The Hard X-ray Telescope (HXT) for the SOLAR-A mission

The Hard X-ray Telescope (HXT) is a Fourier-synthesis imager; a set of spatially-modulated photon count data are taken from 64 independent subcollimators and are Fourier-transformed into an image by using procedures such as the maximum entropy method (MEM) or CLEAN. The HXT takes images of solar flares simultaneously in four energy bands, nominally 15 (or 19)–24, 24–35, 35–57, and 57–100 keV, with an ultimate angular resolution as fine as 5 arc sec and a time resolution 0.5 s. Each subcollimator has a field of view wider than the solar disk. The total effective area of the collimator/detector system reaches 70 cm², about one order of magnitude larger than that of the HINOTORI hard X-ray imager. Thanks to these improvements, HXT will for the first time enable us to take images of flares at photon energies above 30 keV. These higher-energy images will be compared with lower-energy ones, giving clues to the understanding of nonthermal processes in solar flares, i.e., the acceleration and confinement of energetic electrons. It is of particular importance to specify the acceleration site with regard to the magnetic field figuration in a flaring region, which will be achieved by collaborative observations between HXT and the Soft X-ray Telescope on board the same mission.After the launch the name of SOLAR-A has been changed to YOHKOH.     

Introduction of geospatial perspective to the ecology of fish-habitat relationships in Indonesian coral reefs: A remote sensing approach

Coral reef ecosystems worldwide are now being harmed by various stresses accompanying the degradation of fish habitats and thus knowledge of fish-habitat relationships is urgently required. Because conventional research methods were not practical for this purpose due to the lack of a geospatial perspective, we attempted to develop a research method integrating visual fish observation with a seabed habitat map and to expand knowledge to a two-dimensional scale. WorldView-2 satellite imagery of Spermonde Archipelago, Indonesia obtained in September 2012 was analyzed and classified into four typical substrates: live coral, dead coral, seagrass and sand. Overall classification accuracy of this map was 81.3% and considered precise enough for subsequent analyses. Three sub-areas (CC: continuous coral reef, BC: boundary of coral reef and FC: few live coral zone) around reef slopes were extracted from the map. Visual transect surveys for several fish species were conducted within each sub-area in June 2013. As a result, Mean density (Ind. / 300 m²) of Chaetodon octofasciatus, known as an obligate feeder of corals, was significantly higher at BC than at the others (p < 0.05), implying that this species’ density is strongly influenced by spatial configuration of its habitat, like the “edge effect.” This indicates that future conservation procedures for coral reef fishes should consider not only coral cover but also its spatial configuration. The present study also indicates that the introduction of a geospatial perspective derived from remote sensing has great potential to progress conventional ecological studies on coral reef fishes.

     

Chondrites with peculiar rare-earth patterns

Rare-earth elements and Ba in Khohar, Abee, Indarch, Atlanta, Jajh deh Kot Lalu, and Nakhla were determined accurately by isotope dilution technique; for Atlanta only, Fe (total), Mg and Ca were also determined. Khohar shows in two aliquants a strikingly large, positive anomaly for Ce. A fragment of Abee is outstanding in having a large positive Yb anomaly and a zigzag RE pattern. It is considered that the Yb anomaly is not necessarily associated with the zigzaggedness in question. Anyway, these facts corroborate our previous observations that abundances of Ce and/or Yb could be sometimes anomalous in meteoritic and lunar materials.Atlanta also has a significant negative Eu anomaly, similar to the Eu depletions observed in lunar basalts and Ca-poor achondrites by other workers. Besides, this enstatite chondrite has a RE pattern which indicates that this meteorite is cumulate-type (solid-type) material separated perhaps from a considerably fractionated melt. Accordingly, it is suggested that it is not always appropriate to classify this type II enstatite chondrite as “chondrite”. Two fragments from Abee and Atlanta show different RE patterns. It is also observed that Ba abundances are sometimes sporadically and irregularly high.     

REE Tetrad Effects in Rare—metal Granites

Described in this paper are the characteristics of tetrad effects of REE in rare-metal granites.Based on the analytical data and experimental geochemical data available,it is pointed out that the tetrad effects of REE in the granites are produced in the metal-fluid system.Intense fractional crystallization of granitic melt(containing REE accessary minerals)and its interaction with volatile-rich(F,Cl)fluid are the major factors leading to the tetrad effects of REE.From this,this paper presents a composite genetic model for high-degree fractional crystallization-volatile-rich fluid metasomatism of rare-metal granites.With the model,quantitative calculations have been made.Meanwhile,it is pointed out that the tetrad effects of REE can be used as an important indicator to distinguish mineralized granites from barren ones.     

A Microstructural sequence of quartz schists in central Shikoku, south-west Japan

This paper describes a microstructural sequence of quartz schists (metamorphosed chert) in the Asemi river region of the Sambagawa metamorphic terrain in central Shikoku, southwest Japan. The Asemi river region is divided into three areas on the basis of characteristics of microstructures of quartz schists observed under the optical microscope: areas I, II and III, in ascending order of metamorphic grade. Microstructures in area I consist of finer, equant, equidimensional and polygonal quartz grains free from internal deformation features. Microstructures in area II are characterized by oblate or elliptical grains with remarkable undulatory extinction surrounded by serrated grain boundaries. Microstructures in area III consist mainly of coarser and equant grains without distinct internal deformation features.The formation conditions of these microstructures are discussed in the light of recent experimental results.     

A theory of the pressure-induced high-spin—low-spin transition of transition-metal oxides

The pressure-induced high-spin—low-spin transition of the transition-metal ions in octahedral coordination is studied theoretically. The relation between the crossover point and the transition point is discussed and the formula to determine the transition point is given in terms of the crystal-field splitting Δ and the spin-pairing energy Π asΔ = αΠ. The numerical coefficient α is determined by the ratio of the change of the interatomic distances between the transition-metal ion and ligands. It is proved that α is generally less than 1 and takes a value of about 0.95-0.80 for the transition-metal oxides. Based on the discussions on the P–V relation of the low-spin oxides, transition pressures are estimated to be about 700–1300 kbar for MnO, CoO and Fe₂O₃, and about 250–400 kbar for FeO.The magnitude of the shifts of transition pressures due to entropy changes is roughly evaluated to be about 0.1 kbar K^?1 for transition-metal oxides. It is discussed whether the transition at high temperature takes place continuously or not. For MnO, FeO and Fe₂O₃, the high-spin—low-spin transition will take place gradually at temperatures higher than about 2000 K. For CoO, the gradual transition will take place at above 300 K.     

Recognition of conjugate solid-type and liquid-type relationship among the oceanic basalts,with respect to REE

The REE abundances and their chondrite-normalized pattern lead one to consider that the basalt from the Caroline ridge area southeast of the Marianas Arc and the one from the Puerto Rico Trench happen to be equivalent to conjugate liquid-type and solid-type materials, respectively, reflecting an equilibrium of a 20% partial melting. This line of interpretation enables us not only to assess the REE abundances in the original solid-type material (M), but also to estimate the corresponding values in the product (¯L) of a very small (say, less than 1 %) extent of a partial melting. It is also found that the relative REE abundances in a basalt from directly east of the Marianas Trench are quite the same as those thus estimated. Alternatively, it is possible to interpret this basalt as representing the residual liquid left after the primary fractional differentiation of the mantle.It is suggested that the straight-type bulk partition coefficients, the absence of the apparent europium anomaly, and the higher pressure are closely associated.