Relationship between species diversity and reef growth in the Holocene at Ishigaki Island,Pacific Ocean     

Chuki Hongo  Hajime Kayanne 《Sedimentary Geology》2010,223(1-2):86-99

Coral reefs are influenced by global and local factors, and living corals are currently faced with a potential loss of species diversity. Knowledge of the relationship between species diversity and reef growth during the Holocene is important in terms of accurately reconstructing natural conditions prior to recent disturbances (e.g., human impact, pollution, and over-harvesting) and in predicting future scenarios (e.g., abrupt sea-level rise, coastal change, and economic services). This study seeks to characterize the Holocene and present-day reef at Ishigaki Island in the Ryukyu Islands, focusing on spatial and temporal variations in the relationship between species diversity and reef growth. The analysis is based on a drilling core obtained for the Holocene reefs and quantitative species-diversity data (Shannon and Weaver's diversity index, H′) obtained for the present-day reef. H′ was calculated for four coral communities surveyed at the Ibaruma and Fukido reefs. The Holocene sequence was dominated by the corymbose coral community (e.g., Acropora digitifera, A. hyacinthus, Goniastrea retiformis, and Platygyra ryukyuensis), yielding an H′ value of 1.6. The encrusting coral community (e.g., Echinopora lamellose and Pachyseris rugosa) showed the highest diversity at the reef (H′ = 2.2); however, this community was not one of the main reef builders during the Holocene. The massive coral community (e.g., Porites lutea and Favites chinensis) showed the lowest diversity (H′ = 0.6). It also made a minor contribution to reef building; this community appeared in a shallow lagoon once sea level had stabilized. The arborescent coral community (e.g., A. formosa and A. nobilis) was one of the main reef builders, although yielding an H′ value of much less than 1.0. Species diversity is not a prerequisite in terms of Holocene reef growth. Thus, a few species (e.g., A. digitifera, A. hyacinthus, A. formosa, A. nobilis, G. retiformis, and P. ryukyuensis) from two main reef-building communities are important for reef growth. These corals that act as reefs are characterized by high growth rates, having an upward reef growth rate of 2–12 m kyr^? 1 in the Indo-Pacific during the Holocene.  相似文献   

36Cl, 26Al,and O isotopes in an Allende type B2 CAI: Implications for multiple secondary alteration events in the early solar system     

Takayuki Ushikubo  Yunbin Guan  Hajime Hiyagon  Naoji Sugiura  Laurie A. Leshin 《Meteoritics & planetary science》2007,42(7-8):1267-1279

Abstract— We measured ³⁶Cl‐³⁶S and ²⁶Al‐²⁶Mg systematics and O isotopes of secondary phases in a moderately altered type B2 CAI (CAI#2) from the Allende CV3 chondrite. CAI#2 has two distinct alteration domains: the anorthite‐grossular (An‐Grs) domain that mostly consists of anorthite and grossular, and the Na‐rich domain that mostly consists of sodalite, anorthite, and Fe‐bearing phases. Large ³⁶S excesses (up to ～400‰) corresponding to an initial ³⁶Cl/³⁵Cl ratio of (1.4 ± 0.3) × 10^?6 were observed in sodalite of the Na‐rich domain, but no resolvable 26Mg excesses were observed in anorthite and sodalite of the Na‐rich domain (the initial ²⁶Al/²⁷Al ratio < 4.4 × 10^?7). If we assume that the ³⁶Cl‐³⁶S and the ²⁶Al‐²⁶Mg systematics were closed simultaneously, the ³⁶Cl/³⁵Cl ratio would have to be on the order of ～10^?2 when CAIs were formed. In contrast to sodalite in Na‐rich domain, significant ²⁶Mg excesses (up to ～35‰) corresponding to an initial ²⁶Al/²⁷Al ratio of (1.2 ± 0.2) × 10^?5 were identified in anorthite of the An‐Grs domain. The ²⁶Al‐²⁶Mg systematics of secondary phases in CAI#2 suggest that CAIs experienced multiple alteration events. Some of the alteration processes occurred while ³⁶Cl (half‐life is 0.3 Myr) and ²⁶Al (half‐life is 0.72 Myr) were still alive, whereas others took place much later. Assuming that ²⁶Al was homogeneously distributed in the solar nebula, our study implies that alteration of CAIs occurred as early as within 1.5 Myr of CAI formation and as late as 5.7 Myr after.  相似文献   

Jupiter’s Great Red Spot: compactness condition and stability     

Jun-Ichi Yano  Glenn R. Flierl 《Annales Geophysicae》1994,12(1):1-18

Linear Rossby wave dispersion relationships suggest that Jupiter’s Great Red Spot (GRS) is a baroclinic structure embedded in a barotropic shearing zonal flow. Quasi-geostrophic (QG) two-layer simulations support the theory, as long as an infinitely deep zonal flow is assumed. However, once a finite depth of the lower layer is assumed, a self-interaction of the baroclinic eddy component produces a barotropic radiating field, so that the GRS-like eddy can no longer remain compact. Compactness is recovered by explicitly introducing a deep dynamics of the interior for the lower layer, instead of the shallow QG formulation. An implication of the result is a strong coupling of the GRS to a convectively active interior.Paper presented to the NP Symposia of the 1991 Wiesbaden EGS Assembly on “Nonlinear processes in Geophysics”  相似文献   

Oxygen and strontium isotopic characteristics of calc-alkalic volcanic rocks from the central and western Japan arcs: Evaluation of contribution of crustal components to the magmas     

Yukihiro Matsuhisa  Hajime Kurasawa 《Journal of Volcanology and Geothermal Research》1983,18(1-4)

¹⁸O/¹⁶O and ⁸⁷Sr/⁸⁶Sr ratios were determined for Quaternary calc-alkalic volcanic rocks from six volcanic rock suites in the central and western Japan arcs. The δ¹⁸O values relative to SMOW and ⁸⁷Sr/⁸⁶Sr ratios range from +6.3 to +9.9⁰/₀₀ and 0.70357 to 0.70684, respectively. Both the O- and Sr-isotopic compositions are higher than those for island-arc primitive magmas and their differentiates. The isotopic compositions of the calc-alkalic rocks cannot be derived by a simple fractional crystallization of the primitive magmas. On the other hand, the ¹⁸O- and ⁸⁷Sr-enrichment is confined to the rock suites located in well-developed island arcs having thick continental-type crust with low or negative Bouguer anomalies. Involvement of ¹⁸O- and ⁸⁷Sr-rich crustal material in the magma formation is suggested.The isotopic compositions vary remarkably within individual rock suites as well as from volcano to volcano. The data points in δ¹⁸O vs. ⁸⁷Sr/⁸⁶Sr plot accord with a mixing model between primitive magmas and crustal material of dioritic composition on an average, assuming their comparative Sr contents. The primitive magmas involved could not be low-Sr tholeiites, but magmas more or less enriched in incompatible elements including Sr, which correspond to high-alkali tholeiites or alkali basalts and their evolved magmas. The nature of the primitive magmas seems to change from tholeiitic to more alkalic with progressing island-arc evolution.Mixing of crust-derived melts is more plausible than assimilation of solid-rocks for involving 20 to 30% crustal material in the magmas along simple mixing curves. Isotopic variations between the rock suites are ascribed to variable Sr concentration radio of the end-members, variable isotopic compositions of crustal material or variable mixing ratio of the end-members. Extremely high-δ ¹⁸O rocks with moderate increase in ⁸⁷Sr/⁸⁶Sr ratio suggest another mixing process in shallower magma chambers between andesite magmas and metasedimentary rocks having high δ ¹⁸O and ⁸⁷Sr/⁸⁶Sr values but low Sr content. Subsequent fractional crystallization of once-derived magmas would be the prominent process for the rock suites showing gradual increase in ¹⁸O up to 1⁰/₀₀ with uniform ⁸⁷Sr/⁸⁶Sr ratios.  相似文献   

Modeling of Regional High Ozone Episode Observed at Two Mountain Sites (Mt. Tai and Huang) in East China   总被引：3，自引：0，他引：3  

Zifa Wang  Jie Li  Xiquan Wang  Pakpong Pochanart  Hajime Akimoto 《Journal of Atmospheric Chemistry》2006,55(3):253-272

A high O₃ episode was observed during 23–25 May 2004 at two high-mountain sites reflecting the regional pattern of air pollutants over East China. This episode lasted about three days with the maximum hourly O₃ mixing ratios reaching 111 and 114 ppbv at Mt. Tai and Huang, respectively. Backward trajectories and meteorological analysis indicated that regional transport, associated with a weak high pressure system over the East China Sea, might play an important role in the formation of this high ozone episode. The nested air quality prediction modeling system (NAQPMS) was applied to investigate the formation and evolution of this high O₃ event. The comparison of model results with observations showed that NAQPMS successfully reproduced the main observed patterns of O₃ and meteorological parameters during the simulated period. The model results with emission over the Yangtze Delta and the East Central China switched on/off clearly showed that ozone and its precursors transported from the Yangtze Delta and the East Central China enhanced the high ozone episode at two sites, with a contribution of 20%–50% during the episode. In addition, based on process analysis with the model, chemical production and regional transport appeared to be the main causes of high ozone episode involving a large amount of high-ozone air masses and precursors transported from the surrounding areas. The horizontal transport is more active during the period of high ozone episode than that during the non-episode at Mt. Tai as well as Mt. Huang.  相似文献   

The Machangqing copper-molybdenum deposits, Yunnan, China — an example of Himalayan porphyry-hosted Cu-Mo mineralization     

Z. Peng  M. Watanabe  K. Hoshino  S. Sueoka  T. Yano  H. Nishido 《Mineralogy and Petrology》1998,63(1-2):95-117

Summary The Machangqing copper-molybdenum deposits occur in the Shanjian fold belt, Yunnan Province, China. Two types of ores are distinguished: (1) Cu-Mo quartz veinlets in magnetite-series granite porphyry; and (2) Cu-Mo skarns occurring at the contact between the Ordovician sedimentary sequence and the granite porphyry. With decreasing temperature and of hydrothermal fluids initially in equilibrium with K-feldspar, the following alteration patterns developed within the porphyry, from the center outwards: silicification, K-silicate, phyllic and argillic alteration. The paragenetic sequence of alteration minerals observed in the Cu-Mo skarns resulted from decreasing temperature and/or increasing of the hydrothermal fluids initially in equilibrium with grandite garnet. Fluid inclusions in quartz suggest boiling during the mineralization. The mineralization temperatures based on filling temperatures and salinities of quartz are in the following ranges: about 265° to 400 °C and 5.0 to 14.6 wt.% NaCl eq. for the Cu-Mo veinlets; and 200° to 500 °C and 10.2 to 42.0 wt.% NaCl eq. for the Cu-Mo skarns. As is evident from log fo₂-pH diagrams, ores of the early stage of mineralization in the Cu-Mo skarns, characterized by the assemblage magnetite + pyrite + rare pyrrhotite + K-feldspar + quartz, were deposited from highly alkaline and high temperature fluids. With decreasing temperature and fo₂, the pH of the ore fluids was shifted towards slightly alkaline to neutral, with the resultant formation of the main stage ores, characterized by the assemblage chalcopyrite + pyrite + molybdenite + sphalerite + K-feldspar +sericite (muscovite) + epidote + uartz. Very minor amounts of ore minerals, including matildite, bismuthinite and electrum, are associated with a late stage of ore formation.In the case of the Cu-Mo veinlets, it can be stated roughly that both fs₂ and fo₂ conditions were in the stability field of pyrite, with pH of the ore fluids buffered by the assemblage sericite + K-feldspar +quartz ± calcite. K-Ar age determinations were made on the granite porphyry, biotite phenocrysts and hydrothermal biotite in the Cu-Mo skarns, giving ages of 42.5 to 34.6 Ma, 52.3 Ma, and 39.2 to 26.4 Ma, respectively.It is concluded that the Cu-Mo mineralization at Machangqing shows a close spatial and temporal association with the Himalayan felsic magmatism of the magnetite-series type.

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Die Machangqing Kupfer-Molybdän-Lagerstätten, Yunnan, China — Ein Beispiel für prophyrische Cu-Mo Vererzung im Himalaya

Zusammenfassung Die Kupfer-Molybdän-Lagerstätten von Machangqing treten im Shanjian Faltengürtel in der Provinz Yunnan, China, auf. Zwei Erztypen sind unterscheidbar: (1) Cu-Mo Quarzgängchen in einem porphyrischen Granit der Magnetit-Serie; (2) Cu-Mo-Skarne am Kontakt zwischen der ordovizischen Sedimentabfolge und dem porphyrischen Granit. Mit Abnahme der Temperatur und des Verhältnisses der hydrothermalen Fluide, die ursprünglich mit Alkalifeldspat im Gleichgewicht waren, entwickelten sich in diesem Porphyrstock vom Zentrum randwärts folgende Alterationszonen: Silizifizierung, K-silikatische, phyllische und argillische Alteration. Die paragenetische Abfolge der Alterationsminerale, die in den Cu-Mo Skamen zu beobachten sind, sind das Resultat abnehmender Temperatur und/oder einer Zunahme des -Verhältnisses der hydrothermalen Fluide, die ursprünglich mit Grandit-Granat im Gleichgewicht waren. Flüssigkeitseinschlüsse in Quarz weisen auf Siedeprozesse während der Mineralisation hin. Die aus den Einschlußtemperaturen und Salinitäten in Quarz bestimmten Mineralisationstemperaturen liegen für die Cu-Mo-Gängchen zwischen 265–400 °C und zwischen 5–14.6 Gew.% NaCI Äquiv. und zwischen 200–500 °C und 10.2–42 Gew.% NaCI Äquiv. für die Cu-Mo Skarne. Wie aus log fo₂-pH Diagrammen hervorgeht, ist die im Frühstadium der Cu-Mo Skamvererzung entstandene Vergesellschaftung von Magnetit +Pyrit+selten Magnetkies + Alkalifeldspat + Quarz durch Ausfällung aus sehr alkalischen und hochtemperierten Fluiden entstanden. Mit Temperatur- und fo₂-Abnahme wurde der pH der Lösungen leicht alkalisch bis neutral. Dies resultierte in der Bildung der Erze des Hauptstadiums, das durch Chalcopyrit + Pyrit + Molybdänit + Sphalerit + Alkalifeldspat + Serizit (Muscovit) + Epidot + Quarz charakterisiert ist. Sehr geringe Mengen an Erzmineralen inklusive Matildit, Bismuthinit und Elektrum sind dem Spätstadium der Vererzung zuzuordnen. Für die Cu-Mo-Gängchen läßt sich etwas verallgemeinernd feststellen, daß fo₂ und fs₂ im Stabilitätsbereich von Pyrit lagen, wobei der pH der Erzfluide durch die Paragenese Serizit+Alkalifeldspat+Quarz+Calcit gepuffert wurde. K-Ar Altersbestimmungen wurden am porphyrischen Granit, an Biotit-Phänokristallen und an hydrothermal gebildetem Biotit der Cu-Mo Skarne durchgeführt. Sie ergaben Alter von 42.5–34.6, 52.3 bzw. 39.2-26.4 Ma.Die Cu-Mo Vererzung von Machangqing zeigt eine räumliche und zeitliche Assoziation mit dem sauren Magmatismus der Magnetit-Serie im Himalaya.

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With 12 Figures  相似文献   

Star formation in the circumnuclear environment of NGC 1068     

Richard I. Davies  Hajime Sugai  & Martin J. Ward 《Monthly notices of the Royal Astronomical Society》1998,300(2):388-396

We present near-infrared emission-line images of the circumnuclear ring in NGC 1068. We have measured the Brγ fluxes in a number of star-forming complexes and derived the extinction for each of these by comparison with Hα. We investigate the star-forming histories of these regions and find that a short burst of star formation occurred coevally throughout the ring within the last 30–40 Myr, and perhaps as recently as 4–7 Myr ago. The 1–0 S(1) flux and S(1)/Brγ ratios indicate that as well as fluorescence, shock-excited H₂ emission contributes to the total flux. There is excess H₂ flux to the north-west where the ionization cone crosses the ring, and we show that it is possible that the non-stellar continuum from the Seyfert nucleus which produces the high-excitation lines could also be causing fluorescence at the edges of molecular clouds in the ring. The nuclear 1–0 S(1) is more extended than previously realized but only along the bar's major axis, and we consider mechanisms for its excitation.  相似文献   

Cloning and sequencing of the allophycocyanin genes fromSpirulina maxima (Cyanophyta)     

Song  Qin  Kojima  Hiroyuki  Kawata  Yoshikazu  Yano  Shin-ichi  Cheng-kui  Zeng 《中国海洋湖沼学报》1998,16(1):6-11

The genes coding for the α-and β-subunit of allophycocyanin (apcA andapcB) from the cyanophyteSpirulina maxima were cloned and sequenced. The results revealed 44.4% of nucleotide sequence similarity and 30.4% of similarity of deduced amino acid sequence between them. The amino acid sequence identities betweenS. maxima andS. platensis are 99.4% for α subunit and 100% for β subunit.

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Transposable genetic elements inSpirulina and potential applications for genetic engineering     

Kojima  Hiroyuki  Song  Qin  Ajith Kumar  Thankappan  Kawata  Yoshikazu  Yano  Shin-ichi 《中国海洋湖沼学报》1998,16(1):30-39

Transposable elements in cyanobacteria are briefly reviewed. Evidence is presented to show that transposable elements inSpirulina platensis is actually reflected on the phenotype change, i e., helical to straight filaments. Transposition intermediates of DNA were isolated from the extrachromosome and the transposition was related to helical variations inSpirulina. Uses of transposable elements for microalgal recombination are discussed based on the transposition mechanism.

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Oxygen isotopic distribution in an amoeboid olivine aggregate from the Allende CV chondrite: Primary and secondary processes     

Hajime Imai  Hisayoshi Yurimoto 《Geochimica et cosmochimica acta》2003,67(4):765-772

The oxygen isotopic distribution in an amoeboid olivine aggregate (AOA), TTA1-02, from the Allende CV3 chondrite has been determined by secondary ion mass spectrometry. The irregular shaped TTA1- 02 (5×3mm) consists mostly of olivine grains of ca. 5μm in diameter. Olivine grains of Mg-rich (Fo₉₅) and Fe-rich (Fo₆₀) composition are in direct contact with each other, with a sharp compositional boundary. Oxygen isotopic compositions of Fe-rich olivine grains are ¹⁶O-poor (Δ¹⁷O ≅ −5‰), whereas Mg-rich olivine is ¹⁶O-rich (Δ¹⁷O ≅ −25‰). Several Al-rich inclusions (<ca. 500 μm in diameter) are enclosed by olivine grains in the AOA. Oxygen isotopic compositions of spinel and fassaite in Al-rich inclusions are ¹⁶O-rich (Δ¹⁷O ≅ −20‰), whereas those of anorthite, nepheline and phyllosilicate are ¹⁶O-poor (Δ¹⁷O ≅ −5‰). We propose the following sequence of events during the formation of AOAs in the Allende meteorite: 1) Formation of Al-rich inclusions with ¹⁶O-rich oxygen isotopic composition; 2) Accretion of Mg-rich olivine grains with ¹⁶O-rich oxygen isotopic composition around Al-rich inclusions; 3) Accretion into parent body; and 4) Aqueous alteration in the parent body, which led to crystallization of ¹⁶O-poor minerals, Fe-rich olivine, anorthite, nepheline, and phyllosilicate. This is reflecting reactions among primary ¹⁶O-rich AOA minerals and aqueous fluid having ¹⁶O-poor oxygen isotopic composition. Fe-rich olivine grains precipitated from aqueous fluids, which partially dissolved pre-existing Mg-rich olivine grains. Sintering and Mg-Fe diffusion occurred during thermal metamorphism. Anorthite, nepheline and phyllosilicate in Al-rich inclusions replaced primary anorthite or melilite during the aqueous alteration stage.  相似文献