Bücher- und Zeitschriftenschau     

Bubnoff  L. Rutten  Ernst Habetha  Kienow  Strassl  Konrad Richter  Stickel  Gallwitz  Wilckens 《International Journal of Earth Sciences》1937,28(8):629-641

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Non-destructive porosity determinations of antarctic marine sediments derived from resistivity measurements with an inductive method     

S. Gerland  M. Richter  H. Villinger  G. Kuhn 《Marine Geophysical Researches》1993,15(3):201-218

The fractional porosity of marine sediments is one of the fundamental index properties of rocks. For the determination of porosity a nondestructive, inductive method was used on unsplit sediment cores. The results were compared with galvanically measured resistivities using a miniature Wenner array on split cores. The measurements agree well except for cores with high clay content where measurement frequency related effects cause a resistivity difference of about 10%. Porosities were derived from resistivities using a published resistivity-porosity relationship by Boyce (1968) and compared with sample porosities. A comparison of both data sets shows good agreement.  相似文献   

Crystallization of melilite from CMAS-liquids and the formation of the melilite mantle of Type B1 CAIs: Experimental simulations     

Ruslan A. Mendybaev  Frank M. Richter  Andrew M. Davis 《Geochimica et cosmochimica acta》2006,70(10):2622-2642

Type B CAIs are subdivided into B1s, with well-developed melilite mantles, and B2s, with randomly distributed melilite. Despite intensive study, the origin of the characteristic melilite mantle of the B1s remains unclear. Recently, we proposed that formation of the melilite mantle is caused by depletion of the droplet surface in volatile magnesium and silicon due to higher evaporation rates of volatile species compared to their slow diffusion rates in the melt, thus making possible crystallization of melilite at the edge of the CAI first, followed by its crystallization in the central parts at lower temperatures. Here, we present the results of an experimental study that aimed to reproduce the texture observed in natural Type B CAIs. First, we experimentally determined crystallization temperatures of melilite for three melt compositions, which, combined with literature data, allowed us to find a simple relationship between the melt composition, crystallization temperature, and composition of first crystallizing melilite. Second, we conducted a series of evaporation and cooling experiments exposing CAI-like melts to gas mixtures with different oxygen fugacities (f_O2). Cooling of the molten droplets in gases with logf_O2?IW-4 resulted in crystallization of randomly distributed melilite, while under more reducing conditions, melilite mantles have been formed. Chemical profiles through samples quenched right before melilite started to crystallize showed no chemical gradients in samples exposed to relatively oxidizing gases (logf_O2?IW-4), while the near-surface parts of the samples exposed to very reducing gases (logf_O2?IW-7) were depleted in volatile MgO and SiO₂, and enriched in refractory Al₂O₃. Using these experimental results and the fact that the evaporation rate of magnesium and silicon from CAI-like melts is proportional to , we estimate that Type B1 CAIs could be formed by evaporation of a partially molten precursor in a gas of solar composition with . Type B2 CAIs could form by slower evaporation of the same precursors in the same gas with .  相似文献   

Kinetic isotopic fractionation during diffusion of ionic species in water     

Frank M. Richter  Ruslan A. Mendybaev  Ian D. Hutcheon  Neil C. Sturchio 《Geochimica et cosmochimica acta》2006,70(2):277-289

Experiments specifically designed to measure the ratio of the diffusivities of ions dissolved in water were used to determine . The measured ratio of the diffusion coefficients for Li and K in water (D_Li/D_K = 0.6) is in good agreement with published data, providing evidence that the experimental design being used resolves the relative mobility of ions with adequate precision to also be used for determining the fractionation of isotopes by diffusion in water. In the case of Li, we found measurable isotopic fractionation associated with the diffusion of dissolved LiCl (D_⁷Li/D_⁶Li=0.99772±0.00026). This difference in the diffusion coefficient of ⁷Li compared to ⁶Li is significantly less than that reported in an earlier study, a difference we attribute to the fact that in the earlier study Li diffused through a membrane separating the water reservoirs. Our experiments involving Mg diffusing in water found no measurable isotopic fractionation (D_²⁵Mg/D_²⁴Mg=1.00003±0.00006). Cl isotopes were fractionated during diffusion in water (D_³⁷Cl/D_³⁵Cl=0.99857±0.00080) whether or not the co-diffuser (Li or Mg) was isotopically fractionated. The isotopic fractionation associated with the diffusion of ions in water is much smaller than values we found previously for the isotopic fractionation of Li and Ca isotopes by diffusion in molten silicate liquids. A major distinction between water and silicate liquids is that water surrounds dissolved ions with hydration shells, which very likely play an important but still poorly understood role in limiting the isotopic fractionation associated with diffusion.  相似文献   

The first detection of propane on Saturn     

Thomas K. Greathouse  John H. Lacy  Bruno Bézard  Matthew J. Richter  Claudia Knez 《Icarus》2006,181(1):266-271

We report the first detection of propane, C₃H₈, in Saturn's stratosphere. Observations taken on September 8, 2002 UT at NASA's IRTF using TEXES, show multiple emission lines due to the 748 cm⁻¹ν₂₁ band of C₃H₈. Using a line-by-line radiative transfer code, we are able to fit the data by scaling the propane vertical mixing ratio profile from the photochemical model of Moses et al. [2000. Icarus 143, 244-298]. Multiplicative factors of 0.7 and 0.65 are required to fit the −20° and −80° planetocentric latitude spectra. The resultant profiles are characterized by a 5 mbar mixing ratio of 2.7±0.8×¹⁰⁻⁸ at −20° and at −80° latitude. These results suggest that the time scale for meridional circulation lies between the net photochemical lifetimes of C₂H₂ and C₃H₈, ≈30-600 years.  相似文献   

Moisture transport from the Atlantic to the Pacific basin and its response to North Atlantic cooling and global warming     

Ingo Richter  Shang-Ping Xie 《Climate Dynamics》2010,35(2-3):551-566

Atmospheric moisture transport from the Atlantic to the Pacific basin plays an important role in regulating North Atlantic salinity and thus the strength of the thermohaline circulation. Potential changes in the strength of this moisture transport are investigated for two different climate-change scenarios: North Atlantic cooling representative of Heinrich events, and increased greenhouse gas (GHG) forcing. The effect of North Atlantic cooling is studied using a coupled regional model with comparatively high resolution that successfully simulates Central American gap winds and other important aspects of the region. Cooler North Atlantic sea surface temperature (SST) in this model leads to a regional decrease of atmospheric moisture but also to an increase in wind speed across Central America via an anomalous pressure gradient. The latter effect dominates, resulting in a 0.13 Sv (1 Sv = 10⁶ m³ s^?1) increase in overall moisture transport to the Pacific basin. In fresh water forcing simulations with four different general circulation models, the wind speed effect is also present but not strong enough to completely offset the effect of moisture decrease except in one model. The influence of GHG forcing is studied using simulations from the Intergovernmental Panel on Climate Change archive. In these simulations atmospheric moisture increases globally, resulting in an increase of moisture transport by 0.25 Sv from the Atlantic to Pacific. Thus, in both scenarios, moisture transport changes act to stabilize the thermohaline circulation. The notion that the Andes effectively block moisture transport from the Atlantic to the Pacific basin is not supported by the simulations and atmospheric reanalyses examined here. This indicates that such a blocking effect does not exist or else that higher resolution is needed to adequately represent the steep orography of the Andes.  相似文献   

Protokoll über die Geschäftssitzung der Geologischen Vereinigung in Frankfurt a. M. am 4. Januar 1937     

Max Richter 《International Journal of Earth Sciences》1937,28(1-2):135-135

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Die Hochflächen-Treppe der Nordeifel und ihre Beziehungen zum Tertiär und Quartär der Niederrheinischen Bucht     

Priv.-Doz. Dr. Dieter Richter 《International Journal of Earth Sciences》1962,52(1):376-404

The tableland of the northern Eifel consists of a whole series of levelling planations which descend like steps to the plain of the Lower Rhine or form broad terraces along the river valleys. A similar staircase structure can be seen in the Cretaceous range of the Aachener Wald. The oldest obliquely situated plateau of the Hohe Venn is a resurrected fossil peneplain which was formed before the Maastricht formation as can be proved by scanty remains of the flinty chalk (Maastricht) which still overlays this peneplain at the present time. Therefore the great elevation of the northern Eifel to heights of 2280 feet above sea-level did not follow until later than Upper Cretaceous.The indentation of this old Cretaceous peneplain presumably resulted in the formation of an older system of plateaus in Oligocene and in a system of young plateaus in Miocene which had the appearance of a staircase. These tableland systems originated in times of slight elevation in which superficial denudation must have predominated under the influence of a damp climate and intensive chemical decomposition of the rocks. During the Lower Miocene and Pliocene epochs considerable elevatory movements occurred which led occasionally to the formation of steep obsequent slopes at the edges of both systems. During the Lower Pleistocene epoch glacial conditions existed and at this time the main period of terrace formation occurred. In the course of this period there was a great gravel accumulation which was linked with lateral erosion and which, whith the aid of its valley terraces and rubble remains, can be traced as far as the foreland. A later, very marked incision of the rivers can be traced back to great elevations of land which occurred after this period. The rhythmic alternation of periods of elevation and inactivity can be seen in the morphological development of the northern Eifel. The individual periods of tableland and terrace formation can be related to corresponding sediments belonging to the Upper Tertiary and the Quaternary periods.

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Résumé Le paysage en plateaux emboîtés du Nord de l'Eifel se compose de toute une série de surfaces de nivellement qui descendent en gradins vers la plaine basse du Rhin inférieur ou constituent de larges terrasses le long des vallées fluviales. Une pareille structure en plateaux étagés est décelable dans la petite montagne crétacée du Aachener Wald. Le plus ancien haut plateau incliné des Hautes Fagnes représente une ancienne pénépleine à nouveau exhumée qui s'est formée avant le Maastrichtien comme on peut le démontrer par des restes peu abondants d'éluvions à silex (pierre à feu) qui lui servait autrefois de couverture. Le fort soulèvement du Nord de l'Eifel jusqu'à des hauteurs de 760 au dessus du niveau de la mer ne s'est produit par conséquent qu'après le crétacé supérieure.Á l'oligocène, un système plus ancien de surfaces applanies étagées et au miocène, un système de surfaces plus jeunes ont été probablement entaillés en gradins dans cette ancienne pénéplaine crétacée. Ces systèmes de plateaux emboîtés ont pris naissance à des époques de faible soulèvement, où l'érosion en surface a dû prédominer sous l'influence d'un climat humide et d'une décomposition chimique intensive de la roche. Au miocène inférieur et au pliocène ils ont chaque fois produit des mouvements de soulèvement assez forts qui ont entraîné la formation de versants à profil plus abrupt au bord des deux systèmes. Dans les conditions glaciaires, du pleistocène ancien, de l'époque des principales terrasses, il se produisit un important remblaiement de cailloutis uni à une érosion latérale et que l'on peut suivre jusque dans les parties avancées du territoire à l'aide de ses terrasses de vallées et de ses restes de cailloutis. Une forte entaille ultérieure des fleuves remonte à de vastes soulèvements de terrain postérieurs à cette époque. C'est ainsi que dans l'évolution morphologique du Nord de l'Eifel s'exprime l'alternance rythmique de périodes de soulèvement et de repos. Les différentes époques de formations de hauts plateaux étagés et de terrasses peuvent être mises en relation avec des sédiments correspondants parallèles du tertiaire supérieur et du quaternaire de la baie du Rhin inférieur.

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Die rezente hydrothermal-sedimentäre Lagerstätte Atlantis-II-Tief im Roten Meer     

Dr. Harald Bäcker  Helmut Richter 《International Journal of Earth Sciences》1973,62(3):697-737

Zusammenfassung Die in Entstehung befindliche hydrothermal-sedimentäre Lagerstätte Atlantis-II-Tief im Roten Meer wurde in den Jahren 1969, 1971 und 1972 von den Forschungsschiffen Wando River und Valdivia aus genauer untersucht. Die Detailkartierung zeigt eine Fallenstruktur, die hauptsächlich durch NW-streichende Grabenrandverwerfungen hervorgerufen wurde. Die in die se Depression in ihren tiefsten Teil einströmenden metallhaltigen Solen hielten das für die Lagerstättenbildung, besonders das für die Sulfidausfällung nötige Milieu über längere Zeit aufrecht. Diese seit dem ausgehenden Pleistozän anhaltende stabile Situation wurde einige Male von Lava-Ausflüssen, tektonischen Ereignissen und Verlagerung der Quellen unterbrochen. Diese Vorgänge und die komplizierte Morphologie der solegefüllten Becken führten zu einer sehr komplexen Faziesentwicklung und stratigraphischen Abfolge. Insgesamt läßt sich, von den Quellen ausgehend, eine Zonierung von sulfidisch-silikatischer zu manganitischlimonitischer Ausfällung beobachten.

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The Atlantis II Deep, a hydrothermal-sedimentary metal depositin statu nascendi has been investigated in detail 1969, 1971 and 1972 with the research vessels Wando River and Valdivia. The new bathymetric map reveals a trap structure mainly caused by NW-striking faults, limiting local grabens. The metalliferous brines discharging into the deepest part of this depression maintained the conditions necessary for the formation of the deposit, esp. of the sulfides, for a long time.This stabil situation active since the end of the Pleistocene was several times disturbed by lava flows, tectonic events and displacement of the discharge vents.These events and the complicate morphologic structure of the brine-filled deep are responsible for a very complex development of lithologic facies and the stratigraphic sequence. There is a general deposit differentiation from sulfidic-silicatic precipitation near the discharge points and formation of limonite and manganite outside the brines.

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Résumé Pendant les années 1969, 1971 et 1972 les gisements hydrothermaux sédimentaires Atlantis II, en voie de formation dans la Mer Rouge, ont fait l'objet de campagnes scientifiques détaillées entreprises par les navires océanographiques Wando River et Valdivia.La carte morphologique montre une structure de descente qui a été formée principalement par des failles de direction NW délimitant des graben. Les saumures métallifères affluant dans la partie la plus profonde de cette dépression ont maintenu pendant une certaine durée le milieu nécessaire à la formation du gisement, et surtout à la précipitation des sulfures. Cette situation restée stable depuis la fin du Pléistocène a été interrompue plusieurs fois des émissions basaltiques, par des dislocations tectoniques et par le déplacement des sources. Ces événements, ainsi que la morphologie compliquée du bassin rempli de saumures, ont conduit à un développement très complexe des faciès lithologiques et de la séquence stratigraphique. Dans l'ensemble on peut constater une zonation des faciès avec précipitations sulfurosilicatées près des points d'entrée des saumures et manganolimonitiques plus à l'écart.

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Bottom irregularities in the North Sea     

Dr. K. Richter  Dipl.-Phys. B. Schmalfeldt  Dipl.-phys. J. Siebert 《Ocean Dynamics》1976,29(1):1-10

Summary A pressure transducer fixed to a sledge was towed over the bottom of the sea. Pressure variations corresponding to bottom displacement variations were recorded along different profiles in the area west of Sylt. From the time series obtained power spectra of bottom irregularities were computed as a function of wavenumberk or wavelength . Total rms bottom displacement in the wavelength band 50 to 500 m ranges from 3 cm to 36 cm depending on the location of the profile. Presumedly this is due to different types of sediment. Therefore the area cannot be considered as uniform or isotropic concerning the spatial and directional distribution of bottom irregularities. The approximation of spectra byE(k)k– yields -values between 0.4 and 2.9.

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Bodenunebenheiten in der Nordsee

Zusammenfassung Mit Hilfe einer Druckdose, die von einem Schiff aus über den Meeresboden gezogen wurde, konnten auf ausgewählten Profilen westlich von Sylt Bodenunebenheiten registriert werden. Aus den gewonnenen Zeitserien wurden SpektrenE(k) für die Wellenzahlenk bzw. für die Wellenlänge berechnet. Hieraus lassen sich die Amplituden der Bodenunebenheiten im Wellenlängenbereich von 20 bis 500 m bestimmen. Die effektive Bodenwelligkeit im Bereich von 50 bis 500 m liegt je nach Profil zwischen 3 cm und 36 cm. Die Ursache dafür ist möglicherweise in der unterschiedlichen Sedimentzusammensetzung zu suchen. Eine Isotropie des Bodenspektrums im Meßgebiet ist nicht vorhanden. Die Annäherung der Spektren durchE(k)k– ergibt -Werte zwischen 0,4 und 2,9.

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Irrégularités du fond en Mer du Nord

Résumé Un manomètre enregistreur fixé à un traîneau a été remorqué sur le fond de la mer. Les variations de pression correspondant aux variations du fond ont été enregistrées le long de différents profils dans la zone Ouest de Sylt. A partir de la série de mesures obtenues, on a calculé le spectre de puissance des irrégularités du fond en fonction du nombre d'ondek ou de la longueur d'onde . Globalement, les variations du fond dans la bande de longueurs d'onde de 50 à 500 m varient de 3 à 36 cm en moyenne quadratique selon la situation du profil. On présume que cela est dû aux différents types de sédiments. Aussi, la zone ne peut pas être considérée comme uniforme ou isotrope en ce qui concerne la distribution dans l'espace et en direction des irrégularités du fond. L'approximation de spectres parE(k)k– donne des valeurs de comprises entre 0,4 et 2,9.

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