Pressure--Temperature--Time Paths of Regional Metamorphism II. Their Inference and Interpretation using Mineral Assemblages in Metamorphic Rocks

A companion paper (England & Thompson, 1984a) investigatesthe pressure-temperature-time (PTt) paths followed by rocksundergoing burial metamorphism in continental thickening events.This paper discusses problems involved in inferring such pathsfrom the petrological data available in metamorphic rocks and—oncesuch paths are determined—how they may be interpretedin terms of the thermal budgets of metamorphism. Each of theprincipal facies series (glaucophane-jadeite, andalusite- sillimaniteand kyanite-sillimanite) may be encountered by rocks involvedin the thickening and erosion of continental crust in a regimeof average continental heat flow. The inference of a minimumthermal budget required for a given metamorphism depends stronglyon a knowledge of the PTt paths followed by rocks during themetamorphism. Discrimination between possible thermal regimesis greatly enhanced if portions of PTt paths, rather than singlePT points, are available, and additional constraint is possibleif these paths are supplemented by geochronological, structuraland heat flow data.     

Block and boulder accumulations along the coastline between Fins and Sur (Sultanate of Oman): tsunamigenic remains?

The rocky coastline of the Sultanate of Oman between Fins and Sur is decorated by a number of large blocks and boulder accumulations forming ramparts. The blocks occur as individual rocks of up to 40 tons, as imbricated sets and as ??boulder trains.?? Landward, the deposits change into a sand/boulder mixture and distal into sands. The coast is made up of Tertiary folded limestones and beach rock of Quaternary age, both also constitute the megaclasts. The transport distance from the fractured seaward platform of 6?C10?m above mean sea level varies between 20?m and more than 50?m. We found individual blocks of recent corals and overturned blocks with attached oysters and rock pools. Terrestrial laser scanning was used to analyze geomorphologic features as well as for volumetric estimates of the block weights. Tropical cyclones such as Gonu in 2007 or Phet in 2010 are known to have affected Oman??s coastline in the past. The coastal changes during recent cyclones were minor; therefore, we interpret the block deposits as tsunamigenic. However, this interpretation is not unambiguous. The most likely source area for a tsunami is seen in the Makran Subduction Zone situated in the northern Indian Ocean. Here, at least 4?C5 tsunamigenic earthquakes are documented.     

西藏安多剖面沉积物粒度特征及环境意义

对西藏安多剖面的3个层位沉积物与两个现代流动沙丘表层沉积物粒度组成、传统粒度参数及体积分维值进行了对比分析,探讨其粒度特征以及环境指示意义。结果表明：安多剖面的3层代表了3个不同的气候阶段,第一层（0～172 cm）沉积动力为风,其中在0.44～1.08 m深度处是一次风力加强的阶段,第二层（172～224 cm）、第三层（224～232 cm）均在6 Φ附近出现次峰,悬浮组分明显增加,推断为远距离输送的粉砂级颗粒沉降,表明这两个阶段风力有所减弱;安多剖面颗粒比研究区现代流动沙丘颗粒细,表明剖面可能为固定或半固定沙丘沉积;本研究区样品的体积分维值在0.215～1.77,虽然没有实际的物理意义,但作为粒度参数指标,在指示环境变化上是有效的,并且与粘粒、粉砂含量呈现明显的正相关关系,与细砂呈现明显的负相关关系。     

Mechanical shaking and soil water affect the growth of Psammochloa villosa in the Mu Us Sandland

The Mu Us Sandland is basically characterized by water shortage and high wind. Thus, wind-induced mechanical perturbation (MP) and soil water availability are likely to interact to affect plant growth. Since high water availability and MP can induce responses that are in the opposite direction, we hypothesized that MP effects on perennial grasses might be mitigated by increased soil water availability in the Mu Us Sandland. We counducted an experiment in which seedlings of Psammochloa villosa were subjected to two levels of MP (non-MP vs. MP 1 min d⁻¹) and two levels of water availability (200 ml d⁻¹vs. 400 ml d⁻¹) and measured three plant traits. MP significantly decreased plant height, total biomass, and root/shoot ratio. There were significant interactions between MP and soil water availability on plant height and root/shoot ratio. These findings imply that MP alone is a stressful factor for P. villosa and MP effects on its growth can be partially mitigated by increased soil water availability, and also suggest that P. villosa may respond to MP in a way that allows plants to survive in the windy semiarid environments.     

The unusual X-ray light curve of GRB 080307: the onset of the afterglow?

Swift -detected GRB 080307 showed an unusual smooth rise in its X-ray light curve around 100 s after the burst, at the start of which the emission briefly softened. This 'hump' has a longer duration than is normal for a flare at early times and does not demonstrate a typical flare profile. Using a two-component power-law-to-exponential model, the rising emission can be modelled as the onset of the afterglow, something which is very rarely seen in Swift -X-ray light curves. We cannot, however, rule out that the hump is a particularly slow early-time flare, or that it is caused by upscattered reverse shock electrons.     

Coordinated Study on Solar Wind Turbulence During the Venus-Express, ACE and Ulysses Alignment of August 2007

At the end of August 2007, Venus, Earth and Ulysses were aligned within a few degrees. This unusual event gives the opportunity to attempt a coordinated study on the radial evolution of solar wind turbulence and coronal transients like CMEs between 0.7 and 1.4 AU. Interplanetary magnetic field data and moments of proton velocity distribution function such as density, speed and temperature are required for this programme and will be provided by ACE at Earth, Venus Express at Venus and Ulysses at 1.4 AU. This project has been recently proposed as a Coordinated Investigation Programme (CIP35) for the International Heliophysical Year.     

Chromite growth,dissolution and deformation from a morphological view point: SEM investigations

The SEM investigations on some chromite crystals show significant morphological differences between cumulate chromites (from stratiform complexes and from ophiolites) and chromites from podiform deposits (ophiolites). The later exhibit a rounded habit and abundant pits which are both the result of dissolution processes. Accordingly, the interpretation of the silicate inclusions within these chromites and the interpretration of the trace-elements distribution need great care. The nodules, a typical structure of the podiform chromites, are explained by a magmatic growth followed by a progressive recrystallization. The accessory chromites which define the mineral lineation in the tectonite peridotites from ophiolites have been deformed by processes of intracrystalline gliding, stretching and dissolution. In the harzburgites, the orthopyroxene has progressively exsolved at sub-solidus (symplektites) vermicular to massive chromite displaying euhedral forms. In the dunitic lenses, the idiomorphic chromites which are aligned parallel to the lineation may have also recrystallized in a solid state.     

Thermal modelling of magmatic intrusions in the Gjallar Ridge, Norwegian Sea: implications for vitrinite reflectance and hydrocarbon maturation

Extensive magmatic activity took place in the Vøring Basin, offshore Norway, related to the Early Cenozoic rifting. The break‐up of the North‐Atlantic at the Palaeocene–Eocene transition induced strong volcanism. There are numerous magmatic sills below 3 km depth in the area. They are predominantly layer parallel and thin compared with their lateral extent. Igneous intrusions, sills and dykes affected the temperature history, and thus need to be taken into account in petroleum prospect analysis. We have calculated the temperature and maturity effects in the sedimentary layers in the Gjallar area associated with the emplacement of single sill and sill complexes. A 120‐m‐thick sill produces a theoretical vitrinite reflectance (%R₀) 0.8% higher than normal at a distance of 100 m from the sill. Vitrinite reflectance changes caused by a swarm of seven sills varying from 8 to 80 m in thickness were calculated. It is shown that the calculated thermal profile can account for the observed shift in vitrinite reflectance in the well. A two‐dimensional section crossing the Gjallar Ridge, consisting of numerous magmatic intrusions, is also modelled. The modelled geological development and temperature history over the profile show that there are significant maturation effects in the interval under investigation. Based on this work, the sill swarm observed in the area could more than double the fraction of the kerogen that has been transformed to petroleum at the (present) depth of 4 km.