Some instabilities in the 3/1 and 2/1 resonances     

Tadashi Yokoyama  Massae Sato  Masayoshi Tsuchida 《Celestial Mechanics and Dynamical Astronomy》1987,41(1-4):99-105

In a very simple way, it is possible to show the existence of small regions of instability, inside the observed 3/1 and 2/1 Kirkwood Gap, by using the classical Laplace-Lagrange secular theory.  相似文献   

Growth patterns of the last ice age coral terraces at Huon Peninsula   总被引：1，自引：0，他引：1  

Tezer M. Esat  Yusuke Yokoyama   《Global and Planetary Change》2006,54(3-4):216-224

At Huon Peninsula, Papua New Guinea, prolific coral growth during the last-glacial was episodic and in response to a series of sea-level rises. The resultant step-like coral terraces are currently situated from 20 m up to 140 m above sea-level due to continuous tectonic uplift of the Peninsula. The sea-level rises were in response to periodic partial disintegration of Northern Hemisphere ice sheets associated with severe climate swings and occurred within decadal timescales. The relatively rapid 15 m to 35 m rise in sea-levels exposed new head-room for corals to colonize. The resulting terrace structures contain individual corals that do not appear to have grown sequentially in time and with elevation. Additionally, following the peak, sea level fell relatively slowly over several thousand years and corals grew and filled in the flanks of the terrace such that younger corals now occupy lower elevations. We have labeled these structures “pack-up” reefs. This is in contrast to coral terraces formed during major sea-level rises from glacial to interglacial or glacial to interstadial transitions where the rate of sea level rise is commensurate with coral growth rates and corals can keep up with sea-level rise by growing on top of each other in a time orderly sequence. Deriving sea-level information from pack-up terraces is difficult and is likely to be ambiguous. The periodic fluctuations in climate were associated with atmospheric radiocarbon swings that seem to have varied smoothly with time. The same corals that show a scatter in stratigraphic temporal ordering appear regularly distributed in time and with radiocarbon content attesting to the veracity of the age measurements and at the same time confirm the disordered distribution of corals in “pack-up” type reefs.  相似文献   

Energy Balance of Irrigated Intercropping Field in the Middle Reaches of Heihe River Basin     

WU Jinkui DING Yongjian WANG Genxu SHEN Yongping Yusuke YAMAZAKI Jumpei KUBOTA 《中国地理科学(英文版)》2006,16(3):243-248

1 Introduction Most of the solar radiation that ecosystem seizes is con- sumed on latent, sensible and soil heat flux. Among them, latent heat flux shares the biggest part (Gutierrez and Meizer, 1994; Ham et al., 1991; Rachidi et al., 1993). The radiation budget and the energy balance are crucial to water conversion and effective water utilization. Also, they are important parts of research of water-saving ag- riculture (Mo et al., 1997). At present, the researches on radiation budget and e…  相似文献   

Rates of Thermal and Chemical Evolution of Magmas in a Cooling Magma Chamber: a Chronological and Theoretical Study on Basaltic and Andesitic Lavas from Rishiri Volcano, Japan     

Kuritani  Takeshi; Yokoyama  Tetsuya; Nakamura  Eizo 《Journal of Petrology》2007,48(7):1295-1319

Rates of magmatic processes in a cooling magma chamber wereinvestigated for alkali basalt and trachytic andesite lavaserupted sequentially from Rishiri Volcano, northern Japan, bydating of these lavas using ²³⁸U–²³⁰Th radioactive disequilibriumand ¹⁴C dating methods, in combination with theoretical analyses.We obtained the eruption age of the basaltic lavas to be 29·3± 0·6 ka by ¹⁴C dating of charcoals. The eruptionage of the andesitic lavas was estimated to be 20·2 ±3·1 ka, utilizing a whole-rock isochron formed by U–Thfractionation as a result of degassing after lava emplacement.Because these two lavas represent a series of magmas producedby assimilation and fractional crystallization in the same magmachamber, the difference of the ages (i.e. 9 kyr) is a timescaleof magmatic evolution. The thermal and chemical evolution ofthe Rishiri magma chamber was modeled using mass and energybalance constraints, as well as quantitative information obtainedfrom petrological and geochemical observations on the lavas.Using the timescale of 9 kyr, the thickness of the magma chamberis estimated to have been about 1·7 km. The model calculationsshow that, in the early stage of the evolution, the magma cooledat a relatively high rate (>0·1°C/year), and thecooling rate decreased with time. Convective heat flux fromthe main magma body exceeded 2 W/m² when the magma was basaltic,and the intensity diminished exponentially with magmatic evolution.Volume flux of crustal materials to the magma chamber and rateof convective melt exchange (compositional convection) betweenthe main magma and mush melt also decreased with time, from 0·1 m/year to 10^–3 m/year, and from 1 m/yearto 10^–2 m/year, respectively, as the magmas evolved frombasaltic to andesitic compositions. Although the mechanism ofthe cooling (i.e. thermal convection and/or compositional convection)of the main magma could not be constrained uniquely by the model,it is suggested that compositional convection was not effectivein cooling the main magma, and the magma chamber is consideredto have been cooled by thermal convection, in addition to heatconduction. KEY WORDS: convection; magma chamber; heat and mass transport; timescale; U-series disequilibria  相似文献   

Petrogenesis of ultramafic rocks and olivine-rich troctolites from the East Taiwan Ophiolite in the Lichi mélange     

Morishita  Tomoaki  Ghosh  Biswajit  Soda  Yusuke  Mizukami  Tomoyuki  Tani  Ken-ichiro  Ishizuka  Osamu  Tamura  Akihiro  Komaru  Chihiro  Aari  Shoji  Yang  Hsiao-Chin  Chen  Wen-Shan 《Mineralogy and Petrology》2018,112(4):521-534

Mineralogy and Petrology - We examine ultramafic and olivine-rich troctolite blocks of the East Taiwan Ophiolite (ETO) in the Lichi Mélange. Although ultramafic rocks are extensively...  相似文献   

Single planet formation regime in the high-ionization environment:Possible origin of hot Jupiters and super-Earths     

Yusuke Imaeda  Toshikazu Ebisuzaki 《地学前缘(英文版)》2018,9(4):1023-1031

We studied the particle growth in a protoplanetary disk in a high-ionization environment and found that icy planet formation is inactive for a disk with an ionization rate 100 times higher than that of the present Solar System. In particular, in the case of M 10~(-7.4)M_☉yr~(-1), only rocky planet formation occurs. In such a case, all the solid materials in the disk drift inward, eventually reach the inner MRI front,and accumulate there. They form a dense, thin sub-disk of solid particles, which undergoes gravitational instability to form rocky planetesimals. The planetesimals rapidly grow into a planet through pebble accretion. Consequently, rocky planets tend to be much larger than planets formed through other regimes(tandem planet formation regime and dispersed planet formation regime), in which icy planet formation actively takes place. These rocky planets may evolve into hot Jupiters if they grow fast enough to the critical core mass of the runaway gas accretion before the dispersal of the disk gas, or they may evolve into super-Earths if the gas dispersed sufficiently early.  相似文献   

Software Dedicated for the Curation of Geochemical Data Sets in Analytical Laboratories     

Yusuke Yachi  Hiroshi Kitagawa  Tak Kunihiro  Eizo Nakamura 《Geostandards and Geoanalytical Research》2014,38(1):95-102

Software designed for analytical laboratories to guarantee traceability and accessibility of rocks with their geochemical properties has been developed. The software documents the sample origin, current sample location and the location of any sample subsets (e.g., thin sections, solutions, etc.), and archives all associated geochemical data sets. The software can be installed on a personal computer so is available for use in any laboratory and allows curation before and after publication. The software will be of use in integrating and sharing geological reference materials within and among institutes. In this article, the system design and implementation are detailed. All source codes for the software are available at http://dream.misasa.okayama-u.ac.jp/ .  相似文献   

EPMA Chemical Ages of Paleoproterozoic Granitoids in NW India and Their Significance     

S. Biju-Sekhar  K. Yokoyama  M. Santosh  M.K. Pandit  T. Okudaira  M. Yoshida 《Gondwana Research》2001,4(4):577-578

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Depositional process of the Byk-E tephra bed in the Chiba section,central Japan: A marker bed defining the Global Boundary Stratotype Section and Point for the Chibanian Stage     

Yasufumi Satoguchi  Yoshihiro Takeshita  Hiroomi Nakazato  Yusuke Suganuma 《Island Arc》2021,30(1):e12432

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Solidification depth and crystallization age of the Shiaidani Granodiorite: Constraints to the average denudation rate of the Hida Range,central Japan     

Tetsuo Kawakami  Shigeru Sueoka  Tatsunori Yokoyama  Saya Kagami  Georgina E. King  Frédéric Herman  Sumiko Tsukamoto  Takahiro Tagami 《Island Arc》2021,30(1):e12414

Solidification pressure and crystallization age of the ~5 Ma Shiaidani Granodiorite (Hida Mountain Range, central Japan) are determined based on Al-in-hornblende geobarometry and U–Pb zircon dating. Al-poor patchy replacements developed in amphiboles are common in this granite and petrographic study revealed that the replacements include chloritized biotite and albitic plagioclase. These are probably the hydrothermally recrystallized domains, and should not be used for solidification pressure estimates. Magmatic rim of amphibole is characterized by Si < 7.3 a.p.f.u. (Al_IV > 0.7 a.p.f.u.), and utilized in solidification pressure estimate that yielded 0.17–0.29 GPa. The solidification age of the granite is estimated as ~5.6–5.2 Ma using U–Pb zircon dating. From these data, the lower limit of an average denudation rate after ~5.6–5.2 Ma for the area where Shiaidani Granodiorite is exposed is estimated as 0.93–2.5 mm/year.  相似文献