed and analyzed using HFSS simulations. The popularly known UWB antenna technology is now quite matured leading to effective coverage of the communication band of frequencies from 3.1 to 10.6 GHz. This technology is adapted to design, analyze and implement a planar element radiator for array applications covering the 6-18GHz band. The antenna is realized in hardware with a return loss of less than -10dB over 7.2GHz to 22 GHz and good radiation patterns from 6.0 to 15 GHz

    A thermodynamic unification of jamming

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    Fragile materials ranging from sand to fire-retardant to toothpaste are able to exhibit both solid and fluid-like properties across the jamming transition. Unlike ordinary fusion, systems of grains, foams and colloids jam and cease to flow under conditions that still remain unknown. Here we quantify jamming via a thermodynamic approach by accounting for the structural ageing and the shear-induced compressibility of dry sand. Specifically, the jamming threshold is defined using a non-thermal temperature that measures the 'fluffiness' of a granular mixture. The thermodynamic model, casted in terms of pressure, temperature and free-volume, also successfully predicts the entropic data of five molecular glasses. Notably, the predicted configurational entropy avoids the Kauzmann paradox entirely. Without any free parameters, the proposed equation-of-state also governs the mechanism of shear-banding and the associated features of shear-softening and thickness-invariance.Comment: 16 pgs double spaced. 4 figure

    Curvature fluctuations and Lyapunov exponent at Melting

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    We calculate the maximal Lyapunov exponent in constant-energy molecular dynamics simulations at the melting transition for finite clusters of 6 to 13 particles (model rare-gas and metallic systems) as well as for bulk rare-gas solid. For clusters, the Lyapunov exponent generally varies linearly with the total energy, but the slope changes sharply at the melting transition. In the bulk system, melting corresponds to a jump in the Lyapunov exponent, and this corresponds to a singularity in the variance of the curvature of the potential energy surface. In these systems there are two mechanisms of chaos -- local instability and parametric instability. We calculate the contribution of the parametric instability towards the chaoticity of these systems using a recently proposed formalism. The contribution of parametric instability is a continuous function of energy in small clusters but not in the bulk where the melting corresponds to a decrease in this quantity. This implies that the melting in small clusters does not lead to enhanced local instability.Comment: Revtex with 7 PS figures. To appear in Phys Rev

    Structure and Stability of an Amorphous Metal

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    Using molecular dynamics simulations, with a realistic many-body embedded-atom potential, and a novel method to characterize local order, we study the structure of pure nickel during the rapid quench of the liquid and in the resulting glass. In contrast with previous simulations with pair potentials, we find more crystalline order and fewer icosahedra for slower quenching rates, resulting in a glass less stable against crystallization. It is shown that there is not a specific amorphous structure, only the arrest of the transition from liquid to crystal, resulting in small crystalline clusters immersed in an amorphous matrix with the same structure of the liquid.Comment: 4 pages, 4 ps figs., to appear in Phys. Rev. Let

    Molecular dynamics simulations of non-equilibrium systems

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    Peer reviewe

    The Energy Density of Solar Wind and its Correlation with Cosmic Ray Intensity

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    Short-Term Correlations of Decameter Radio Emission from Jupiter and Solar Activity.

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