Zircon U–Pb geochronology of “Sashu mylonite”, eastern extension of Higo Plutono‐metamorphic Complex,Southwest Japan: Implication for regional tectonic evolution     

Kenta Kawaguchi  Yasutaka Hayasaka  Kaushik Das  Tomoyuki Shibata  Kosuke Kimura 《Island Arc》2020,29(1)

Geochronological and geochemical studies reveal the possible origin of the restricted body of mylonite rocks occurring at the eastern edge of Kyushu Island, Japan, just in contact with the Sashu Fault, a part of the Paleo‐Median Tectonic Line (Paleo‐MTL). The LA‐ICP‐MS zircon U–Pb dating of the quartz diorite mylonite in this mylonitic body indicates a crystallization age of 114.0 ±1.7 Ma. Moreover, the two tonalite samples appear as thin layers within the Permian fine‐grained mafic mylonite; a part of the same body yields the age of 113.7 ±2.3 Ma and 116.9 ±1.3 Ma, with extremely low Th/U ratio. These quartz diorite mylonite and tonalite are consistent with the late Early Cretaceous magmatism and coeval metamorphism similar to those in the Higo Plutono‐metamorphic Complex in western Kyushu, Japan. This newly characterized complex occurs just south of the Cretaceous Sambagawa metamorphic rocks. The newly characterized mylonitic rocks are lying structurally above the Sambagawa Metamorphic Complex and are distributed along the Paleo‐MTL. The extension of the Higo Plutonometamorphic Complex, as well as the structural relationship between this complex and the Sambagawa Metamorphic Complex, is still controversial but holds a key to reconstruct the tectonic evolution of Southwest Japan during the Late Mesozoic to Early Cenozoic period. Hence, this article provides new insight into the reconstruction of the evolution history of East Asia as an active convergent margin.  相似文献   

Jumping mechanisms of Trojan asteroids in the planar restricted three- and four-body problems     

Kenta Oshima  Tomohiro Yanao 《Celestial Mechanics and Dynamical Astronomy》2015,122(1):53-74

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Effect of heavy oil on the development of the nervous system of floating and sinking teleost eggs     

Irie K  Kawaguchi M  Mizuno K  Song JY  Nakayama K  Kitamura S  Murakami Y 《Marine pollution bulletin》2011,63(5-12):297-302

Heavy oil (HO) on the sea surface penetrates into fish eggs and prevents the normal morphogenesis. To identify the toxicological effects of HO in the context of the egg types, we performed exposure experiments using floating eggs and sinking eggs. In the course of development, HO-exposed embryos of floating eggs showed abnormal morphology, whereas early larva of the sinking eggs had almost normal morphology. However, the developing peripheral nervous system of sinking eggs showed abnormal projections. These findings suggest that HO exposed fishes have problems in the developing neurons, although they have no morphological malformations. Through these observations, we conclude that HO is strongly toxic to floating eggs in the morphogenesis, and also affect the neuron development in both floating and sinking eggs.  相似文献   

Long-traveling landslides in deep snow conditions induced by the 2011 Nagano Prefecture earthquake,Japan     

Shintaro Yamasaki  Hidehisa Nagata  Takayuki Kawaguchi 《Landslides》2014,11(4):605-613

Earthquakes in mountainous areas may produce many landslides that involve abundant snow, but few observations have been made of these hazardous phenomena. The 12 March 2011 north Nagano Prefecture earthquake (M_JMA 6.7) occurred in a mountainous part of Japan that typically has an annual snow cover of more than 2 m, and it induced many snowy landslides. Some of these traveled relatively long distances. We examined the snowy Tatsunokuchi landslide to reconstruct the landsliding processes over deep snow. We infer that the Tatsunokuchi landslide occurred by collapse of a rock debris mass of 5?×?10⁴ m³ that plunged into the abundant snow, forming a mixture of snow and rock debris, which then traveled on top of the snow. Later, the displaced mass included a large amount of snow which was pushed forward at the front and to the sides. The velocity of the landslide was estimated to be approximately 14 m/s. It appears that the displaced mass, having only a small proportion of rock debris, had a low enough density to travel easily on top of the snow. Our observations suggest that there was much liquid water at the base of the displaced mass shortly after the event. Our results suggest that landslides may damage wider areas than expected if they travel over deep snow.  相似文献   

Subglacial drainage system changes of the Gulkana Glacier,Alaska: discharge and sediment load observations and modelling     

Daisaku Kido  Kazuhisa A. Chikita  Kenta Hirayama 《水文研究》2007,21(3):399-410

Hydrological characteristics of englacial and subglacial drainage systems in Gulkana Glacier, Alaska, were examined by analysing temporal variations of discharge and sediment load in the proglacial Phelan Creek in 2001. From data plots on semi‐log paper, it appeared appropriate to separate both discharge and sediment load into fast and slow components. The two components were possibly produced by two different drainage systems: an englacial and subglacial, ‘channellized’ system in the ablation zone, and a subglacial, ‘distributed’ system in the accumulation zone. The data indicate the occurrence of an event during which part of the ‘distributed’ drainage system changed into the ‘channellized’ drainage system. The daily time‐series of discharge and sediment load were represented using a tank model. In the model, the drainage from an additional tank was added, supposing that a subglacial reservoir full of water and sediment collapsed slowly when the subglacial drainage system changed from distributed to channellized. The simulation with the collapsed tank gave much more reasonable results than those with no collapsed tank. The contribution of the collapsed tank to total sediment load is 24%, which is much larger than 9% to total discharge. Copyright © 2006 John Wiley & Sons, Ltd.  相似文献   

Japanese VLBI Network Observations of a Gamma-Ray Narrow-Line Seyfert 1 Galaxy 1H 0323+342     

Kiyoaki?WajimaEmail author  Kenta?Fujisawa  Masaaki?Hayashida  Naoki?Isobe 《Journal of Astrophysics and Astronomy》2014,35(3):215-218

We made simultaneous single-dish and VLBI observations of a gamma-ray narrow-line Seyfert 1 (NLS1) galaxy 1H 0323+342. We found significant flux variation at 8 GHz on a time scale of one month. The total flux density varied by 5.5% in 32 days, corresponding to a variability brightness temperature of 7.0 × 10¹¹ K. We also obtained brightness temperatures of greater than 5.2 × 10¹⁰ K from the VLBI images. These high brightness temperatures suggest that the source has nonthermal processes in the central engine. The source structure could be modelled by two elliptical Gaussian components on the parsec scales. The flux of the central component decreases in the same way as the total flux density, showing that the short-term variability is mainly associated with this component.  相似文献   

The Solar Optical Telescope for the Hinode Mission: An Overview     

S. Tsuneta  K. Ichimoto  Y. Katsukawa  S. Nagata  M. Otsubo  T. Shimizu  Y. Suematsu  M. Nakagiri  M. Noguchi  T. Tarbell  A. Title  R. Shine  W. Rosenberg  C. Hoffmann  B. Jurcevich  G. Kushner  M. Levay  B. Lites  D. Elmore  T. Matsushita  N. Kawaguchi  H. Saito  I. Mikami  L. D. Hill  J. K. Owens 《Solar physics》2008,249(2):167-196

The Solar Optical Telescope (SOT) aboard the Hinode satellite (formerly called Solar-B) consists of the Optical Telescope Assembly (OTA) and the Focal Plane Package (FPP). The OTA is a 50-cm diffraction-limited Gregorian telescope, and the FPP includes the narrowband filtergraph (NFI) and the broadband filtergraph (BFI), plus the Stokes Spectro-Polarimeter (SP). The SOT provides unprecedented high-resolution photometric and vector magnetic images of the photosphere and chromosphere with a very stable point spread function and is equipped with an image-stabilization system with performance better than 0.01 arcsec rms. Together with the other two instruments on Hinode (the X-Ray Telescope (XRT) and the EUV Imaging Spectrometer (EIS)), the SOT is poised to address many fundamental questions about solar magnetohydrodynamics. This paper provides an overview; the details of the instrument are presented in a series of companion papers. M. Otsubo is a former NAOJ staff scientist.  相似文献   

The Solar Optical Telescope of Solar-B (Hinode): The Optical Telescope Assembly     

Y. Suematsu  S. Tsuneta  K. Ichimoto  T. Shimizu  M. Otsubo  Y. Katsukawa  M. Nakagiri  M. Noguchi  T. Tamura  Y. Kato  H. Hara  M. Kubo  I. Mikami  H. Saito  T. Matsushita  N. Kawaguchi  T. Nakaoji  K. Nagae  S. Shimada  N. Takeyama  T. Yamamuro 《Solar physics》2008,249(2):197-220

The Solar Optical Telescope (SOT) aboard the Solar-B satellite (Hinode) is designed to perform high-precision photometric and polarimetric observations of the Sun in visible light spectra (388 – 668 nm) with a spatial resolution of 0.2 – 0.3 arcsec. The SOT consists of two optically separable components: the Optical Telescope Assembly (OTA), consisting of a 50-cm aperture Gregorian with a collimating lens unit and an active tip-tilt mirror, and an accompanying Focal Plane Package (FPP), housing two filtergraphs and a spectro-polarimeter. The optomechanical and optothermal performance of the OTA is crucial to attain unprecedented high-quality solar observations. We describe in detail the instrument design and expected stable diffraction-limited on-orbit performance of the OTA, the largest state-of-the-art solar telescope yet flown in space.  相似文献   

Morphological study of the solar granulation     

Reizaburo Kitai  Ichiro Kawaguchi 《Solar physics》1979,64(1):3-12

High resolution images of the solar granulation show the presence of the small dot-like dark regions in the granulation cells. From the study of the characteristics of these dark regions, it is found that the dark regions are formed without any relations to the presence of the magnetic field. Moreover, it is observed that a granulation cell splits in a few minutes after the formation of the dark regions in the cell. Similarities and differences between the granules with the dark regions and the so-called exploding granules are discussed.  相似文献   

A search for absorption of Mg and Ca compounds in molecular clouds towards Galactic continuum sources     

Seiichi Sakamoto    Glenn J. White    Kentarou Kawaguchi    Masatoshi Ohishi    Kumiko S. Usuda  & Tetsuo Hasegawa 《Monthly notices of the Royal Astronomical Society》1998,301(3):872-880

Absorption lines of MgH and CaH N  = 1 − 0 transitions were searched for in foreground molecular clouds towards the continuum sources associated with Sgr B2 (M) and W49A (N). None of these lines was detected with our sensitivity level of ∼20 mK. Millimetric absorption lines of MgO, MgOH, CaO and CaOH were also searched for towards Sgr B2 (M) without success. The fractional abundances relative to molecular hydrogen are ≲ 1.0 × 10⁻¹¹ for MgH, ≲ 7.9 × 10⁻¹³ for MgO, ≲ 1.6 × 10⁻¹⁰ for MgOH, ≲ 1.6 × 10⁻⁹ for CaH, ≲ 2.0 × 10⁻¹² for CaO, and ≲ 2.5 × 10⁻¹⁰ for CaOH, respectively. The low abundances measured in absorption indicate that a significant fraction of interstellar magnesium and calcium cannot be tied up in their monohydrides, monoxides and monohydroxides. The low abundance of MgH also implies that grain-surface chemistry involving magnesium is not efficient and that magnesium is depleted on to grains to a factor of ≳ 10^2.5 in well-shielded molecular clouds.  相似文献