Bulk density effects on soil hydrologic and thermal characteristics: A numerical investigation          下载免费PDF全文

Yuki Kojima  Joshua L. Heitman  Masaru Sakai  Chihiro Kato  Robert Horton 《水文研究》2018,32(14):2203-2216

Soil bulk density (ρ_b) is commonly treated as static in studies of land surface dynamics. Magnitudes of errors associated with this assumption are largely unknown. Our objectives were to (a) quantify ρ_b effects on soil hydrologic and thermal properties and (b) evaluate effects of ρ_b on surface energy balance and heat and water transfer. We evaluated 6 soil properties, volumetric heat capacity, thermal conductivity, soil thermal diffusivity, water retention characteristics, hydraulic conductivity, and vapour diffusivity, over a range of ρ_b, using a combination of 6 models. Thermal conductivity, water retention, hydraulic conductivity, and vapour diffusivity were most sensitive to ρ_b, each changing by fractions greater than the associated fractional changes in ρ_b. A 10% change in ρ_b led to 10–11% change in thermal conductivity, 6–11% change in saturated and residual water content, 49–54% change in saturated hydraulic conductivity, and 80% change in vapour diffusivity. Subsequently, 3 field seasons were simulated with a numerical model (HYDRUS‐1D) for a range of ρ_b values. When ρ_b increased 25% (from 1.2 to 1.5 Mg m^?3), soil temperature variation decreased by 2.1 °C in shallow layers and increased by 1 °C in subsurface layers. Surface water content differed by 0.02 m³ m^?3 for various ρ_b values during drying events but differences mostly disappeared in the subsurface. Matric potential varied by >100 m of water. Surface energy balance showed clear trends with ρ_b. Latent heat flux decreased 6%, sensible heat flux increased 9%, and magnitude of ground heat flux varied by 18% (with a 25% ρ_b increase). Transient ρ_b impacted surface conditions and fluxes, and clearly, it warrants consideration in field and modelling investigations.  相似文献   

Layout design of rockbolts for natural ground reinforcement     

Junji Kato  Keiichiro Ishii  Kenjiro Terada  Takashi Kyoya 《国际地质力学数值与分析法杂志》2014,38(3):236-255

The present study addresses a layout design of rockbolts for reinforcing natural ground structures applying a special optimization method, called multiphase layout optimization. Rockbolts are used to tighten loosed natural ground, and the layout of rockbolts are determined without sufficient information about the physical properties of the ground materials. Because of this uncertainty, unexpected deformation often occurs at the excavation surface of natural ground. In that case, it is requested to determine an effective layout of the additional rockbolts promptly with respect to the actual deformation at the construction site. However, it is not easy to determine the optimal layout because of its complexity, and consequently, it has no choice but to determine the layout in an empirical way. This study introduces a numerical approach to determine an optimal layout of rockbolts with respect to arbitrarily possible deformation of natural ground. The objective is to maximize the stiffness of the overall ground structure reinforced with rockbolts. For optimization, a gradient‐based optimization scheme is applied because of its numerical efficiency. It was verified from a series of numerical examples that this method has great potential to improve the stiffness of the overall ground structure and shows a certain applicability to a practical design. Copyright © 2013 John Wiley & Sons, Ltd.  相似文献   

Late Paleozoic serpentinites and mafic schists from the Coast Range accretionary complex,central Chile: their relation to aeromagnetic anomalies     

E. Godoy  T. Kato 《International Journal of Earth Sciences》1990,79(1):121-130

Regional structural trends within the poorly exposed metamorphic basement complex of central Chile between 39°30' and 41°30'S latitudes are evident on total intensity aeromagnetic maps. Field and laboratory measurements of magnetic susceptibility indicate that anomalies are related to relic magnetite and rare ilmenite phase concentrations in serpentinites and lower greenschist facies mafic schists.Serpentinites and mafic schists representing fragmented ophiolites are common throughout a broad, highly magnetic central zone which separates a low-magnetic metaturbidites terrain in the Northeast from a southwestern, low susceptibility, metavolcanic rich area with isolated anomalies. One of the isolated anomalies represents a polyphase deformed serpentinite emplacement overlain by coarse grained eclogitic blueschist, highly magnetic undeformed serpentinites and amphibolite boulders thought to have been transported within the ultramafic body.The trend of the regional magnetic anomaly pattern is controlled by the main foliation, a crenulation cleavage (S2), rather than by primary factors, such as emplacement pattern of the ultramafics. This structural grain was established during the early Carboniferous event which culminated pre-Andean accretion in the area. The overall zonation, however, seems to reflect the composition of slices in a composite prism accreted during oblique subduction along the margin of Gondwanaland.

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Zusammenfassung Reliktische präkinematische (prä-S2) Magnetitanreicherungen kommen in Serpentiniten und Metabasiten der Grünschieferfazies des spätpaläozoischen Grundgebirges der Küstenkordillere Chiles häufig vor. Zwischen 39°30' und 41 °30' südlicher Breite wurden magnetische Messungen in situ in diesen Gesteinen durchgeführt, die deren enge räumliche Beziehung zu regionalen NW-SO streichenden Anomalien bestätigen.Die Serpentinite stellen Teile eines zerscherten Ophiolithkomplexes dar, der zwischen einer schwach-magnetischen Metaturbidit-Zone und einer schlecht aufgeschlossenen Metapyroklastit-Zone diapirartig intrudierte. Ein mehrfach deformierter Serpentinitkörper ist von Gerollen aus eklogitischem Blauschiefer überlagert, die höchstwahrscheinlich ursprünglichen tektonischen Einschlüssen entsprechen.Der regionale Trend der Anomalien ist eher vom Streichen und Einfallen der Hauptschieferung als von primären Strukturen kontrolliert. Es handelt sich um eine Krenulationsschieferung (S2) die durch eine frühkarbonische Phase entstanden ist. Sie stellt den Höhepunkt einer prä-Andinen Schrägakkretion dar. Die regionale lithologische Gliederung scheint jedoch die Zusammensetzung der einzelnen Akkretionskeile widerzuspiegeln.

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Résumén Serpentinitas y esquistos máficos metamorfizados en condiciones de facies esquistos verdes baja forman parte del basamento metamorfico de la Cordillera de la Costa de Chile central entre los 39°30' y los 41°30'l.s. Mediciones in situ y en laboratorio de suceptibilidad magnética muestran que sus concentraciones de magnetita pretectonica con respecto a la foliación principal son responsables de anomalías de rumbo NW-SE.Las serpentinitas constituyen parte de una asociación »ofiolítica« fragmentada que aflora dentro de una ancha banda entre metaturbiditas débilmente magnéticas al NE y metapiroclastitas con aisladas anomalías al SW. Una serpentinita del último sector presenta evidencias de deformación polifásica y esta recubierta por bolones de esquistos azules eclogíticos y anfibolitas, los cuales podrían representar inclusiones originalmente transportadas por el cuerpo ultramáfico.El diseño regional de las anomalías magnéticas está controlado por la actitud de la foliación principal, más que por el diseño del emplazamiento original. Esta, un clivaje de crenuación S2, se originó durante un evento carbonífero temprano que representa el climax de la acreción pre-andina en el área. La zonación litológica regional, sin embargo, parece reflejar más bien la composición de lonjas individuales dentro de un prisma compuesto acrecionado mediante subducción oblicua.

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- (prä-S2) . 39°30 41°30 in situ , , NW-SO. , , . , , , , , . , . (S2), . - . .

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Atmospheric Corrections Using MODTRAN for TOA and Surface BRDF Characteristics from High Resolution Spectroradiometric/ Angular Measurements from a Helicopter Platform     

Yaping Zhou  Ken C. Rutledge Analytical Service & Material  Inc  Hampton  VA  USA Thomas P. Charlock Atmospheric Sciences Division  NASA Langley Research Center Hampton  VA  USA Norman G. Loeb  Seiji Kato Hampton University  Hampton  VA  USA 《大气科学进展》2001,(5)

l. IntroductionThe cIassicaI definition of bi--directional reflectance--distribution function (BRDF) is aderivative, distribution function, relatlng the irradiance incident from one given direction tolts contribution to the radiance renected in another direct1on (N1codemus et al., l977).f r (0,, rp,; 0,, rp, )= dL, (0,, P,; 0,, 9,; E, )/ dE, (0,, 9,) [sr-- 1 ], (l)where 0 (zenith angle) and 9 (azimuth angle) together indicate a direction, the subscr1pt i indi-cates quantities associated wi…  相似文献   

Micro- and nano-inclusions in a superdeep diamond from São Luiz,Brazil     

Hiroyuki Kagi  Dmitry A. Zedgenizov  Hiroaki Ohfuji  Hidemi Ishibashi 《Geochemistry International》2016,54(10):834-838

We report cloudy micro- and nano-inclusions in a superdeep diamond from São-Luiz, Brazil which contains inclusions of ferropericlase (Mg, Fe)O and former bridgmanite (Mg, Fe)SiO₃ and ringwoodite (Mg, Fe)₂SiO₄. Field emission-SEM and TEM observations showed that the cloudy inclusions were composed of euhedral micro-inclusions with grain sizes ranging from tens nanometers to submicrometers. Infrared absorption spectra of the cloudy inclusions showed that water, carbonate, and silicates were not major components of these micro- and nano-inclusions and suggested that the main constituent of the inclusions was infrared-inactive. Some inclusions were suggested to contain material with lower atomic numbers than that of carbon. Mineral phase of nano- and micro-inclusions is unclear at present. Microbeam X-ray fluorescence analysis clarified that the micro-inclusions contained transition metals (Cr, Mn, Fe, Co, Ni, Cu, Zn) possibly as metallic or sulfide phases. The cloudy inclusions provide an important information on the growth environment of superdeep diamonds in the transition zone or the lower mantle.  相似文献   

Special issue of the Second Asian Marine Biology Symposium — Toward the Blue Sea,Asian Seas in a changing world     

Jae-Sang Hong  Hiroaki Tsutsumi 《Ocean Science Journal》2016,51(3):411-412

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An anthophyllite-hornblende pair from Japan     

Tokiko Tiba  Mitsuo Hashinoto  Akira Kato 《Lithos》1970,3(4):335-340

Chemical, optical and X-ray powder data on coexisting anthophyllite and hornblende in an amphibolite are presented. Some chemical features of amphibole pairs are briefly discussed.  相似文献   

Log N — log S of radio sources at 10 GHz with flat spectra     

Ko Aizu  Hiroto Tabara  Tatsuji Kato  Makoto Inoue 《Astrophysics and Space Science》1986,119(1):257-261

A logN — logS relation at 10 GHz is constructed for sources with the flat spectra 0.5 (flux densitySv ^–) from observations at NRO, MPIfR and others. Based on the source distribution on log (Luminosity) volume plane we obtain an epoch-depending luminosity function which explains the above relation.Paper presented at the IAU Third Asian-Pacific Regional Meeting, held in Kyoto, Japan, between 30 September–6 October, 1984.Nobeyama Radio Observatory, a branch of the Tokyo Astronomical Observatory, University of Tokyo, is a facility open for general use by researchers in the field of astronomy and astrophysics.  相似文献   

One-armed oscillations of a non-selfgravitating polytropic disk     

Atsuo T. Okazaki  Shoji Kato 《Astrophysics and Space Science》1986,119(1):109-110

One-armedglobal oscillations in a non-selfgravitating polytropic disk rotating around a star are investigated. The unperturbed disk is axisymmetric, geometrically thin, and extends infinitely in the radial direction keeping its thickness constant. Perturbations considered are inviscid and adiabatic. It is found that there are one-armed retrograde wave modes which are trapped in an inner region of the disk. The eignefrequency of the lowest order mode is given by _K(r _s)(z ₀/r _s)₂, wherer _s is the radius of the central star,z ₀ is the half-thickness of the disk, and _K(r _s) is the Keplerian angular frequency at the surface of the star.Paper presented at the IAU Third Asian-Pacific Regional Meeting, held in Kyoto, Japan, between 30 September–6 October, 1984.  相似文献   

Solar brightness distribution at 8.6 mm from interferometer observations     

K. Kawabata  M. Fujishita  T. Kato  H. Ogawa  T. Omodaka 《Solar physics》1980,65(2):221-227

The radial brightness distribution of the quiet Sun at 8.6 mm is synthesized from observations using a sixteen element east-west interferometer in Nagoya. The observed brightness is flat from the disk center to 0.8R . A slight darkening appeared between 0.8R and the limb. No evidence of the bright ring near the limb is found. The radio radius at 8.6 mm is 1.015±0.005R . In addition there exists a coronal component just outside the radio limb.  相似文献