An FDTD method for analysis of scattering from rough fluid-fluidinterfaces     

Hastings  F.D. Schneider  J.B. Broschat  S.L. Thorsos  E.I. 《Oceanic Engineering, IEEE Journal of》2001,26(1):94-101

A finite-difference time-domain (FDTD) method for scattering by one-dimensional, rough fluid-fluid interfaces is presented, modifications to the traditional FDTD algorithm are implemented which yield greater accuracy at lower computational cost. These modifications include use of a conformal technique, in which the grid conforms locally to the interface, and a correction for the numerical dispersion inherent to the FDTD algorithm, Numerical results are presented for fluid-fluid cases modeling water-sediment interfaces. Two different roughness spectra, the single-scale Gaussian roughness spectrum and a multiscale modified power-law spectrum, are used. The Gaussian results are calculated as a function of the dimensionless parameters kh and kl, where k is the wavenumber in water, h is the rms surface height, and l is the surface correlation length. For the modified power-law spectrum, statistical parameters consistent with an insonification frequency of 7.5 kHz are used. Results are compared with those obtained using an integral equation technique both for scattering from single-surface realizations and for Monte Carlo averages of scattering from an ensemble of surface realizations. Scattering strengths are calculated as a function of scattering angle for an incident angle of 70° (20° grazing). The results agree well over all scattering angles for the cases examined  相似文献   

Panchromatic properties of 99 000 galaxies detected by SDSS, and (some by) ROSAT, GALEX, 2MASS, IRAS, GB6, FIRST, NVSS and WENSS surveys     

M. Obri&#;  &#;. Ivezi&#;  P. N. Best  R. H. Lupton  C. Tremonti  J. Brinchmann  M. A. Agüeros  G. R. Knapp  J. E. Gunn  C. M. Rockosi  D. Schlegel  D. Finkbeiner  M. Ga&#;e&#;a  V. Smol&#;i&#;  S. F. Anderson  W. Voges  M. Juri&#;  R. J. Siverd  W. Steinhardt  A. S. Jagoda  M. R. Blanton  D. P. Schneider 《Monthly notices of the Royal Astronomical Society》2006,370(4):1677-1698

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Early enrichment of quasars by the first stars     

A. Venkatesan  R. Schneider †  A. Ferrara 《Monthly notices of the Royal Astronomical Society》2004,349(3):L43-L48

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On the Interpretation of Continuous Resistivity Distributions in the Magnetotelluric Method     

D. Rankin  I. K. Reddy  K. Schneider 《Geophysical Journal International》1976,45(1):89-95

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Holocene climate variability as derived from alkenone sea surface temperature and coupled ocean-atmosphere model experiments     

N.?RimbuEmail author  G.?Lohmann  S.?J.?Lorenz  J.?H.?Kim  R.?R.?Schneider 《Climate Dynamics》2004,23(2):215-227

Holocene climate modes are identified by the statistical analysis of reconstructed sea surface temperatures (SSTs) from the tropical and North Atlantic regions. The leading mode of Holocene SST variability in the tropical region indicates a rapid warming from the early to mid Holocene followed by a relatively weak warming during the late Holocene. The dominant mode of the North Atlantic region SST captures the transition from relatively warm (cold) conditions in the eastern North Atlantic and the western Mediterranean Sea (the northern Red Sea) to relatively cold (warm) conditions in these regions from the early to late Holocene. This pattern of Holocene SST variability resembles the signature of the Arctic Oscillation/North Atlantic Oscillation (AO/NAO). The second mode of both tropical and North Atlantic regions captures a warming towards the mid Holocene and a subsequent cooling. The dominant modes of Holocene SST variability emphasize enhanced variability around 2300 and 1000 years. The leading mode of the coupled tropical-North Atlantic Holocene SST variability shows that an increase of tropical SST is accompanied by a decrease of SST in the eastern North Atlantic. An analogy with the instrumental period as well as the analysis of a long-term integration of a coupled ocean-atmosphere general circulation model suggest that the AO/NAO is one dominant mode of climate variability at millennial time scales.  相似文献   

Assessing selected natural and anthropogenic impacts on freshwater lens morphology on small barrier Islands: Dog Island and St. George Island, Florida, USA   总被引：3，自引：2，他引：1  

James C. Schneider  Sarah E. Kruse 《Hydrogeology Journal》2006,14(1-2):131-145

Abstract The freshwater lens morphologies of the barrier islands Dog Island and St. George Island on the panhandle coast of Florida (FL), USA, are controlled to varying degrees by both natural and anthropogenic factors. Variable-density groundwater flow models confirm that spatial variability of recharge values can account for the observed lens asymmetry on these islands. The depth to the base of the lens does not vary significantly seasonally. Human development has altered recharge patterns in some areas, locally thinning the freshwater lens. Aqueduct water supply to St. George Island represents 7–25% of natural recharge; higher recharge rates are required to simulate the lens on St. George Island than on Dog Island. On both islands, coastal erosion rates are sufficiently rapid that the freshwater lens may not be in equilibrium with current boundary conditions.

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Resumen Las morfologías de los lentes de agua dulce en las islas de barrera: Islas Dog y St. George, en la costa alargada y estrecha de Florida, EUA, están controladas en diferentes grados por factores antropogénicos y naturales. Los modelos de flujo con densidad variable del agua subterránea, confirman que la variabilidad espacial de los valores de recarga, pueden ser la causa de la asimetría observada en los lentes de estas islas. La profundidad hasta la base de los lentes no varía significativamente con las estaciones climáticas. El desarrollo humano ha alterado las tendencias de recarga en algunas áreas, causando adelgazamiento local de los lentes de agua dulce. El abastecimiento de agua del acueducto en la Isla St. George, representa entre 7% y 25% de la recarga natural; por otro lado se necesitan cantidades mayores de recarga para simular los lentes en la Isla St. George que en la Isla Dog. En ambas islas, las tasas de erosión costera son tan rápidas, que las lentes de agua dulce podrían no estar en equilibrio con las condiciones actuales de frontera.

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Résumé La morphologie des lentilles deau douce des îles de Dog et de St. George, situés dans le district côtier de Florida-Etats Unis est contrôlé dans une mesure variable par des facteurs naturelles et humaines. Les modèles découlement à densité variable des eaux souterraines confirment que la variation spatiale de la recharge peut expliquer les asymétries observées des lentilles des cettes îles. La profondeur des lentilles ne présente pas des variations saisonnières importantes. Les activités humaines ont modifié la recharge dans certaines zones en amincissant localement les lentilles deau douce. Lalimentation en eaux de lîle de St. George représente 7–25% de la recharge naturelle; pour simuler les lentilles de lîle de Dog il a été nécessaire dintroduire des valeurs plus élevées de la recharge par rapport aux ceux utilisés pour lîle de St. George. Pour les deux îles lérosion côtière est assez rapide ainsi que les lentilles de eau douce ne sont pas en équilibre avec les conditions à la frontière.

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On the interpolation of precipitation data over complex terrain     

M. Dorninger  S. Schneider  R. Steinacker 《Meteorology and Atmospheric Physics》2008,101(3-4):175-189

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Climatic Change Letters inaugural editorial     

Stephen H. Schneider  Michael Oppenheimer 《Climatic change》2009,97(1-2):1-2

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Stellar sources of dust in the high-redshift Universe     

Rosa Valiante  Raffaella Schneider  Simone Bianchi  Anja C. Andersen 《Monthly notices of the Royal Astronomical Society》2009,397(3):1661-1671

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Relative clustering and the joint halo occupation distribution of red sequence and blue-cloud galaxies in COMBO-17     

P. Simon  M. Hetterscheidt  C. Wolf  K. Meisenheimer  H. Hildebrandt  P. Schneider  M. Schirmer  T. Erben 《Monthly notices of the Royal Astronomical Society》2009,398(2):807-831

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