998 resultados para Sugar addition


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Vanadium Oxide has been a frontrunner in the field of oxide electronics because of its metal-insulator transition (MIT). The interplay of different structures of VO2 has played a crucial role in deciding the magnitude of the first order MIT. Substitution doping has been found to introduce different polymorphs of VO2. Hence the role of substitution doping in stabilizing the competing phases of VO2 in the thin film form remains underexplored. Consequently there have been reports both discounting and approving such a stabilization of competing phases in VO2. It is reported in the literature that the bandwidth of the hysteresis and transition temperature of VO2 can be tuned by substitutional doping of VO2 with W. In this work, we have adopted a novel technique called, Ultrasonic Nebulized Spray Pyrolysis of Aqueous Combustion Mixture (UNSPACM) to deposit VO2 and W- doped VO2 as thin films. XRD and Raman spectroscopy were used to investigate the role of tungsten on the structure of VO2 thin films. Morphology of the thin films was found to be consisting of globular and porous nanoparticles of size similar to 20nm. Transition temperature decreased with the addition of W. We found that for 2.0 at % W doping in VO2, the transition temperature has reduced from 68 degrees C to 25 degrees C. It is noted that W-doping in the process of reducing the transition temperature, alters the local structure and also increases room temperature carrier concentration. (c) 2016 Author(s).

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Minor yttrium addition can improve the glass-forming ability of Cu-Zr-Al ternary alloys via suppression of the growth of eutectic clusters. Yttrium addition also makes the room temperature ductility of the alloys decrease, and both the compressive strength and elastic strain limits increase slightly.

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An attempt has been made to prepare a YBa2Cu3O 7-δ (YBCO) thin film doped with ferromagnetic CoFe 2O4. Transmission electron microscopy of the resultant samples shows, however, that Y(Fe, Co)O3 forms as a nanoparticulate dispersion throughout the film in preference to CoFe2O4, leaving the YBCO yttrium deficient. As a consequence, the superconducting properties of the sample are poor, with a self-field critical current density of just 0.25 MA cm-2. Magnetic measurements indicate however that the Y(Fe, Co)O3 content, together with any other residual phases, is also ferromagnetic, and some interesting features are present in the in-field critical current behaviour, including a reduced dependence on applied field and a strong c-axis peak in the angular dependence. The work points the way towards future attempts utilising YFeO3 as an effective ferromagnetic pinning additive for YBCO. © 2009 Elsevier B.V. All rights reserved.

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A kind of novel Ti-based composites was developed by introducing different amounts of carbon element to the Ti-50 Cu-23 Ni-20 Sn-7 bulk metallic glass forming alloys. The thermal stability and microstructural evolution of the composites were investigated. Room temperature compression tests reveal that the composite samples with 1% and 3% (mass fraction) carbon additions have higher fracture strength and obvious plastic strain of 2 195 MPa, 3.1% and 1 913 MPa, 1.3% respectively, compared with those of the corresponding carbon-free Ti-50 Ni-20 Cu-23 Sn-7 alloys. The deformation mechanisms of the composites with improved mechanical properties were also discussed.

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Se hizo un experimento para determinar el efecto de periodos de protección de plagas del follajes y frutos sobre el rendimiento y la ganancia neta en el cultivo de sandía para exportación. el experimento fue ubicado entre Nagarote y la paz centro, realizándose en los meses de febrero a abril de 1988, bajo riego. Para la protección del cultivo de las plagas se utilizó el insecticida prfenofos más riopcord (tambo 880 ecu). La dinámica poblacional mostró que las plagas que provocaron daños directo a los frutos como larvas de spodoptera spp. (lepidóptera: noctuidae) y heliothis ssp. (Lepidóptera: noctuidae), se acentuaron desde los 40 días después de la emergencia (DDE) de las plantas hasta el final de la cosecha. Las plagas que afectaron principalmente los follajes como lyriomiza spp. (Díptera: agromizidae) y aphis spp. Homóptera: aphididae) fueron más constante pero que a partir de los 38 DDE aumentaron sus poblaciones y provocaron un daño severo. El tratamiento que fue protegido desde la emergencia de la planta hasta la cosecha ocupo el primer lugar en fruto/mz, pero sin diferencias significativas entre los periodo de protección a excepción del testigo (sin protección). Así también se colocó en el primer lugar en el número de cajas con frutos exportables por su tamaño/mz, pero sin diferencia significativas con los periodos protegidos desde los 19 y 43 DDE hasta la cosecha. El periodo protegido en ninguna fase de cultivo y el periodo protegido desde la emergencia hasta los 43 DDE ocuparon el primer lugar en fruto no exportable por su tamaño demasiado pequeño. El tratamiento protegido desde los 19 DDE hasta la cosecha presento la mayor ganancia neta. Se presentó deformación de frutos entre 70 y80 %, no presentándose efecto de periodo de protección.

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The influence of the momentum addition, which may be associated with the average or fluctuation transverse component of the magnetic field or others, on the acceleration the solar wind or stellar wind is studied in a local streamtube. The results show that the larger the momentum addition the stronger the acceleration of the wind. For example, if the typical transverse magnetic field is about 0.1 of the longitudinal field, the velocity of the solar wind at 1 AU may be increased by 40%. The coronal hole may be considered as a streamtube, the presence of a high stream from the coronal hole may be explained by the existence of an average or fluctuation transverse magnetic field in the streamtube. A similar conclusion may be applied to the polar region, where the velocity of the solar wind will be larger than elsewhere as if there is a transverse component of magnetic field, as well as to the stellar wind. The influence of other parameters on the acceleration of the solar wind is also discussed. From the viewpoint of the solar wind mechanism, the present paper shows that the momentum addition in the subsonic flow region can increase the velocity of the solar wind at 1 AU.

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