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  • 1
    Publication Date: 2022-05-26
    Description: Author Posting. © The Authors, 2005. This is the author's version of the work. It is posted here by permission of Elsevier B. V. for personal use, not for redistribution. The definitive version was published in Deep Sea Research Part I: Oceanographic Research Papers 52 (2005): 2315-2332, doi:10.1016/j.dsr.2005.08.004.
    Description: A Video Plankton Recorder (VPR) and remotely operated vehicle (ROV) were utilized on three cruises in the oligotrophic North Pacific Subtropical Gyre (NPSG) between 1995 and 2002 to quantify the size and abundance of marine snow and Rhizosolenia diatom mats within the upper 305 m of the water column. Quantitative image analysis of video collected by the VPR and an ROV-mounted particle imaging system provides the first transect of marine snow size and abundance across the central North Pacific gyre extending from 920 km NW of Oahu to 555 km off Southern California. Snow abundance in the upper 55 m was surprisingly high for this oligotrophic region, with peak values of 6.0-13.0 x 103 aggregates m-3 at the western and eastern-most stations. At stations located in the middle of the transect (farthest from HI and CA), upper water column snow abundance displayed values of ~0.5-1.0 x 103 aggregates m-3. VPR and ROV imagery also provided in-situ documentation of the presence of nitrogen-transporting, vertically migrating Rhizosolenia mats from the surface to 〉300 m with mat abundances ranging from 0-10 mats m-3. There was clear evidence that Rhizosolenia mats commonly reach sub-nutricline depths. The mats were noted to be a common feature in the North Pacific gyre, with the lower salinity edge of the California Current appearing to be the easternmost extent of their oceanic distribution. Based on ROV observations at depth, flux by large (〉1.5 cm) mats is revised upward 4.5 fold, yielding an average value of 40 µmol N m-2 d-1, a value equaling previous estimates that included much smaller mats visible only to towed optical systems. Our results suggest that the occurrence across a broad region of the NPSG of particulate organic matter (POM) production events represented by high concentrations of Rhizosolenia mats, associated mesozooplankton, and abundant detrital marine aggregates may represent significant stochastic components in the overall carbon, nitrogen and silica budgets of the oligotrophic subtropical gyre. Likewise, their presence has important implications for the proposed climate-driven, ecosystem reorganization or domain shift occurring in the NPSG.
    Description: This project was primarily supported by NSF Biological Oceanography Program grant OCE-9423471 to C. Pilskaln, OCE-9415923 and OCE-9414372/OCE-0094591 to T. Villareal, and assisted by OCE-9314533 to D. Caron.
    Keywords: Biogeochemical cycles ; Carbon cycle ; Nitrogen cycle ; Particle flux ; North Pacific Subtropical Gyre ; 24–32°N ; 168–123°W
    Repository Name: Woods Hole Open Access Server
    Type: Preprint
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  • 2
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] The surface of Saturn’s haze-shrouded moon Titan has long been proposed to have oceans or lakes, on the basis of the stability of liquid methane at the surface. Initial visible and radar imaging failed to find any evidence of an ocean, although abundant evidence was found that flowing ...
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  • 3
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Cassini's Titan Radar Mapper imaged the surface of Saturn's moon Titan on its February 2005 fly-by (denoted T3), collecting high-resolution synthetic-aperture radar and larger-scale radiometry and scatterometry data. These data provide the first definitive identification of ...
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  • 4
    Electronic Resource
    Electronic Resource
    Oxford, UK; Malden, USA : Blackwell Science Ltd
    Journal of fish biology 66 (2005), S. 0 
    ISSN: 1095-8649
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Biology
    Notes: Rainbow trout Oncorhynchus mykiss fry in moderately hard water were exposed to control or high levels of dietary Cu (c. 6 and 580 ug Cu g food−1) at one of three levels of Na (1·5, 3·0 or 4·5%) in the diet, i.e. six experimental groups. Fish were fed a 4% body mass ration daily for 28 days and 10 individuals from each group were sampled every 7 days. Concentrations of Cu and Na were measured in the gills, liver, gut and remaining carcass of sampled fish. Growth was not affected and no consistent differences were found in mass, total lengths (LT) or indices of body condition among any of the groups on any sampling day. Copper concentration was significantly higher in tissues of Cu-exposed groups, although within treatment types (control Cu v. high Cu diet), it did not differ consistently among groups that received different levels of dietary Na. Tissue Na concentration did not differ among any of the groups and did not show any marked changes over time. In Cu-exposed groups, the proportion of total body Cu burden contained in the liver approximately doubled over time, from c. 30% on day 7 to c. 60% on day 28. In unexposed fish, the liver maintained c. 25% of the total Cu burden throughout the experiment. In contrast, the proportion of the total body Cu burden contained in the gut decreased somewhat over time in Cu-exposed fish, from c. 40% on day 7 to c. 30% on day 28, and remained fairly stable at c. 25–30% in control groups, i.e. approximately equal to liver values. In all groups, the carcass contained by far the largest portion of the total Na content (〉80%). Measurements made 36 h post-feeding indicated that all six groups had much higher Na efflux relative to influx, suggesting that the fish were eliminating excess Na taken up from the diet, and differences in Na influx rates were small. Na efflux rate was significantly higher in the high Cu and high Na group than in the high Cu and low Na group. The results indicate that at the concentrations used in this experiment, dietary Na has little effect on dietary Cu uptake by juvenile rainbow trout, and dietary Cu has little effect on Na homeostasis.
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  • 5
    Electronic Resource
    Electronic Resource
    Springer
    Earth, moon and planets 7 (1973), S. 440-452 
    ISSN: 1573-0794
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract This paper discusses formation of ‘pathological’ cases of crater morphology due to interaction of craters with molten lavas. Terrestrial observations of such a process are discussed. In lunar maria, a number of small impact craters (D 〈 10 km) may have been covered by thin layers of fluid lavas, or formed in molten lava. Some specific lunar examples are discussed, including unusual shallow rings resembling experimental craters deformed by isostatic filling.
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  • 6
    Electronic Resource
    Electronic Resource
    Springer
    Earth, moon and planets 3 (1971), S. 3-78 
    ISSN: 1573-0794
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract This paper summarizes current data and new observations on lunar basin systems. Parts 1–4 review earlier literature and give new crater-counts used to reconstruct basin histories. Among the results are: basin rings are defined by faults, hills, craters, and/or wrinkle ridges; all of these are inter-related; √2 plays a special role in the ratios of ring diameters; flooding occurred in many basins prior to the formation of the familiar front-side maria; 3 km is a typical depth of lava flooding in basins. Parts 5–11 interpret these results in terms of origin and evolution of basins. Polar concentrations of basins and old, large craters are found (Figures 28 and 29). Basins originated by impacts of very early planetesimals left over from or created during formation of the Moon (6). Concentric fractures were produced by the impacts. Concentric rings developed along fractures during subsequent sagging of the basin into partially melted substrata, along the lines of theory and experiments by Lance and Onat (1962) (Figures 36 and 37). There is marginal empirical evidence that some rings formed significantly after their basins (8). The structure of specific rings depended on the nature of volcanic products extruded. Wrinkle ridges, ‘peak-rings’, rings of craters, concentric graben, and central peaks are all consequences of basin-forming evolutionary processes (9, Figure 41), Flooding by lava was a final stage in basin evolution. Lava extruded from concentric ring-faults, wrinkle ridges, and crater and basin rims (10). Mascons are directly correlated with the amount of mare lava, but not correlated with basin age or morphology (11). Section 12 summarizes the results and compares them to those of other authors.
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  • 7
    Electronic Resource
    Electronic Resource
    Springer
    Earth, moon and planets 3 (1972), S. 408-411 
    ISSN: 1573-0794
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract A new catalogue of lunar crater diameters, depths and morphologies based on Orbiter photography is described. Preliminary shadow length reductions indicate that previous depths determined by ACIC and Baldwin are systematically about 500 m too shallow.
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  • 8
    Electronic Resource
    Electronic Resource
    Springer
    Earth, moon and planets 3 (1972), S. 412-447 
    ISSN: 1573-0794
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract In this paper we consider the origin of rilles on the lunar maria, both sinuous and those having straight line segments, from the point of view of lava tubes formed in surface lava flows, and also in terms of collapses along active fissures. Terrestrial examples of tube formation and collapse, as well as the large-scale collapse of a chain of craters built over an active fissure were observed on the Island of Hawaii by the writers and serve as the basis of comparison with lunar topography shown on Orbiter photographs of the Moon. We also consider the origin of apparent flow channels on steep slopes on the Moon, and conclude that these are often related to early stages in the formation of covered lava tubes.
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  • 9
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    In:  Geological Society Special Publication 271: 309-322.
    Publication Date: 2007-10-08
    Description: Soft wall capping, which involves placing a cap of soil and turf (or other vegetation) on the top of ruined walls, is a potentially low cost, easy to maintain, ecologically sensitive and effective method of conserving ruined monuments. An integrated programme of laboratory and field testing has been designed to test the performance of soft capping in comparison with hard capping at a range of sites in England. A sample of ruined walls has been soft capped and monitored using repeat photography, with more detailed wooden dowel monitoring of wall moisture and electronic monitoring of temperatures and moisture levels at the base of soft caps at some sites. Experiments designed to test the thermal blanketing capability of the soft caps have been run in an environmental cabinet on scaled-down versions of soft and hard caps, and similar set-ups have also been monitored outdoors in Oxford. Short-term data from both field trials and laboratory tests illustrate the success of soft wall capping under a wide range of environmental conditions, but longer-term monitoring is needed to evaluate more fully the conservation benefits of soft capping.
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  • 10
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