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Not AvailableThe integration of genome information into fisheries and aquaculture management is important to ensure long-term sustainable fishery harvest and aquaculture production. In the present study, a combination of PacBio, Illumina, and Arima Hi-C technologies were applied to construct the genome assembly of M. cephalus, an economically important brackish water aquaculture species.ICAR-CR

Diffusion studies in the β (B2), β′ (bcc), and γ (fcc) Fe-Ni-Al alloys at 1000 °C

Diffusion studies were carried out in the Fe-Ni-Al system at 1000°C with solid-solid diffusion couples assembled with β (B2), β′ (bcc), and γ (fcc) single-phase alloys for the development of diffusion structures, diffusion paths, and for the determination of interdiffusion and intrinsic diffusion coefficients. The diffusion structures were examined by optical and scanning electron microscopy, and the concentration profiles were determined by electron microprobe analysis. Diffusion couples included several series of β vs γ and β′ vs γ diffusion couples characterized by a common terminal alloy bonded to several terminal alloys with varying compositions. The development of planar and nonplanar interfaces, as well as two-phase layers, as observed in various couples, were related to the diffusion paths. The interdiffusion fluxes of individual components were calculated directly from the experimental concentration profiles, and the diffusional interactions among components were examined in the light of zero-flux planes (ZFPs) and flux reversals, which were identified in several couples. Ternary interdiffusion coefficients (D̃i.jFe (i, j = Al, Ni)), with Fe considered as the dependent concentration variable, were evaluated at composition points of the intersection of diffusion paths of single-phase couples and of multiphase couples that developed planar interfaces. The interdiffusion coefficients were the largest in magnitude for the β′ alloys, especially near the β/β′ miscibility gap, and decreased for the β and γ alloys. In the β and γ phases, the main interdiffusion coefficient for Al was larger than those for Ni and Fe. Also, Fe interdiffused faster than Ni in the Fe-rich β and β′ phases. The cross-interdiffusion coefficients (D̃AlNiFe and D̃NiAlFe) were negative in all three phases. In general, the D̃AlNiFe coefficients were larger in magnitude than the D̃NiAlFe coefficients; however, the magnitude of D̃NiAlFe was greater than that of D̃AlNiFe near the β/(β + γ) phase boundary on the ternary isotherm. In the β phase, the magnitude of D̃ijFe (i, j = Al, Ni) coefficients increased over 1 to 2 orders of magnitude with a decrease in the Al concentration and increase in the Fe/Ni concentration ratio. Interdiffusion coefficients, extrapolated from the ternary coefficients for binary alloys, were consistent with those in literature. Intrinsic diffusion coefficients were also determined at selected compositions. In addition, tracer diffusion coefficients were estimated for the binary Fe-Al and Ni-Al alloys at selected compositions, from an extrapolation of ternary interdiffusion coefficients

Tracking India within precambrian supercontinent cycles

The term supercontinent generally implies grouping of formerly dispersed continents and/or their fragments in a close packing accounting for about 75% of earth’s landmass in a given interval of geologic time. The assembly and disruption of supercontinents rely on plate tectonic processes, and therefore, much speculation is involved particularly considering the debates surrounding the applicability of differential plate motion, the key to plate tectonics during the early Precambrian. The presence of Precambrian orogenic belts in all major continents is often considered as the marker of ancient collisional or accretionary sutures, which provide us clues to the history of periodic assembly of ancient supercontinents. Testing of any model assembly/breakup depends on precise age data and paleomagnetic pole reconstruction. The record of dispersal of the continents and release of enormous stress lie in extensional geological features, such as rift valleys, regionally extensive flood basalts, granite-rhyolite terrane, anorthosite complexes, mafic dyke swarms, and remnants of ancient mid-oceanic ridges. Indian shield with extensive Precambrian rock records is known to bear signatures of the past supercontinents in a fragmentary manner. Vast tracts of Precambrian rocks exposed in peninsular India and in the Lesser Himalaya and the Shillong plateau further north and east provide valuable clues to global tectonic reconstructions and the geodynamics of the respective periods. The Indian shield is a mosaic of Archean cratonic nuclei surrounded by Proterozoic orogenic belts, which preserve the records of geologic events since the Paleoarchean/Eoarchean. Here we discuss the sojourn of the Indian plate from the Archean through Proterozoic, in light of available models for supercontinent assembly and breakup in the Precambrian. We also discuss the issues in constraining the configuration, which is mainly due to scanty exposures, lack of reliable paleomagnetic poles from different cratons, and their time of formation or amalgamation. In this chapter, we briefly review Precambrian geology of India to track her participation in the making of the supercontinents through time.Sarbani Patranabis-Deb, Dilip Saha, and M. Santos