Field Test of Enhanced Remedial Amendment Delivery Using a Shear‐Thinning Fluid

Heterogeneity of hydraulic properties in aquifers may lead to contaminants residing in lower‐permeability zones where it is difficult to deliver remediation amendments using conventional injection processes. The focus of this study is to examine use of a shear‐thinning fluid (STF) to improve the uniformity of remedial amendment distribution within a heterogeneous aquifer. Previous studies have demonstrated the significant potential of STFs for improving remedial amendment delivery in heterogeneous aquifers, but quantitative evaluation of these improvements from field applications is lacking. A field‐scale test was conducted that compares data from successive injection of a tracer in water followed by injection of a tracer in an STF to evaluate the impact of the STF on tracer distribution uniformity in the presence of permeability contrasts within the targeted injection zone. Data from tracer breakthrough at multiple depth‐discrete monitoring intervals and electrical resistivity tomography (ERT) showed that inclusion of STF in the injection solution improved the distribution of the injected fluid within the targeted treatment zone. One improvement was a reduction in the movement of injected fluids through high‐permeability pathways, as evidenced by slower breakthrough of tracer at monitoring locations where breakthrough in baseline tracer‐only injection data was faster. In addition, STF‐amended injection solutions arrived faster and to a greater extent in monitoring locations within low‐permeability zones. ERT data showed that the STF injection covered a higher percentage of a two‐dimensional cross section within the injection interval between the injection well and a monitoring well about 3 m away.     

Geometry and architecture of faults in a syn-rift normal fault array: The Nukhul half-graben, Suez rift, Egypt

The geometry and architecture of a well exposed syn-rift normal fault array in the Suez rift is examined. At pre-rift level, the Nukhul fault consists of a single zone of intense deformation up to 10 m wide, with a significant monocline in the hanging wall and much more limited folding in the footwall. At syn-rift level, the fault zone is characterised by a single discrete fault zone less than 2 m wide, with damage zone faults up to approximately 200 m into the hanging wall, and with no significant monocline developed. The evolution of the fault from a buried structure with associated fault-propagation folding, to a surface-breaking structure with associated surface faulting, has led to enhanced bedding-parallel slip at lower levels that is absent at higher levels. Strain is enhanced at breached relay ramps and bends inherited from pre-existing structures that were reactivated during rifting. Damage zone faults observed within the pre-rift show ramp-flat geometries associated with contrast in competency of the layers cut and commonly contain zones of scaly shale or clay smear. Damage zone faults within the syn-rift are commonly very straight, and may be discrete fault planes with no visible fault rock at the scale of observation, or contain relatively thin and simple zones of scaly shale or gouge. The geometric and architectural evolution of the fault array is interpreted to be the result of (i) the evolution from distributed trishear deformation during upward propagation of buried fault tips to surface faulting after faults breach the surface; (ii) differences in deformation response between lithified pre-rift units that display high competence contrasts during deformation, and unlithified syn-rift units that display low competence contrasts during deformation, and; (iii) the history of segmentation, growth and linkage of the faults that make up the fault array. This has important implications for fluid flow in fault zones.     

Sr–Nd isotope geochemistry of the early Precambrian sub-alkaline mafic igneous rocks from the southern Bastar craton, Central India

Sr–Nd isotope data are reported for the early Precambrian sub-alkaline mafic igneous rocks of the southern Bastar craton, central India. These mafic rocks are mostly dykes but there are a few volcanic exposures. Field relationships together with the petrological and geochemical characteristics of these mafic dykes divide them into two groups; Meso-Neoarchaean sub-alkaline mafic dykes (BD1) and Paleoproterozoic (1.88 Ga) sub-alkaline mafic dykes (BD2). The mafic volcanics are Neoarchaean in age and have very close geochemical relationships with the BD1 type. The two groups have distinctly different concentrations of high-field strength (HFSE) and rare earth elements (REE). The BD2 dykes have higher concentrations of HFSE and REE than the BD1 dykes and associated volcanics and both groups have very distinctive petrogenetic histories. These rocks display a limited range of initial ¹⁴³Nd/¹⁴⁴Nd but a wide range of apparent initial ⁸⁷Sr/⁸⁶Sr. Initial ¹⁴³Nd/¹⁴⁴Nd values in the BD1 dykes and associated volcanics vary between 0.509149 and 0.509466 and in the BD2 dykes the variation is between 0.510303 and 0.510511. All samples have positive ? _Nd values; the BD1 dykes and associated volcanics have ? _Nd values between +0.3 and +6.5 and the BD2 dykes between +1.9 to +6.0. Trace element and Nd isotope data do not suggest severe crustal contamination during the emplacement of the studied rocks. The positive ? _Nd values suggest their derivation from a depleted mantle source. Overlapping positive ? _Nd values suggest that a similar mantle source tapped by variable melt fractions at different times was responsible for the genesis of BD1 (and associated volcanics) and BD2 mafic dykes. The Rb–Sr system is susceptible to alteration and resetting during post-magmatic alteration and metamorphism. Many of the samples studied have anomalous apparent initial ⁸⁷Sr/⁸⁶Sr suggesting post-magmatic changes of the Rb–Sr system which severely restricts the use of Rb–Sr for petrogenetic interpretation.     

Microseismicity and structure of the Germencik area, western Turkey

Microseismicity at the boundary between two segments of the Büyük Menderes active normal fault zone, western Turkey, was monitored for two weeks during 1990 April and May, using a dense network of six portable seismographs with spacing ∼1–2 km. Extension rate across this fault zone is investigated by three independent methods; our preferred estimate is 1.2 ± 0.4 mm yr⁻¹. The area contains a geothermal field, but microseismicity appears unrelated to geothermal well positions and was thus lower than expected; six local events were recorded, none larger than magnitude 2. Microearthquakes in this size range contribute negligibly to local tectonic deformation. However, frequency of occurrence of these and local magnitude 7 events both satisfy the standard Gutenberg-Richter relationship. The local geomorphology includes an example of river capture associated with elevation changes accompanying changing patterns of slip on individual fault segments, which appears to have occurred less than 1 Myr ago.     

A study of the long-term behaviour patterns of the variation of the emission lines in the spectra of some Be type stars

The ratio of the line intensity to that of the nearby continuum for an emission line, has been derived from objective prism spectra taken, at the Norman Lockyer Observatory, over the period, 1914 to 1959, for six stars ( Cassiopeia, and Persei, HD 20336, 25 Orionis, Piscium). This has been combined with information already in the literature, to study the long-period behaviour of the stars. Long-term variations have been looked for, and it is found that, with the exception of one of the stars which is a spectroscopic binary, the variations tend to occur in outbursts which may last for 10 to 20 years, and which may show signs of semi-regular periodicities during the outburst.It is suggested, that while no stable long-term periodicities have been found, the outbursts may recur after long intervals, and that this possibility is demonstrated by one of these stars ( Cassiopeia). It is also suggested that the semi-regular variations that occur during some of the outbursts may be ralated to an intrinsic cycle connected with the surface of the star, and possibly akin to the solar sunspot cycle. Top: Far-encounter picture (No. 73) of Mars, taken by the Mariner 7 spacecraft on 4 August 1969 from a distance of 471 750 km from the planet.Bottom: Near-encounter picture (No. 21) of Mars, taken by Mariner 6 on 30 July 1969 at the time of its closest approach to the surface of the planet. The size of the field is approximately 690×890 km on the Martian surface This photograph recorded more than 100 individual craters, the largest of which is about 260 km in diameter.Reproduced by courtesy of the Jet Propulsion Laboratory, California Institute of Technology.     

Turbulence statistics of a Kelvin–Helmholtz billow event observed in the night-time boundary layer during the Cooperative Atmosphere–Surface Exchange Study field program

An apparent shear flow instability occurred in the stably stratified night-time boundary layer on 6 October 1999 over the Cooperative Atmosphere–Surface Exchange Study (CASES-99) site in southeast Kansas. This instability promoted a train of billows which appeared to be in different stages of evolution. Data were collected by sonic anemometers and a high-frequency thermocouple array distributed on a 60 m tower at the site, and a high resolution Doppler lidar (HRDL), situated close to the tower. Data from these instruments were used to analyze the characteristics of the instability and the billow event. The instability occurred in a layer characterized by a minimum Richardson number Ri0.13, and where an inflection in the background wind profile was also documented. The billows, which translated over the site for approximately 30 min, were approximately L320 m in length and, after billow evolution they were contained in a layer depth H30 m. Their maximum amplitude, determined by HRDL data, occurred at a height of 56 m. Billow overturns, responsible for mixing of heat and momentum, and high-frequency intermittent turbulence produce kurtosis values above the Gaussian value of 3, particularly in the lower part of the active layer.     

Stratigraphic and structural expression of the lateral growth of thrust fault-propagation folds: results and implications from kinematic modelling

In order to better understand the development of thrust fault‐related folds, a 3D forward numerical model has been developed to investigate the effects that lateral slip distribution and propagation rate have on the fold geometry of pre‐ and syn‐tectonic strata. We consider a fault‐propagation fold in which the fault propagates upwards from a basal decollement and along‐strike normal to transport direction. Over a 1 Ma runtime, the fault reaches a maximum length of 10 km and accumulates a maximum displacement of 1 km. Deformation ahead of the propagating fault tip is modelled using trishear kinematics while backlimb deformation is modelled using kink‐band migration. The applicability of two different lateral slip distributions, namely linear‐taper and block‐taper, are firstly tested using a constant lateral propagation rate. A block‐taper slip distribution replicates the geometry of natural fold‐thrusts better and is then used to test the sensitivity of thrust‐fold morphology to varied propagation rates in a set of fault‐propagation folds that have identical final displacement to length (D_max/L_max) ratios. Two stratigraphic settings are considered: a model in which background sedimentation rates are high and no topography develops, and a model in which a topographic high develops above the growing fold and local erosion, transport and deposition occur. If the lateral propagation rate is rapid (or geologically instantaneous), the fault tips quickly become pinned as the fault reaches its maximum lateral extent (10 km), after which displacement accumulates. In both stratigraphic settings, this leads to strike‐parallel rotation of the syn‐tectonic strata near the fault tips; high sedimentation rates relative to rates of uplift result in along‐strike thinning over the structural high, while low sedimentation rates result in pinchout against it. In contrast, slower lateral propagation rates (i.e. up to one order of magnitude greater than slip rate) lead to the development of along‐strike growth triangles when sedimentation rates are high, whereas when sedimentation rates are low, offflap geometries result. Overall we find that the most rapid lateral propagation rates produce the most realistic geometries. In both settings, time‐equivalent units display both nongrowth and growth stratal geometries along‐strike and the transition from growth to nongrowth has the potential to delineate the time of fault/fold growth at a given location. This work highlights the importance of lateral fault‐propagation and fault tip pinning on fault and fold growth in three dimensions and the complex syn‐tectonic geometries that can result.     

Normal fault growth and early syn-rift sedimentology and sequence stratigraphy: Thal Fault, Suez Rift, Egypt

This paper investigates the tectono‐stratigraphic development of a major, segmented rift border fault (Thal Fault) during ca. 6 Myr of initial rifting in the Suez Rift, Egypt. The Thal Fault is interpreted to have evolved by the progressive linkage of at least four fault segments. We focus on two contrasting structural settings in its hangingwall: Gushea, towards the northern tip of the fault, and Musaba Salaama, ca. 20 km along‐strike to the south, towards the centre of the fault. The early syn‐rift stratigraphic succession passes upwards from continental facies, through a condensed marginal marine shell‐rich facies, into fully marine shoreface sandstone and offshore mudstone. Regionally correlatable stratal surfaces within this succession define time‐equivalent stratal units that exhibit considerable along‐strike variability in thickness and facies architecture. During the initial ca. 6 Myr of rifting, the thickest stratigraphy developed towards the centre of the array of fault segments that subsequently hard linked to form the Thal Fault. Thus, a displacement gradient existed between fault segments at the centre and tip of the fault array, suggesting that the fault segments interacted, and a fixed length was established for the fault array, at an early stage in rifting. Towards the centre of the Thal Fault the early syn‐rift succession shows pronounced thickening away from the fault and towards a series of intra‐block antithetic faults that were active for up to ca. 6 Myr. This indicates that a large proportion of fault‐controlled subsidence during the initial ca. 6 Myr of rifting occurred in the hangingwalls of antithetic intra‐block faults, and not the present‐day Thal Fault. The antithetic faults progressively switched off during rifting such that after ca. 6 Myr of rifting, fault‐activity had localised on the Thal Fault enabling it to accrue to the present‐day high level of displacement. Aspects of the development of the Thal Fault appear to be in contrast to many models of fault evolution that predict large‐displacement rift‐climax faults to have always had the greatest displacement during fault population evolution. This study has implications for tectono‐stratigraphic development during early rift basin evolution. In particular, we stress that caution must be taken when relating final rift‐climax fault structure to the early tectono‐stratigraphy, as these may differ considerably.