Age of the Taishu Group,southwestern Japan,and implications for the origin and evolution of the Japan Sea     

Takashi Ninomiya  Shoichi Shimoyama  Koichiro Watanabe  Kenji Horie  Daniel J. Dunkley  Kazuyuki Shiraishi 《Island Arc》2014,23(3):206-220

The Taishu Group, a marine formation with a thickness of >5400 m, crops out on Tsushima Island, located in the southwestern Japan Sea. The group, which is generally regarded as early Eocene to early Miocene in age, provides important information about the tectonic setting of the Japan Sea. In this study, we present new SHRIMP U–Pb dates for igneous zircons from the Kunehama Tuff, which is in the basal part of the Taishu Group, and the Oobaura Tuff, which is in the uppermost part of the group. Results show that the Taishu Group was deposited rapidly, during the short interval of 17.9–15.9 Ma (early–middle Miocene), and is equivalent to other early–middle Miocene strata found in the Japan Sea region. Our results provide new constraints on the geological history of the Japan Sea and its islands.  相似文献   

江豚的分娩及相关行为观察   总被引：4，自引：0，他引：4  

杨健  张先锋  堀由纪子  藤本朝海 《海洋与湖沼》1998,29(1):41-46

于１９９３年４月１０日,在日本江之岛水族馆,江豚顺利分娩,对其分娩过程,以及与之相关的呼吸,活动行为进行较详细的观察和研究,结果表明,母豚将小母豚发尾部生以占分娩的绝大部分时间,分娩后期段平均呼吸频率减缓,游动速度放慢,水面活动增多,并趋于单独活动,此外,还记录到母豚的喷水,跳水,收腹,摆尾,转游等分娩时的特殊行为及出生后幼豚的行为。  相似文献   

Acoustic properties of deformed rocks in the Nobeoka thrust,in the Shimanto Belt,Kyushu, Southwest Japan          下载免费PDF全文

Yoshitaka Hashimoto  Shogo Abe  Hiroki Tano  Gaku Kimura  Asuka Yamaguchi  Rina Fukuchi  Jun Kameda  Yohei Hamada  Yujin Kitamura  Koichiro Fujimoto  Mio Eida 《Island Arc》2017,26(4)

Laboratory measurements for compressional and shear wave velocities (Vp and Vs, respectively) and porosity were conducted with core samples from the Nobeoka Thrust Drilling Project (NOBELL) under controlled effective pressure (5–65 MPa at 5 MPa intervals) and wet conditions. Samples were classified according to deformation texture as phyllite, foliated cataclasite, or non‐foliated cataclasite. Measured values of Vp, Vs, and porosity are within a range of 5.17–5.57 km/s, 2.60–2.71 km/s, and 2.75–3.10 %, respectively, for phyllite; 4.89–5.23 km/s, 2.46–2.57 km/s, and 3.58–4.53 %, respectively, for foliated cataclasite; and 4.90–5.32 km/s, 2.51–2.63 km/s, and 3.79–4.60 %, respectively, for non‐foliated cataclasite, which are all consistent with the previous laboratory experiments conducted with outcrop samples under dry conditions. However, our results also indicate higher Vp and Vs and lower porosity than those measured by the previous studies that adopted the wire‐line logging methods. The variations in Vp, Vs, and porosity are controlled by deformation structure and are greater for phyllite and foliated cataclasite than for non‐foliated cataclasite.  相似文献   

Accurate ocean tide modeling in southeast Alaska and large tidal dissipation around Glacier Bay     

Daisuke Inazu  Tadahiro Sato  Satoshi Miura  Yusaku Ohta  Kazuyuki Nakamura  Hiromi Fujimoto  Christopher F. Larsen  Tomoyuki Higuchi 《Journal of Oceanography》2009,65(3):335-347

An accurate prediction of ocean tides in southeast Alaska is developed using a regional, barotropic ocean model with a finite difference scheme. The model skill is verified by the observational tidal harmonics in southeast Alaska including Glacier Bay. The result is particularly improved in Glacier Bay compared to the previous model described by Foreman et al. (2000). The model bathymetry dominates the model skill. We re-estimate tidal energy dissipation in the Alaska Panhandle and suggest a value for tidal energy dissipation of 3.4 GW associated with the M₂ constituent which is 1.5 times the estimation of Foreman et al. (2000). A large portion of the M₂ energy budget entering through Chatham Strait is dissipated in the vicinity of Glacier Bay. Moreover, it is shown that the developed model has the potential to correct the ocean tide loading effect in geodetic data more efficiently than the model of Foreman et al. (2000), especially around Glacier Bay.  相似文献   

Geological applications potential of DEM,ETM+, and gravity data in arid and semi-arid regions with special reference to south Western Desert,Egypt   总被引：1，自引：0，他引：1  

Mohamed Abdel Zaher  Nureddin M. Saadi  Koichiro Watanabeb 《Arabian Journal of Geosciences》2014,7(5):1705-1716

The study area comprises the southeastern part of the Western Desert of Egypt. The aims of the present study are to delineate the major surface and subsurface structures and to evaluate tectonic framework of the study area. Surface studies of the present work are based mainly on data from two different types of remote sensing systems: 15 cloud-free Landsat Enhanced Thematic Mapper Plus (ETM+) images and Shuttle Radar Topography Mission (SRTM) DEM data. The remote sensing data were used to recognize and extract geological lineaments by calculating and interpreting DEM derivatives, including shaded relief maps, slope maps, and traverse profiles. A Bouguer anomaly map (scale 1:500,000) was used to delineate a detailed picture of the subsurface structure in the study area. The analysis of surface data, including SRTM DEM and ETM+, was combined with subsurface data, including Bouguer anomaly map, and gave new insight into the tectonic and structure patterns of the study area.  相似文献   

An experimental study on impact-induced alterations of planetary organic simulants          下载免费PDF全文

Yasuhito Sekine  Kenya Kodama  Takamichi Kobayashi  Seiji Obata  Yu Chang  Nanako O. Ogawa  Yoshinori Takano  Naohiko Ohkouchi  Koichiro Saiki  Toshimori Sekine 《Meteoritics & planetary science》2018,53(6):1267-1282

The present study systematically investigates shock-induced alteration of organic simulants of planetary bodies (OSPBs) as a function of peak shock pressure and temperature by impact experiments. Our results show that the composition and structure of OSPBs are unchanged upon impacts at peak pressures ≤~5 GPa and temperatures ≤~350 °C. On the other hand, these are dramatically changed upon impacts at >7–8 GPa and > ~400 °C, through loss of hydrogen-related bonds and concurrent carbonization, regardless of the initial compositions of OSPBs. Compared with previous results on static heating of organic matter, we suggest that shock-induced alteration cannot be distinguished from static heating only by Raman and infrared spectroscopy. Our experimental results would provide a proxy indicator for assessing degree of shock-induced alteration of organic matter contained in carbonaceous chondrites. We suggest that a remote-sensing signature of the 3.3–3.6 μm absorption due to hydrogen-related bonds on the surface of small bodies would be a promising indicator for the presence of less-thermally-altered (i.e., <350 °C) organic matter there, which will be a target for landing to collect primordial samples in sample-return spacecraft missions, such as Hayabusa2 and OSIRIS-REx.  相似文献   

ASCA Observations of X-ray Emission from Ultra-luminous Infrared Galaxies     

Takao Nakagawa  Tsuneo Kii  Ryuichi Fujimoto  Toshiyuki Miyazaki  Hajime Inoue  Yasushi Ogasaka  Ryohei Kawabe 《Astrophysics and Space Science》1999,266(1-2):43-48

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Amplification of flood discharge caused by the cascading failure of landslide dams     

Shoki Takayama  Masamitsu Fujimoto  Yoshifumi Satofuka 《国际泥沙研究》2021,36(3):430-438

The cascading failure of multiple landslide dams can trigger a larger peak flood discharge than that caused by a single dam failure.Therefore,for an accurate numerical simulation,it is essential to elucidate the primary factors affecting the peak discharge of the flood caused by a cascading failure,which is the purpose of the current study.First,flume experiments were done on the cascading failure of two landslide dams under different upstream dam heights,downstream dam heights,and initial downstream reservoir water volumes.Then,the experimental results were reproduced using a numerical simulation model representing landslide dam erosion resulting from overtopping flow.Finally,the factors influencing the peak flood discharge caused by the cascading failure were analyzed using the numerical simulation model.Experimental results indicated that the inflow discharge into the downstream dam at the time when the downstream dam height began to rapidly erode was the main factor responsible for a cascading failure generating a larger peak flood discharge than that generated by a single dam failure.Furthermore,the results of a sensitivity analysis suggested that the upstream and downstream dam heights,initial water volume in the reservoir of the downstream dam,upstream and downstream dam crest lengths,and distance between two dams were among the most important factors in predicting the flood discharge caused by the cascading failure of multiple landslide dams.  相似文献   

日本岛根县石见银矿区英安质火山岩中的黑云母矿物学特征及其K-Ar和40Ar-39Ar年代学研究     

曾南石  渡边公一郎  井泽英二  本村庆信 《矿物岩石》2005,25(4):17-22

以显微镜、X射线衍射仪和电子探针等方法,对日本岛根县石见银矿区所产英安质火山岩中的黑云母进行了详细的研究．观察到部分黑云母经受了不同程度的热液蚀变作用。根据对未蚀变、或仅受到轻微蚀变作用的黑云母所进行的^40Ar-^39Ar同位素年龄测定,它们主要为第四纪产物。但是,从经受强热液蚀变作用的黑云母所获得的^40Ar-^39Ar同位素结果表明,后期的高温热液活动可以破坏晶体中的原始K—Ar同位素平衡,使得其。^40Ar-^39Ar同位素年龄与高于从未蚀变矿物所获得的结果,从而产生严重的年代失真。所以,对来自热液蚀变带的样品需要进行详细的矿物学研究。估计对黑云母的原始KAr同位素体系产生破坏的热扰动临界温度可能在200℃左右。  相似文献   

EIDOSCOPE: particle acceleration at plasma boundaries     

A. Vaivads  G. Andersson  S. D. Bale  C. M. Cully  J. De Keyser  M. Fujimoto  S. Grahn  S. Haaland  H. Ji  Yu. V. Khotyaintsev  A. Lazarian  B. Lavraud  I. R. Mann  R. Nakamura  T. K. M. Nakamura  Y. Narita  A. Retinò  F. Sahraoui  A. Schekochihin  S. J. Schwartz  I. Shinohara  L. Sorriso-Valvo 《Experimental Astronomy》2012,33(2-3):491-527

We describe the mission concept of how ESA can make a major contribution to the Japanese Canadian multi-spacecraft mission SCOPE by adding one cost-effective spacecraft EIDO (Electron and Ion Dynamics Observatory), which has a comprehensive and optimized plasma payload to address the physics of particle acceleration. The combined mission EIDOSCOPE will distinguish amongst and quantify the governing processes of particle acceleration at several important plasma boundaries and their associated boundary layers: collisionless shocks, plasma jet fronts, thin current sheets and turbulent boundary layers. Particle acceleration and associated cross-scale coupling is one of the key outstanding topics to be addressed in the Plasma Universe. The very important science questions that only the combined EIDOSCOPE mission will be able to tackle are: 1) Quantitatively, what are the processes and efficiencies with which both electrons and ions are selectively injected and subsequently accelerated by collisionless shocks? 2) How does small-scale electron and ion acceleration at jet fronts due to kinetic processes couple simultaneously to large scale acceleration due to fluid (MHD) mechanisms? 3) How does multi-scale coupling govern acceleration mechanisms at electron, ion and fluid scales in thin current sheets? 4) How do particle acceleration processes inside turbulent boundary layers depend on turbulence properties at ion/electron scales? EIDO particle instruments are capable of resolving full 3D particle distribution functions in both thermal and suprathermal regimes and at high enough temporal resolution to resolve the relevant scales even in very dynamic plasma processes. The EIDO spin axis is designed to be sun-pointing, allowing EIDO to carry out the most sensitive electric field measurements ever accomplished in the outer magnetosphere. Combined with a nearby SCOPE Far Daughter satellite, EIDO will form a second pair (in addition to SCOPE Mother-Near Daughter) of closely separated satellites that provides the unique capability to measure the 3D electric field with high accuracy and sensitivity. All EIDO instrumentation are state-of-the-art technology with heritage from many recent missions. The EIDOSCOPE orbit will be close to equatorial with apogee 25-30 RE and perigee 8-10 RE. In the course of one year the orbit will cross all the major plasma boundaries in the outer magnetosphere; bow shock, magnetopause and magnetotail current sheets, jet fronts and turbulent boundary layers. EIDO offers excellent cost/benefits for ESA, as for only a fraction of an M-class mission cost ESA can become an integral part of a major multi-agency L-class level mission that addresses outstanding science questions for the benefit of the European science community.  相似文献