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991.
992.
993.
Landscapes on the edge: examining the role of climatic interactions in shaping coastal watersheds using a coastal–terrestrial landscape evolution model 下载免费PDF全文
Incised coastal gullies (ICGs) are dynamic features found at the terrestrial‐coastal interface. Their geomorphic evolution is driven by the interactions between processes of fluvial knickpoint migration and coastal cliff erosion. Under scenarios of future climate change the frequency and magnitude of the climatological drivers of both terrestrial (fluvial and hillslope) and coastal (cliff erosion) processes are likely to change, with an adjunct impact on these types of coastal features. Here we explore the response of an incised coastal gully to changes in both terrestrial and coastal climate in order to elucidate the key process interactions which drive ICG evolution. We modify an extant landscape evolution model, CHILD, to incorporate processes of soft‐cliff erosion. This modified version, termed the Coastal‐Terrestrial‐CHILD (CT‐CHILD) model, is then employed to explore the interactions between changing terrestrial and coastal driving forces on the future evolution of an ICG found on the south‐west Isle of Wight, UK. It was found that the magnitude and frequency of storm events will play a key role in determining the future trajectory of ICGs, highlighting a need to understand the role of event sequencing in future projections of landscape evolution. Furthermore, synergistic (positive) and antagonistic (negative) interactions were identified between coastal and terrestrial parameters, such as wave height intensity and precipitation duration, which act to modulate the impact of changes in any one parameter. Of note was the role played by wave height intensity in driving coastal erosion, which was found to play a more important role than sea‐level rise in determining rates of coastal erosion. This highlights the need for a greater focus on wave height in studies of soft‐cliff erosion. Copyright © 2014 John Wiley & Sons, Ltd. 相似文献
994.
Alireza Karimzadeh Somarin Stephen A. Kissin Donald D. Heerema Daniel J. Bihari 《Resource Geology》2009,59(2):107-120
The Archean mafic–ultramafic complex of Lac des Iles, Ontario, Canada, hosts economic platinum group elements (PGE)-Au-Cu-Ni mineralization in the Roby Zone. All lithologies in the North Roby Zone have been affected by hydrothermal alteration. The alteration products include talc (the most dominant mineral), anthophyllite, serpentine, actinolite, tremolite, chlorite, hornblende, zoisite, clinozoisite, epidote and sericite. In the altered rocks, light rare earth elements (La, Ce, Nd, Sm), Pb, Rb, Ba, Cs, S and possibly Y have been added by hydrothermal solution whereas Eu and heavy rare earth elements (Yb, Gd, Dy, Er) remained immobile. There are five types of fluid inclusions in the pegmatitic plagioclase with homogenization temperature and salinity ranging from 240°C to 445°C and 15.37 to 48.52 wt% equivalent NaCl, respectively. The δ18 O and δD of talc range form 6.2‰ to 6.9‰ and −28‰ to −48‰, respectively. δ18 O and δD water in equilibrium with talc during the hydrothermal alteration suggest a modified source for the hydrothermal solution. Microthermometry and stable isotope studies suggest that high temperature–high salinity fluid was diluted by, and mixed with, low temperature–low salinity meteoric solution. This mechanism precipitated the hydrothermal assemblage and redistributed trace elements during and after pegmatite formation in the North Ruby Zone. 相似文献
995.
Stephen G. Monismith James L. Hench Derek A. Fong Nicholas J. Nidzieko William E. Fleenor Laura P. Doyle S. Geoffrey Schladow 《Estuaries and Coasts》2009,32(1):100-110
In this paper, we discuss observations of temperature variability in the tidal portion of the San Joaquin River in California.
The San Joaquin River makes up the southern portion of the Sacramento San Joaquin Delta, the eastern end of San Francisco
Bay. Observations made in August 2004 and August 2005 show significant diurnal variations in temperature in response to surface
heat exchange. However, to account for observed changes in heat content a sizeable downstream heat flux (approximately 100 W
m−2) must be added to the surface heat flux. To account for this flux via Fickian dispersion, a flow-dependent dispersion coefficient
varying from 500 to 4,000 m2 s−1 is needed. These values are much larger than would be predicted for a river of this size, suggesting that the complex topology
of the Delta greatly enhances longitudinal dispersion. Building on these observations, we present a simple theory that explores
how the subtidal temperature field varies in response to changes in flow rate, dispersion, and heat exchange. 相似文献
996.
Stephen T. Ross W. Todd Slack Ryan J. Heise Mark A. Dugo Howard Rogillio Bryant R. Bowen Paul Mickle Richard W. Heard 《Estuaries and Coasts》2009,32(2):360-374
Gulf sturgeon are anadromous, spawning in freshwater and returning to the marine environment to feed. Herein, we document
the marine distribution and timing of movement in and out of the marine environment of Gulf sturgeon natal to the Pascagoula
and Pearl rivers (MS and LA). From 1999 to 2004, we attached sonic transmitters to 194 fish averaging 151 (MS) to 160 (LA)
cm in fork length. We located 56 different Gulf sturgeon in the estuarine or marine environments, some multiple times. Fish
were distributed nonrandomly, being found primarily in shallow water (mean = 3.9 m) in barrier island passes. Benthic samples
taken at Gulf sturgeon telemetry location sites were dominated by Florida lancelets, sand dollars, annelids, haustoriid amphipods,
and mollusks—all documented prey of Gulf sturgeon. Movement into salt water consistently occurred in October and November;
movement back into rivers or low salinity estuaries was complete by the end of March. 相似文献
997.
In addition to the previously reported 25-norhopanes and 25-norhopanoic acids, for the first time we report the identification of 25-norbenzohopanes. The hydrocarbon composition of the bitumen from Palaeozoic carbonates in northern Alberta displays molecular evidence for severe levels of biodegradation characterised by the removal of C30–C35 hopanes. Biodegradation is also indicated by the removal of C32 and C33 benzohopanes. The appearance of C31 and C32 25-norbenzohopanes corresponds to the decrease in C32 and C33 benzohopanes, suggesting that 25-norbenzohopanes originate by demethylation of benzohopane counterparts. Demethylation at C-10 in the hopanoids affects a broader class of compounds that so far includes the hopanes and hopanoic acids, as well as the benzylated hopanoid species. 相似文献
998.
999.
Ralph D. Lorenz Rosaly M. Lopes Jonathan I. Lunine Karl L. Mitchell Ellen R. Stofan Melissa Myers Jani Radebaugh Stephen D. Wall the Cassini RADAR Team 《Planetary and Space Science》2008,56(8):1132-1144
Cassini radar images show a variety of fluvial channels on Titan's surface, often several hundreds of kilometers in length. Some (predominantly at low- and mid-latitude) are radar-bright and braided, resembling desert washes where fines have been removed by energetic surface liquid flow, presumably from methane rainstorms. Others (predominantly at high latitudes) are radar-dark and meandering and drain into or connect polar lakes, suggesting slower-moving flow depositing fine-grained sediments. A third type, seen predominantly at mid- and high latitudes, have radar brightness patterns indicating topographic incision, with valley widths of up to 3 km across and depth of several hundred meters. These observations show that fluvial activity occurs at least occasionally at all latitudes, not only at the Huygens landing site, and can produce channels much larger in scale than those observed there. The areas in which channels are prominent so far amount to about 1% of Titan's surface, of which only a fraction is actually occupied by channels. The corresponding global sediment volume inferred is not enough to account for the extensive sand seas. Channels observed so far have a consistent large-scale flow pattern, tending to flow polewards and eastwards. 相似文献
1000.
The flow within a canopy of large bluff bodies is highly turbulent and spatially heterogeneous. Results from direct numerical
simulations over groups of cubical obstacles are analysed using the double-averaging methodology. The obstacles occupy a significant
fraction of the canopy space; this gives rise to substantial dispersive stresses within the canopy. The underlying bluff-body
turbulent dynamics is different from typical canopy turbulence, and this is reflected in the double-averaged statistics. The
spatially-averaged velocities, stresses and drag force depend significantly upon the layout of the obstacles. An ongoing challenge
is to parameterise these spatially-averaged quantities in terms of the obstacle geometry and layout. 相似文献