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381.
382.
Pavel SPURNÝ Jiří BOROVIČKA Javor KAC Pavel KALENDA Jure ATANACKOV Gregor KLADNIK Dieter HEINLEIN Thomas GRAU 《Meteoritics & planetary science》2010,45(8):1392-1407
Abstract– We report an analysis of instrumental observations of a very bright fireball which terminated with a meteorite fall near the town of Jesenice in Slovenia on April 9, 2009, at 0h59m46s UT. The fireball designated EN090409 was recorded photographically and photoelectrically by two southern stations of the Czech part of the European Fireball Network (EN). Simultaneously, a part of the luminous trajectory was also captured by two all‐sky CCD systems and one video camera of the Slovenian meteor network. In addition to these optical recordings, the sonic booms produced by the Jesenice fireball were detected at 16 seismic stations located within 150 km of the trajectory. From all these records, we reconstructed the fireball’s atmospheric trajectory, basic geophysical data, the possible impact area, and the original heliocentric orbit of the meteoroid. Using a detailed fireball light curve, we modeled the atmospheric fragmentation of the meteoroid. Both the atmospheric behavior and the heliocentric orbit proved to be quite normal in comparison with other observed meteorite falls. The Jesenice orbit is markedly different from the P?íbram and Neuschwanstein orbital meteorite pair, which fell on similar dates (April 7, 1959, and April 6, 2002, respectively). Three meteorites with a total weight of 3.6 kg (until April 2010) were found in a high mountain area near the town of Jesenice. They are classified as L6 ordinary chondrites ( Bischoff et al. 2010 ). 相似文献
383.
Lutz Nasdala John M. Hanchar Dieter Rhede Allen K. Kennedy Tamás Váczi 《Chemical Geology》2010,269(3-4):290-300
Mesoproterozoic (~ 1050 Ma; Stenian) zircon crystals from the Saranac Prospect, Bancroft, Ontario, contain up to ~ 1 wt.% U and ~ 0.15 wt.% Th and, correspondingly, they are for the most part extensively radiation-damaged (calculated total α-doses 2.3?35.3 × 1018/g). The crystals show textures of complex, intense chemical alteration that is attributed to multiple, low-T replacement events along fluid-controlled reaction fronts. Centers of crystals appear totally replaced; the primary zoning is virtually erased and the material has high porosity and numerous inclusions. Interior regions surrounding the central reworked areas still exhibit primary igneous-type zoning; in those regions the alteration emanates from fractures and then follows the more radiation-damaged growth zones. Altered areas are typically recognized by their high porosity, low BSE intensity, and deficient analytical totals. Those regions often have lost a significant fraction of their radiogenic Pb. They are in general somewhat depleted in Zr, Si, and U, and are notably enriched in Ca and Fe. Element maps reveal elevated concentrations of Al and Y within filled fractures. Our observations indicate that the fluid-driven ion exchange is mainly controlled by the accessibility of micro-areas with elevated levels of radiation damage to transporting fluids via “fast pathways”. Most importantly, there is apparent Zr?Si?U equilibrium between initially existing and newly formed zircon. The retention of U after the chemical replacement (94 ± 14% relative to the original U content in the respective zones) does not significantly fall below the retention of two major cations Zr (95 ± 4%) and Si (95 ± 2%). In spite of the partially extreme hydrothermal alteration overprinting, the original U zoning in the crystals is well preserved. These observations suggest that preferential chemical leaching of U from zircon is clearly not a general feature of this mineral. This in turn seems to question the general validity of hydrothermal experiments to low-T, fluid-driven alteration of zircon in geological environments. The observed apparent immobility of U may affect the interpretation of U?Pb discordance in zircon, and the performance assessment of this mineral as potential waste form for actinides. 相似文献
384.
Júlia Dégi Rainer Abart Kálmán Török Enikő Bali Richard Wirth Dieter Rhede 《Contributions to Mineralogy and Petrology》2010,159(3):293-314
The complex microstructure of kelyphitic rims around garnet in lower crustal garnet granulite xenoliths from the Bakony–Balaton
Highland Volcanic Field, Central Pannonian Basin has been studied in order to identify controls on garnet breakdown. Symplectites
comprised of a vermicular intergrowth of submicron sized anorthite, orthopyroxene and spinel replace garnet at a sharp reaction
front. Based on element distribution maps the transformation of garnet to symplectite is isochemical. Phase diagram calculations
indicate that this reaction was induced by a pressure decrease and/or a temperature increase. In site-specific TEM foils prepared
by focused ion beam technique and oriented parallel and perpendicular to the reaction front 200 nm wide rods of anorthite
and 20 nm wide rods of spinel are identified. The rods are oriented approximately perpendicular to the replacement front and
are embedded in an orthopyroxene matrix. The regular spacing of the symplectite phases along the reaction front suggests that
their growth is controlled by diffusion. The kinetics of symplectite formation has been modelled based on irreversible thermodynamics.
During interaction of the xenolith with the host basalt the microstructure and chemistry of the An–Opx–Spl symplectite was
significantly modified and it was partially replaced by an olivine bearing symplectite. In contrast to primary symplectite
formation, these processes were metasomatic in nature including addition of sodium, titanium and some trace elements from
the basaltic melt and can clearly be discerned from the garnet breakdown. Based on these observations it is inferred that
symplectite formation took place within the deep crust during the extension of the Pannonian Basin between 15 and 30 km depth
at high temperature (850–1,050°C) prior to the volcanic transport to the surface. 相似文献
385.
Spatial and temporal variability of urban tree canopy temperature during summer 2010 in Berlin, Germany 总被引:1,自引:0,他引:1
Trees form a significant part of the urban vegetation. Their meteorological and climatological effects at all scales in urban environments make them a flexible tool for creating a landscape oriented to the needs of an urban dweller. This study aims at quantifying the spatio-temporal patterns of canopy temperature (T C) and canopy-to-air temperature difference (?T C) in relation to meteorological conditions and tree-specific (physiological) and urban site-specific characteristics. We observed T C and ?T C of 67 urban trees (18 species) using a high-resolution thermal-infrared (TIR) camera and meteorological measurements in the city of Berlin, Germany. TIR images were recorded at 1-min intervals over a period of 2?months from 1st July to 31st August 2010. The results showed that ?T C depends on tree species, leaf size and fraction of impervious surfaces. Average canopy temperature was nearly equal to air temperature. Species-specific maximum ?T C varied between 1.9?±?0.3?K (Populus nigra), 2.9?±?0.3?K (Quercus robur), 3.2?±?0.5?K (Fagus sylvatica), 3.9?±?1.0?K (Platanus acerifolia), 4.6?±?0.2?K (Acer pseudoplatanus), 5.0?±?0.5?K (A. platanoides) and 5.6?±?1.1?K (A. campestre). We analysed ?T C for a hot and dry period (A) and a warm and wet period (B). The range of species-specific ?T C at noon was nearly equal, i.e. 4.4?K for period A and 4.2?K for period B. Trees surrounded by high fraction of impervious surfaces showed consistently higher ?T C. Knowledge of species-specific canopy temperature and the impacts of urban structures are essential in order to optimise the benefits from trees in cities. However, comprehensive evaluation and optimisation should take the full range of climatological effects into account. 相似文献
386.
The combination of the O-shell theory of Heymann and Dziczkaniec and the supernova theory of Woosley and Howard clearly identifies the astrophysical sites for the formation of the anomalous light Xe component in carbonaceous chondrites. These sites are the O- and Ne-shells, and possibly C-shell of a massive star. Most of the 124Xe and 126Xe are formed in the O-shell during hydrostatic core silicon-burning, when a seed of heavy nuclei is exposed to an effective temperature near T9 = 2.0. 128Xe is formed via 128Ba in the O-shell, but the amounts appear too small to satisfy the deduced 128Xe/124Xe and 128Xe/126Xe yield ratios from the chondrites. However, substantial amounts of 128Xe can be formed in the adjacent Ne- and C-shells during the explosion. The formation of 128Ba in the O-shell would increase if the (γ, α) photodisintegration rate in 128Ba is actually smaller than calculated by Woosley and Howard. Lewis et al. have proposed that the anomalous light Xe component is mass-fractionated normal Xe. It is in this sense that the process of stellar nucleosynthesis of the present paper mimicks mass-fractionation. 相似文献
387.
Dieter Lorenz-Petzold 《Astrophysics and Space Science》1984,98(2):249-254
We present the general stiff matter and radiation solutions for thek=0, 1, –1 Friedmann-Robertson-Walker space-times in the Brans-Dicke scalar-tensor theory. 相似文献
388.
Dieter Breitschwerdt 《Astrophysics and Space Science》2001,276(1):163-176
The state of our observational and theoretical knowledge of the localinterstellar medium (LISM) is reviewed. The LISM stretches out from thelocal Cloud, surrounding the solar system to the boundary of the LocalBubble, which is a region of distinct anticorrelation between HI (N
H< 1020 cm-2) and 1/4 keV diffuse soft X-rays. After discussingsome key observations in soft X-rays, obtained by ROSAT and DXS, and inthe EUV by the EUVE satellite and the EURD instrument onboard Minisat, Iwill critically review models of the LISM. Since we cannot determine theplasma state (temperature, density, etc.) directly, the best plasmadiagnostic tool is high resolution spectroscopy. The interpretationof the data then has to rely heavily on plasma emission models. I willpoint out several caveats in the standard procedure. Preference is givento dynamical models of the Local Bubble in general and to non-equilibriumplasma emission models in particular, which have to be calculatedself-consistently. Such a model can explain (i) the deficiency of EUVlines as observed by EUVE, (ii) the dispersion measure and scintillationproperties of a nearby pulsar, (iii) the existence of local neutral HIclouds, and (iv) OVI absorption line widths. New model spectra of theLISM will be presented and briefly compared with DXS, EUVE and preliminaryEURD results. 相似文献
389.
Dieter Lorenz-Petzold 《Astrophysics and Space Science》1983,96(2):351-354
We investigate the Einstein field equations for tilted spatially self-similar Bianchi type-fV spacetimes. The solutions represent anisotropic models which can be made consistent with the observed isotropy. 相似文献
390.
Kenneth R. Meyer Dieter S. Schmidt 《Celestial Mechanics and Dynamical Astronomy》1982,28(1-2):201-207
The fundamental matrix solutionT for the variational equations of a Hamiltonian system is symplectic. We use this fact to completeT when it is only partially known. We discuss three cases. The last one gives an easy proof for the method invented by Brown in his lunar theory.Paper presented at the 1981 Oberwolfach Conference on Mathematical Methods in Celestial Mechanics.Dedicated to Victor Szebehely. 相似文献