Hitoshi Sakai (1930–2008)     

Ken Sakai 《Applied Geochemistry》2012

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Patterns of Surf Smelt, Hypomesus pretiosus, Intertidal Spawning Habitat Use in Puget Sound, Washington State     

Timothy Quinn  Kirk Krueger  Ken Pierce  Daniel Penttila  Kurt Perry  Tiffany Hicks  Dayv Lowry 《Estuaries and Coasts》2012,35(5):1214-1228

Surf smelt Hypomesus pretiosus are an important part of the Salish Sea food web and obligate beach spawners, yet little is known about the spatiotemporal distribution of spawning and beach characteristics related to spawning success. We counted smelt eggs at 51 sites around Camano Island, Puget Sound, Washington every 2?weeks for 1?year and at 13 of those 51 sites each month in the following year. At each site, we measured beach characteristics hypothesized to affect spawning habitat suitability as measured by egg abundance and mortality. Eggs were collected at 45 sites and pooled by month for analyses. Few sites (N?=?10, 19.6?%) contributed 87?% of total eggs and 89?% of all live eggs collected. Mean total egg counts at sites were higher (p?<?0.019) in Jul?CSep (1,790.7, SE?=?829.5) than in Jan?CMar (26.1, SE?=?10.2). Principal component and regression analyses suggested that aspect, fetch, solar radiation, and beach temperature predicted egg abundance but not mortality. Because a small proportion of sites appear to support most spawning activity, a conclusion consistent with year?2 egg counts, impacts to relatively few beaches could greatly affect surf smelt production.  相似文献   

Subsidence Analysis and Burial History of the Late Carboniferous to Early Jurassic Soutpansberg Basin, Limpopo Province, South Africa     

Ntokozo MALAZA  LIU Ken  ZHAO Baojin 《《地质学报》英文版》2016,90(6):2000-2007

The subsidence history of the Soutpansberg Basin was reconstructed by a tectonic subsidence analysis coupled with backstripping calculations based on data of newly interpreted sequence boundaries. Furthermore,burial and time plots were constructed in order to understand the burial and thermal history of the basin. Input data were based on facies,lithostratigraphic models and tectonic interpretations. The studied succession is up to 1000 m and is underlain by the Achaean Limpopo Mobile Belt. The subsidence within the basin supports the primary graben system which must have been centred within the present basins,and later became a region of faulting. The subsidence and burial history curves suggests two phases of rapid subsidence during the Early-Late Permian(300–230 Ma) and Middle Triassic(215–230 Ma). The areas of greater extension subsided more rapidly during these intervals. Two slow subsidence phases are observed during the Late Triassic(215–198 Ma) and Early Jurassic(198–100 Ma). These intervals represent the post-rift thermal subsidence and are interpreted as slow flexural subsidence. Based on these observations on the subsidence curves,it is possible to infer that the first stage of positive inflexion(300 Ma) is therefore recognised as the first stage of the Soutpansberg Basin formation.  相似文献   

Shear Strength Development with Burial in Eel River Margin Slope Sediments     

Jacques Locat  Homa Lee  Robert Kayen  Ken Israel  Marie-Claude Savoie  Éric Boulanger 《Marine Georesources & Geotechnology》2013,31(2):111-135

As part of the STRATAFORM project, a series of cores were obtained from the Eel River Margin area of Eureka, California. The geotechnical analysis of intact specimens and of reconstituted samples provides some insight on the development of shear strength with burial. The results show the effect of bioturbation in the early part of the lifetime of a sediment. SEDCON tests were used to proposed various relationships which help predict the changes in density, liquidity index, and strength as a function of depth. These relationships are found useful from near the water sediment-interface down to a depth of at least 400 m in the sediment column.  相似文献   

Dr Russell Gavin Cole (1963–2013)     

Ken R Grange 《新西兰海洋与淡水研究杂志》2013,47(4):428-429

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81Kr‐Kr age and multiple cosmic‐ray exposure history of the Vaca Muerta mesosiderite     

Ken‐ichi BAJO  Keisuke NAGAO 《Meteoritics & planetary science》2011,46(4):556-573

Abstract– Noble gas isotopic compositions were measured for a eucritic pebble and bulk material of a silicate–metal mixture from the Vaca Muerta mesosiderite as well as pyroxene and plagioclase separated from the eucritic pebble by total melting and stepwise heating methods. Trapped noble gases were degassed completely by a high‐temperature thermal event, probably at the formation of the Vaca Muerta parent body (VMPB). The presence of fissiogenic Xe isotopes from extinct ²⁴⁴Pu in the bulk samples might be a result of rapid cooling from an early high‐temperature metamorphism. High concentrations of cosmogenic noble gases enabled us to determine precise isotopic ratios of cosmogenic Kr and Xe. Spallogenic Ne from Na and unique Ar isotopic compositions were observed. The ⁸¹Kr‐Kr exposure age of 168 ± 8 Myr for the silicate pebble is distinctly longer than the age of 139 ± 8 Myr for the bulk samples. The precursor of the pebble had been irradiated on the surface of the VMPB for more than 60 Myr (first stage irradiation), with subsequent incorporation into bulk materials approximately 4 Gyr ago. The Vaca Muerta meteorite was excavated from the VMPB 140 Myr ago (second stage irradiation). Relative diffusion rates among the cosmogenic Ar, Kr, and Xe based on data obtained by stepwise heating indicate that Kr and Xe can be partially retained in pyroxene and plagioclase under the condition that resets the K‐Ar system. This result supports the presence of fission Xe and of excess concentration of cosmogenic Kr, which could have survived the thermal event approximately 3.8 Gyr ago.  相似文献   

The stability and equation of state for the cotunnite phase of TiO2 up to 70 GPa     

Daisuke Nishio-Hamane  Asa Shimizu  Ritsuko Nakahira  Ken Niwa  Asami Sano-Furukawa  Taku Okada  Takehiko Yagi  Takumi Kikegawa 《Physics and Chemistry of Minerals》2010,37(3):129-136

The stability and equation of state for the cotunnite phase in TiO₂ were investigated up to a pressure of about 70 GPa by high-pressure in situ X-ray diffraction measurements using a laser-heated diamond anvil cell. The transition sequence under high pressure was rutile → α-PbO₂ phase → baddeleyite phase → OI phase → cotunnite phase with increasing pressure. The cotunnite phase was the most stable phase at pressures from 40 GPa to at least 70 GPa. The equation of state parameters for the cotunnite phase were established on the platinum scale using the volume data at pressures of 37–68 GPa after laser annealing, in which the St value, an indicator of the magnitude of the uniaxial stress component in the samples, indicates that these measurements were performed under quasi-hydrostatic conditions. The third-order Birch-Murnaghan equation of state at K ₀′ = 4.25 yields V ₀ = 15.14(5) cm³/mol and K ₀ = 294(9), and the second-order Birch-Murnaghan equation of state yields V ₀ = 15.11(5) cm³/mol and K ₀ = 306(9). Therefore, we conclude that the bulk modulus for the cotunnite phase is not comparable to that of diamond.  相似文献   

Structural and stratigraphic evolution of Abu Dhabi in the context of Arabia     

Ken W. Glennie 《Arabian Journal of Geosciences》2010,3(4):331-349

The Emirate of Abu Dhabi is famed for its coastal carbonate, sabkhas and sand dunes; it is located in the NE part of the Arabian Plate, which formed during the Late Neoproterozoic (~820–750 Ma) by the accretion of island arcs and microcontinents to early Gondwana. Most of Arabia seems to have spent its existence within the Southern Hemisphere until it crossed the Equator during the Mesozoic; parts were involved in four glaciations, two in the Proterozoic (~750–630 Ma—Iceball or Slushball Earth?), and two more in the Palaeozoic (Late Ordovician and Permo-Carboniferous transition). In the early Palaeozoic the Arabian Plate was oriented about 90° counter clockwise relative to today’s poles. Gondwana later skirted the South Pole, migrating to the other side of the planet, eventually emerging the ‘right-way up’ with the Arabian Plate oriented to the poles more or less as seen today. Cold and temperate climate conditions ensured that for much of its early existence, Arabia was the site of mainly quartz-rich deposits. Later in the Neoproterozoic, however, extensive stromatolitic carbonate deposition took the lead, culminating around the Cambro-Precambrian boundary with deposition of the extensive Ara and Hormuz evaporites. Since south Arabia’s Permo-Carboniferous glaciation, the Arabian plate has been drifting northward, crossing temperate climatic zones conducive to fluvial and aeolian sandstone deposition and, from the later Permian, to tropical shallow-marine carbonates and evaporites In parallel with the above, the rifting of Gondwana opened an oceanic trough in the Late Permian off the NE flank of Arabia. Slope carbonates and deepwater Hawasina turbidites with a clear flow to the NE were deposited until they were obducted (together with associated ophiolites) in the Late Cretaceous on the edge of the Arabian plate in Oman and Iran. The deposition of widespread Early Silurian hydrocarbon source rocks in east-central Arabia was followed in the later Permian by extensive reservoir rocks with more during the mid-Late Mesozoic, giving rise to major oilfields both on- and off-shore, including Abu Dhabi. Arabia and Africa began to separate late in the Miocene with the opening of the Red Sea and Gulf of Aden. SSW–NNE compressive stresses caused uplift and volcanic activity in west Saudi Arabia and Yemen. Some products of erosion flowed eastward into Abu Dhabi. At the NE margin of Arabia, the Tethys Ocean narrowed, the NE flank of the newly forming Zagros Mountains of Iran is being subducted beneath southern Asia. To the SE, roughly coeval crustal compression adjacent to the Gulf of Oman led to uplift of the Oman Mountains and deposition of erosional products flanking the mountains mainly to the W and SW. The Oman Mountains are currently rising at about 2 mm/a, while northern Musandam is subsiding into the Strait of Hormuz at some 6 mm/a in association with subduction of the Arabian plate margin below the Eurasian plate. Alternations between polar glaciations and interglacials over the past few 100 ka resulted in considerable climatic changes over Arabia; slow glacial build-ups lasting some 80 to 120 ka led, somewhat erratically, to a fall in sea level of up to 130 m, to strong winds and the building of systems of extensive sand dunes such as the Rub’ al Khali. The joint Tigris–Euphrates river system flowed through a desert landscape, reaching the ocean only SE of the Strait of Hormuz. The peak of the last glaciation about 21 ka was followed by its rapid collapse and flooding of the Arabian Gulf to its present level between about 12 or 10 and 6 ka, a horizontal marine advance of some 200–300 m/a. Abu Dhabi is now the site of shallow-marine carbonates offshore and classical sabkhas and carbonate-rich sand dunes onshore.  相似文献