Pliocene climate change of the Southwest Pacific and the impact of ocean gateways     

Cyrus Karas  Dirk Nürnberg  Ralf Tiedemann  Dieter Garbe-Schönberg 《Earth and Planetary Science Letters》2011,301(1-2):117-124

The transition from the early Pliocene “Warmhouse” towards the present “Icehouse” climate and the role of Gateway dynamics are intensively debated. Both, the constrictions of the Central American Seaway and the Indonesian Gateway affected ocean circulation and climate during the Pliocene epoch. Here, we use combined δ¹⁸O and Mg/Ca ratios of planktonic foraminifera (marine protozoa) from surface and subsurface levels to reconstruct the thermal structure and changes in salinities from the Southwest Pacific Deep Sea Drilling Project (DSDP) Site 590B from 6.5 to 2.5 Ma. Our data suggest a gradual cooling of ~ 2 °C and freshening of the sea surface during ~ 4.6–4 Ma with an increased meridional temperature gradient between the West Pacific Warm Pool and the Southwest Pacific when the closing of the Central American Seaway reached a critical threshold. After ~ 3.5 Ma, the restricted Indonesian Gateway might have amplified the East Australian Current, allowing enhanced heat transport towards the Southwest Pacific with reduced meridional temperature gradients when the global climate gradually cooled. At the same time our data suggest a cooling and freshening of Subantarctic Mode Water (SAMW) or/and an increased northward flow of SAMW towards Site 590B, possibly a first step towards the present Antarctic Frontal System.  相似文献   

Sensitivity of multi-gas climate policy to emission metrics     

Steven J. Smith  Joseph Karas  Jae Edmonds  Jiyong Eom  Andrew Mizrahi 《Climatic change》2013,117(4):663-675

The Global Warming Potential (GWP) index is currently used to create CO₂-equivalent emission totals for multi-gas greenhouse targets. While many alternatives have been proposed, it is not possible to uniquely define a metric that captures the different impacts of emissions of substances with widely disparate atmospheric lifetimes, which leads to a wide range of possible index values. We examine the sensitivity of emissions and climate outcomes to the value of the index used to aggregate methane emissions using a technologically detailed integrated assessment model. The methane index is varied between 4 and 70, with a central value of 21, which is the 100-year GWP value currently used in policy contexts. We find that the sensitivity to index value is, at most, 10–18 % in terms of methane emissions but only 2–3 % in terms of the maximum total radiative forcing change, with larger regional emissions differences in some cases. The choice of index also affects estimates of the cost of meeting a given end of century forcing target, with total two-gas mitigation cost increasing by 7–9 % if the index is increased, and increasing in most scenarios from 4 to 23 % if the index is lowered, with a slight (1 %) decrease in total cost in one case. We find that much of the methane abatement occurs as the induced effect of CO₂ abatement rather than explicit abatement, which is one reason why climate outcomes are relatively insensitive to the index value. We also find that the near-term climate benefit of increasing the methane index is small.  相似文献   

水体扰动对多种赤潮藻生长的影响   总被引：4，自引：0，他引：4  

李冬梅  高永利  田甜  劉駿豪  殷克东 《热带海洋学报》2010,29(6)

水体扰动是海洋环境的一个重要特征.扰动通过对藻细胞周围的营养盐边界层厚度的影响,进而影响藻细胞的生长.在其他环境因子统一的条件下,通过室内实验研究扰动条件为主要影响因素对藻类生长的影响.研究结果发现扰动对中肋骨条藻、具齿原甲藻等10个藻种生长存在不同影响,实验数据显示,100r·min-1扰动对新月菱形藻Nitzschia closterium,中肋骨条藻Skeletonema costatum、具齿原甲藻Prorocentrum dentatum、针胞藻Fibrocapsa japonica、棕囊藻Phaeocystis spp.、定鞭金藻Prymnesium patelliferium有显著作用(P<0.05),对赤潮异弯藻Heterosigma akashiwo、亚心形扁藻Platymonas subcordiformis、青岛大扁藻Platymonas helgolandica var Tsing-taoensis、塔胞藻Pyramimonas sp.、Pyramidomonas作用不明显(P>0.05).扰动促进了棕囊藻和定鞭金藻的生长,使之达到最大生物量,并延长了藻细胞的生长时间;同时100r·min-1扰动抑制了新月菱形藻,中肋骨条藻、具齿原甲藻、针胞藻的生长.这些不同的藻类对水体扰动有不同生长反应,结果表明水体扰动是藻类种间竞争的的选择推动力之一.  相似文献   

Response of the mesozooplankton community of the St Lucia estuary,South Africa,to a mouth-opening event during an extended drought     

Hendrik L. Jerling  Leon VivierDigby P. Cyrus 《Estuarine, Coastal and Shelf Science》2010

Mesozooplankton samples were collected between March 2005 and November 2008 in St Lucia, the largest estuarine lake system in South Africa. St Lucia experienced an extended period of drought before and during the present study. This drought led to natural closing of the estuary mouth as a result of flood-tide marine sediment deposition in 2002. In March 2007 the mouth was washed open by exceptionally high tidal and wave conditions. This resulted in an influx of a large volume of seawater. The mouth closed again in August 2007. Before opening of the mouth salinities in the Estuary were below 10 and large parts of North Lake dried up while South Lake retained a relatively stable waterbody with salinities between 10 and 30. When the mouth opened seawater flooded the system and salinities changed to about 35. After the mouth had closed again in August 2007 salinities increased in the lakes and decreased in the Estuary. The mesozooplankton community was dominated by copepods during all sampling sessions, especially by the estuarine calanoids Pseudodiaptomus stuhlmanni and Acartia natalensis. Mean mesozooplankton densities were significantly higher in South Lake before the mouth opened in March 2007. While zooplankton density decreased when the mouth opened species richness increased with the influx of coastal marine species, especially in the Estuary. Overall zooplankton densities declined progressively as salinity increased to hypersaline levels after mouth closure. Multivariate analyses supported significant differences between the lakes and the Estuary in terms of mesozooplankton community composition. Taxa mostly responsible for the similarities within and dissimilarity between sections of the system were the copepods P. stuhlmanni and A. natalensis with the meroplankton, crab zoeae and mollusc larvae, also contributing significantly after the mouth-opening event.  相似文献   

Between an Uncomfortable Decision and an Absurd One     

Cyrus M. Hester  John Coleman 《Ground water》2014,52(5):645-646

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Boron-polymetallic metallogeny of the north and northeast of the Sino-Korean Craton     

V. V. Ratkin  V. I. Gvozdev  O. A. Karas’ 《Russian Journal of Pacific Geology》2014,8(5):379-389

Based on published data and original investigations, it has been shown that the combination of widely known Ag, Fe, and Fe-Mn ore deposits, as well as boron and Pb-Zn world-class deposits, is typical for metallogenic zones in the north and northeast of the Sino-Korean Craton. The ore genesis was spatially inherited and lasted from the Archean to Mesozoic. The Archean metallogenic zones are related to the protocontinental margin terranes of the craton basement and they comprise banded iron ore and Cu-Zn sulfide deposits. The proterozoic-Early Paleozoic metallogenic zones are related to rift basins, where the ore-bearing Archean folded basement is overlain by volcanic and sedimentary complexes. The Proterozoic metallogenic zones host quartz veins and schistosity zone-related Au deposits, banded iron and Cu-Zn ore deposits, large sedimentary-metamorphogenic borate and magnesite deposits, Cu-W deposits in tourmalinites, exhalation-sedimentary Pb-Zn ore deposits, and large polygenic REE-Fe-Nb ore deposits. The Riphean-Cambrian terrigenous-carbonate strata are represented by stratiform Pb-Zn and fluorite deposits. Mesozoic metallogenic zones related to volcano-plutonic complexes of intraplate series coincide with zones where the folded basement is made of Precambrian ore-bearing series. Gold deposits are typical of all the metallogenic zones, but most of them are related to Mesozoic volcano-plutonic complexes.  相似文献   

Book reviews     

Vladimír Karas  Hans Joachim Haubold 《Astrophysics and Space Science》1990,166(1):167-168

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Stellar dynamics in a galactic centre surrounded by a massive accretion disc — I. Newtonian description     

D. Vokrouhlický  & V. Karas 《Monthly notices of the Royal Astronomical Society》1998,298(1):53-66

The long-term evolution of stellar orbits bound to a massive centre is studied in order to understand the cores of star clusters in central regions of galaxies. Stellar trajectories undergo tiny perturbations, the origins of which are twofold: (i) the gravitational field of a thin gaseous disc surrounding the galactic centre, and (ii) cumulative drag arising from successive interactions of the stars with the material of the disc. Both effects are closely related because they depend on the total mass of the disc, assumed to be a small fraction of the central mass. It is shown that, in contrast to previous works, most of the retrograde (with respect to the disc) orbits are captured by the central object, presumably a massive black hole. Initially prograde orbits are also affected, so that statistical properties of the central star cluster in quasi-equilibrium may differ significantly from those deduced in previous analyses.  相似文献   

N. Ashby,D. F. Bartlett and W. Wyss (eds.),general relativity and gravitation, 1989, Cambridge University Press,Cambridge, 1990, xiv + 502 pp., ISBN 0-521-38428-1, hard cover £35.00/$49.50     

V. Karas 《Astrophysics and Space Science》1993,201(1):154-155

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A Preliminary Analysis of Disturbance Tracksover the Mediterranean Basin     

S. Karas  A. Zangvil 《Theoretical and Applied Climatology》1999,64(3-4):239-248

Summary  The Mediterranean basin experiences considerable cyclone activity mostly during fall, winter and spring and diminished activity during summer. In this study we present results of synoptic disturbance track analysis for two contrasting winter months and two, near average, summer months over the eastern Mediterranean. The surface and 500 hPa disturbance tracks were subjectively analyzed from two points of view. First, looking at tracks of conventionally defined cyclone centers (eddies) based on actual pressure and height distribution and second, looking at tracks of transient cyclonic disturbances (TRADs), defined as centers of negative deviations from the time mean. The second type of analysis demonstrated a considerable increase in the number of detectable tracks. Over the Mediterranean and vicinity the ratio between the number of surface TRAD tracks to cyclone tracks is, about 2, whereas at 500 hPa the ratio is much higher, about 5. However, the average life span of transient disturbances was only slightly longer than that of conventional cyclones (mainly at 500 hPa). At the surface and at 500 hPa about 50% of the cyclone tracks coincided to a certain extent with TRAD tracks. In summer, when conventional analysis over the eastern Mediterranean yields mostly quasi‐stationary low pressure centers associated with the Persian Gulf Trough, we detected clear signs of transient disturbances. Some interpretations of the differences between cyclones and TRADs in terms of weather in the eastern Mediterranean are also made. Received January 19, 1999Revised June 23, 1999  相似文献