Systematic errors in weak lensing: application to SDSS galaxy–galaxy weak lensing     

Rachel Mandelbaum  Christopher M. Hirata  Uro&#; Seljak  Jacek Guzik  Nikhil Padmanabhan  Cullen Blake  Michael R. Blanton  Robert Lupton  Jonathan Brinkmann 《Monthly notices of the Royal Astronomical Society》2005,361(4):1287-1322

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A new approach for mobile and expandable real-time deep seafloorobservation - adaptable observation system     

Kawaguchi  K. Hirata  K. Nishida  T. Obana  S. Mikada  H. 《Oceanic Engineering, IEEE Journal of》2002,27(2):182-192

Although submarine cable in-line seafloor observation systems are very effective tools for real-time/long-term geo-scientific measurements,, there are technological difficulties for deploying as many sensors as on land. To solve this problem, JAM-STEC developed an expandable and replaceable satellite measurement station called the adaptable observation system (AOS). The AOS is a battery operated mobile observatory connected to the backbone cable system by a 10 km long thin fiber cable to ensure real-time data recovery. The system consists of a branching system, a junction box, a fiber cable, and a battery system for a six-month operation. Installation and construction of the AOS will be conducted by a towed vehicle and an ROV. A thin fiber cable-laying system was developed and tested for practical operation. This observation system provides a chance to extend existing seafloor networks from an in-line area to a wider area  相似文献   

Crustal and upper mantle structure in the Ryukyu Island Arc deduced from deep seismic sounding   总被引：4，自引：0，他引：4  

T. Iwasaki  N. Hirata  T. Kanazawa  J. Melles  K. Suyehiro  T. Urabe  L. Möller  J. Makris  H. Shimamura 《Geophysical Journal International》1990,102(3):631-651

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Can non-Gaussian cosmological models explain the WMAP high optical depth for reionization?     

Xuelei Chen  Asantha Cooray  Naoki Yoshida  Naoshi Sugiyama 《Monthly notices of the Royal Astronomical Society》2003,346(3):L31-L35

The first-year Wilkinson Microwave Anisotropy Probe data suggest a high optical depth for Thomson scattering of  0.17 ± 0.04  , implying that the Universe was reionized at an earlier epoch than previously expected. Such early reionization is likely to be caused by ultraviolet (UV) photons from first stars, but it appears that the observed high optical depth can be reconciled within the standard structure formation model only if star formation in the early Universe was extremely efficient. With normal star formation efficiencies, cosmological models with non-Gaussian density fluctuations may circumvent this conflict as high density peaks collapse at an earlier epoch than in models with Gaussian fluctuations. We study cosmic reionization in non-Gaussian models and explore to what extent, within available constraints, non-Gaussianities affect the reionization history. For mild non-Gaussian fluctuations at redshifts of 30 to 50, the increase in optical depth remains at a level of a few per cent and appears unlikely to aid significantly in explaining the measured high optical depth. On the other hand, within available observational constraints, increasing the non-Gaussian nature of density fluctuations can easily reproduce the optical depth and may remain viable in underlying models of non-Gaussianity with a scale-dependence.  相似文献   

Fractal structure of spatial distribution of microfracturing in rock   总被引：10，自引：0，他引：10  

Takayuki Hirata  Takashi Satoh  Keisuke Ito 《Geophysical Journal International》1987,90(2):369-374

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Galaxy halo masses and satellite fractions from galaxy–galaxy lensing in the Sloan Digital Sky Survey: stellar mass, luminosity, morphology and environment dependencies     

Rachel Mandelbaum  Uro&#; Seljak  Guinevere Kauffmann  Christopher M. Hirata  Jonathan Brinkmann 《Monthly notices of the Royal Astronomical Society》2006,368(2):715-731

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Wouthuysen–Field coupling strength and application to high-redshift 21-cm radiation     

Christopher M. Hirata 《Monthly notices of the Royal Astronomical Society》2006,367(1):259-274

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Trace Element Composition and Classification of the Chinga Iron Meteorite     

K. D. Litasov  A. Ishikawa  I. S. Bazhan  D. S. Ponomarev  T. Hirata  N. M. Podgornykh  N. P. Pokhilenko 《Doklady Earth Sciences》2018,478(1):62-66

A complete microelement analysis of the Chinga meteorite was performed, and the possibility of attributing it together with a number of other iron meteorites into the IVC subgroup, which is transition between IVA and IVB is proposed.  相似文献   

Secular change in lifetime of granitic crust and the continental growth: A new view from detrital zircon ages of sandstones     

Hikaru Sawada  Yukio Isozaki  Shuhei Sakata  Takafumi Hirata  Shigenori Maruyama 《地学前缘(英文版)》2018,9(4):1099-1115

U-Pb ages of detrital zircons were newly dated for 4 Archean sandstones from the Pilbara craton in Australia, Wyoming craton in North America, and Kaapvaal craton in Africa. By using the present results with previously published data, we compiled the age spectra of detrital zircons for 2.9, 2.6, 2.3,1.0, and0.6 Ga sandstones and modern river sands in order to document the secular change in age structure of continental crusts through time. The results demonstrated the following episodes in the history of continental crust:(1) low growth rate of the continents due to the short cycle in production/destruction of granitic crust during the Neoarchean to Paleoproterozoic(2.9-23 Ga),(2) net increase in volume of the continents during Paleo-to Mesoproterozoic(2.3-1.0 Ga), and(3) net decrease in volume of the continents during the Neoproterozoic and Phanerozoic(after 1.0 Ga). In the Archean and Paleoproterozoic, the embryonic continents were smaller than the modern continents, probably owing to the relatively rapid production and destruction of continental crust. This is indeed reflected in the heterogeneous crustal age structure of modern continents that usually have relatively small amount of Archean crusts with respect to the post-Archean ones. During the Mesoproterozoic, plural continents amalgamated into larger ones comparable to modern continental blocks in size. Relatively older crusts were preserved in continental interiors, whereas younger crusts were accreted along continental peripheries.In addition to continental arc magmatism, the direct accretion of intra-oceanic island arc around continental peripheries also became important for net continental growth. Since 1.0 Ga, total volume of continents has decreased, and this appears consistent with on-going phenomena along modern active arc-trench system with dominant tectonic erosion and/or arc subduction. Subduction of a huge amount of granitic crusts into the mantle through time is suggested, and this requires re-consideration of the mantle composition and heterogeneity.  相似文献   

Age and associated stress field of middle Miocene back-arc basalt magmatism in Northeast Japan     

Jun Hosoi  Atsushi Yamaji  Hideki Iwano  Tohru Danhara  Takafumi Hirata 《Island Arc》2021,30(1):e12379

A large volume of middle Miocene basaltic rocks is widely distributed across the back-arc region of Northeast Japan, including around the Dewa Mountains. Petrological research has shown that basaltic rocks of the Aosawa Formation around the Dewa Mountains were generated as a result of the opening of the Sea of Japan. To determine the precise ages of the middle Miocene basaltic magmatism, we conducted U–Pb and fission-track (FT) dating of a rhyolite lava that constitutes the uppermost part of the Aosawa Formation. In addition, we estimated the paleostress field of the volcanism using data from a basaltic dike swarm in the same formation. The rhyolite lava yields a U–Pb age of 10.73 ±0.22 Ma (2σ) and a FT age of 10.6 ±1.6 Ma (2σ), and the paleostress analysis suggests a normal-faulting stress regime with a NW–SE-trending σ₃-axis, a relatively high stress ratio, and a relatively high magma pressure. Our results show that the late Aosawa magmatism occurred under NW–SE extensional stress and ended at ~ 11 Ma.  相似文献