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Yoshiki Shirahama Yukari Miyashita Masao Kametaka Yuji Suzuki Yosuke Miyairi Yusuke Yokoyama 《Island Arc》2021,30(1):e12376
The NE-trending Hinagu fault zone, length 81 km, is one of the major active faults in Kyushu, Japan. From north to south, it is divided into three segments based on geomorphic features and paleoseismic behavior: the Takano-Shirahata, Hinagu, and Yatsushiro Sea segments. The 2016 Kumamoto earthquake produced a 6-km-long surface rupture with a dextral strike-slip displacement on the northern part of the Takano-Shirahata segment. Surface rupture, a faint east-side-up flexure with a vertical offset of less than 8 cm, was observed near the middle of the Takano-Shirahata segment. To examine past surface-rupturing earthquakes on the Takano-Shirahata segment, including rupture frequency and timing, we conducted a paleoseismic study with boring and trenching at Yamaide. A trench across the surface rupture exposed multiple fault strands associated with multiple surface-rupturing events that deformed several strata of fine-grained sediments. By structural and stratigraphic interpretation, high-density radiocarbon dating and tephra analysis, and Bayesian modeling, we constrained the timing of seven events, Events 1–7, to 0.84–1.25, 1.31–7.06, 9.99–11.0, 10.8–12.1, 12.0–13.0, 14.2–15.1, and before 14.8 kcal BP. Slip during Events 1–6 was obviously larger than the 2016 slip. The estimated average recurrence interval was about 2596–2860 years, but the interval between Events 2 and 3 was much longer than other intervals. Moreover, the vertical throw associated with Event 2 was larger than that of other events. This implies that the Takano-Shirahata segment has a period with rare larger earthquakes and a period with frequent smaller earthquakes. Some events might have produced ruptures on both the Takano-Shirahata and the northern part of the Hinagu segments simultaneously or in a short time. The variety of recurrence intervals suggests that the seismic activity has been affected by one or both activities of the Futagawa fault zone and the Hinagu segment. 相似文献
95.
Ryoichi Nakada Yoshio TakahashiUrumu Tsunogai Guodong ZhengHiroshi Shimizu Keiko H. Hattori 《Applied Geochemistry》2011,26(7):1065-1076
A comprehensive study was performed to characterize, for the first time, the mud, water, and gases released from onshore mud volcanoes located in the southern margin of the Junggar Basin, northwestern China. Chemical compositions of mud, along with the geology of the basin, suggest that a source of the mud is Mesozoic or Cenozoic shale. Oxygen and H isotope compositions of the released water suggest a local meteoric origin. Combined with the positive Eu anomalies of the water, a large 18O shift of the water suggests extensive interaction with rocks. Gases discharged from the mud volcanoes are predominantly thermogenic hydrocarbons, and the high δ13C values (>+20‰ VPDB) for CO2 gases and dissolved carbonate in muddy water suggest secondary methanogenesis with CO2 reduction after oil biodegradation.The enrichments of Eu and 18O in water and the low thermal gradient of the area suggest that the water-rock interactions possibly occur deeper than 3670 ± 200 m. On the other hand, considering the relationship to the petroleum reservoir around the mud volcanoes, the depth of the gases can be derived from about 3600 m, a depth that is greater than that generally estimated for reservoirs whose gas is characterized by 13C-enriched CO2. Oil biodegradation with CO2 reduction likely occurs at a shallower depth along the seepage system of the mud volcano. The results contribute to the worldwide data set of gas genesis in mud volcanoes. Moreover, they further support the concept that most terrestrial mud volcanoes release thermogenic gas produced in very deep sediments and may be early indicators of oil biodegradation, an important problem in the petroleum industry. 相似文献
96.
Shiho Hirotani Masao Ban Mitsuhiro Nakagawa 《Contributions to Mineralogy and Petrology》2009,157(6):709-734
Eruptive products of the Shirataka volcano (0.9–0.7 Ma) in NE Japan are calc-alkaline andesite–dacite, and are divisible into
six petrologic groups (G1–G6). Shirataka rocks possess mafic inclusions—basalt–basaltic andesite, except for G3 and G4. All
rocks show mixing and mingling of the mafic and silicic end-members, with trends defined by hosts and inclusions divided into
high-Cr and low-Cr types; both types coexist in G1, G2, and G5. Estimated mafic end-members are high-Cr (1120–1170°C, 48–51%
SiO2, olv ± cpx ± plg) and low-Cr type magmas (49–52% SiO2, cpx ± plg) except for the Sr isotopic composition. In contrast, the silicic end-members of both types have similar petrologic
features (790–840°C, 64–70% SiO2, hbl ± qtz ± px + plg). High-Cr type mafic and corresponding silicic end-members have lower 87Sr/86Sr ratios than the low-Cr ones in each group. The trace element model calculations suggest that the low-Cr type mafic end-member
magma is produced through ca. 20% fractional crystallization (olv ± cpx ± plg) from the high-Cr type one with assimilation
of granitoids (r = 0.02–0.05). The silicic magmas are producible through <30% partial remelting of previously emplaced basaltic magma with
assimilation of crustal components. The compositional difference between the low-K and medium-K basalts in the Shirataka volcano
is mainly attributed to the different degrees of the effect of subduction derived fluid by dehydration of phlogopite.
Electronic supplementary material The online version of this article (doi:) contains supplementary material, which is available to authorized users. 相似文献
97.
Y. K. Yang N. Nakada L. Zhao H. Tanaka 《International Journal of Environmental Science and Technology》2017,14(9):1989-1998
Rapid increases in the amounts of fullerene C60 nanoparticles (nC60) being produced and used will inevitably lead to increases in the amounts released into the aquatic environment. This will have implications for human and ecosystem health. Wastewater treatment plants are key barriers to nC60 being released into aquatic systems, but little information is available on how adsorption processes in wastewater treatment plants affect the fates of nC60. We investigated the effects of the surface properties of activated sludge on the adsorption of nC60 and related mechanisms by modeling the adsorption kinetics and equilibrium process and performing correlation analyses. The adsorption of nC60 closely followed the pseudo-second-order kinetic model (R > 0.983), the Freundlich isotherm model (R > 0.990), and the linear partitioning isotherm model (R > 0.966). Different adsorption coefficients, 1.070–4.623 for the Freundlich partitioning model and 1.788–6.148 for the linear partitioning model, were found for different types of activated sludge. The adsorption coefficients significantly positively correlated with the zeta (ζ) potential (R = 0.877) and hydrophobicity (R = 0.661) and negatively correlated with particle size (R = ?0.750). The results show that nC60 adsorption is strongly affected by the surface properties of activated sludge because changes in surface properties cause changes in the electrostatic and hydrophobic interactions that occur. 相似文献
98.
Satoko Takahashi Masao Saito Shigehisa Takakuwa Ryohei Kawabe 《Astrophysics and Space Science》2008,313(1-3):165-168
We have performed millimeter- and submilli- meter-wave survey observations using the Nobeyama millimeter array (NMA) and the
Atacama Submillimeter Telescope Experiment (ASTE) in one of the nearest intermediate-mass (IM) star-forming regions: Orion
Molecular Cloud-2/3 (OMC-2/3). Using the high-resolution capabilities offered by the NMA (∼several arcsec), we observed dust
continuum and H13CO+(1–0) emission in 12 pre- and proto-stellar candidates identified previously in single-dish millimeter observations. We unveiled
the evolutionary changes with variations of the morphology and velocity structure of the dense envelopes traced by the H13CO+(1–0) emission. Furthermore, using the high-sensitivity capabilities offered by the ASTE, we searched for large-scale molecular
outflows associated with these pre- and proto-stellar candidates observed with the NMA. As a result of the CO(3–2) observations,
we detected six molecular outflows associated with the dense gas envelopes traced by H13CO+(1–0) and 3.3 mm continuum emission. The estimated CO outflow momentum increases with the evolutionary sequence from early
to late type of the protostellar cores. We also found that the 24 μm flux increases as the dense gas evolutionary sequence.
We propose that the enhancement of the 24 μm flux is caused by the growth of the cavity (i.e. the CO outflow destroys the
envelope) as the evolutionary sequence. Our results show that the dissipation of the dense gas envelope plays an essential
role in the evolution of the IM protostars. The extremely high-sensitivity and high-angular resolution offered by ALMA will
reveal unprecedented details of the inner ∼50 AU of these protostars, which will provide us a break through in the classic
scenario of IM star/disk formation. 相似文献
99.
T. Tanabé S. Nishida Y. Nakada T. Onaka I.S. Glass M. Sauvage 《Astrophysics and Space Science》1997,255(1-2):407-413
We report preliminary results of our systematic survey for infrared stars in the globular clusters of the Magellanic Clouds.
In the course of an ISOCAM survey for AGB stars in the intermediate-age clusters, we have discovered extremely red AGB stars
in NGC 419 and NGC 1978. From their colours and luminosities, they are thought to be experiencing intense mass-loss and to
be in the final or superwind phase of the AGB evolution. However, they seem to be of somewhat lower luminosity than the corresponding
visible AGB stars when only the mid-infrared data are taken into account. This suggests that hitherto unobserved infrared
excesses may exist at longer wavelengths.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
100.
M. P. Nakada 《Solar physics》1969,7(2):302-320
Some trends in the composition of the lower solar corona due to mixing and diffusion have been examined. Mixing has been treated through plausible inference from the thermal gradient and through analogy with the neutral atmosphere of the earth. These indicate that diffusion may be important in the lower corona. Changes in composition due to pressure and thermal gradients have been calculated with multi-component diffusion equations. Results indicate that (i) large enhancements of heavy elements are possible and (ii) the composition of the corona can show large variations with values of the thermal gradient in the lower corona. 相似文献