Vergleichende Messungen der SO2-Immissions-Konzentration mit den Meßgeräten Picoflux und SO2-Monitor     

Ing. Kurt Chalupa 《Theoretical and Applied Climatology》1971,19(2):225-230

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Solar radiation extinction,sky radiation,sky light polarization and aerosol particle total number and size distribution on the Island Maui (Hawaii)     

Kurt Bullrich  Reiner Eiden  Ruprecht Jaenicke  Wolfram Nowak 《Pure and Applied Geophysics》1968,69(1):280-319

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Röntgenographische Gefügeanalyse mit dem Texturgoniometer am Beispiel von Quarziten aus kaledonischen Überschiebungszonen     

Dr. Kurt v. Gehlen  Dr. Gerhard Voll 《International Journal of Earth Sciences》1962,51(2):440-450

Zusammenfassung Quantitative Gefügediagramme können röntgenographisch mit einem Zählrohr-Textur-Goniometer gemessen werden. Diese Methode kommt besonders in Frage bei sehr feinkörnigen Gesteinen oder aber dann, wenn etwa bei einachsigen Mineralen auch die Regelung anderer Gitterrichtungen außer der c-Achsen-Richtung interessiert. Das beim Quarz anzuwendende Verfahren wird behandelt und gezeigt, wie man hier im Einzelfall Prismenregelungen nachweisen kann. Als praktische Beispiele werden Quarzitgefüge mit Prismenregelung aus kaledonischen Überschiebungszonen Schottlands und Norwegens abgebildet und ihre Entstehung diskutiert. Die Messungen scheinen darauf hinzuweisen, daß beim Quarz bevorzugt Translation mit (11¯20) als Gleitfläche und c als Gleitgerade maßgebend war.  相似文献   

Rare gases and fossil particle tracks in the Kenna ureilite     

Laurel L. Wilkening  Kurt Marti 《Geochimica et cosmochimica acta》1976,40(12):1465-1466

Fossil particle tracks and spallation-produced He and Ne in the Kenna ureilite indicate that it existed in space as a small object for 23 m.y. In our study of Kenna, we found no evidence of trapped He or Ne. Large amounts of heavy rare gases occur in Kenna in concentrations typical of ureilites. In a step-wise release of gases, the isotopic compositions of Kr and Xe were found to be constant above 600°C, revealing the presence of a single retentively sited component. The Xe isotopic abundances are characterized by 124:126:128:129:130:131:132:134:136 = 0.471:0.414:8.280:103.61: 16.296:81.92:100:37.70:31.23. This isotopic composition is distinct from AVCC (average carbonaceous chondritic), but similar to compositions known for some time in certain temperature fractions of Renazzo, Murray and Murchison. Kenna-type Xe appears to be one of the several components found in carbonaceous chondrites.

Binz et al. (Geochim. Cosmochim. Acta 39, 1576–1579, 1975) have recently found that many volatile trace elements are strongly depleted in ureilites. Thus, the relatively large amounts of heavy rare gases present in ureilites did not result from a mixture of a volatile-rich component with the ureilite host. It appears that some material rich in carbon and heavy rare gases was incorporated into a differentiated ureilite host. All current hypotheses which purport to explain the origin of trapped gases in meteorites encounter difficulty in accounting for trapped gases in ureilites in a straightforward manner.  相似文献   

The mass and moment of inertia of the Earth     

Barbara Romanowicz  Kurt Lambeck 《Physics of the Earth and Planetary Interiors》1977,15(1):P1-P4

Recent revisions of geodetic and astronomical constants by the International Association of Geodesy and the International Astronomical Union lead to improved values for the earth's mass and moment of inertia. Corrections to be applied to these values before they are used as constraints in the inversion of seismic data are discussed.  相似文献   

Nickel,and the existence of high-MgO liquids in nature     

D.B. Clarke  M.J. O&#x;Hara 《Earth and Planetary Science Letters》1979,44(1):153-158

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Vulkanogene Glasscherben-Relikte in Kohlentonsteinen des Saar-Lothringer Oberkarbons sowie Herkunft und Menge der Pyroklastika     

Dr. Kurt Burger 《International Journal of Earth Sciences》1990,79(3):659-691

Zusammenfassung Obwohl Kohlentonsteine aus dem Saar-Lothringer Oberkarbon seit etwa 170 Jahren bekannt sind, gelang erst in jüngster Zeit der Nachweis und die Identifikation vulkanogener Relikte im petrographischen Stoffbestand. Diese befinden sich in Kohlentonsteinen des Stefan A: KTst 0=950; Westfal D: KTst 1=700; Westfal C: KTst 3 =400, KTst 4a=330, KTst 4aß=322, KTst 4=320, KTst 5=300 und im KTst 6=270. Das entspricht einem Anteil von ca. 18 % an der Gesamtzahl der in diesem limnischen Steinkohlenrevier beobachteten Kohlentonsteine, die hier große praktische und wissenschaftliche Bedeutung besitzen. Die pseudomorphen Relikte bestehen aus kleinen Splittern, kleinen und größeren Fragmenten mit teilweise gut erhaltenem blasigen Gefüge von Vitroklasten — sie zeigen die für Aschenschmelztuffe typisch verschweißte Scherbentextur. Die Glassubstanz ist meist zu mikrokristallinem Kaolinit devitrifiziert. Der eindeutige Nachweis dieser Relikte ist für die Genese bedeutungsvoll, liefern sie doch nun den sicheren Beweis, daß der primäre Stoffbestand aus aerisch abgelagertem pyroklastischen Material bestand, das intensive chemische Verwitterungs- und diagenetische Umbildungsprozesse erfahren hat. Für die 43 Kohlentonsteine des Saar-Lothringer Oberkarbons wird eine pyroklastische Eruptionsmenge von mindestens 8,2 km³ Festvolumen bzw. 20,5 km³ Lokkervolumen angenommen. Die Eruptionen erfolgten vermutlich aus der in der Nähe befindlichen Metz-Hunsrück-Südrand-Tiefenstörung, die nach Reflexionsseismik bis unter die Moho reicht.

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Tonsteins in the Carboniferous of the Saar-Lorraine basin are known since about 170 years. Volcanic glass remains, however, have been proven as constituents of the tonstein only recently. They occur in tonsteins of Stephanian A: KTst 0=950; Westphalian D: KTst 1=700; Westphalian C: KTst 3=400, KTst 4a=330, KTst 4aß= 322, KTst 4=320, KTst 5=300 and KTst 6=270. Tonsteins with volcanic glass fragments amount to 18% of the total tonsteins observed in the limnic Saar-Lorraine basin. They are important to applied geology, e.g. for seam identification and correlation, as well as for scientific reasons, namely for the determination of provenance and genesis of tonsteins.The volcanic remains consist of tiny glass splinters, glass fragments, and of fragments with well preserved gasbubble texture. The welded splinter texture is typical of welded pyroclastic ash deposits. Much of the glass has been devitrified to microcrystalline kaolinite. The indisputable evidence of volcanic remains is essential when considering the genesis of tonsteins, as they provide proof that tonsteins are primarily composed of eolian pyroclastic constituents which were altered by chemical weathering and diagenesis.For the 43 horizons of the coal tonsteins found in the Upper Carboniferous of the Saar-Lorraine basin, a pyroclastic eruption quantity of at least 8.2 km³ of solid volume or 20.5 km³ of bulk volume is assumed. The eruptions possibly took place along the nearby deep-seated Metz fault at the southern rim of the Hunsrück. This fault, reaches below the Moho according to reflection seismic.

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Résumé Bien que des tonstein du Carbonifère supérieur de SarreLorraine soient connus depuis 170 ans c'est seulement il y a peu de temps que des fragments de verre volcanique y ont été identifiés. Ces fragments ont été rencontrés dans les niveaux de tonstein suivants: Stephanien A: KTst 0=950; Westphalien D: KTst 1=700; Westphalien C: KTst 3=400, KTst 4a=330, KTst 4aß=322, KTst 4=320, KTst 5=300 et KTst 6=270. Ces niveaux représentent une proportion de l'ordre de 18% dans le total des couches de tonstein carbonifère rencontrées dans ce bassin houiller limnique où elles présentent un grand intérêt tant au point de vue pratique que scientifique. Les verres se présentent en esquilles et en fragments de tailles diverses, montrant parfois une structure bulleuse bien conservée; ils présentent également les structures d'agglomération propres aux tufs soudés à chaud. Le verre est le plus souvent dévitrifié en kaolinite microcristalline. La présence de ces fragments est d'un intérêt particulier pour la genèse du dépôt puisqu'elle fournit la preuve que celui-ci était constitué de matériaux primaires pyroclastiques sédimentés dans l'air, matériaux qui ont subi ensuite des altérations chimiques et des transformations diagénétiques intenses.Pour l'ensemble des 43 horizons de tonstein du Carbonifère supérieur de la Sarre-Lorraine, on admet un volume de matières pyroclastiques d'au moins 8,2 km³ (volume à l'état monolithique) ou de 20,5 km³ (volume à l'état fragmenté). Ces éruptions ont probablement pour origine la faille de Metz, située à proximité, qui forme la limite sud du Hunsrück et que la sismique-réflexion permet de prolonger jusqu'au Moho.

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Das Thema dieser Arbeit war Gegenstand des KurzvortragesBurger &Wolf (1987) auf dem XI. ICC in Peking (31. 8. bis 4. 9. 1987). Vorliegende Bearbeitung stellt die originäre Fassung dar.  相似文献   

Astron observations of the Rapid Burster MXB 1730-335 and constraints on burster parameters from spectra of trailing bursts     

A. D. Kaminker  G. G. Pavlov  Yu. A. Shibanov  V. G. Kurt  E. Yu. Shafer  A. S. Smirnov  V. M. Shamolin  I. F. Kopaeva  E. K. Sheffer 《Astrophysics and Space Science》1990,173(2):171-189

We report on eight X-ray bursts detected by ASTRON from the Rapid Burster (RB) on 13 and 28 April and 16 August, 1983. Six of them (trailing bursts), with durations of 1.5–2 min, rise times of 5–10 s and intervals of 1–1.5 hours, exhibit spectral softening during the burst decay and may be related to the type I bursts. Two of the bursts (triangle bursts) observed on 28 April at interval of 28 min with much longer rise times (30–50 s) and longer durations (3 min), do not show distinct spectral softening. Persistent flux from RB on 16 August was estimated asF _p(2.0–2.4)×10^–9 erg cm^–2 s^–1. Spectral evolution of two trailing bursts was investigated by fitting their spectra in consecutive time intervals with the blackbody (BB), isothermal scattering photosphere (SP) and thermal bremsstrahlung (TB) models. Around the burst maxima the SP model fits the data best whereas in the burst tails the TB model is generally better. The BB model is worse than at least one of the two others. Interpretation of the burst spectra in terms of the BB radiation leads to improbably small neutron star mass and radius (M<0.86M ,R _NS<5 km) if the peak luminosity does not exceed the Eddington limit. Interpretation of the spectra around the burst maxima (3–15 s from the burst onset) in terms of an isothermal SP yields reasonable constraints onM,R _NS, and distanceD. For instance, for the hydrogen photosphere we obtainedM=(1.0–2.1)M R _NS=(7.1–16.4) km ifD=11 kpc. If one postulatesM=1.4M , thenD=(8.5–13) kpc for hydrogen photosphere; if, besides,D=11 kpc, thenR _NS=(8.1–13.3) km. It follows also from the SP-interpretation that the photosphere radius may increase up to 20–30 km in maxima of the trailing bursts when the luminosity becomes close to the Eddington luminosity.  相似文献   

A method to estimate hydraulic conductivity while drilling     

Kurt I. Srensen  Flemming Effers  Esben Auken  Louise Pellerin 《Journal of Hydrology》2002,260(1-4):15-29

A field test and analysis method has been developed to estimate the vertical distribution of hydraulic conductivity in shallow unconsolidated aquifers. The field method uses fluid injection ports and pressure transducers in a hollow auger that measure the hydraulic head outside the auger at several distances from the injection point. A constant injection rate is maintained for a duration time sufficient for the system to become steady state. Exploiting the analogy between electrical resistivity in geophysics and hydraulic flow two methods are used to estimate conductivity with depth: a half-space model based on spherical flow from a point injection at each measurement site, and a one-dimensional inversion of an entire dataset.

The injection methodology, conducted in three separate drilling operations, was investigated for repeatability, reproducibility, linearity, and for different injection sources. Repeatability tests, conducted at 10 levels, demonstrated standard deviations of generally less than 10%. Reproducibility tests conducted in three, closely spaced drilling operations generally showed a standard deviation of less than 20%, which is probably due to lateral variations in hydraulic conductivity. Linearity tests, made to determine dependency on flow rates, showed no indication of a flow rate bias. In order to obtain estimates of the hydraulic conductivity by an independent means, a series of measurements were made by injecting water through screens installed at two separate depths in a monitoring pipe near the measurement site. These estimates differed from the corresponding estimates obtained by injection in the hollow auger by a factor of less than 3.5, which can be attributed to variations in geology and the inaccurate estimates of the distance between the measurement and the injection sites at depth.  相似文献   

Laboratory Studies Of Wind Stress Over Surface Waves   总被引：4，自引：0，他引：4  

B. Mete Uz  Mark A. Donelan  Tetsu Hara  Erik J. Bock 《Boundary-Layer Meteorology》2002,102(2):301-331

Simultaneous laboratory observations of wind speed, wind stress, and surfacewind-wave spectra are made under a variety of wind forcing patterns using cleanwater as well as water containing an artificial surfactant. Under typical experimentalconditions, more than half of the total stress is supported by the wave-induced stressrather than by the surface viscous stress. When the surfactant reduces the shortwind-wave spectra, the wind stress also decreases by as much as 20–30% at agiven wind speed. When the wind forcing is modulated in time, the wind stresstends to be higher under decreasing wind than under increasing wind at a givenwind speed, mainly because the response of short wind-wave spectra to varyingwind forcing is delayed in time. These examples clearly demonstrate that therelationship between the wind speed and the wind stress can be significantlymodified if the surface wave field is not in equilibrium with the wind forcing.Next, we examine whether the wind stress is estimated accurately if the wave-inducedstress by all surface wave components is explicitly evaluated by linear superpositionand is added to the surface viscous stress. It is assumed that the surface viscous stressis uniquely related to the wind speed, and that the wind input rate is determined by thelocal, reduced turbulent stress rather than the total stress. Our wind stress estimatesincluding the wave contributions agree well with observed wind stress values, evenif the surface wave field is away from its equilibrium with the wind in the presenceof surface films and/or under time-transient wind forcing. These observations stronglysuggest that the wind stress is accurately evaluated as a sum of the wave-induced stressand the surface viscous stress. At very high winds, our stress estimates tend to be lowerthan the observations. We suspect that this is because of the enhancement of wind stressover very steep (or breaking) short wind-waves.  相似文献