29,845 research outputs found

    Calculations of radar backscattering coefficient of vegetation-covered soils

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    A model for simulating the measured backscattering coefficient of vegetation-covered soil surfaces includes both coherent and incoherent components of the backscattered radar pulses from a rough sil surface. The effect of vegetation canopy scattering is also incorporated into the model by making the radar pulse subject to two-way attenuation and volume scattering when it passes through the vegetation layer. Model results agree well with the measured angular distributions of the radar backscattering coefficient for HH polarization at the 1.6 GHz and 4.75 GHz frequencies over grass-covered fields. It was found that the coherent scattering component is very important at angles near nadir, while the vegetation volume scattering is dominant at incident angles 30 degrees

    Analytical Approximations to Galaxy Clustering

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    We discuss some recent progress in constructing analytic approximations to the galaxy clustering. We show that successful models can be constructed for the clustering of both dark matter and dark matter haloes. Our understanding of galaxy clustering and galaxy biasing can be greatly enhanced by these models.Comment: 10 pages, Latex, crckapb.sty, figure included, to appear in the proceedings of Ringberg Workshop on Large-Scale Structure (ed. D. Hamilton; Kluwer Academic Publishers

    Calculations of the spectral nature of the microwave emission from soils

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    The brightness temperatures for a set of soil profiles observed at USDA facilities in Arizona and Georgia were calculated at the wavelengths of 2.8, 6, 11, 21, and 49 cm using a coherent radiative transfer model. The soil moisture sampling depth is found to be a function of wavelength and is in the range 0.06 to 0.1 of a wavelength. The thermal sampling depth also depends on wavelength and is approximately equal to one wavelength at dry soil condition and 0.1 - 0.5 wavelengths at wet soil conditions. Calculated values of emissivity show strong diurnal variations when the soils are wet, while there is little diurnal change when the soil is dry. The soil moistures within the four depth intervals of 0-2, 0-5, 0-9, and 0-15 cm were parameterized as function of the calculated emissivity and brightness temperature. Best-fit parameters and correlation coefficients are presented for five wavelengths. Interrelationships among the effective temperature, surface temperature, and emissivity are displayed

    Albedo and flux extinction coefficient of impure snow for diffuse shortwave radiation

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    Impurities enter a snowpack as a result of fallout of scavenging by falling snow crystals. Albedo and flux extinction coefficient of soot contaminated snowcovers were studied using a two stream approximation of the radiative transfer equation. The effect of soot was calculated by two methods: independent scattering by ice grains and impurities and average refractive index for ice grains. Both methods predict a qualitatively similar effect of soot; the albedo is decreased and the extinction coefficient is increased compared to that for pure snow in the visible region; the infrared properties are largely unaffected. Quantitatively, however, the effect of soot is more pronounced in the average refractive index method. Soot contamination provides a qualitative explanation for several snow observations

    Lagrangian bias in the local bias model

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    It is often assumed that the halo-patch fluctuation field can be written as a Taylor series in the initial Lagrangian dark matter density fluctuation field. We show that if this Lagrangian bias is local, and the initial conditions are Gaussian, then the two-point cross-correlation between halos and mass should be linearly proportional to the mass-mass auto-correlation function. This statement is exact and valid on all scales; there are no higher order contributions, e.g., from terms proportional to products or convolutions of two-point functions, which one might have thought would appear upon truncating the Taylor series of the halo bias function. In addition, the auto-correlation function of locally biased tracers can be written as a Taylor series in the auto-correlation function of the mass; there are no terms involving, e.g., derivatives or convolutions. Moreover, although the leading order coefficient, the linear bias factor of the auto-correlation function is just the square of that for the cross-correlation, it is the same as that obtained from expanding the mean number of halos as a function of the local density only in the large-scale limit. In principle, these relations allow simple tests of whether or not halo bias is indeed local in Lagrangian space. We discuss why things are more complicated in practice. We also discuss our results in light of recent work on the renormalizability of halo bias, demonstrating that it is better to renormalize than not. We use the Lognormal model to illustrate many of our findings.Comment: 14 pages, published on JCA

    Decays of J/ψJ/\psi and ψ\psi^\prime into vector and pseudoscalar meson and the pseudoscalar glueball-qqˉq\bar{q} mixing

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    We introduce a parametrization scheme for J/ψ(ψ)VPJ/\psi(\psi^\prime)\to VP where the effects of SU(3) flavor symmetry breaking and doubly OZI-rule violation (DOZI) can be parametrized by certain parameters with explicit physical interpretations. This scheme can be used to clarify the glueball-qqˉq\bar{q} mixing within the pseudoscalar mesons. We also include the contributions from the electromagnetic (EM) decays of J/ψJ/\psi and ψ\psi^\prime via J/ψ(ψ)γVPJ/\psi(\psi^\prime)\to \gamma^*\to VP. Via study of the isospin violated channels, such as J/ψ(ψ)ρηJ/\psi(\psi^\prime)\to \rho\eta, ρη\rho\eta^\prime, ωπ0\omega\pi^0 and ϕπ0\phi\pi^0, reasonable constraints on the EM decay contributions are obtained. With the up-to-date experimental data for J/ψ(ψ)VPJ/\psi(\psi^\prime)\to VP, J/ψ(ψ)γPJ/\psi(\psi^\prime)\to \gamma P and PγγP\to \gamma\gamma, etc, we arrive at a consistent description of the mentioned processes with a minimal set of parameters. As a consequence, we find that there exists an overall suppression of the ψ3g\psi^\prime\to 3g form factors, which sheds some light on the long-standing "ρπ\rho\pi puzzle". By determining the glueball components inside the pseudoscalar η\eta and η\eta^\prime in three different glueball-qqˉq\bar{q} mixing schemes, we deduce that the lowest pseudoscalar glueball, if exists, has rather small qqˉq\bar{q} component, and it makes the η(1405)\eta(1405) a preferable candidate for 0+0^{-+} glueball.Comment: Revised version to appear on J. Phys. G; An error in the code was corrected. There's slight change to the numerical results, while the conclusion is intac

    D2.7 Online mapping of Chinese and European ICT industrial associations – Final report

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    This document is a deliverable of CHOICE project task 2.2 Bringing together European and Chinese Industrial Associations. This task will, at the end of the project, have delivered a final version of an online database of relevant Chinese and European ICT industrial associations. This document is a report on the information gathered for the development of the online database of relevant Chinese and European ICT industrial associations. It maps Chinese industrial associations to European industrial associations in ICT. It does this by providing details of the Chinese industrial associations and other relevant bodies that are a Chinese priority for collaboration with their EU counterparts related to EU-China collaborative ICT R&D&I. Other such Chinese bodies that are not a Chinese priority for such collaboration that map to European industrial associations in ICT are then summarised so that a complete mapping of Chinese industrial associations and related bodies to European industrial associations in ICT can be made. Mappings are made based on the best matches in terms of the subject matter covered by the associations, in each case the best match based on this criteria is identified and highlighted by being given in bold type. If a mapped Chinese association is not a priority for collaboration it is identified in italics. The Chinese selection of Chinese bodies that are a priority for collaboration with EU counterparts reflects the relevant policy guidance provided on behalf of the Chinese government on how the aims of the "Twelfth Five-Year" National Strategic Emerging Industry Development Plan are to be achieved. An overview of the policy guidance relevant to ICT R&D&I is given in section one of CHOICE deliverable D2.4: Handbook for China ICT Industrial Support Services. Based on this mapping opportunities to foster interaction between the associations in China and Europe are identified. A DVD of the modest database that exists on the basis of the mapping presented in this report accompanies the report

    Calculations of microwave brightness temperature of rough soil surfaces: Bare field

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    A model for simulating the brightness temperatures of soils with rough surfaces is developed. The surface emissivity of the soil media is obtained by the integration of the bistatic scattering coefficients for rough surfaces. The roughness of a soil surface is characterized by two parameters, the surface height standard deviation sigma and its horizontal correlation length l. The model calculations are compared to the measured angular variations of the polarized brightness temperatures at both 1.4 GHz and 5 GHz frequences. A nonlinear least-squares fitting method is used to obtain the values of delta and l that best characterize the surface roughness. The effect of shadowing is incorporated by introducing a function S(theta), which represents the probability that a point on a rough surface is not shadowed by other parts of the surface. The model results for the horizontal polarization are in excellent agreement with the data. However, for the vertical polarization, some discrepancies exist between the calculations and data, particularly at the 1.4 GHz frequency. Possible causes of the discrepancy are discussed

    New Angle on the Strong CP and Chiral Symmetry Problems from a Rotating Mass Matrix

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    It is shown that when the mass matrix changes in orientation (rotates) in generation space for changing energy scale, then the masses of the lower generations are not given just by its eigenvalues. In particular, these masses need not be zero even when the eigenvalues are zero. In that case, the strong CP problem can be avoided by removing the unwanted θ\theta term by a chiral transformation in no contradiction with the nonvanishing quark masses experimentally observed. Similarly, a rotating mass matrix may shed new light on the problem of chiral symmetry breaking. That the fermion mass matrix may so rotate with scale has been suggested before as a possible explanation for up-down fermion mixing and fermion mass hierarchy, giving results in good agreement with experiment.Comment: 14 page

    A parameterization of effective soil temperature for microwave emission

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    A parameterization of effective soil temperature is discussed, which when multiplied by the emissivity gives the brightness temperature in terms of surface (T sub o) and deep (T sub infinity) soil temperatures as T = T sub infinity + C (T sub o - T sub infinity). A coherent radiative transfer model and a large data base of observed soil moisture and temperature profiles are used to calculate the best-fit value of the parameter C. For 2.8, 6.0, 11.0, 21.0 and 49.0 cm wavelengths. The C values are respectively 0.802 + or - 0.006, 0.667 + or - 0.008, 0.480 + or - 0.010, 0.246 + or - 0.009, and 0,084 + or - 0.005. The parameterized equation gives results which are generally within one or two percent of the exact values
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