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1.
We present the results of our tests of an acousto-optical imaging spectrophotometer with a CCD detector for astronomical observations. The tunable acousto-optical filter, based on a paratellurite single crystal with a 13 Å pass band operates in the wavelength range 6300–11000 Å. We obtained image spectra for the planetary nebula NGC 7027 in the Hα line and for Saturn in the methane absorption band, as well as Hα and continuum images for the nuclear region of the Seyfert galaxy NGC 1068.  相似文献   
2.

The aim of this study is to investigate the accretion of matter onto a compact gravitating remnant (neutron star) in the central region of the expanding shell of a Type II supernova. Computations of an explosion with the energetics of a Type II supernova have been performed to derive the structure of matter in the vicinity of the neutron star. The energy of the expanding shell and the parameters of the presupernova correspond to the known values for SN 1987A. This accretion leads to the formation of a layer of fairly dense and hot gas at the surface of the compact remnant, providing the conditions for nucleosynthesis reactions. Thus, one result of the study is to demonstrate the importance of the r and rbc processes, or explosive nucleosynthesis, in the compact envelope of a neutron star. A second result is the production of emission lines from unstable elements formed in the central part of the neutron-star envelope.

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3.
The results of X-ray structural, electron-microscopic, and X-ray spectral microprobe studies of Al-based metal solid solutions that underwent nuclear disintegration and that were discovered in nature for the first time are presented. Based on the similarity to technical counterparts, it is suggested to recognize the previously unknown alloys as natural duralumin.  相似文献   
4.
The aerosol longwave radiative forcing of the atmosphere and heating rate of the near-surface aerosol layer are estimated for the extreme smoke conditions in the Moscow region in summer 2010. Thermal radiation fluxes in the atmosphere are determined using the integral transmission function and semiempirical aerosol model developed on the basis of standard aerosol models and measurements at the Zvenigorod Scientific Station, Obukhov Institute of Atmospheric Physics, Russian Academy of Sciences. The aerosol radiative forcing reached 33 W/m2 at the lower atmospheric boundary and ranged between–1.0 and 1.0 W/m2 at the upper atmospheric boundary. The heating rate of the 10-m atmospheric layer near surface was up to 0.2 K/h during the maximum smoke conditions on August 7–9. The sensitivity of the aerosol longwave radiative forcing to the changes in the aerosol absorption coefficient and aerosol optical thickness are estimated.  相似文献   
5.
Solar System Research - The article proposes a “tagged cosmic particle” method that uses the natural flux of high-energy particles of Galactic Cosmic Rays to study the composition of...  相似文献   
6.
Diamond crystals 0.05–0.2 mm (rarely up to 0.7 mm) in size were found in lavas of the Tolbachik fissure eruption (TFE, Kamchatka, 2012–2013). The TFE basaltic lavas with diamonds in the pores are similar in chemical composition to the lavas of the Great Tolbachik Fissure Eruption (GTFE, Kamchatka, 1975–1976); however, the basalts of the new eruption contain slightly more SiO2 and higher Fe relative to those of GTFE. Basalts of both eruptions are close in trace element composition. The diamonds were identified using electron microscopy and X-ray diffraction. The crystals, as a rule, represent a combination of cubes and octahedrons, with rare rhombododecahedrons. The TFE diamond has a typical cubic cell with a cube edge a = 3.574 Å and belongs to the spatial group of Fd-3m. The X-ray diffraction pattern of some grains contain reflexes with fractional indices, which indicate the twinning of the diamond along the plane {111}, which is confirmed by crystal morphological analysis. The TFE diamond was formed at the early stage of eruption with typical intense gaseous-pyroclastic jets to a height of 250 m and more. The finding of diamonds in fresh products of basaltic eruption of an active volcano may be considered as evidence of its magmatic source. Such numerous (hundreds) diamond grains in lavas of the active volcano were found for the first time in the world.  相似文献   
7.
Samples from the surface of lava flows discharged by the 2012–2013 Tolbachik Fissure Eruption were found to contain oxysulfates of copper, sodium, and potassium: K2Cu3O(SO4)2 (fedotovite), NaKCu2O(SO4)2, and Na3K5Cu8O4(SO4)8. The last two phases have no naturally occurring or synthetic analogues that we are aware of. They form flattened crystals of prismatic to long-prismatic habits. The crystals of Na3K5Cu8O4(SO4)8 have a chemical composition corresponding to the empirical formula Na2.22K5.47Cu8.02S8.05O36. An X-ray analysis of this compound showed that it has a monoclinic symmetry, P2/c, a = 13.909(4), b = 4.977(1), c = 23.525(6) Å, β = 90.021(5)°, V = 1628.3(7) Å3. The crystal structure was determined by direct techniques and refined to yield R 1 for 3955 reflexes//web// with F 2 > 4σF. The compound NaKCu2O(SO4)2 also belongs to the monoclinic system, P2/c, a = 14.111(4), b = 4.946(1), c = 23.673(6) Å, β = 92.052(6)°, V = 1651.1(8) Å3. The structure was determined by direct techniques to yield a tentative structural model that has been refined up to R 1 = 0.135 for 4088 reflexes with F 2 > 4σF. The crystal structure of Na3K5Cu8O4(SO4)8 is based on chains of [O2Cu4]4+ consisting of rib-coupled oxy-centered tetrahedrons of (OCu4)6+. The chains are surrounded by sulfate radicals, resulting in columns of {[O2Cu4](SO4)4}4? aligned along the b axis. The interchain space contains completely ordered positions of Na+ and K+ cations. The principle underlying the connection of NaKCu2O(SO4)2 columns in the crystal structure of {[O2Cu4](SO4)4}4? is different, in view of the relation Na:K = 1 as contrasted with 3:5 for the compound Na3K5Cu8O4(SO4)8. The presence of oxy-centered tetrahedrons in the structure of these new compounds furnishes an indirect hint at the importance of polynuclear copper-oxygen radicals with centering oxygen atoms as forms of transport of copper by volcanic gases.  相似文献   
8.
The first historical eruption of Kambalny volcano began on March 24, 2017 with the powerful ash emission from the summit crater reaching as high as 6 km above sea level. The explosive activity continued without interruption from March 24 to March 30. The most powerful ash emission was registered on March 25–26, when the ash plume drifted several thousand kilometers SW, S, and SE from the volcano. On April 2 and April 9, after several calm days, powerful ash explosions occurred generating ash plumes up to 7 km high. The area of the land and sea over which the ash plume drifted during the day of March 25, was 650000 km2; the area of the ash accumulation on the land that was formed from March 24 to April 9, exceeded 1500 km2. These parameters were measured using the satellite-based data in the VolSatView information system. Domination of the silty fraction and the presence of secondary minerals (pyrite, gypsum, sulfur, and others) in the ash point to the phreatic character of the volcanic eruption.  相似文献   
9.
Geology of Ore Deposits - Abstract—Yellow volborthite Cu2.95(V1.91P0.09)Σ2O7(OH)1.90·2H2O, and turquoise atacamite, Cu2[Cl0.98(OH)0.02]Σ1.00(OH)3 have been found incrusting...  相似文献   
10.
Geology of Ore Deposits - A new mineral, deltalumite, which is an analogue of the spinel-type synthetic δ-Al2O3, the second natural modification of alumina after corundum, α-Al2O3, has...  相似文献   
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