Turbulent heat fluxes by profile and inertial dissipation methods: analysis of the atmospheric surface layer from shipboard measurements during the SOFIA/ASTEX and SEMAPHORE experiments

Heat flux estimates obtained using the inertial dissipation method, and the profile method applied to radiosonde soundings, are assessed with emphasis on the parameterization of the roughness lengths for temperature and specific humidity. Results from the inertial dissipation method show a decrease of the temperature and humidity roughness lengths for increasing neutral wind speed, in agreement with previous studies. The sensible heat flux estimates were obtained using the temperature estimated from the speed of sound determined by a sonic anemometer. This method seems very attractive for estimating heat fluxes over the ocean. However allowance must be made in the inertial dissipation method for non-neutral stratification. The SOFIA/ASTEX and SEMAPHORE results show that, in unstable stratification, a term due to the transport terms in the turbulent kinetic energy budget, has to be included in order to determine the friction velocity with better accuracy. Using the profile method with radiosonde data, the roughness length values showed large scatter. A reliable estimate of the temperature roughness length could not be obtained. The humidity roughness length values were compatible with those found using the inertial dissipation method.     

The ilmenite/titano-magnetite assemblage: kinetics of re-equilibration

Compositions of coexisting ilmenite and titano-magnetite commonly have been used to establish the conditions of formation for igneous and metamorphic rocks (Buddington-Lindsley geothermometer/oxybarometer). Temperatures so determined for some rocks are lower than might be expected for magmatic crystallization. These low temperatures are the result of re-equilibration of the Fe-Ti oxides during slow cooling. This process is one in which titano-magnetites are oxidized and ilmenites are reduced upon cooling along a buffer curve or in the presence of a fluid of constant composition. Textural studies indicate that the reduction of the ilmenite-hematite phase may be the slower reaction consequently, the rate-controlling step of the re-equilibration.The kinetics of the reduction reactions in the two-phase region between the joins for the ilmenite-hematite and magnetite-ulvöspinel solid solution series were studied by thermogravimetric analysis at controlledf_O2. With experiments conducted near the Ni/NiO and QFM buffers, annealed ilmenite(ss) synthetic charges were reduced isothermally. The temperature range for the experiments was 900–1250°C, with total gas-flow rates of 0.35 and 1.0 cm/s. Kinetic data were collected by measuring the weight change during each experiment as a function of time. Additionally, a cooling-rate (0.5°C/hr) experiment was conducted near the QFM buffer from 1150 to 985°C starting with an ilmenite-saturated spinel phase.At 1200°C and 0.35 cm/s flow rate, the reaction mechanism is an interfacial process where mass transport of the reacting gases is the rate-controlling step. In isothermal experiments at 1100°C and lower, diffusion of reactants through a solid product layer was the controlling mechanism. The activation energy for this diffusion process is 59±6 kcal/mole. Significant enhancement of diffusion occurs along grain boundaries.Although the individual phases may re-equilibrate internally upon cooling, the Fe-Ti contents must remain unchanged for proper use of this mineral indicator-i.e. no external re-equilibration. It is imperative that the kinetics of the situation be appreciated. These preliminary kinetic experiments indicate that extreme caution must be exercised when applying this ilmenite/titano-magnetite geothermometer/oxybarometer. These phases may only truly “quench” in the parameters of formation in the case of certain hypabyssal and extrusive occurrences     

Exsolution in the mss-pentlandite system: Textural and genetic implications for Ni-sulfide ores

Experimentation in synthetic systems is essential for a correct interpretation of ore-mineral textures such as the pyrrhotite-pentlandite (po-pn) intergrowths of Ni-sulfide deposits. Within the Fe-Ni-S system, isothermal and cooling exsolution experiments were performed on monosulfide solid solution (mss) of various compositions using sealed, evacuated silica-glass tubes. The charges were annealed between 400° and 200°C for periods ranging from 20 minutes to 5 weeks; also, charges were cooled from 500° to 100°C at 1°C/h. Early-formed isothermal textures form by nucleation and growth, and depend on the initial degree of supersaturation and metal diffusivities; the final textures result from further growth and coarsening of the early forms and are particularly sensitive to the diffusivities, which are a function of temperature. The cooling-rate experiments indicate that massive pn develops by exsolution between 610° and about 250°C during slow cooling from temperatures above the mss-pn solvus; coarsened pn forms along basal planes in the mss matrix between about 250° and 150°C; pn "Flames" result at 150°C or slightly below. Crossing pn lamellae, obtained isothermally at high degrees of supersaturation and virtually unknown in ores, cannot form during slow cooling.     

The reproductive cycle of the bay scallop,Argopecten irradians irradians (Lamarck), in a small coastal embayment on Cape Cod,Massachusetts

The spawning activity of the bay scallop Argopecten irradians irradians (Lamarck) was monitored from May through September in a small embayment on Cape Cod, Massachusetts and compared with changes in hydrographic conditions. Spawning activity of bay scallops began in May and continued through July with some minor activity occurring during August and September. Activity was most closely related to changes in ambient temperature and occurred predominantly before the summer maximum temperature was recorded. As temperatures declined in the late summer and early fall, increased gametogenic activity was evident. A longer period of spawning activity was observed than was previously reported for New England waters.     

Geochemistry of Archean shales from the Pilbara Supergroup,Western Australia

Archean clastic sedimentary rocks are well exposed in the Pilbara Block of Western Australia. Shales from turbidites in the Gorge Creek Group (ca. 3.4 Ae) and shales from the Whim Creek Group (ca. 2.7 Ae) have been examined. The Gorge Creek Group samples, characterized by muscovite-quartzchlorite mineralogy, are enriched in incompatible elements (K, Th, U, LREE) by factors of about two, when compared to younger Archean shales from the Yilgarn Block. Alkali and alkaline earth elements are depleted in a systematic fashion, according to size, when compared with an estimate of Archean upper crust abundances. This depletion is less notable in the Whim Creek Group. Such a pattern indicates the source of these rocks underwent a rather severe episode of weathering. The Gorge Creek Group also has fairly high B content (85 ± 29 ppm) which may indicate normal marine conditions during deposition.Rare earth element (REE) patterns for the Pilbara samples are characterized by light REE enrichment ($\text{La}{}_{\mathrm{N}}\text{Yb}{}_{\mathrm{N}}\text{≥ 7.5}$) and no or very slight Eu depletion ($\text{Eu}\text{Eu}{}^1\text{= 0.82 – 0.99}$). A source comprised of about 80% felsic igneous rocks without large negative Eu-anomalies (felsic volcanics, tonalites, trondhjemites) and 20% mafic-ultramafic volcanics is indicated by the trace element data. Very high abundances of Cr and Ni cannot be explained by any reasonable provenance model and a secondary enrichment process is called for.     

Selective concentration of cesium in analcime during hydrothermal alteration,Yellowstone National Park,Wyoming

Chemical and mineralogical studies of fresh and hydrothermally altered rhyolitic material in Upper and Lower Geyser Basins, Yellowstone National Park, show that all the altered rocks are enriched in Cs and that Cs is selectively concentrated in analcime. The Cs content of unaltered rhyolite lava flows, including those from which the altered sediments are derived, ranges from 2.5 to 7.6 ppm. The Cs content of analcime-bearing altered sedimentary rocks is as high as 3000 ppm, and in clinoptilolite-bearing altered sedimentary rocks Cs content is as high as 180 ppm. Altered rhyolite lava flows which were initially vitrophyres, now contain up to 250 ppm Cs, and those which were crystallized prior to hydrothermal alteration contain up to 14 ppm. Mineral concentrates of analcime contain as much as 4700 ppm Cs. The Cs must have been incorporated into the analcime structure during crystallization, rather than by later cation substitution, because analcime does not readily exchange Cs. The $\text{Cs}\text{Cl}$ of the fluids circulating through the hydrothermal system varies, suggesting that Cs is not always a conservative ion and that Cs is lost from upflowing thermal waters due to water-rock interaction resulting in crystallization of Cs-bearing analcime.The source of Cs for Cs enrichment of the altered rocks is from leaching of rhyolitic rocks underlying the geyser basins, and from the top of the silicic magma chamber that underlies the area.Analcime is an important natural Cs sink, and the high Cs concentrations reported here may prove to be an important indicator of the environment of analcime crystallization.     

Towards evaluating cloud response to climate change using clustering technique identification of cloud regimes

Most of the discrepancies in the climate sensitivity of general circulation models (GCMs) are believed to be due to differences in cloud radiative feedback. Analysis of cloud response to climate change in different ‘regimes’ may offer a more detailed understanding of how the cloud response differs between GCMs. In which case, evaluation of simulated cloud regimes against observations in terms of both their cloud properties and frequency of occurrence will assist in assessing confidence in the cloud response to climate change in a particular GCM. In this study, we use a clustering technique on International Satellite Cloud Climatology Project (ISCCP) data and on ISCCP-like diagnostics from two versions of the Hadley Centre GCM to identify cloud regimes over four different geographical regions. The two versions of the model are evaluated against observational data and their cloud response to climate change compared within the cloud regime framework. It is found that cloud clusters produced by the more recent GCM, HadSM4, compare more favourably with observations than HadSM3. In response to climate change, although the net cloud response over particular regions is often different in the two models, in several instances the same basic processes may be seen to be operating. Overall, both changes in the frequency of occurrence of cloud regimes and changes in the properties (optical depth and cloud top height) of the cloud regimes contribute to the cloud response to climate change.     

Improved magnetic anomalies of the Antarctic lithosphere from satellite and near-surface data

The Antarctic magnetic anomaly map compiled marine and airborne surveys collected south of 60°S through 1999 and used Magsat data to help fill in the regional gaps between the surveys. Ørsted and CHAMP satellite magnetic observations with greatly improved measurement accuracies and temporal and spatial coverage of the Antarctic, have now supplanted the Magsat data. We combined the new satellite observations with the near-surface survey data for an improved magnetic anomaly map of the Antarctic lithosphere. Specifically, we separated the crustal from the core and external field components in the satellite data using crustal thickness variations estimated from the terrain and the satellite-derived free-air gravity observations. Regional gaps in the near-surface surveys were then filled with predictions from crustal magnetization models that jointly satisfied the near-surface and satellite crustal anomalies. Comparisons in some of the regional gaps that also considered newly acquired aeromagnetic data demonstrated the enhanced anomaly estimation capabilities of the predictions over those from conventional minimum curvature and spherical harmonic geomagnetic field models. We also noted that the growing number of regional and world magnetic survey compilations involve coverage gaps where these procedures can contribute effective near-surface crustal anomaly estimates.