The origin of high-amplitude magnetic anomalies at the intersection of the Juan de Fuca ridge and Blanco fracture zone     

Robert S. Detrick  Walter S. Lynn 《Earth and Planetary Science Letters》1975,26(1):105-113

The intersection of the Juan de Fuca ridge and Blanco fracture zone is characterized by unusually high amplitude magnetic anomalies (over 1500 nT) which appear to be associated with a body roughly 50 km in length and 20 km in width aligned along the fracture zone. Simple three-dimensional magnetic models indicate that this anomaly is probably caused by a highly magnetized block of material situated in the western end of the Blanco fracture zone near its intersection with the Juan de Fuca ridge. Rock magnetization studies of tholeiitic basalts dredged from this area confirm the presence of highly magnetized basalts near the ridge crest/transform fault intersection. These tholeiitic basalts are enriched in iron and titanium relative to “normal” oceanic tholeiites, apparently the result of extensive shallow fractionation involving olivine, plagioclase, and clinopyroxene. Magnetic model studies indicate that an average thickness of no more than 500 m of these iron-rich basalts is necessary to produce the observed anomaly pattern. Comparison of these basalts with samples previously dredged from the Juan de Fuca ridge crest suggests that these Fe-rich, highly magnetized basalts probably “leaked” out of the southernmost portion of the Juan de Fuca ridge.  相似文献   

Zur Stratigraphie,Petrologie und Genese einer Bentonit-Lage aus dem oberen Mittel-Turon (Oberkreide) des südöstlichen Münsterlandes     

Dr. Ekbert Seibertz  Dr. Walter Vortisch 《International Journal of Earth Sciences》1979,68(2):649-679

Zusammenfassung Die Bentonit-Lage kann möglicherweise mit der Lage M₆₈ aus dem Turon von Lüneburg (Norddeutschland) korreliert werden. Identifiziert wurden vulkanische Glasfragmente, Quarz, Na-, K-Feldspat, Oligoklas, Biotit, Muskovit, Calcit, Schwerminerale (u. a. Olivin, Hornblende) und Tonminerale (Kaolinit, Illit, mixed-layer Illit/Smektit, FeBeidellit - z. T. in großen Aggregaten). Die vulkanoklastischen Gläser zeigen alle Übergänge von intakt zu völlig devitriert. Mit Hilfe der Elektronenstrahl-Mikrosonde konnten, bei Berücksichtigung der Kathoden-Lumineszenz, die Feldspäte chemisch analysiert und genetisch in solche mit niedrigerer und solche mit höherer (vulkanoklastisch) Bildungstemperatur gegliedert werden. Von den Schwermineralen dürften vor allem Olivin und Hornblende vulkanogener Herkunft sein. Untersuchungen der durch Umwandlung vulkanischen Materials entstandenen kompakten Smektit-Aggregate mittels Mikrosonde, Röntgendiffraktometrie und Mössbauer-Spektroskopie zeigten, daß es sich hier um ein AI-reiches Glied der Mischungsreihe Nontronit-Beidellit (Fe-reicher Beidellit) handelt. Differentialthermoanalytische Untersuchungen ergaben für Fe-reiche, dioktaedrische, smektitische Tonminerale typische Kurven. Das Ausgangsmaterial des Bentonits war intermediär bis basisch. Äolischer oder kombiniert äolischer und mariner Transport von Exhalationspunkten im mitteleuropäischen Raum werden diskutiert.

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The bentonite can probably be correlated with horizon M₆₈ in the Turonian of Lüneburg in northern Germany. Volcanic glass fragments, quartz, Na and K feldspars, oligoclase, biotite, muscovite, calcite, heavy minerals (i. a. olivine, hornblende) and clay minerals (kaolinite, illite, mixed-layer illite/smectite and Fe-beidellite) were identified. The glass shows a spectrum of all states from unaltered to completely devitrified. Analysis of feldspars by means of electron microprobe and cathodo-luminescence has allowed to divide them into genetically high (pyroclastic) and low temperature forms. Of the heavy minerals, olivine and hornblende most clearly are of volcanic origin. Examinations of smectite aggregates (alteration products of volcanic material) by electron microprobe, x-ray diffractometry, and Mössbauer spectroscopy demonstrated the presence of a member of the continuous series nontronite-beidellite (Fe-rich beidellite). Differential thermal analysis gave typical curves for dioctahedral Fe-rich smectites. The chemical composition of the original material of the bentonite was intermediate to basic. Eolian or eolian and marine current transport from sources in central Europe are considered.

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Résumé La couche de bentonite peut probablement être corrélée avec la couche M₆₈ du Turonien de Lunebourg (au nord de l'Allemagne). Des fragments de verre volcanique, du quartz, du feldspath sodique, du feldspath potassique, de l'oligoclase de la biotite, de la muscovite, de la calcite, des minéraux lourds (p. ex. olivine, hornblende) et des minéraux argileux (kaolinite, illite, mixed-layer illite/smectite, beidellite ferreux — en partie en grands agrégates) ont été identifiés. Les verres pyroclastiques montrent tous les passages du verre intact jusqu'au verre entièrement dévitrifié. A l'aide de la microsonde électronique et en prenant en considération la cathodoluminescence, les feldspaths pouvaient être analysés chimiquement et ordonnés génétiquement selon leur température de formation. Ceux à haute temperature de formation sont pyroclastiques. Parmi les minéraux lourds pouvaient avant tout être d'origine volcanogène, l'olivine et la hornblende. Les études des agrégats de smectites compacts formés par la transformation de matériaux volcaniques montrent grâce à la microsonde, la diffractométrie X et de la spectrométrie de Mössbauer qu'il s'agit dans ce cas là d'un membre riche en Al de la série des mélanges nontronite-beidellite (beidellite ferreux). Des analyses thermiques différentielles donnèrent des courbes typiques pour les minéraux argileux smectitiques, dioctaédriques et riches en Fe. La matière de base de la bentonite était intermédiaire à basique. Transport éolien ou transport combiné, éolien et marin des points d'exhalation dans l'espace européen central seront dicutés.

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Polycyclic aromatic hydrocarbons in Recent lake sediments—I. Compounds having anthropogenic origins     

Stuart G. Wakeham  Christian Schaffner  Walter Giger 《Geochimica et cosmochimica acta》1980,44(3):403-413

Polycyclic aromatic hydrocarbons (PAH) in sediment cores from Lake Lucerne, Lake Zürich, and Greifensee, Switzerland, and Lake Washington, northwest U.S.A., have been isolated, identified and quantified by glass capillary gas chromatography and gas chromatography/mass spectrometry. Surface sediment layers are greatly enriched in PAH—up to 40 times—compared to deeper layers. In addition, concentration increases in upper sediments generally correspond to increasing industrialization and urbanization in the catchment basins of the lakes. Few PAH could be detected in pre-industrial revolution sediments, indicating that background levels for most PAH in aquatic sediments are extremely low.These results are consistent with an anthropogenic source for most of the aromatic hydrocarbons present in the modern sediments. A comparison of PAH distributions in the sediments and in possible source materials shows that urban runoff of street dust may be the most important PAH input to these lacustrine sediments. There is evidence that a significant contribution to the PAH content of street dust comes from material associated with asphalt.  相似文献   

Poly cyclic aromatic hydrocarbons in Recent lake sediments—II. Compounds derived from biogenic precursors during early diagenesis     

Stuart G. Wakeham  Christian Schaffner  Walter Giger 《Geochimica et cosmochimica acta》1980,44(3):415-429

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Growth rates of manganese nodules in Oneida Lake,New York     

Willard S. Moore  Walter E. Dean  S. Krishnaswami  D.V. Borole 《Earth and Planetary Science Letters》1980,46(2):191-200

²²⁶Ra is used to document the growth histories of six manganese nodules from Oneida Lake, New York. Detailed sectioning and analysis reveal that there are discontinuous gradients in²²⁶Ra content in these samples. These gradients result from periods of rapid growth (>1 mm/100 years) separated by periods of no growth of erosion. Although the²²⁶Ra “age” of the nodules approximates the age of Oneida Lake, the nodules are not sediment-covered because they occur only in areas of the lake where fine-grained sediments are not accumulating.  相似文献   

An assessment of the use of stabilized coal and oil ash for construction of artificial fishing reefs: Comparison of fishes observed on small ash and concrete reefs   总被引：2，自引：0，他引：2  

Frederic E. Vose  Walter G. Nelson   《Marine pollution bulletin》1998,36(12):980-988

Fishes present on small artificial reefs located 2 km off the central east coast of Florida (USA) were surveyed to determine the acceptability of using stabilized oil and coal ash residue as a component material in construction of artificial fishing reefs. Species richness was not significantly different over 2.5 yr on stabilized oil and coal ash reefs compared to concrete control reefs. Of 19 species tested for significant differences in mean abundance, lane snapper was observed at significantly higher mean abundances on fossil-fuel ash reefs (stabilized oil ash/coal fly ash), while three reef species (hairy blenny, porkfish and gray snapper) were significantly more common on concrete control reefs. Further study is needed to determine whether contaminants (Cu, V, Ni and Zn) from stabilized ash blocks can cause abundance differences for some fishes. Plausible alternate explanations for the differences in mean abundance include both interspecific interactions (competition and predation) and differences in the attraction or retention of fish among reef replicates due to slight variations in reef dimensions.  相似文献   

Distribution and source of tar on the Pacific Ocean     

C.S Wong  David R Green  Walter J Cretney 《Marine pollution bulletin》1976,7(6):102-106

Petroleum residues, or tar lumps, are concentrated in the northwestern portion of the Pacific Ocean, particularly in the Kuroshio current system. The source of the tar appears to be tank washings from tankers on the very large Middle East to Japan route. Tar pollutants apparently are discharged by tankers south of Japan, become entrained in the Kuroshio current, and create a plume of contamination which extends downstream for 7000 km across the Pacific.  相似文献   

Complex formation in the ternary system Mg(II)-CO₂-H₂O     

Walter Riesen  Heinz Gamsjäger  Paul W. Schindler 《Geochimica et cosmochimica acta》1977,41(9):1193-1200

The carbonato and hydrogencarbonato complexes of Mg²⁺ were investigated at 25 and 50° in solutions of the constant ClO₄^? molality (3 M) consisting preponderantly of NaClO₄. The experimental data could be explained assuming the following equilibria: Mg²⁺ + CO_2B + H₂O ag MgHCO⁺₃ + H⁺, $\text{log}{}^1\text{β}{}_1\text{= ?7.64}{}_4\text{± 0.01}{}_7\text{(25°), ?7.46}{}_2\text{± 0.01}{}_1\text{(50°)}$, Mg²⁺ + 2 CO_2g + 2 H₂Oag Mg(HCO₃)⁰₂ ± 2 H⁺, $\text{log}{}^1\text{β}{}_2\text{= ?15.00 ± 0.14 (25°)}$, ?15.37 ± 0.39 (50°), Mg²⁺ + CO_2g + H₂Oag MgCO⁰₃ + 2 H⁺, $\text{log}{}^1\text{k}{}_1\text{= ?15.64 ± 0.06 (25°)}$,?15.23 ± 0.02 (50°), with the assumption γ_MgCO3⁰ = γ_Mg(HCO3)⁰2, ΔG⁰(I = 0) for the reaction MgCO⁰₃ + CO_2g + H₂O = Mg(HCO₃)⁰₂ was estimated to be ?3.9₁ ± 0.8₆ and 0.6 ± 2.4 kJ/mol at 25 and 50°C, respectively. The abundance of carbonate linked Mg(II) species in fresh water systems is discussed.  相似文献   

Biogeochemistry of Mono Lake,California     

Walter E. Reed 《Geochimica et cosmochimica acta》1977,41(9):1231-1245

Modern sediments of Mono Lake show marked variation in lipid composition with depositional environment. Constituents derived from the drainage basin, characterized by high molecular weight alkane hydrocarbons (C₂₅–C₃₁), and the steroids β-sitosterol and brassicasterol, predominate in near-shore environments. In the deepest part of the lake, sediments exhibit a combination of externally-derived constituents, and lipids derived from the lake biota; the latter characterized by low molecular-weight alkanes and alkenes (C₁₅–C₁₇), phytane, and the steroids ergost-7-en-3β-ol and 24-ethylcholest-7-en-3-β-ol. Steranes, 4-methylsteranes, and the C₁₈ and C₁₉ isoprenoids appear to be forming in the intensely reducing bottom sediments at the present time.The compositions of samples from the Pleistocene succession of Mono Basin suggest that sample-to-sample variation within the same stratum is negligible so long as unweathered samples from the same depositional environment are compared. Sediments having equivalent lithologies may or may not have similar compositions, but sediments having similar fossil contents do show similar lipid compositions. Subaerial weathering of sediments causes a marked decrease in the amount of extractable organic material, as well as distinct changes in its hydrocarbon composition. Specifically, weathered sediments exhibit a decrease in relative content of low molecular weight hydrocarbons and a relative increase in nC₂₂.Organic composition of sediments from the Pleistocene stratigraphie column cannot be correlated with depth of burial. Compositional changes with stratigraphie position are probably related to paleo-ecological factors such as population or productivity rather than depth of burial. Lithology and organic composition provide mutually-corroborating evidence regarding glacial advances in the adjacent Sierra Nevada Mountains. During glaciations, the lake sediments are rich in sandstones, and the organic composition shows a predominance of externally-derived debris, with no evidence for contributions from the lake biota.  相似文献   

Variations in 24-μm morphologies among galaxies in the Spitzer Infrared Nearby Galaxies Survey: new insights into the Hubble sequence     

G. J. Bendo  D. Calzetti  C. W. Engelbracht  R. C. Kennicutt Jr    M. J. Meyer  M. D. Thornley  F. Walter  D. A. Dale  A. Li  E. J. Murphy 《Monthly notices of the Royal Astronomical Society》2007,380(4):1313-1334

To study the distribution of star formation and dust emission within nearby galaxies, we measured five morphological parameters in the 3.6- and 24-μm wavebands for 65 galaxies in the Spitzer Infrared Nearby Galaxies Survey (SINGS) and eight galaxies that were serendipitously observed by SINGS. The morphological parameters demonstrate strong variations along the Hubble sequence, including statistically significant differences between S0/a-Sab and Sc-Sd galaxies. Early-type galaxies are generally found to be compact, centralized, symmetric sources in the 24-μm band, while late-type galaxies are generally found to be extended, asymmetric sources. These results suggest that the processes that increase the real or apparent sizes of galaxies' bulges also lead to more centralized 24-μm dust emission. Several phenomena, such as strong nuclear star formation, Seyfert activity, or outer ring structures, may cause galaxies to deviate from the general morphological trends observed at 24 μm. We also note that the 24-μm morphologies of Sdm-Im galaxies are quite varied, with some objects appearing very compact and symmetric but others appearing diffuse and asymmetric. These variations reflect the wide variation in star formation in irregular galaxies as observed at other wavelengths. The variations in the 24-μm morphological parameters across the Hubble sequence mirror many of the morphological trends seen in other tracers of the ISM and in stellar emission. However, the 24-μm morphological parameters for the galaxies in this sample do not match the morphological parameters measured in the stellar wavebands. This implies that the distribution of dust emission is related to but not equivalent to the distribution of stellar emission.  相似文献