Carbon dioxide in magmas and implications for hydrothermal systems   总被引：21，自引：0，他引：21  

Jacob B. Lowenstern 《Mineralium Deposita》2001,36(6):490-502

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Neuere Ergebnisse der Braunkohlen- und Torf-Petrographie. Gedanken zur Mazeral-Klassifikation     

Dr. H. Jacob 《International Journal of Earth Sciences》1962,51(2):530-546

Zusammenfassung Die Mazeral-Klassifikation von Torf und Weichbraunkohle muß tunlichst auf die Steinkohlen-Nomenklatur Bezug nehmen und nach gleichen bzw. ähnlichen Prinzipien erfolgen. Ferner hat sie technologischen Gesichtspunkten Rechnung zu tragen. Die vom Verfasser vorgeschlagene Nomenklatur wird diesen Anforderungen gerecht. Da Torfe und Weichbraunkohlen heterogener als Steinkohlen sind, ist eine stärkere Gliederung erforderlich. 5 Gruppen (Exinit, Xylinit, Detrinit, Dopplerinit und Inertinit) werden jeweils in 3 Untergruppen eingeteilt. Diese erfahren eine weitere Gliederung nach Mazeralen. Abschließend weist der Verfasser darauf hin, daß durch Kombination der Weichbraunkohlen- und Steinkohlen-Klassifikation auch den Belangen der Hartbraunkohlen-Petrographie Rechnung getragen werden kann.  相似文献   

The impact of seasonality on multi-scale feature extraction techniques     

Brian Moore  Jacob J. McKee 《International Journal of Digital Earth》2020,13(1):9-21

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Detailed correlation of type III radio bursts with Hα activity     

T. B. H. Kuiper  Jay M. Pasachoff 《Solar physics》1973,28(1):187-196

We compare observations of type III impulsive radio bursts made at the Clark Lake Radio Observatory with high-spatial-resolution cinematographic observations taken at the Big Bear Solar Observatory. Use of the log-periodic radio interferometer allows us to localize the radio emission uniquely. This study concentrates on the particularly active region close to the limb on 22 May 1970. Sixteen of the 17 groups were associated with some H activity, 11 of them with the start of such activity.as of September 1972: Williams College-Hopkins Observatory, Williamstown, Massachusetts 01267.  相似文献   

Jacob Bear: an autobiography     

Bear J 《Ground water》2003,41(3):393-396

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Planetary Embryos Never Formed in the Kuiper Belt     

A. MorbidelliC. Jacob  J.-M. Petit 《Icarus》2002,157(1):241-248

We study the orbital evolutions of various systems of planetary embryos in the transneptunian region, undergoing mutual scattering and perturbations from the giant planets. We show that about 15-20% of the original embryos should survive in the transneptunian region at the current epoch. The orbital dispersion of the surviving embryos depends on their individual mass, so that only lunar mass embryos could survive with semimajor axis smaller than 50 AU. In all cases, we show by a Monte Carlo model that at least one of the surviving embryos should have already been discovered by one of the most effective Kuiper-belt surveys. This implies that planetary embryos did not form in the transneptunian region (or have been removed by some external and unknown mechanism). Therefore, we conclude that the Kuiper belt was not excited by resident planetary embryos, unlike the asteroid belt. We also compute with the Monte Carlo model that a significant number (order 10) of Pluto-size bodies could exist only on very eccentric and long-periodic orbits, typical of the scattered disk, while the existence of about 30 bodies brighter than absolute magnitude 4 in the classical belt is compatible with the discovery of Varuna by the Spacewatch survey.  相似文献   

An intercomparison of regional climate simulations for Europe: assessing uncertainties in model projections   总被引：2，自引：0，他引：2  

M. Déqué  D. P. Rowell  D. Lüthi  F. Giorgi  J. H. Christensen  B. Rockel  D. Jacob  E. Kjellström  M. de Castro  B. van den Hurk 《Climatic change》2007,81(1):53-70

Ten regional climate models (RCM) have been integrated with the standard forcings of the PRUDENCE experiment: IPCC-SRES A2 radiative forcing and Hadley Centre boundary conditions. The response over Europe, calculated as the difference between the 2071–2100 and the 1961–1990 means can be viewed as an expected value about which various uncertainties exist. Uncertainties are measured here by variance in eight sub-European boxes. Four sources of uncertainty can be evaluated with the material provided by the PRUDENCE project. Sampling uncertainty is due to the fact that the model climate is estimated as an average over a finite number of years (30). Model uncertainty is due to the fact that the models use different techniques to discretize the equations and to represent sub-grid effects. Radiative uncertainty is due to the fact that IPCC-SRES A2 is merely one hypothesis. Some RCMs have been run with another scenario of greenhouse gas concentration (IPCC-SRES B2). Boundary uncertainty is due to the fact that the regional models have been run under the constraint of the same global model. Some RCMs have been run with other boundary forcings. The contribution of the different sources varies according to the field, the region and the season, but the role of boundary forcing is generally greater than the role of the RCM, in particular for temperature. Maps of minimum expected 2m temperature and precipitation responses for the IPCC-A2 scenario show that, despite the above mentioned uncertainties, the signal from the PRUDENCE ensemble is significant.  相似文献   

Numerical simulation of NAPL flow in the subsurface     

L.K. Kuiper  T.K. Illangasekare 《Computational Geosciences》1998,2(3):171-189

A three-dimensional, three-phase numerical model is presented for simulating the movement of immiscible fluids, including nonaqueous-phase liquids (NAPLs), through porous media. The model is designed to simulate soil flume experiments and for practical application to a wide variety of contamination scenarios involving light or dense NAPLs in heterogeneous subsurface systems. The model is derived for the three-phase flow of water, NAPL, and air in porous media. The basic governing equations are based upon the mass conservation of the constitutents within the phases. The descretization chosen to transform the governing equations into the approximating equations, although logically regular, is very general. The approximating equations are a set of simultaneous coupled nonlinear equations which are solved by the Newton-Raphson method. The linear system solutions needed for the Newton-Raphson method are obtained using a matrix of preconditioner/accelerator iterative methods. Because of the special way the governing equations are implemented, the model is capable of simulating many of the phenomena considered necessary for the sucessful simulation of field problems including entry pressure phenomena, entrapment, and preferential flow paths. The model is verified by comparing it with several exact analytic test solutions and three soil flume experiments involving the introduction and movement of light nonaqueous-phase liquid (LNAPL) or dense nonaqueous-phase liquid (DNAPL) in heterogeneous sand containing a watertable. This revised version was published online in August 2006 with corrections to the Cover Date.  相似文献   

The first multi-wavelength campaign of AXP 4U 0142+61 from radio to hard X-rays     

P. R. den Hartog  L. Kuiper  W. Hermsen  N. Rea  M. Durant  B. Stappers  V. M. Kaspi  R. Dib 《Astrophysics and Space Science》2007,308(1-4):647-653

For the first time a quasi-simultaneous multi-wavelength campaign has been performed on an Anomalous X-ray Pulsar from the radio to the hard X-ray band. 4U 0142+61 was an INTEGRAL target for 1 Ms in July 2005. During these observations it was also observed in the X-ray band with Swift and RXTE, in the optical and NIR with Gemini North and in the radio with the WSRT. In this paper we present the source-energy distribution. The spectral results obtained in the individual wave bands do not connect smoothly; apparently components of different origin contribute to the total spectrum. Remarkable is that the INTEGRAL hard X-ray spectrum (power-law index 0.79±0.10) is now measured up to an energy of ～230 keV with no indication of a spectral break. Extrapolation of the INTEGRAL power-law spectrum to lower energies passes orders of magnitude underneath the NIR and optical fluxes, as well as the low ～30 μJy (2σ) upper limit in the radio band.  相似文献   

Exsolution and shock microstructures of igneous pyroxene clasts in the Northwest Africa 7533 Martian meteorite          下载免费PDF全文

Hugues Leroux  Damien Jacob  Maya Marinova  Roger H. Hewins  Brigitte Zanda  Sylvain Pont  Jean‐Pierre Lorand  Munir Humayun 《Meteoritics & planetary science》2016,51(5):932-945

Northwest Africa (NWA) 7533 is a Martian regolith breccia. This meteorite (and its pairings) offers a good opportunity to study (near‐) surface processes that occurred on early Mars. Here, we have conducted a transmission electron microscope study of medium‐ and coarse‐grained (a few tens to hundreds of micrometers) Ca‐rich pyroxene clasts in order to define their thermal and shock histories. The pyroxene grains have a high‐temperature (magmatic) origin as revealed by the well‐developed pigeonite–augite exsolution microstructure. Exsolution lamella characteristics (composition, thickness, and spacing) indicate a moderately slow cooling. Some of the pyroxene clasts display evidence for local decomposition into magnetite and silica at the submicron scale. This phase decomposition may have occurred at high temperature and occurred at high oxygen fugacity at least 2–3 log units above the QFM buffer, after the formation of the exsolution lamellae. This corresponds to oxidizing conditions well above typical Martian magmatic conditions. These oxidizing conditions seem to have prevailed early and throughout most of the history of NWA 7533. The shock microstructure consists of (100) mechanical twins which have accommodated plastic deformation. Other pyroxene shock indicators are absent. Compared with SNC meteorites that all suffered significant shock metamorphism, NWA 7533 appears only mildly shocked. The twin microstructure is similar from one clast to another, suggesting that the impact which generated the (100) twins involved the compacted breccia and that the pyroxene clasts were unshocked when they were incorporated into the NWA 7533 breccia.  相似文献