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  • 1
    Online Resource
    Online Resource
    Münster : Inst. für Infektiologie, Zentrum für Molekularbiologie der Entzündung, Westfäl. Wilhelms-Univ.
    Keywords: Forschungsbericht
    Description / Table of Contents: Molecular biology, pertussis toxin, membrane-anchored synthetic peptides, epitope-mapping, ADP-ribosylation, G-proteins, retrograde transport, diagnosis
    Type of Medium: Online Resource
    Pages: 22 p. = 245 kB, text and images
    Edition: [Electronic ed.]
    Language: German , English
    Note: Contract No.: BMBF 01KI 9206/0 , Differences between the printed and electronic version of the document are possible
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  • 2
    Online Resource
    Online Resource
    Berlin, Heidelberg :Springer Berlin / Heidelberg,
    Keywords: Polymers. ; Electronic books.
    Type of Medium: Online Resource
    Pages: 1 online resource (239 pages)
    Edition: 1st ed.
    ISBN: 9783540487647
    Series Statement: Advances in Polymer Science Series ; v.150
    DDC: 547.7/046
    Language: English
    Note: 150 Advances in Polymer Science -- New Developments in Polymer Analytics I -- Copyright -- Preface -- Contents -- Contents of Volume 151 -- Hyphenated Techniques in Liquid Chromatography of Polymers -- Field-Flow Fractionation Techniques for Polymer and Colloid Analysis -- Capillary Electrophoresis in Polymer Analysis -- Author Index Volumes 101-150 -- Subject Index.
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  • 3
    Online Resource
    Online Resource
    San Diego :Elsevier Science & Technology,
    Keywords: Sulfur. ; Electronic books.
    Type of Medium: Online Resource
    Pages: 1 online resource (232 pages)
    Edition: 1st ed.
    ISBN: 9781483158655
    Language: English
    Note: Front Cover -- The Chemistry of Sulphur, Selenium, Tellurium and Polonium -- Copyright Page -- Table of Contents -- PREFACE -- PART 23: SULPHUR -- CHAPTER 1. THE ELEMENT -- 1.1. HISTORY -- 1.2. THE OCCURRENCE OF SULPHUR AND ITS COMPOUNDS -- 1.3. PRODUCTION OF SULPHUR -- 1.4. INDUSTRIAL USE OF SULPHUR -- 1.5. PURIFICATION OF SULPHUR IN LABORATORY SCALE -- 1.6. ALLOTROPE MODIFICATIONS OF SULPHUR -- 1.7. NUCLEAR PROPERTIES OF SULPHUR -- 1.8. PHYSICAL PROPERTIES OF SULPHUR -- 1.9. CHEMISTRY AND CHEMICAL PROPERTIES OF SULPHUR -- 10.1. INTERCHALCOGEN COMPOUNDS (OXIDES EXCLUDED) -- 1.11. BIOLOGICAL ACTIVITIES OF SULPHUR AND ITS COMPOUNDS -- CHAPTER 2. SULPHUR COMPOUNDS -- 2.1. SULPHANES -- 2.2. SULPHUR HALIDES -- 2.3. OXIDES OF SULPHUR -- 2.4. OXYACIDS OF SULPHUR -- 2.5. COMPOUNDS CONTAINING SULPHUR AND NITROGEN -- 2.6. COMPOUNDS COMPOSED OF SULPHUR, NITROGEN AND HALOGEN -- 2.7. COMPOUNDS CONTAINING SULPHUR, NITROGEN, OXYGEN AND HYDROGEN -- 2.8. COMPOUNDS COMPOSED OF SULPHUR, NITROGEN AND CARBON -- 2.9. SULPHUR COMPOUNDS OF Vb ELEMENTS -- 2.10. SULPHUR COMPOUNDS OF IVb ELEMENTS -- 2.11. SULPHUR COMPOUNDS OF GROUP Illb -- 2.12. SULPHUR COMPOUNDS OF GROUP Ia AND IIa ELEMENTS -- 2.13. SULPHUR COMPOUNDS OF TRANSITION ELEMENTS -- 2.14. MOLECULAR TRANSITION METAL SULPHIDES -- 2.15. SULPHUR COMPOUNDS OF LANTHANIDES AND ACTINIDES -- 2.16. ANALYTICAL USE OF HYDROGEN SULPHIDE -- PART 24: SELENIUM, TELLURIUM AND POLONIUM -- CHAPTER 1. THE ELEMENTS -- 1.1 INTRODUCTION AND HISTORICAL -- 1.2. OCCURRENCE AND DISTRIBUTION -- 1.3. PRODUCTION -- 1.4. NDUSTRIAL USES -- 1.5. PURIFICATION -- 1.6. ALLOTROPY -- 1.7. NUCLEAR PROPERTIES -- 1.8. PHYSICAL PROPERTIES OF THE ELEMENTS -- 1.9. CHEMISTRY OF THE ELEMENTS -- 1.10. HEALTH HAZARDS -- 1.11. ANALYTICAL CHEMISTRY -- CHAPTER 2. COMPOUNDS OF THE ELEMENTS -- 2.1. INTRODUCTION -- 2.2. ALLOYS -- 2.3. HYDRIDES. , 2.4. CARBONYL COMPOUNDS -- 2.5. HALIDES -- 2.6. CYANIDES, THIOCYANATES, SELENOCYANATES AND BISTRIFLUOROMETHYL NITROXIDES -- 2.7. OXIDES AND PEROXIDES -- 2.8. HYDROXIDES AND OXO-ACIDS -- 2.9. SULPHIDES -- 2.10. NITRIDES AND AZIDES -- 2.11. CARBON SELENIDES AND TELLURIDE -- 2.12. CARBONATES -- 2.13. SALTS OF ORGANIC ACIDS -- 2.14. ALKOXIDES -- 2.15. NITRATES -- 2.16. PHOSPHATES -- 2.17. SULPHATES, SELENATES AND TELLURATES -- 2.18. "SULPHOXIDES" AND "SELENOXIDES -- 2.19. CHROMATES -- 2.20. HALATES AND PERHALATES -- 2.21. ORGANO-COMPOUNDS -- 2.22. COMPLEXES -- INDEX -- Contents of Comprehensive Inorganic Chemistry -- INDEPENDENT OPINION.
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  • 4
    In: Geochimica et cosmochimica acta, New York, NY [u.a.] : Elsevier, 1950, 68(2004), 21, Seite 4405-4427, 0016-7037
    In: volume:68
    In: year:2004
    In: number:21
    In: pages:4405-4427
    Description / Table of Contents: During ODP Leg 193, 4 sites were drilled in the active PACMANUS hydrothermal field on the crest of the felsic Pual Ridge to examine the vertical and lateral variations in mineralization and alteration patterns. We present new data on clay mineral assemblages, clay and whole rock chemistry and clay mineral strontium and oxygen isotopic compositions of altered rocks from a site of diffuse low-temperature venting (Snowcap, Site 1188) and a site of high-temperature venting (Roman Ruins, Site 1189) in order to investigate the water-rock reactions and associated elemental exchanges. The volcanic succession at Snowcap has been hydrothermally altered, producing five alteration zones: (1) chlorite ± illite-cristobalite-plagioclase alteration apparently overprinted locally by pyrophyllite bleaching at temperatures of 260-310°C; (2) chlorite ± mixed-layer clay alteration at temperatures of 230°C; (3) chlorite and illite alteration; (4) illite and chlorite ± illite mixed-layer alteration at temperatures of 250-260°C; and (5) illite ± chlorite alteration at 290-300°C. Felsic rocks recovered from two holes (1189A and 1189B) at Roman Ruins, although very close together, show differing alteration features. Hole 1189A is characterized by a uniform chlorite-illite alteration formed at 2̃50°C, overprinted by quartz veining at 350°C. In contrast, four alteration zones occur in Hole 1189B: (1) illite ± chlorite alteration formed at 3̃00°C; (2) chlorite ± illite alteration at 235°C; (3) chlorite ± illite and mixed layer clay alteration; and (4) chlorite ± illite alteration at 220°C. Mass balance calculations indicate that the chloritization, illitization and bleaching (silica-pyrophyllite assemblages) alteration stages are accompanied by different chemical changes relative to a calculated pristine precursor lava. The element Cr appears to have a general enrichment in the altered samples from PACMANUS. The clay concentrate data show that Cr and Cu are predominantly present in the pyrophyllites. Illite shows a significant enrichment for Cs and Cu relative to the bulk altered samples. Considerations of mineral stability allow us to place some constraints on fluid chemistry. Hydrothermal fluid pH for the chloritization and illitization was neutral to slightly acidic and relatively acidic for the pyrophyllite alteration. In general the fluids, especially from Roman Ruins and at intermediate depths below Snowcap, show only a small proportion of seawater mixing (〈10%). Fluids in shallow and deep parts of the Snowcap holes, in contrast, show stronger seawater influence.
    Type of Medium: Online Resource
    Pages: graph. Darst
    ISSN: 0016-7037
    Language: English
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  • 5
    Publication Date: 2022-09-27
    Description: Calcareous foraminifer shells (tests) represent one of the most important archives for paleoenvironmental and paleoclimatic reconstruction. To develop a mechanistic understanding of the relationship between environmental parameters and proxy signals, knowledge of the fundamental processes operating during foraminiferal biomineralization is essential. Here, we apply microscopic and diffraction‐based methods to address the crystallographic and hierarchical structure of the test wall of different hyaline foraminifer species. Our results show that the tests are constructed from micrometer‐scale oriented mesocrystals built of nanometer‐scale entities. Based on these observations, we propose a mechanistic extension to the biomineralization model for hyaline foraminifers, centered on the formation and assembly of units of metastable carbonate phases to the final mesocrystal via a non‐classical particle attachment process, possibly facilitated by organic matter. This implies the presence of metastable precursors such as vaterite or amorphous calcium carbonate, along with phase transitions to calcite, which is relevant for the mechanistic understanding of proxy incorporation in the hyaline foraminifers.
    Description: Plain Language Summary: Foraminifers are single celled marine organisms typically half a millimeter in size, which form shells made of calcium carbonate. During their life, the chemical composition of their shells records environmental conditions. By analyzing fossil shells, past conditions can be reconstructed to understand ancient oceans and climate change. To do that correctly, we need to know exactly how foraminifers form their shell. We find that foraminifers build micrometer‐sized mesocrystals which are made of smaller building blocks. This means that the smallest building blocks form first and assemble to form a larger grain, which is oriented in a specific direction. To align all the building blocks, it is possible that they are first unstable and undergo transformation on assembly, during which their composition may change. By understanding and quantifying this process, the composition of the final fossil shell may be understood, ultimately leading to more reliable reconstructions of past environmental change.
    Description: Key Points: Hyaline foraminiferal shells are built of micrometer sized mesocrystalline units. Biomineralization likely includes the formation and assembly of nanoparticles. Nanometer sized units suggest non‐classical crystal growth.
    Description: https://doi.org/10.17617/3.D7HN3I
    Keywords: ddc:561.9 ; ddc:549
    Language: English
    Type: doc-type:article
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  • 6
    Publication Date: 2020-02-12
    Language: English
    Type: info:eu-repo/semantics/article
    Format: application/pdf
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  • 7
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    In:  International Symposium on Advancing Geodesy in a Changing World : Proceedings of the IAG Scientific Assembly, Kobe, Japan, July 30 – August 4, 2017 | International Association of Geodesy symposia ; 149
    Publication Date: 2020-02-12
    Description: The thermosphere causes by far the largest non-gravitational perturbing acceleration of near-Earth orbiting satellites. Especially between 80 km and 1,000 km, the thermospheric density distribution and variations are required to model accurately this acceleration for precise orbit determination (POD), ephemeris computation and re-entry prediction of the Low-Earth Orbiting (LEO) satellites. So far, mostly on-board accelerometers are used to measure the thermospheric density. However, such type of satellite is usually of complex shape and any error or mismodelling in the satellite drag coefficient and satellite effective cross-sectional area will directly propagate into the derived thermospheric density values. At GFZ, an empirical model of the thermospheric mass density denoted as “CH-Therm-2018” has been developed by using 9 years (2001–2009) of CHAMP observations. A completely different approach for thermospheric density determination is based on using satellite laser ranging (SLR) measurements to LEO satellites equipped with retro-reflectors to determine an accurate satellite orbit. These measurements are sensitive to small perturbations acting on the satellite. In order to minimize the error induced by imprecise satellite macro-models, we use in our investigation SLR observations to satellites with a simple spherical shape and thus, relate estimated scaling factors to the thermospheric density. In this paper, we use SLR observations to two ANDE-2 satellites – ANDE-Castor and ANDE-Pollux – as well as SpinSat with altitudes between 248 km and 425 km to calibrate the CH-Therm-2018 model, as well as four other empirical models of thermospheric density, namely CIRA86, NRLMSISE00, JB2008 and DTM2013. For our tests, we chose a period from 16 August 2009 to 26 March 2010 of low solar activity and a period from 29 December 2014 to 29 March 2015 of high solar activity. Using data of a few geodetic satellites obtained at the same and different time intervals allows us to investigate the reliability of the scaling factors of the thermospheric densities provided by the models. We have found that CIRA86 and NRLMSISE00 most significantly overestimate the thermospheric density at the period of low solar activity among the models tested. The JB2008 model is the least scaled model and provides reliable values of the thermospheric density for the periods of both low and high solar activity. The GFZ CH-Therm-2018 model, on the contrary, underestimates the thermospheric density at the time interval of low solar activity. Using SLR observations at longer time intervals should allow to investigate temporal evolution of the scaling factors of these models more precisely.
    Language: English
    Type: info:eu-repo/semantics/bookPart
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  • 8
    Publication Date: 2020-02-12
    Language: English
    Type: info:eu-repo/semantics/bookPart
    Format: application/pdf
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  • 9
    Publication Date: 2022-02-08
    Description: The following authors were omitted from the original version of this Data Descriptor: Markus Reichstein and Nicolas Vuichard. Both contributed to the code development and N. Vuichard contributed to the processing of the ERA-Interim data downscaling. Furthermore, the contribution of the co-author Frank Tiedemann was re-evaluated relative to the colleague Corinna Rebmann, both working at the same sites, and based on this re-evaluation a substitution in the co-author list is implemented (with Rebmann replacing Tiedemann). Finally, two affiliations were listed incorrectly and are corrected here (entries 190 and 193). The author list and affiliations have been amended to address these omissions in both the HTML and PDF versions. © 2021, This is a U.S. government work and not under copyright protection in the U.S.; foreign copyright protection may apply.
    Language: English
    Type: info:eu-repo/semantics/article
    Format: application/pdf
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  • 10
    Publication Date: 2020-02-12
    Description: In this study, we present an empirical model, named CH-Therm-2018, of the thermospheric mass density derived from 9-year (from August 2000 to July 2009) accelerometer measurements from the CHAllenging Mini-satellite Payload (CHAMP) satellite at altitudes from 460 to 310km. The CHAMP dataset is divided into two 5-year periods with 1-year overlap (from August 2000 to July 2005 and from August 2004 to July 2009) to represent the high-to-moderate and moderate-to-low solar activity conditions, respectively. The CH-Therm-2018 model describes the thermospheric density as a function of seven key parameters, namely the height, solar flux index, season (day of year), magnetic local time, geographic latitude and longitude, as well as magnetic activity represented by the solar wind merging electric field. Predictions of the CH-Therm-2018 model agree well with CHAMP observations (within 20%) and show different features of thermospheric mass density during the two solar activity levels, e.g., the March–September equinox asymmetry and the longitudinal wave pattern. From the analysis of satellite laser ranging (SLR) observations of the ANDE-Pollux satellite during August–September 2009, we estimate 6h scaling factors of the thermospheric mass density provided by our model and obtain the median value equal to 1.267±0.60. Subsequently, we scale up our CH-Therm-2018 mass density predictions by a scale factor of 1.267. We further compare the CH-Therm-2018 predictions with the Naval Research Laboratory Mass Spectrometer Incoherent Scatter Radar Extended (NRLMSISE-00) model. The result shows that our model better predicts the density evolution during the last solar minimum (2008–2009) than the NRLMSISE-00 model.
    Language: English
    Type: info:eu-repo/semantics/article
    Format: application/pdf
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