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61.
Harlan D. Shannon George S. Young Michael A. Yates Mark R. Fuller William S. Seegar 《Boundary-Layer Meteorology》2002,104(2):167-199
An examination of boundary-layer meteorological and avian aerodynamic theories suggests that soaring birds can be used to measure the magnitude of vertical air motions within the boundary layer. These theories are applied to obtain mixed-layer normalized thermal updraft intensity over both flat and complex terrain from the climb rates of soaring American white pelicans and from diagnostic boundary-layer model-produced estimates of the boundary-layer depth zi and the convective velocity scale w*. Comparison of the flatland data with the profiles of normalized updraft velocity obtained from previous studies reveals that the pelican-derived measurements of thermal updraft intensity are in close agreement with those obtained using traditional research aircraft and large eddy simulation (LES) in the height range of 0.2 to 0.8 zi. Given the success of this method, the profiles of thermal vertical velocity over the flatland and the nearby mountains are compared. This comparison shows that these profiles are statistically indistinguishable over this height range, indicating that the profile for thermal updraft intensity varies little over this sample of complex terrain. These observations support the findings of a recent LES study that explored the turbulent structure of the boundary layer using a range of terrain specifications. For terrain similar in scale to that encountered in this study, results of the LES suggest that the terrain caused less than an 11% variation in the standard deviation of vertical velocity. 相似文献
62.
Jerry Shannon Mathew E. Hauer Alexis Weaver Sarah Shannon 《The Professional geographer》2018,70(1):84-93
Although general patterns of food insecurity in the United States are known, few studies have attempted to estimate small area food security or account for ongoing socioeconomic changes. Here we address these issues by producing small area estimates of food insecurity in the Atlanta metropolitan area using two methodologies: fixed effects modeling and demographic metabolism. In both cases, we use county-level data from the Current Population Survey to determine the association between food insecurity and demographic predictors. These associations are then applied to tract-level data from the 2009 to 2013 American Community Survey and projected data for 2020 to create small area estimates of food insecurity. We find broad consensus between our two methods. For both time periods, food insecurity is highest in southern sections of the city of Atlanta and its neighboring suburbs. Projections to 2020, however, show that food insecurity rates are projected to increase in outer-ring suburbs east and west of the city while decreasing in the urban core. These results highlight the need to further adapt antihunger efforts for often sprawling suburban communities, where poverty rates are increasing but spatial mismatch combined with poor transit access might hinder access to food assistance. 相似文献
63.
Paquin Jean-Philippe Lu Youyu Taylor Stephanne Blanken Hauke Marcotte Guillaume Hu Xianmin Zhai Li Higginson Simon Nudds Shannon Chanut Jérôme Smith Gregory C. Bernier Natacha Dupont Frédéric 《Ocean Dynamics》2020,70(3):365-385
Ocean Dynamics - In the context of Canada’s Ocean Protection Plan (OPP), improved coastal and near-shore modelling is needed to enhance marine safety and emergency response capacity in the... 相似文献
64.
Shannon Gore J. Andrew G. Cooper Derek W.T. Jackson Lianna Jarecki 《地球表面变化过程与地形》2019,44(9):1860-1875
Beaches of tropical island coasts exhibit high levels of diversity in composition and form in comparison with their continental counterparts. To investigate the nature and origin of this diversity, individual beach morphology and sedimentology was investigated in the British Virgin Islands (BVI), a Caribbean archipelago of > 60 high volcanic and low reef islands. The islands exhibit a diversity of orientations (some facing the Atlantic and some the Caribbean), elevation and gradient, rock type and wave energy. An examination of 100 beaches in the archipelago revealed a first-order division into sand (70 beaches) and coral rubble (30 beaches). These beaches occur in seven planform types (determined by the antecedent geological framework) and are further subdivided according to shoreface type (seagrass, sandy shoreface, or reef). Mainland-attached headland-embayment beaches are the most common form of sand beach while coral rubble beaches usually occur as barriers that enclose salt ponds and wetlands. Among sand beaches, carbonate content is greatest on Atlantic-facing beaches, and coral rubble beaches are more common on Caribbean-facing beaches. Grain size characteristics on sandy beaches are highly variable and range from fine to very coarse sands while coral rubble beaches range up to boulder-sized clasts. The local source material is a primary determinant of sediment composition. The local factors such as the underlying geology, source and availability of sediments are the primary determinants of beach form, composition and texture in the BVI. Oceanographic and climatic conditions such as the prevailing easterly trade winds and waves which seasonally range in direction from east-northeast to southeast as well as beach orientation to Atlantic- or Caribbean-facing waves also contribute to the variability, but in a secondary role. © 2019 John Wiley & Sons, Ltd. 相似文献
65.
Loren W. Acton 《Solar physics》2018,293(10):137
We present a new derivation of the X-ray spectral sensitivity of the Soft X-ray Telescope (SXT) experiment onboard Yohkoh. The recalibration is based upon the hypothesis that, during the first 15 months of the mission, an absorbing material gradually built up on the entrance filters of the telescope. We have also re-evaluated the times and sizes of ruptures of the SXT entrance filters. The impact of this recalibration on derived filter-ratio temperature, emission measure, and calculated spectral irradiance is substantial, especially for SXT data prior to November 1992. 相似文献
66.
We examine the nature of the surface layer in Gale Crater as determined from high-resolution thermal and visible Mars Odyssey Thermal Emission Imaging System (THEMIS) data as well as how our conclusions compare to past analyses. At THEMIS resolution, the thermal surface structure is dominated by local control, thus providing us with detailed images that contain thermophysical information as well. Using these data sets we have created a map of the area, defining units based primarily on their geomorphology as determined from the daytime thermal and visible images and then using the nighttime thermal data to interpret the nature of the surface layer within each unit. Seven units have been defined: (i) partially blanketed knobby plateaus, (ii) crater walls with terrain similar to that on the plateaus on the upper half and exposed, rocky surfaces on the lower half, (iii)-(v) three floor units with varying combinations of bedrock and indurated and/or particulate deposits, (vi) sand sheets, and (vii) a central mound, consisting of indurated and/or rocky material forming layers, terraces, and slides, covered by particulate material that tapers in thickness downslope. Additionally, dozens of channels have been observed on the crater walls and central mound. The results indicate that aeolian processes have played a major role in shaping much of the present surface layer within Gale and may still be active today. Because of the dramatic size and structure of Gale, the winds are most likely controlled by the local topography. Additionally, the presence and frequency of channels within Gale bolster hypotheses involving aqueous episodes in the history of the crater. 相似文献
67.
The margins of the deep-water sedimentary basins west of Ireland contain a number of large clusters (provinces) of spectacular
carbonate mounds and build-ups. These basins have a complex development history involving the interplay of rift tectonics,
thermal subsidence, igneous activity and oceanographic variations. The Porcupine and Rockall basins both rest upon thin continental
crust, the consequence of major rift episodes in Permo-Triassic, Late Jurassic and Early Cretaceous times. Phases of volcanism
occurred in the Early Cretaceous and especially in the Early Cenozoic. Fluid flow within the basins is likely to have been
controlled by the overall basin geometry and by the distribution and linkage of permeable strata with fault systems, stratal
surfaces and unconformities. A number of regional unconformities, controlled by both basin tectonic and regional oceanographic
effects, can be mapped and correlated throughout the Porcupine and Rockall basins. The youngest of these unconformities (C10:
Early Pliocene) can be traced throughout much of the NW European Atlantic margin. It forms the horizon on which virtually
all the carbonate mounds in the basins develop, suggesting a geologically instantaneous mound nucleation and growth event.
Although the control on their development is uncertain, the mound clusters show a spatial association with lithified strata,
buried contourite and deltaic deposits, slope failure features and with the basin margins. Analysis of these relationships
points to a combination of geological and oceanographic processes controlling mound initiation and growth. 相似文献
68.
The Magellan mound province in the Porcupine Basin 总被引:5,自引:0,他引:5
V. A. I. Huvenne W. R. Bailey P. M. Shannon J. Naeth R. di Primio J. P. Henriet B. Horsfield H. de Haas A. Wheeler K. Olu-Le Roy 《International Journal of Earth Sciences》2007,96(1):85-101
The Magellan mound province is one of the three known provinces of carbonate mounds or cold-water coral banks in the Porcupine
Seabight, west of Ireland. It has been studied in detail using a large and varied data set: 2D and 3D seismic data, sidescan
sonar imagery and video data collected during ROV deployment have been used to describe the mounds in terms of origin, growth
processes and burial. The aim of this paper is to present the Magellan mounds and their setting in an integrated, holistic
way.
More than 1,000 densely spaced and mainly buried mounds have been identified in the area. They all seem to be rooted on one
seismic reflection, suggesting a sudden mound start-up. Their size and spatial distribution characteristics are presented,
together with the present-day appearance of the few mounds that reach the seabed. The underlying geology has been studied
by means of fault analysis and numerical basin modelling in an attempt to identify possible hydrocarbon migration pathways
below or in the surroundings of the Magellan mounds.
Although conclusive evidence concerning the processes of mound initiation proves to be elusive, the results of both fault
analysis and 2D numerical modelling failed to identify, with confidence, any direct pathways for focused hydrocarbon flow
to the Magellan province. Diffuse seepage however may have taken place, as drainage area modelling suggests a possible link
between mound position and structural features in the Hovland-Magellan area. During mound development and growth, the interplay
of currents and sedimentation seems to have been the most important control. Mounds which could not keep pace with the sedimentation
rates were buried, and on the few mounds which maintained growth, only a few corals survive at present. 相似文献
69.
70.