Sketch of the geology of the Birmingham District: With special reference to the long excursion of 1898     

C. Lapworth  W.W. Watts  W. Jerome Harrison 《Proceedings of the Geologists' Association. Geologists' Association》1898,15(9):313-IN3

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Palygorskite as a sediment dispersal tracer in the eastern Mediterranean     

Daniel Jean Stanley  Harrison Sheng  Christian Blanpied 《Geo-Marine Letters》1981,1(1):49-55

Palygorskite is a clay mineral widely distributed in late Quaternary deposits of the eastern Mediterranean, where, locally, it proves an ideal tracer of sediment dispersal. This study shows that the origin of this mineral is not limited to African sources. Cores containing late Pleistocene to recent sediment record the transport of palygorskite from the Plain of Helos on the Peloponnesus to specific deep basins along the Hellenic Arc. Palygorskite, commonly concentrated in the silt size fraction, may be overlooked in studies that focus only on the <2 μm fraction. In this region we find that the detrial palygorskite distribution is partially controlled by size-sorting effects related to gravity-induced transport processes. In consequence, comprehensive compositional analyses should be made both on the silt and clay fractions.  相似文献   

Spatial and temporal variability in coccolithophore abundance and production of PIC and POC in the NE subarctic Pacific during El Niño (1998), La Niña (1999) and 2000     

M.S. Lipsen  D.W. Crawford  P.J. Harrison 《Progress in Oceanography》2007,75(2):304-325

Seasonal variations in coccolithophore abundance, chlorophyll, nutrients and production of particulate organic and inorganic carbon (POC and PIC) were determined along a coastal to oceanic east-west transect (Line P) culminating at Ocean Station Papa in the northeastern subarctic Pacific between 1998 and 2000. Offshore stations generally exhibited low seasonality in chlorophyll concentrations, with moderate seasonality in POC production. Near shelf stations showed a similar pattern to offshore stations, but were also characterized by sporadic events of higher POC productivity. During the 1998 El Niño, June was characterized by low chlorophyll and POC productivity along the transect, presumably as a result of depleted surface nitrate. In contrast, during the 1999 La Niña, and in 2000, higher POC productivity and surface nitrate occurred along the transect in June. Chlorophyll and POC productivity were similar in late summer in all 3 years. The coccolithophore population was usually numerically dominated by Emiliania huxleyi, particularly in June. Along the transect, abundance of coccolithophores was much higher in June during the 1998 El Niño (mean of 221 cells ml⁻¹) than in the 1999 La Niña (mean of 40 cells ml⁻¹), with their abundance in late summers of both years being very low. Abundances were even higher along the transect in June and the late summer of 2000 with sporadic ‘blooms’ of >1000 cells ml⁻¹ at some stations (cruise averages 395 and 552 cell ml⁻¹, respectively). Production rates of PIC did not consistently correlate with areas of high coccolithophore abundance. PIC production was high (100-250 mg C m⁻² d⁻¹) along the transect during June 1998, and low (1-40 mg C m⁻² d⁻¹) during both winters, June 1999 and during late summers of 1998 and 1999. The year 2000 was more complicated, with high rates of PIC production accompanying high abundance of coccolithophores in late summer, but lower rates of PIC production accompanying high coccolithophore numbers in June. Our data suggest that the abundance of coccolithophores and the production rates of PIC in the subarctic are higher than previously thought. Occasional PIC:POC production ratios of 1 or greater in 1998 and 2000 suggest that coccolithophores in this region could have a significant impact on the efficiency of the biological carbon pump.  相似文献   

Station Papa Time Series: Insights into Ecosystem Dynamics     

Paul J. Harrison 《Journal of Oceanography》2002,58(2):259-264

The Northeast Pacific has one of the longest time series of any open ocean station, primarily as a result of the weathership station at Station P from the 1950s to 1981. This review summarizes our understanding of the plankton ecosystem for this station and examines interannual variability for the primary producers. The weathership era characterized a period of high temporal sampling resolution with a limited number of parameters being measured. In contrast, the post-weathership period focussed on seasonal sampling (usually three times per year), but a wider range of parameters were measured and sediment traps were deployed to estimate carbon and opal flux rates. The mixed layer depth is shallow compared to the Atlantic Ocean, ranging from 40 to 120 m in late summer and winter respectively. Nitrate, silicate and phosphate are saturating year round with only a few exceptions in the 1970s. Winter and summer Si:N ratios are the same (1.5:1). Ammonium and urea are 0.5 uM in winter and near detection limits (∼0.1 uM) in late summer. Iron is limiting (∼0.05 nM) in late spring and summer for the growth of large diatoms, but iron is co-limiting with irradiance in winter. Chlorophyll and primary productivity are low and show little seasonal variation (about 2 times). Summer chl is about 20 mg m⁻² while primary productivity ranges from 400–850 mg C m⁻²d⁻¹. The f-ratio of 0.25 does not vary with seasons and indicates that primary productivity is fueled by regenerated nitrogen (e.g. NH₄ and urea). Small cells (<5 um) are normally abundant and they utilize regenerated nitrogen produced by the micrograzers; they do not appear to be Fe-limited, but rather controlled by the micrograzers. Shipboard carboy experiments indicate that large diatoms become dominant when iron is added. Therefore top down control is exerted by the micrograzers on the small cells, while there is bottom up control of the large phytoplankton due to low Fe concentrations. This revised version was published online in August 2006 with corrections to the Cover Date.  相似文献   

Partitioning of metals among metal-binding proteins in the bay mussel, Mytilus edulis     

F.L. Harrison  J.R. Lam  J. Novacek 《Marine environmental research》1988,24(1-4)

Metabolism of metals was assessed in populations of Mytilus edulis exposed to metals in the laboratory and in the field. Chronic exposure to metals in both environments resulted in increased concentrations of metals in both the low molecular weight metal-binding protein fraction, which contains metallothioneins, and in the high molecular weight metal-binding protein fraction, which contains metalloenzymes. Our results from analysis of laboratory-exposed populations and from monitoring indigenous and transplanted populations indicate that the capacity for production of metallothioneins is limited and that the quantities present differ greatly with seasonal changes in the environment.  相似文献   

Semiconductors exposed to oils in pressure-tolerant electronic systems     

Daniel E. Gilbert  John R. Hauser  James W. Harrison  Jimmie J. Wortman 《Ocean Engineering》1974,2(6):265-273

The present study indicates that most semiconductor components are fabricated such that they are not affected by operation in a dielectric oil environment. A quantitative estimate of the conditions under which oil-soluble ions will invert semiconductor surfaces and interfere with proper device operation is developed. The results are discussed in terms of pressure-tolerant electronic systems—solid-state components operated immersed in chemically inert dielectric oils when these components are subject to, and experience, ambient hydrostatic pressures of the ocean depths. The feasibility of pressure-tolerant electronic systems is demonstrated.  相似文献   

Reproductive success as an indicator of genotoxicity in the polychaete worm, Neanthes arenaceodentata     

Florence L. Harrison  Susan L. Anderson 《Marine environmental research》1989,28(1-4)

The effects on reproduction of single or chronic exposure to the direct-acting mutagen, radiation, were evaluated using Neanthes arenaceodentata as the model animal. In the first set of experiments, mated pairs were irradiated when oocytes were visible in the female and were given a single dose of either 0·5, 1·0, 2·0, 5·0, 10 or 50 Gy. In the second set of experiments, lifetime exposure was initiated upon the spawning of the P₁ female and was terminated upon the spawning of the F₁ female; the average total doses (0·55, 6·5 and 54 Cy) were delivered at a rate of 0·19, 2·1 or 17 mGyH⁻¹. Our results on embryo abnormalities and mortalities indicated that lethal mutations were most likely induced in the germ cells and had an adverse effect on reproductive success by reducing the survival of early life stages. Except for those mated pairs exposed acutely to 10 or 50 Gy or exposed chronically to 17 mGyh⁻¹, there was no evidence of gamete killing. However, evidence was obtained for mutagen-damage accumulation in developing gametes from continuous exposure to radiation.  相似文献   

East-west trending magnetic anomalies in the Southern Hemisphere of Mars: Modeling analysis and interpretation   总被引：1，自引：0，他引：1  

Lon L. Hood  Nicola C. Richmond  Keith P. Harrison 《Icarus》2007,191(1):113-131

Maps of the vector components of the martian crustal magnetic field over the strongly magnetized Terra Cimmeria/Sirenum region are constructed using Mars Global Surveyor magnetometer data. Although pronounced east-west trending anomalies are present on the radial and north field component maps at the mapping altitude (∼360-380 km), these trends are much less prominent at the lower aerobraking altitude (∼90-150 km). Comparisons with similar maps produced using artificial data at the aerobraking altitude indicate that elongated sources in this region may have maximum lengths along the martian surface of ∼500 km and maximum aspect ratios of ∼2. Iterative forward modeling of several relatively isolated anomalies in the mapped region yields paleomagnetic pole positions consistent with those estimated in previous studies of other anomalies using mapping phase and science phasing orbit data. On this basis, it is inferred that sources in the studied region are most probably magnetized primarily in northward or southward directions. Using this additional constraint, iterative forward modeling is then applied to determine a magnetization distribution that is consistent with data at both the aerobraking altitude and the mapping altitude. The model magnetization distribution, which includes 41 discrete sources, again indicates no highly elongated sources. An examination of surface geology in the region as well as a consideration of the global distribution of anomalies suggests that magmatic intrusions (e.g., subsurface dike swarms), cooling in the presence of water, are the most likely sources of the magnetic anomalies.  相似文献   

The Heliospheric Imagers Onboard the STEREO Mission   总被引：1，自引：0，他引：1  

C. J. Eyles  R. A. Harrison  C. J. Davis  N. R. Waltham  B. M. Shaughnessy  H. C. A. Mapson-Menard  D. Bewsher  S. R. Crothers  J. A. Davies  G. M. Simnett  R. A. Howard  J. D. Moses  J. S. Newmark  D. G. Socker  J.-P. Halain  J.-M. Defise  E. Mazy  P. Rochus 《Solar physics》2009,254(2):387-445

Mounted on the sides of two widely separated spacecraft, the two Heliospheric Imager (HI) instruments onboard NASA’s STEREO mission view, for the first time, the space between the Sun and Earth. These instruments are wide-angle visible-light imagers that incorporate sufficient baffling to eliminate scattered light to the extent that the passage of solar coronal mass ejections (CMEs) through the heliosphere can be detected. Each HI instrument comprises two cameras, HI-1 and HI-2, which have 20° and 70° fields of view and are off-pointed from the Sun direction by 14.0° and 53.7°, respectively, with their optical axes aligned in the ecliptic plane. This arrangement provides coverage over solar elongation angles from 4.0° to 88.7° at the viewpoints of the two spacecraft, thereby allowing the observation of Earth-directed CMEs along the Sun?–?Earth line to the vicinity of the Earth and beyond. Given the two separated platforms, this also presents the first opportunity to view the structure and evolution of CMEs in three dimensions. The STEREO spacecraft were launched from Cape Canaveral Air Force Base in late October 2006, and the HI instruments have been performing scientific observations since early 2007. The design, development, manufacture, and calibration of these unique instruments are reviewed in this paper. Mission operations, including the initial commissioning phase and the science operations phase, are described. Data processing and analysis procedures are briefly discussed, and ground-test results and in-orbit observations are used to demonstrate that the performance of the instruments meets the original scientific requirements.  相似文献   

Multiscalarity of the Nutrient–Chlorophyll Relationship in Coastal Phytoplankton     

William K. W. Li  Marlon R. Lewis  W. Glen Harrison 《Estuaries and Coasts》2010,33(2):440-447

The relationship between nitrogen (N) and phytoplankton chlorophyll a (Chl) establishes a basis for understanding eutrophication in coastal marine ecosystems. A substantial literature exists on cross-ecosystem analysis of this relationship, but there is little information on cross-scale patterns. A collection of observational records in Bedford Basin (Canada) was used to construct the N–Chl relationship at four time scales: intra-day, intra-annual, interannual, and interdecadal. Additionally, a dataset of contingent observations from 16 biogeochemical ocean provinces was used to construct the N–Chl relationship at large spatial scale. In Bedford Basin, N statistically predicts Chl at time scales that are short (intra-day, intra-annual) and long (interdecadal) but not intermediate (interannual). There is an apparent stoichiometric regularity in the dependence of Chl on N that crosses time scales. Further, an apparent similitude exists between the local pattern at long time scale and the global pattern at large space scale.  相似文献