388 research outputs found

    Development of a long life design procedure for Australian asphalt pavements

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    This project examined the incorporation of the Fatigue Endurance Limit concept into a pavement design procedure. The result of the project was the development of a validated method based off fundamental laboratory testing, which can be used to determine the maximum thickness of an asphalt pavement, beyond which any increase in design thickness will result in little to no increase in the structural capacity of the pavement

    The upper Derwent : long-term landscape archaeology in the Peak District.

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    This thesis is concerned with writing a long-term archaeological landscape history of the Upper Derwent, situated in the Peak District. It is based on fieldwork I have undertaken or directed on behalf of the Peak District National Park Authority between 1994 and 2002 while employed as a Survey Archaeologist. Original field data, gathered by field survey, fieldwalking and excavation, documentary sources and the recorded results of research are discussed as the archaeological evidence for occupation and activity in, and perceptions of, the area. This evidence is integrated into an interpretation of the landscape history of the Upper Derwent, covering a period from the approximate end of the last Ice Age to the modern day. The nature, scale, visibility and chronological resolution of archaeological evidence vary enormously over time. The limitations posed by this variability are addressed, and the opportunities for more in-depth analysis acknowledged. The thesis also explores Andrew Fleming's proposition that we can only interpret the long-term landscape archaeology of an area by exploring the detail of the local evidence in relation to its wider context (Fleming 1990). This takes the 'face-to-face' community as the main focus of study. There are two fundamental issues that have to be addressed in attempting such a study, which are related to reconciling different scales of time and geography. One, is how to write long-term landscape history that covers a time-span extending way beyond a person's comprehension of their past world as understood through personal memory, story-telling and folklore or by other forms of archive. The second is to try to interpret how occupants of a local geographical area interact with regional trends and broader social institutions. I have primarily based my approach on that outlined by Fleming, while also incorporating elements of theoretical developments in landscape archaeology since 1990. Implications of this approach for landscape archaeology are discussed

    Integration of Mirror Design with Suspension System using NASA's New Mirror Modeling Software

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    Advances in mirror fabrication is making very large space based telescopes possible. In the many applications, only monolithic mirrors meet the performance requirements. The existing and near-term planned heavy launch vehicles place a premium on lowest possible mass. Again, available and planned payload shroud size limits near term designs to 4 meter class mirror. Practical 8 meter and beyond designs could encourage planners to include larger shrouds if it can be proven that such mirrors can be manufactured. These two factors lower mass and larger mirrors, presents the classic optimization problem. There is a practical upper limit to how large a mirror can be supported by a purely kinematic mount system and be launched. This paper shows how the design of the suspension system and mirror blank needs to be designed simultaneously. We will also explore the concepts of auxiliary support systems, which act only during launch and disengage on orbit. We will define required characteristics of these systems and show how they can substantially reduce the mirror mass. The AMTD project is developing and maturing the processes for future replacements for HUBBLE, creating the design tools, validating the methods and techniques necessary to manufacture, test and launch extremely large optical missions. This paper will use the AMTD 4 meter "design point" as an illustration of the typical use of the modeler in generating the multiple models of mirror and suspension systems used during the conceptual design phase of most projects. The influence of Hexapod geometry, mirror depth, cell size and construction techniques (Exelsis Deep Core Low Temperature Fusion (c) versus Corning Frit Bonded (c) versus Schott Pocket Milled Zerodur (c) in this particular study) are being evaluated. Due to space and time consideration we will only be able to present snippets of the study in this paper. The advances in manufacturing techniques for lightweight mirrors, such as EXELSIS deep core low temperature fusion, Corning's continued improvements in the Frit bonding process and the ability to cast large complex designs, combined with water-jet and conventional diamond

    Sedimentation of the Middle Precambrian Tyler Formation of Northcentral Wisconsin and Northwestern Michigan

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    A Thesis submitted to the faculty of the Graduate School of the University of Minnesota by Bevan William Alwin in partial fulfillment of the requirements for the degree of Master of Science, June 1976. Plates I-II referenced in the thesis are also attached to this record.The Tyler Formation crops out in a northeasterly-trending belt in Northcentral Wisconsin and Northwestern Michigan along the Gogebic Iron Range. Good exposures are found along several of the major streams draining the area, road cuts and railroad right-of-ways. The Tyler is considered Late Middle Precambrian in age, the Wisconsin equivalent of the Baraga Group of Michigan's Marquette Range Supergroup. The formation was warped and slightly metamorphosed during the Penokean Orogeny (1.7 b. y.). Primary sedimentary structures have been generally preserved. The sedimentologic aspects of seven outcrops in the Hurley, Wisconsin area were studied in detail and a measured stratigraphic section was established. Three distinct lithologies are present, sandstone (graywacke), siltstone and shale in varying degrees of metamorphism. Forty-one percent of the beds measured are argillites or slates and fifty-nine percent are sandstones or siltstones. Volumetrically, the sandstones and siltstones are more abundant than the shale units. A thinning-upward trend in the shale beds suggests a decreasing rate of sedimentation up section which in turn suggests increasing tectonic stability in the source area relative to the depocenter. Alternatively, the thinning-upward trend in the shales may reflect increased periodicity of the events which deposited the coarser-grained elastic beds. A corresponding volumetric increase in sandstones and siltstones up section is explained by the peculiarities of local basin bottom topography. Primary sedimentary structures including alternation of sand-mud units, laterally extensive bedding, graded bedding, rnicrocross-bedding, sole marks, rip-up clasts and Bouma sequences suggest a turbidity current mechanism for sediment transport and deposition in a realtively deep water environment. Twenty-four percent of the beds studied in detail are recognizable turbidites while thirty-five percent do not contain specific telltale sedimentary structures. A grain-flow origin for at least some of these latter beds is suspected. Because of the similarity between the lithologies and facies of the Tyler Formation and the ideal facies sequences of submarine fans, it is suggested that that part of the Tyler Formation which was studied in detail was deposited as part of a submarine fan complex. Indicators of current movement found in the rocks of the Tyler are of several types including both interstratal and intrastratal. Sole marks and cross-bedding are most useful. The currents which deposited the Tyler sediments moved from the east-southeast toward the west-northwest. A new type of sole mark, called a ridge mold or negative groove, is described and a possible method of formation is suggested. Two different methods for estimating current velocity were employed, one based on maximum clast size and one based on spacing of ridge molds. Both methods yielded velocities of a few tens of centimeters per second and primary slope is estimated at 0°10'. Petrology reveals that the major framework constituents of the Tyler graywackes are quartz, plagioclase and rock fragments set in a chlorite- and mica-rich matrix. The "average" graywacke is a lithic graywacke with 28% matrix. Quartz and chert comprise 73% of the framework grains, rock fragments 17% and feldspar 10%. The source terrain was probably mostly granitic with some contribution from older sedimentary, metamorphic and volcanic rocks. The Lower Precambrian rocks to the south and southeast of the Tyler outcrop belt were the probable source. Paleoslope was probably at right angles to current flow. Thus a southern limit to the extent of the Middle Precambrian depositional basin is defined. Similarity of the Tyler and other Middle Precambrian sedimentary rocks in the Lake Superior region suggests a common depocenter in a cratonic basin but at different depositional loci. Reconstruction of current movement and probable source area for the Tyler, Rove and Virginia (Thomson) Formations suggest that the depocenter was landlocked on three sides but may have been open to the northeast

    Integration of Mirror Design with Suspension System Using NASA's New Mirror Modeling Software

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    Advances in mirror fabrication are making very large space based telescopes possible. In many applications, only monolithic mirrors can meet the performance requirements. The existing and near-term planned heavy launch vehicles place a premium on lowest possible mass, and then available payload shroud sizes limit near term designs to 4 meter class mirrors. Practical 8 meter class and beyond designs could encourage planners to include larger shrouds, if it can be proven that such mirrors can be manufactured. These two factors, lower mass and larger mirrors, present the classic optimization problem. There is a practical upper limit to how large of a mirror can be supported by a purely kinematic mount system handling both operational and launch loads. This paper shows how the suspension system and mirror blank need to be designed simultaneously. We will also explore the concepts of auxiliary support systems which act only during launch and disengage on orbit. We will define required characteristics of these systems and show how they can substantially reduce the mirror mass

    Evaluation of the Status of the Kemp\u27s Ridley Sea Turtle After the 2010 Deepwater Horizon Oil Spill

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    Coincident with the 2010 Deepwater Horizon oil spill, unprecedented numbers of Kemp’s ridley sea turtles (Lepidochelys kempii) stranded on northern Gulf of Mexico beaches and the number of nests recorded on the primary nesting beaches plummeted far below expected levels. High levels of strandings have continued since 2010 and the number of nests recovered to approximately 2009 levels in 2011, and improved slightly in 2012. A stock assessment conducted in 2012 indicated that a mortality event occurred in 2010, and that the number of nests should once more exhibit an increasing trend from 2013 and beyond. This has not happened; rather, the number of nests declined sharply in 2013. We conducted a new stock assessment to evaluate additional scenarios, including 1) three stock-recruitment options; 2) the potential that a new source of ongoing mortality is present; and 3) the potential that the number of nests-per-adult-female is dependent on the size of the age-2+ benthic population. The latter model provided the best fit to the data. Further, the preliminary estimate of actual nesting in 2014 is consistent with model projections. The reduction in reproductive output could be due to the combination of a large population and reduced prey levels. Together these may have increased the remigration interval or reduced the number of nests per female. However, research is needed to evaluate this and other plausible hypotheses. Nesting may be highly variable in the future depending on feeding conditions on the foraging grounds

    Integration of Mirror Design with Suspension System using NASA's New Mirror Modeling Software

    Get PDF
    Advances in mirror fabrication are making very large space based telescopes possible. In many applications, only monolithic mirrors can meet the performance requirements. The existing and near-term planned heavy launch vehicles place a premium on lowest possible mass, and then available payload shroud sizes limit near term designs to 4 meter class mirrors. Practical 8 meter class and beyond designs could encourage planners to include larger shrouds, if it can be proven that such mirrors can be manufactured. These two factors, lower mass and larger mirrors, present the classic optimization problem. There is a practical upper limit to how large of a mirror can be supported by a purely kinematic mount system handling both operational and launch loads. This paper shows how the suspension system and mirror blank need to be designed simultaneously. We will also explore the concepts of auxiliary support systems which act only during launch and disengage on orbit. We will define required characteristics of these systems and show how they can substantially reduce the mirror mass
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