Ocean-atmosphere interaction in high southern latitudes     

D.James Baker Jr. 《Dynamics of Atmospheres and Oceans》1979,3(2-4)

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Effects of stem density upon sediment retention by salt marsh cord grass,Spartina alterniflora loisel   总被引：1，自引：0，他引：1  

Mark L. Gleason  Deborah A. Elmer  Natalie C. Pien  John S. Fisher 《Estuaries and Coasts》1979,2(4):271-273

A laboratory experiment was conducted to determine whether retention of waterborne sand by salt marsh cordgrass, Spartina alterniflora Loisel, is directly related to the number of stems per unit area. Waves generated in a trough washed over a sloping beach planted with S. alterniflora sprigs: a range of stem densities (0–108 stems/m²) was examined in separate trials. The amount of sand accumulated after 60 waves is a positive nonlinear function of stem density. The greatest accretion coincided with the highest stem density tested. Shape of the beach profile was also strongly influenced by the number of stems per m².  相似文献   

Geochronology of upper Tertiary volcanic activity in the Andes of north Chile     

Mr. M. C. W. Baker 《International Journal of Earth Sciences》1977,66(1):455-465

25 new K-Ar data are presented for Upper Cenozoic andesites and ignimbrites from the Andes of north Chile between 20° 30 S and 22° 30 S. The original simple volcanic stratigraphy of andesites overlying ignimbrites has been refined. A more complicated stratigraphy, with some andesites predating the ignimbrites, is described. The sequence and timing of volcanic events differ along the length of the north Chilean Andes. Ages of the earliest widespread ignimbrite eruptions range from 21 m. y. to 10 m. y., in different segments of the volcanic chain. The existence of two large acid extrusives of Quaternary age suggests that generation of acid magmas has continued until recently.

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Zusammenfassung 25 neue K-Ar-Daten von känozoischen Andesiten und Ignimbriten der nordchilenischen Anden zwischen 20° 30 S und 22° 30 S werden vorgestellt. Die ursprünglich einfache Stratigraphie — Andesite überlagern Ignimbrite — wurde verfeinert, und eine komplexere Stratigraphie, bei der einige Andesite älter sind als die Ignimbrite, wird beschrieben. Die Reihenfolge und der zeitliche Ablauf vulkanischer Tätigkeit sind in den nordchilenischen Anden komplex. Die ältesten ausgedehnten Ignimbritdecken reichen in den verschiedenen Abschnitten der Vulkanzone von 21 bis 10 Mio. Jahre. Das Vorhandensein von zwei großen sauren quartären Extrusionszyklen läßt vermuten, daß die Bildung von sauren Magmen bis in die Gegenwart andauerte.

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Resumen Se presentan 25 nuevas edades radiométricas de lavas y ignimbritas Cenozoicas de los Andes del Norte Chileno, entre los meridianos 20° 30 S y 22° 30 S. La estratigrafía primera de las rocas volcanicas (las lavas sobre las ignimbritas) se ha refinado. Se describe una estratigrafia mas complicada, en que algunas lavas antedatan las ignimbritas. La sucesión y las edades de los eventos volcanicos diferen a lo largo de los Andes del Norte Chileno. Las edades de las erupciones mas tempranas y extensivas varian entre 21 M. a. y 10 M. a. en segmentas diferentes de la zona volcanica. La existencia de dos grandes derrames acidos de edad cuaternaria sugere que la producción de magmas acidas continuó hasta el tiempo reciente.

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Résumé On présente 25 valeurs nouvelles sur l'âge radiométrique des andésites et des ignimbrites du Cénozoïque supérieur des Andes du nord du Chili entre les latitudes 20° 30 et 22° 30 S. L'ancienne stratigraphie simplifiée où les andésites surmontent les ignimbrites a été révisée, et remplacée par une stratigraphie plus compliquée où quelques andéseites précèdent les ignimbrites. La succession et la chronologie des éruptions volcaniques diffèrent le long des Andes du nord du Chili. Dans les différentes parties de la chaîne volcanique, l'âge des premières grandes eruptions d'ignimbrites varie entre 21 et 10 M. a. La présence de deux grandes coulées acides d'âge quaternaire permet de supposer que des magmas acides continuent à se former.

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26 ( K/Ar) - 20°30 22°30 . — — , , , . - , , . 21 22 . , .

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Petrology and geochemistry of Easter Island     

P. E. Baker  F. Buckley  J. G. Holland 《Contributions to Mineralogy and Petrology》1974,44(2):85-100

Easter Island has developed around three volcanoes—Poike, an older (3 m.y.) strato-volcano, Rano Kau, a caldera, and the fissure complex of Terevaka and its associated cones. The lavas show a wide compositional spread from tholeiites and olivine tholeiites to hawaiites, mugearites, benmoreites, trachytes and rhyolites (comendites). Hawaiite is by far the most abundant rock type and trachytes and rhyolites are relatively rare. Intermediate and acid rocks are concentrated in the southwestern part of the island on or around Rano Kau.The basaltic rocks, which are plagioclase-phyric or aphyric, are transitional hypersthenenormative types characterized by high contents of Fe, Ti and Zr but low K and Mg. The Poike basalts are marginally lower in Zr, Nb, Y and Zn compared with those of the younger volcanoes, but the trachytes from this centre show anomalously high concentrations of Rb, Zr and Nb.The island's youngest flow, the Roiho basalt, is an olivine tholeiite with distinctly more alkaline affinities: it is olivine-microphyric with relatively high contents of Mg, Ni and K.The study was initiated whilst this author was at Department of Geology and Mineralogy, University of Oxford.  相似文献   

Characterizing the effects of policy instruments on the future costs of carbon capture for coal power plants     

Gregory F. Nemet  Erin Baker  Bob Barron  Samuel Harms 《Climatic change》2015,133(2):155-168

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Whole-disk spectrophotometric properties of Mercury: Synthesis of MESSENGER and ground-based observations     

Deborah L. Domingue  Faith Vilas  Johan Warell  Scott L. Murchie  David T. Blewett  Brian J. Anderson 《Icarus》2010,209(1):101-124

Disk-integrated and disk-resolved measurements of Mercury’s surface obtained by both the Mercury Dual Imaging System (MDIS) and the Mercury Atmospheric and Surface Composition Spectrometer (MASCS) onboard the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft were analyzed and compared with previous ground-based observations of Mercury at 11 wavelengths. The spectra show no definitive absorption features and display a red spectral slope (increasing reflectance with increasing wavelength) typical of space-weathered rocky surfaces. The MDIS spectra show evidence of phase reddening, which is not observed in the MASCS spectra. The MDIS spectra are commensurate with ground-based observations to within 10%, whereas the MASCS spectra display greater discrepancies with ground-based observations at near-infrared wavelengths. The derived photometric calibrations provide corrections within 10% for observations taken at phase angles less than ∼100°. The derived photometric properties are indicative of a more compact regolith than that of the lunar surface or of average S-type asteroids. The photometric roughness of the surface is also much smoother than the Moon’s. The calculated geometric albedo (reflectance at zero phase) is higher than lunar values. The lower reflectance of immature units on Mercury compared with immature units on the Moon, in conjunction with the higher geometric albedo, is indicative of more complicated grain structures within Mercury’s regolith.  相似文献   

Flow patterns of lobate debris aprons and lineated valley fill north of Ismeniae Fossae, Mars: Evidence for extensive mid-latitude glaciation in the Late Amazonian     

David M.H. Baker  James W. Head 《Icarus》2010,207(1):186-209

A variety of Late Amazonian landforms on Mars have been attributed to the dynamics of ice-related processes. Evidence for large-scale, mid-latitude glacial episodes existing within the last 100 million to 1 billion years on Mars has been presented from analyses of lobate debris aprons (LDA) and lineated valley fill (LVF) in the northern and southern mid-latitudes. We test the glacial hypothesis for LDA and LVF along the dichotomy boundary in the northern mid-latitudes by examining the morphological characteristics of LDA and LVF surrounding two large plateaus, proximal massifs, and the dichotomy boundary escarpment north of Ismeniae Fossae (centered at 45.3°N and 39.2°E). Lineations and flow directions within LDA and LVF were mapped using images from the Context (CTX) camera, the Thermal Emission Imaging Spectrometer (THEMIS), and the High Resolution Stereo Camera (HRSC). Flow directions were then compared to topographic contours derived from the Mars Orbiter Laser Altimeter (MOLA) to determine the down-gradient components of LDA and LVF flow. Observations indicate that flow patterns emerge from numerous alcoves within the plateau walls, are integrated over distances of up to tens of kilometers, and have down-gradient flow directions. Smaller lobes confined within alcoves and superposed on the main LDA and LVF represent a later, less extensive glacial phase. Crater size-frequency distributions of LDA and LVF suggest a minimum (youngest) age of 100 Ma. The presence of ring-mold crater morphologies is suggestive that LDA and LVF are formed of near-surface ice-rich bodies. From these observations, we interpret LDA and LVF within our study region to result from formerly active debris-covered glacial flow, consistent with similar observations in the northern mid-latitudes of Mars. Glacial flow was likely initiated from the accumulation and compaction of snow and ice on plateaus and in alcoves within the plateau walls as volatiles were mobilized to the mid-latitudes during higher obliquity excursions. Together with similar analyses elsewhere along the dichotomy boundary, these observations suggest that multiple glacial episodes occurred in the Late Amazonian and that LDA and LVF represent significant reservoirs of non-polar ice sequestered below a surface lag for hundreds of millions of years.  相似文献   

Mercury’s magnetospheric magnetic field after the first two MESSENGER flybys     

Igor I. Alexeev  Elena S. Belenkaya  Haje Korth  Daniel N. Baker  Catherine L. Johnson  Menelaos Sarantos 《Icarus》2010,209(1):23-1862

The “paraboloid” model of Mercury’s magnetospheric magnetic field is used to determine the best-fit magnetospheric current system and internal dipole parameters from magnetic field measurements taken during the first and second MESSENGER flybys of Mercury on 14 January and 6 October 2008. Together with magnetic field measurements taken during the Mariner 10 flybys on 29 March 1974 and 16 March 1975, there exist three low-latitude traversals separated in longitude and one high-latitude encounter. From our model formulation and fitting procedure a Mercury dipole moment of 196 nT ·  (where R_M is Mercury’s radius) was determined. The dipole is offset from Mercury’s center by 405 km in the northward direction. The dipole inclination to Mercury’s rotation axis is relatively small, ∼4°, with an eastern longitude of 193° for the dipole northern pole. Our model is based on the a priori assumption that the dipole position and the moment orientation and strength do not change in time. The root mean square (rms) deviation between the Mariner 10 and MESSENGER magnetic field measurements and the predictions of our model for all four flybys is 10.7 nT. For each magnetic field component the rms residual is ∼6 nT or about 1.5% of the maximum measured magnetic field, ∼400 nT. This level of agreement is possible only because the magnetospheric current system parameters have been determined separately for each flyby. The magnetospheric stand-off distance, the distance from the planet’s center to the inner edge of the tail current sheet, the tail lobe magnetic flux, and the displacement of the tail current sheet relative to the Mercury solar-magnetospheric equatorial plane have been determined independently for each flyby. The magnetic flux in the tail lobes varied from 3.8 to 5.9 MWb; the subsolar magnetopause stand-off distance from 1.28 to 1.43 R_M; and the distance to the inner edge of the current sheet from 1.23 to 1.32 R_M. The differences in the current systems between the first and second MESSENGER flybys are attributed to the effects of strong magnetic reconnection driven by southward interplanetary magnetic field during the latter flyby.  相似文献   

Elevated concentrations of formate, acetate and dissolved organic carbon found at the Lost City hydrothermal field   总被引：1，自引：0，他引：1  

Susan Q. Lang  David A. Butterfield  Deborah S. Kelley 《Geochimica et cosmochimica acta》2010,74(3):941-5748

Fluids from the ultramafic-hosted Lost City hydrothermal field were analyzed for total dissolved organic carbon and dissolved organic acids. Formate (36-158 μmol/kg) and acetate (1-35 μmol/kg) concentrations are higher than in other fluids from unsedimented hydrothermal vents, and are a higher ratio of the total dissolved organic carbon than has been found in most marine geothermal systems. Isotopic evidence is consistent with an abiotic formation mechanism for formate, perhaps during serpentinization processes in the sub-surface. Further support comes from previous studies where the abiological formation of low molecular weight organic acids has been shown to be thermodynamically favorable during hydrothermal alteration of olivine, and laboratory studies in which the reduction of carbon dioxide to formate has been confirmed. As the second most prevalent carbon species after methane, formate may be an important substrate to microbial communities in an environment where dissolved inorganic carbon is limited. Acetate is found in locations where sulfate reduction is believed to be important and is likely to be a microbial by-product, formed either directly by autotrophic metabolic activity or indirectly during the fermentative degradation of larger organic molecules. Given the common occurrence of exposed ultramafic rocks and active serpentinization within the worlds ocean basins, the abiotic formation of formate may be an important process supporting life in these high pH environments and may have critical implications to understanding the organic precursors from which life evolved.  相似文献   

Thallium isotope variations in an ore-bearing continental igneous setting: Collahuasi Formation, northern Chile     

R.G.A. Baker  M. Rehkämper  C. Ihlenfeld  R. Coggon 《Geochimica et cosmochimica acta》2010,74(15):4405-4416

Thallium is a highly incompatible element and a large fraction of the bulk silicate Earth Tl budget is, therefore, expected to reside in the continental crust. Nonetheless, the Tl isotope systematics of continental rocks are essentially unexplored at present. Here, we present new Tl isotope composition and concentration data for a suite of 36 intrusive and extrusive igneous rocks from the vicinity of porphyry Cu deposits in the Collahuasi Formation of the Central Andes in northern Chile. The igneous lithologies of the rocks are variably affected by the hydrothermal alteration that accompanied the formation of the Cu deposits.The samples display Tl concentrations that vary by more than an order of magnitude, from 0.1 to 3.2 μg/g, whilst ε²⁰⁵Tl ranges between −5.1 and +0.1 (ε²⁰⁵Tl is the deviation of the ²⁰⁵Tl/²⁰³Tl isotope ratio of a sample from a standard in parts per 10⁴). These variations are primarily thought to be a consequence of hydrothermal alteration processes, including metasomatic transport of Tl, and formation/breakdown of Tl-bearing minerals, which are associated with small but significant Tl isotope effects. The Tl abundances show excellent correlations with both K and Rb concentrations but no co-variation with Cu. This demonstrates that Tl displays only limited chalcophile affinity in the continental crust of the Collahuasi Formation, but behaves as a lithophile element with a distribution that is primarily governed by partitioning of Tl⁺ into K⁺-bearing phases. Collahuasi samples with propylitic alteration features, which are derived from the marginal parts of the hydrothermal systems, have, on average, slightly lighter Tl isotope compositions than rocks from the more central sericitic and argillic alteration zones. This small but statistically significant difference most likely reflects preferential retention of isotopically heavy Tl in alteration phases, such as white micas and clays, which formed during sericitic and argillic alteration.  相似文献