A Basic Water Quality Model for the River Neckar: Part 1 – model development,parameter sensitivity and identifiability,calibration and validation     

Ingo Haag 《洁净——土壤、空气、水》2006,34(6):533-548

  相似文献   

The updated ESA Earth System Model for future gravity mission simulation studies   总被引：1，自引：1，他引：0  

Henryk Dobslaw  Inga Bergmann-Wolf  Robert Dill  Ehsan Forootan  Volker Klemann  Jürgen Kusche  Ingo Sasgen 《Journal of Geodesy》2015,89(5):505-513

  相似文献   

Monsoon triggered formation of Quaternary alluvial megafans in the interior of Oman     

Ingo Blechschmidt  Albert Matter  Frank Preusser  Dirk Rieke-Zapp 《Geomorphology》2009,110(3-4):128-139

A vast bajada consisting of coalescing low-gradient (< 0.3°) alluvial fans exceeding 100 km in length formed along the southwestern margin of the Oman Mountains. It comprises an old fan sequence of inferred Miocene to Pliocene age termed Barzaman Formation, diagenetically highly altered to dolomitic clays, and a thin veneer of weakly cemented Quaternary gravels. A combination of remote sensing, lithological analyses and luminescence dating is used to interpret the complex aggradation history of the Quaternary alluvial fans from the interior of Oman in the context of independent regional climate records. From satellite imagery and clast analysis four fans can be discerned in the study area. While two early periods of fan formation are tentatively correlated to the Miocene–Pliocene and the Early Pleistocene, luminescence dating allows the distinction of five phases of fan aggradation during the Middle–Late Pleistocene. These phases are correlated with pluvial periods from Marine Isotope Stage (MIS) 11 through 3, when southern Arabia was affected by monsoonal precipitation. It is concluded that the aggradation of the alluvial fans was triggered by the interplay of increased sediment production during arid periods and high rainfall with enhanced erosion of hillslopes and transport rates during strong monsoon phases. However, the lack of fine-grained sediments, bioturbation and organic material implies that although the Quaternary fans are sourced by monsoonal rains they formed in a semi-arid environment. Thus, it appears that, in contrast to the Oman Mountains, the interior was not directly affected by monsoonal precipitation.  相似文献   

Temporal Gravity Variations near Shrinking Vatnajökull Ice Cap, Iceland     

Wolfgang R. Jacoby  Oliver Hartmann  Herbert Wallner  Peter L. Smilde  Stefan Bürger  Lars E. Sjöberg  Sigurdur Erlingsson  Detlef Wolf  Volker Klemann  Ingo Sasgen 《Pure and Applied Geophysics》2009,166(8-9):1283-1302

Repeated gravity measurements were carried out from 1991 until 1999 at sites SE of Vatnajökull, Iceland, to estimate the mass flow and deformation accompanying the shrinking of the ice cap. Published GPS data show an uplift of about 13 ± 5 mm/a near the ice margin. A gravity decrease of –2 ± 1 μGal/a relative to the Höfn base station, was observed for the same sites. Control measurements at the Höfn station showed a gravity decrease of –2 ± 0.5 µGal/a relative to the station RVIK 5473 at Reykjavík (about 250 km from Höfn). This is compatible, as a Bouguer effect, with a 10 ± 3 mm/a uplift rate of the IGS point at Höfn and an uplift rate of ~20 mm/a near the ice margin. Although the derived gravity change rates at individual sites have large uncertainties, the ensemble of the rates varies systematically and significantly with distance from the ice. The relationship between gravity and elevation changes and the shrinking ice mass is modelled as response to the loading history. The GPS data can be explained by 1-D modelling (i.e., an earth model with a 15-km thick elastic lithosphere and a 7·10¹⁷ Pa·s asthenosphere viscosity), but not the gravity data. Based on 2-D modelling, the gravity data favour a low-viscosity plume in the form of a cylinder of 80 km radius and 10¹⁷ to 10¹⁸ Pa·s viscosity below a 6 km-thick elastic lid, embedded in a layered PREM-type earth, although the elevation data are less well explained by this model. Strain-porosity-hydrology effects are likely to enhance the magnitude of the gravity changes, but need verification by drilling. More accurate data may resolve the discrepancies or suggest improved models.  相似文献   

C. R. Kitchin: Optical Astronomical Spectroscopy. Institute of Physics Publishing,Bristol and Philadelphia,XVII + 272 + XVII Seiten,Preis (paperback): $ 40,OO. ISBN 0 7503 0246 8     

Ingo Lehmann 《Astronomische Nachrichten》1996,317(6):422-422

  相似文献   

A better characterization of the chemical composition of exoplanets atmospheres with ARIEL     

Olivia Venot  Benjamin Drummond  Yamila Miguel  Ingo P. Waldmann  Enzo Pascale  Tiziano Zingales 《Experimental Astronomy》2018,46(1):101-134

  相似文献   

The Kumtag 016 L5 strewn field,Xinjiang Province,China     

Xiaojia Zeng  Shijie Li  Ingo Leya  Shijie Wang  Thomas Smith  Yang Li  Peng Wang 《Meteoritics & planetary science》2018,53(6):1113-1130

The Kumtag 016 strewn field was found in the eastern part of the Kumtag desert, Xinjiang Province, China. In this study, 24 recovered meteorites have been characterized by a suite of different analytical techniques to investigate their petrography, mineralogy, bulk trace elements, noble gas isotopic composition, density, and porosity. We attribute to the strewn field 22 L5 chondrites with shock stage S4 and weathering grade W2–W3. Two different meteorites, Kumtag 021, an L4 chondrite and Kumtag 032, an L6 chondrite, were recognized within the strewn field area. Moreover, Kumtag 003, an H5 chondrite, was previously found in the same area. We infer that the Kumtag 016 strewn field most likely consists of at least four distinct meteorite falls. The effects of terrestrial weathering on the studied meteorites involve sulfide/metal alteration, chemical changes (Sr, Ba, Pb, and U enrichments and depletion in Cr, Co, Ni, and Cs abundances), and physical modifications (decrease of grain density and porosity). Measurements of the light noble gases indicate that the analyzed Kumtag L5 samples contain solar wind-implanted noble gases with a ²⁰Ne/²²Ne ratio of ~12.345. The cosmic-ray exposure (CRE) ages of the L5 chondrites are in a narrow range (3.6 ± 1.4 Ma to 5.2 ± 0.4 Ma). For L4 chondrite Kumtag 021 and L6 chondrite Kumtag 032, the CRE ages are 5.9 ± 0.4 Ma and 4.7 ± 0.8 Ma, respectively.  相似文献   

A noble gas data collection of lunar meteorites     

Marianna Mészáros  Beda A. Hofmann  Ingo Leya 《Meteoritics & planetary science》2018,53(5):1104-1107

We collected the published noble gas data of altogether 35 lunar meteorites. This compilation includes the stable isotopes of He, Ne, Ar, Kr, and Xe. We also give a summary of cosmogenic, trapped, and radiogenic noble gas components of lunar meteorites for which data are available in the literature.  相似文献   

Determination of Zr and Hf in a Flux-Free Fusion of Whole Rock Samples using Laser Ablation Inductively Coupled Plasma-Mass Spectrometry (LA-ICP-MS) with Isotope Dilution Calibration     

Joy E. Reid  Ingo Horn  Henry P. Longerich  Lance Forsythe  George A. Jenner 《Geostandards and Geoanalytical Research》1999,23(2):149-155

Isotope dilution calibration has been applied to the determination of Zr and Hf in whole rocks by laser ablation (LA)-ICP-MS. Enriched isotopes were added during the preparation of flux-free, synthetic whole rock glasses and homogenised through a combination of grinding and fusion. This method avoids problems, such as solution instability and the chemical resistance of minerals such as zircon, inherent in acid digestion sample preparation. The use of isotope dilution removes the need for external calibration using certified reference material glasses such as NIST SRM 612 for which certified Zr and Hf values are not available. The precision of Zr and Hf determinations were found to be < 1% and 3.5% respectively, limited by Poisson counting statistics which contributed to 50% of the final precision of analysis. Measured values correlate closely with compiled literature values.  相似文献   

Petrology,mineralogy, porosity,and cosmic‐ray exposure history of Huaxi ordinary chondrite          下载免费PDF全文

Shijie Li  Shijie Wang  Ingo Leya  Yang Li  Xiongyao Li  Thomas Smith 《Meteoritics & planetary science》2017,52(5):937-948

A meteorite fall was heard and collected on July 13, 2010 at about 18:00 (local time) in the Shibanjing village of the Huaxi district of Guiyang, Guizhou province, China. The total mass of the fall is estimated to be at least 1.6 kg; some fragments are missing. The meteorite consists mainly of olivine, low‐Ca pyroxene, high‐Ca pyroxene, plagioclase, kamacite, taenite, and troilite. Minor phases include chromite and apatite. Various textural types of chondrules exist in this meteorite: most chondrule textures can be easily defined. The grain sizes of secondary plagioclase in this meteorite range from 2 to 50 μm. The chemical composition of olivine and low‐Ca pyroxene are uniform; Fa in olivine and Fs in low‐Ca pyroxene are, respectively, 19.6 ± 0.2 and 17.0 ± 0.3 (mole%). Huaxi has been classified as an H5 ordinary chondrite, with a shock grade S2, and weathering W0. The weak shock features, rare fractures, and the high porosity (17.6%) indicates that Huaxi is a less compacted meteorite. The preatmospheric radius of Huaxi is ~11 cm, corresponding to ~21 kg. The meteorite experienced a relatively short cosmic‐ray exposure of about 1.6 ± 0.1 Ma. The ⁴He and ⁴⁰Ar retention ages are older than 4.6 Ga implying that Huaxi did not degas after thermal metamorphism on its parent body.  相似文献