(Table 1) Physical properties of sediments at DSDP Holes 79-545 and 79-547A

Laboratory measurements of the acoustic and physical properties of deep-sea sediments and rocks are important for the interpretation of seismic reflection and refraction data and estimation of in situ physical property values. Furthermore, the results of such measurements can be used to design geoacoustic models of the upper oceanic crust that can relate the physical properties of deep-sea sediments to lithology, depth of burial, and diagenetic effects (Hamilton, 1980; Milholland et al., 1980). The purpose of this paper is to report the results of laboratory measurements of wet-bulk density, compressionalwave velocity, and velocity anisotropy on sediments cored during DSDP Leg 79. The sample suite consists of 11 calcareous claystones and clay-rich chalks recovered between 370 to 720 m sub-bottom at Holes 545 and 547A.

Temperature measured in permafrost borehole at ICDP site 5011-3 in El'gygytgyn Crater, 2008-2011

This study focuses on the temperature field observed in boreholes drilled as part of interdisciplinary scientific campaign targeting the El'gygytgyn Crater Lake in NE Russia. Temperature data are available from two sites: the lake borehole 5011-1 located near the center of the lake reaching 400 m depth, and the land borehole 5011-3 at the rim of the lake, with a depth of 140 m. Constraints on permafrost depth and past climate changes are derived from numerical simulation of the thermal regime associated with the lake-related talik structure. The thermal properties of the subsurface needed for these simulations are based on laboratory measurements of representative cores from the quaternary sediments and the underlying impact-affected rock, complemented by further information from geophysical logs and data from published literature. The temperature observations in the lake borehole 5011-1 are dominated by thermal perturbations related to the drilling process, and thus only give reliable values for the lowermost value in the borehole. Undisturbed temperature data recorded over more than two years are available in the 140 m deep land-based borehole 5011-3. The analysis of these observations allows determination of not only the recent mean annual ground surface temperature, but also the ground surface temperature history, though with large uncertainties. Although the depth of this borehole is by far too insufficient for a complete reconstruction of past temperatures back to the Last Glacial Maximum, it still affects the thermal regime, and thus permafrost depth. This effect is constrained by numerical modeling: assuming that the lake borehole observations are hardly influenced by the past changes in surface air temperature, an estimate of steady-state conditions is possible, leading to a meaningful value of 14 ± 5 K for the post-glacial warming. The strong curvature of the temperature data in shallower depths around 60 m can be explained by a comparatively large amplitude of the Little Ice Age (up to 4 K), with low temperatures prevailing far into the 20th century. Other mechanisms, like varying porosity, may also have an influence on the temperature profile, however, our modeling studies imply a major contribution from recent climate changes.

(Table 1) Summary of acoustic properties at DSDP Holes 60-453 and 60-459B

Laboratory measurements of physical properties are important because the results may be applied to the interpretation of seismic and other types of geophysical data, and because they can be used to estimate the in situ physical properties of different lithologies present beneath the sea floor. In this chapter, wet-bulk densities and compressional-wave velocities, measured at elevated confining pressures, are reported for a suite of seven sediment samples recovered on DSDP Leg 60. Of the seven samples studied, two are mudstones, two are vitric tuffs, and three are chalks. All but one of the samples are from Hole 459B, near the eastern limit of the Mariana fore-arc region. In five cases, velocities were measured parallel and perpendicular to bedding to test for velocity anisotropy.

Wave-generated flow on coral reefs - an analysis for two-dimensional horizontal reef-tops with steep faces

Waves breaking on the seaward rim of a coral reef generate a flow of water from the exposed side of the reef to the sheltered side and/or to either channels through the reef-rim or lower sections of the latter. This wave-generated flow is driven by the water surface gradient resulting from the wave set-up created by the breaking waves. This paper reviews previous approaches to modelling wave-generated flows across coral reefs and discusses the influence of reef morphology and roughness upon these flows. Laboratory measurements upon a two-dimensional horizontal reef platform with a steep reef face provide the basis for extending a previous theoretical analysis for wave set-up on a reef in the absence of a flow [Gourlay, M.R., 1996b. Wave set-up on coral reefs. 2. Set-up on reefs with various profiles. Coastal Engineering 28, 1755] to include the interaction between a unidirectional flow and the wave set-up. The laboratory model results are then used to demonstrate that there are two basic reef-top flow regimes-reef-top control and reef-rim control. Using open channel flow theory, analytical relationships are derived for the reef-top current velocity in terms of the offreef wave conditions, the reef-top water depth and the physical characteristics of the reef-top topography. The wave set-up and wave-generated flow relationships are found to predict experimental values with reasonable accuracy in most cases. The analytical relationships are used to investigate wave-generated flows into a boat harbour channel on Heron Reef in the southern Great Barrier Reef. (c) 2005 Elsevier B.V. All rights reserved.

Swimming performance of hatchling green turtles is affected by incubation temperature

In an experiment repeated for two separate years, incubation temperature was found to affect the body size and swimming performance of hatchling green turtles (Chelonia mydas). In the first year, hatchlings from eggs incubated at 26 degrees C were larger in size than hatchlings from 28 and 30 degrees C, whilst in the second year hatchlings from 25.5 degrees C were similar in size to hatchings from 30 degrees C. Clutch of origin influenced the size of hatchlings at all incubation temperatures even when differences in egg size were taken into account. In laboratory measurements of swimming performance, in seawater at 28 degrees C, hatchlings from eggs incubated at 25.5 and 26 degrees C had a lower stroke rate frequency and lower force output than hatchlings from 28 and 30 degrees C. These differences appeared to be caused by the muscles of hatchlings from cooler temperatures fatiguing at a faster rate. Clutch of origin did not influence swimming performance. This finding that hatchling males incubated at lower temperature had reduced swimming ability may affect their survival whilst running the gauntlet of predators in shallow near-shore waters, prior to reaching the relative safety of the open sea.

An experimental study of the jet of a boat propeller

An experimental study of the velocity and concentration (scalar) fields of a propeller is presented. Field and laboratory measurements were undertaken. The former were up to 50 diameters downstream. Important findings were that the mean velocity and scalar fields quickly become Gaussian while further downstream they both become irregular sometimes approaching approximately linear profiles. Propeller turbulence causes rapid mixing giving an initial concentration dilution factor of 1/20,000 after fifty propeller diameters. Some preliminary comparisons with field measurements of an actual boat in a natural waterway are made. Considerably more work is needed to gain a full understanding of the complex problem of propeller mixing.

(Table 1) Comparisons of dynamic and static Young's moduli of basalt at DSDP Holes 69-504B, 70-504B and 83-504B

Compressional- and shear-wave velocity logs (Vp and Vs, respectively) that were run to a sub-basement depth of 1013 m (1287.5 m sub-bottom) in Hole 504B suggest the presence of Layer 2A and document the presence of layers 2B and 2C on the Costa Rica Rift. Layer 2A extends from the mudline to 225 m sub-basement and is characterized by compressional-wave velocities of 4.0 km/s or less. Layer 2B extends from 225 to 900 m and may be divided into two intervals: an upper level from 225 to 600 m in which Vp decreases slowly from 5.0 to 4.8 km/s and a lower level from 600 to about 900 m in which Vp increases slowly to 6.0 km/s. In Layer 2C, which was logged for about 100 m to a depth of 1 km, Vp and Vs appear to be constant at 6.0 and 3.2 km/s, respectively. This velocity structure is consistent with, but more detailed than the structure determined by the oblique seismic experiment in the same hole. Since laboratory measurements of the compressional- and shear-wave velocity of samples from Hole 504B at Pconfining = Pdifferential average 6.0 and 3.2 km/s respectively, and show only slight increases with depth, we conclude that the velocity structure of Layer 2 is controlled almost entirely by variations in porosity and that the crack porosity of Layer 2C approaches zero. A comparison between the compressional-wave velocities determined by logging and the formation porosities calculated from the results of the large-scale resistivity experiment using Archie's Law suggest that the velocity- porosity relation derived by Hyndman et al. (1984) for laboratory samples serves as an upper bound for Vp, and the noninteractive relation derived by Toksöz et al. (1976) for cracks with an aspect ratio a = 1/32 serves as a lower bound.

Dynamique de l'oxygène et l'activité microbienne dans les lacs de fonte du pergélisol subarctique

Les lacs de thermokarst (lacs peu profonds créés par le dégel et l’érosion du pergélisol riche en glace) sont un type unique d’écosystèmes aquatiques reconnus comme étant de grands émetteurs de gaz à effet de serre vers l’atmosphère. Ils sont abondants dans le Québec subarctique et ils jouent un rôle important à l’échelle de la planète. Dans certaines régions, les lacs de thermokarst se transforment rapidement et deviennent plus grands et plus profonds. L’objectif de cette étude était d’améliorer la compréhension et d’évaluer quelles variables sont déterminantes pour la dynamique de l’oxygène dans ces lacs. C’est pourquoi j’ai examiné les possibles changements futurs de la dynamique de l’oxygène dans ces lacs dans un contexte de réchauffement climatique. Une grande variété de méthodes ont été utilisées afin de réaliser cette recherche, dont des analyses in situ et en laboratoire, ainsi que la modélisation. Des capteurs automatisés déployés dans cinq lacs ont mesuré l’oxygène, la conductivité et la température de la colonne d’eau en continu de l’été 2012 jusqu’à l’été 2015, à des intervalles compris entre 10 à 60 minutes. Des analyses en laboratoire ont permis de déterminer la respiration et les taux de production bactériens, les variables géochimiques limnologiques, ainsi que la distribution de la production bactérienne entre les différentes fractions de taille des communautés. La température de l’eau et les concentrations d’oxygène dissous d’un lac de thermokarst ont été modélisées avec des données du passé récent (1971) au climat futur (2095), en utilisant un scénario modéré (RCP 4.5) et un scénario plus extrême (RCP 8.5) de réchauffement climatique. Cette recherche doctorale a mis en évidence les conditions anoxiques fréquentes et persistantes présentes dans de nombreux lacs de thermokarst. Aussi, ces lacs sont stratifiés pendant l’hiver comme des concentrations élevées d’ions s’accumulent dans leurs hypolimnions à cause de la formation du couvert de glace (cryoconcentration) et de la libération des ions avec la respiration bactérienne. Les différences de température contribuent également à la stabilité de la stratification. La dynamique de mélange des lacs de thermokarst étudiés était contrastée : la colonne d’eau de certains lacs se mélangeait entièrement deux fois par année, d’autres lacs se mélangeaient qu’une seule fois en automne, alors que certains lacs ne se mélangeaient jamais entièrement. Les populations bactériennes étaient abondantes et très actives, avec des taux respiratoires comparables à ceux mesurés dans des écosystèmes méso-eutrophes ou eutrophes des zones tempérées de l’hémisphère nord. L’érosion des matériaux contenus dans le sol des tourbières pergélisolées procure un substrat riche en carbone et en éléments nutritifs aux populations bactériennes, et ils constituent des habitats propices à la colonisation par des populations de bactéries associées aux particules. Le modèle de la concentration d’oxygène dissous dans un lac a révélé que le réchauffement des températures de l’air pourrait amincir le couvert de glace et diminuer sa durée, intensifiant le transfert de l’oxygène atmosphérique vers les eaux de surface. Ainsi, la concentration en oxygène dissous dans la colonne d’eau de ce lac augmenterait et les périodes de conditions anoxiques pourraient devenir plus courtes. Finalement, cette thèse doctorale insiste sur le rôle des lacs de thermokarst comme des réacteurs biogéochimiques pour la dégradation du carbone organique, qui était retenu dans les sols gelés, en gaz à effet de serre libérés dans l’atmosphère. L’oxygène est un indicateur sensible du mélange de la colonne d’eau et de la dynamique chimique des lacs, en plus d’être une variable clé des processus métaboliques.

Validation of single photon absorptiometry for on-farm measurement of density and mineral content of tail bone in cattle

A validation study examined the accuracy of a purpose-built single photon absorptiometry (SPA) instrument for making on-farm in vivo measurements of bone mineral density (BMD) in tail bones of cattle. In vivo measurements were made at the proximal end of the ninth coccygeal vertebra (Cy9) in steers of two age groups (each n = 10) in adequate or low phosphorus status. The tails of the steers were then resected and the BMD of the Cy9 bone was measured in the laboratory with SPA on the resected tails and then with established laboratory procedures on defleshed bone. Specific gravity and ash density were measured on the isolated Cy9 vertebrae and on 5-mm2 dorso-ventral cores of bone cut from each defleshed Cy9. Calculated BMD determined by SPA required a measure of tail bone thickness and this was estimated as a fraction of total tail thickness. Actual tail bone thickness was also measured on the isolated Cy9 vertebrae. The accuracy of measurement of BMD by SPA was evaluated by comparison with the ash density of the bone cores measured in the laboratory. In vivo SPA measurements of BMD were closely correlated with laboratory measurements of core ash density (r = 0.92). Ash density and specific gravity of cores, and all SPA measures of BMD, were affected by phosphorus status of the steers, but the effect of steer age was only significant (P < 0.05) for steers in adequate phosphorus status. The accuracy of SPA to determine BMD of tail bone may be improved by reducing error associated with in vivo estimation of tail bone thickness, and also by adjusting for displacement of soft tissue by bone mineral. In conclusion a purpose-built SPA instrument could be used to make on-farm sequential non-invasive in vivo measurements of the BMD of tailbone in cattle with accuracy acceptable for many animal studies.

Exploration of Ground Penetrating Radar and Time Domain Reflectometry Methods for the Determination of Pavement Dielectric Constant

Traditionally, densities of newly built roadways are checked by direct sampling (cores) or by nuclear density gauge measurements. For roadway engineers, density of asphalt pavement surfaces is essential to determine pavement quality. Unfortunately, field measurements of density by direct sampling or by nuclear measurement are slow processes. Therefore, I have explored the use of rapidly-deployed ground penetrating radar (GPR) as an alternative means of determining pavement quality. The dielectric constant of pavement surface may be a substructure parameter that correlates with pavement density, and can be used as a proxy when density of asphalt is not known from nuclear or destructive methods. The dielectric constant of the asphalt can be determined using ground penetrating radar (GPR). In order to use GPR for evaluation of road surface quality, the relationship between dielectric constants of asphalt and their densities must be established. Field measurements of GPR were taken at four highway sites in Houghton and Keweenaw Counties, Michigan, where density values were also obtained using nuclear methods in the field. Laboratory studies involved asphalt samples taken from the field sites and samples created in the laboratory. These were tested in various ways, including, density, thickness, and time domain reflectometry (TDR). In the field, GPR data was acquired using a 1000 MHz air-launched unit and a ground-coupled unit at 200 and 500 MHz. The equipment used was owned and operated by the Michigan Department of Transportation (MDOT) and available for this study for a total of four days during summer 2005 and spring 2006. The analysis of the reflected waveforms included “routine” processing for velocity using commercial software and direct evaluation of reflection coefficients to determine a dielectric constant. The dielectric constants computed from velocities do not agree well with those obtained from reflection coefficients. Perhaps due to the limited range of asphalt types studied, no correlation between density and dielectric constant was evident. Laboratory measurements were taken with samples removed from the field and samples created for this study. Samples from the field were studied using TDR, in order to obtain dielectric constant directly, and these correlated well with the estimates made from reflection coefficients. Samples created in the laboratory were measured using 1000 MHz air-launched GPR, and 400 MHz ground-coupled GPR, each under both wet and dry conditions. On the basis of these observations, I conclude that dielectric constant of asphalt can be reliably measured from waveform amplitude analysis of GJPR data, based on the consistent agreement with that obtained in the laboratory using TDR. Because of the uniformity of asphalts studied here, any correlation between dielectric constant and density is not yet apparent.

La datation du site Mailhot-Curran : application de la luminescence optique sur des poteries iroquoiennes du Saint-Laurent

La luminescence optique (OSL) a été mesurée sur dix-sept fragments de poterie collectés à Mailhot-Curran (BgFn-2), un site archéologique du Sylvicole supérieur tardif localisé dans le sud-ouest du Québec. Le but principal de ce projet était de dater ce site qui est considéré jusqu’à maintenant comme le plus récent site préhistorique de la concentration de Saint-Anicet, afin de poser un jalon dans la chronologie des sites de cette région. L’OSL a été utilisée conjointement à la datation par radiocarbone (14C) et la sériation du matériel archéologique. L’hypothèse archéologique propose que le village aurait été occupé pendant les années 1518 à 1530 de notre ère (Chapdelaine 2015a). Les résultats que nous proposons dans ce présent mémoire appuient cette proposition. Nous avons obtenu un âge de 490 ± 49 ans (année de référence : 2013), correspondant à l’année 1523 de notre ère avec une probabilité d’occupation du site Mailhot-Curran entre les années 1474 et 1572. Le programme de datation par luminescence optique a été réalisé sur des fragments de poterie domestique composés d’argile de la Mer de Champlain datant de la période du Quaternaire récent. La datation par stimulation infrarouge (IRSL) a été préférentiellement utilisée sur des aliquotes de grains fins polyminéraliques. Pour la détermination des doses équivalentes, un protocole SAR (Murray et Wintle 2000) modifié pour la mesure des feldspaths et incluant un lessivage optique a été utilisé (Lamothe et al. 2004). Les valeurs g ont été mesurées en suivant le protocole proposé par Auclair et al. (2003). La correction de Huntley et Lamothe (2001) a été utilisée afin de corriger les doses équivalentes mesurées pour la décroissance anormale du signal feldspathique. Les doses annuelles ont pour leur part été déterminées par des mesures réalisées in situ et en laboratoire. Les résultats que nous présentons dans ce mémoire sont affectés par une dispersion assez large. Cette variabilité a été prise en compte par des méthodes statistiques pour la détermination de l’âge probable de l’occupation du site Mailhot-Curran.

La datation du site Mailhot-Curran : application de la luminescence optique sur des poteries iroquoiennes du Saint-Laurent

La luminescence optique (OSL) a été mesurée sur dix-sept fragments de poterie collectés à Mailhot-Curran (BgFn-2), un site archéologique du Sylvicole supérieur tardif localisé dans le sud-ouest du Québec. Le but principal de ce projet était de dater ce site qui est considéré jusqu’à maintenant comme le plus récent site préhistorique de la concentration de Saint-Anicet, afin de poser un jalon dans la chronologie des sites de cette région. L’OSL a été utilisée conjointement à la datation par radiocarbone (14C) et la sériation du matériel archéologique. L’hypothèse archéologique propose que le village aurait été occupé pendant les années 1518 à 1530 de notre ère (Chapdelaine 2015a). Les résultats que nous proposons dans ce présent mémoire appuient cette proposition. Nous avons obtenu un âge de 490 ± 49 ans (année de référence : 2013), correspondant à l’année 1523 de notre ère avec une probabilité d’occupation du site Mailhot-Curran entre les années 1474 et 1572. Le programme de datation par luminescence optique a été réalisé sur des fragments de poterie domestique composés d’argile de la Mer de Champlain datant de la période du Quaternaire récent. La datation par stimulation infrarouge (IRSL) a été préférentiellement utilisée sur des aliquotes de grains fins polyminéraliques. Pour la détermination des doses équivalentes, un protocole SAR (Murray et Wintle 2000) modifié pour la mesure des feldspaths et incluant un lessivage optique a été utilisé (Lamothe et al. 2004). Les valeurs g ont été mesurées en suivant le protocole proposé par Auclair et al. (2003). La correction de Huntley et Lamothe (2001) a été utilisée afin de corriger les doses équivalentes mesurées pour la décroissance anormale du signal feldspathique. Les doses annuelles ont pour leur part été déterminées par des mesures réalisées in situ et en laboratoire. Les résultats que nous présentons dans ce mémoire sont affectés par une dispersion assez large. Cette variabilité a été prise en compte par des méthodes statistiques pour la détermination de l’âge probable de l’occupation du site Mailhot-Curran.

The spectral albedo of sea ice and salt crusts on the tropical ocean of Snowball Earth: II. Optical modeling

During the Snowball Earth events of the Neoproterozoic, tropical regions of the ocean could have developed a precipitated salt lag deposit left behind by sublimating sea ice. The major salt would have been hydrohalite, NaCl•2H2O. The crystals in such a deposit can be small and highly scattering, resulting in an allwave albedo similar to that of snow. The snow-free sea ice from which such a crust could develop has a lower albedo, around 0.5, so the development of a crust would substantially increase the albedo of tropical regions on Snowball Earth. Hydrohalite crystals are much less absorptive than ice in the near- infrared part of the solar spectrum, so their presence at the surface would increase the overall albedo as well as altering its spectral distribution. In this paper, we use laboratory measurements of the spectral albedo of a hydrohalite lag deposit, in combination with a radiative transfer model, to infer the inherent optical properties of hydrohalite as functions of wavelength. Using this result, we model mixtures of hydrohalite and ice representing both artificially created surfaces in the laboratory and surfaces relevant to Snowball Earth. The model is tested against sequences of laboratory measurements taken during the formation and the dissolution of a lag deposit of hydrohalite. We present a parameterization for the broadband albedo of cold, sublimating sea ice as it forms and evolves a hydrohalite crust, for use in climate models of Snowball Earth.