Buchbesprechungen     

F. Zebender  P. Zimmermann  R. Märki  A. Hörler  H. Ambübl 《Aquatic Sciences - Research Across Boundaries》1961,23(1):296-308

Ohne Zusammenfassung  相似文献   

Zur Frage der Geschwindigkeit des Deckenschubes     

Univ.-Prof. Dr. Alexander Tollmann 《International Journal of Earth Sciences》1972,61(3):965-974

Zusammenfassung In den folgenden Ausführungen werden Daten über die Geschwindigkeit der Bewegung von Schubdecken in der Hauptbewegungsphase geliefert. Die hierfür verwendeten Beispiele stammen aus den Ostalpen und Westkarpaten. Eine sichere Geschwindigkeits-Bestimmung ist derzeit noch nicht durchführbar. Es können aber Minimalbewegungswerte von etwa 1,5 mm/Jahr errechnet werden. Die reale Transportgeschwindigkeit könnte auch wesentlich höher liegen, vielleicht bei 10–20 mm/Jahr.

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This paper presents facts pertaining to the velocity of the overthrust of nappes during a tectonical phase by means of examples from the Eastern Alps and the Western Carpathians. An exact determination of this velocity is still not possible. One can calculate minimum values of near 1,5 mm/year. The real velocity of the overthrusts of nappes might be much higher, perhaps 10–20 mm/year.

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Résumé L'article expose des données sur la vitesse des mouvements des nappes de charriage pendant la phase principale de transport. Les exemples présentés proviennent des Alpes orientales et des Carpathes occidentales. Il n'est pas possible jusqu'à présent de faire une détermination plus exacte de cette vitesse. Mais on peut calculer un minimum de transport d'environ 1,5 mm/an. La vitesse réelle des mouvements de translation pourrait même être nettement plus élevée, et atteindre peut-être 10–20 mm/ an.

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. . . 1,5 /. , 10–20 /.

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Stratabound barite deposits in Nevada     

R. A. Zimmermann 《Mineralium Deposita》1969,4(4):401-409

The barite deposits in the Shoshone Range contain rhythmic layering of several types. One type includes interlayered barite and clay seams with iron oxide grains and stains, where the barite beds gradually change in thickness upwards. Top-bottom (geopetal) features are present but differ from those observed in the Arkansas Stanley Shale deposits. Chert and very fine-grained quartz are interlayered with the barite. The thickest barite beds lie where the chert and shaly layers are thinnest. These are features one would normally find in a sediment. These and other observations suggest a formation by syn-diagenetic processes.

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Zusammenfassung Die Schwerspatlagerstätten der Shoshone Range in Nevada zeigen rhythmische Lagen verschiedener Arten. So gibt es eine Wechsellagerung von Schwerspat mit Tonhäutchen, die Eisenoxidkörner und -filme enthalten. Bei diesem Typ schwankt die Schichtmächtigkeit von unten nach oben. Die Lagen sind sehr reich an Geopetalgefügen aber unterscheiden sich von denjenigen in den Schwerspatlagerstätten von Stanley Shale, Arkansas. Die rhythmischen Lagen bestehen aus Flint (Chert), feinkörnigem Quarz und Schwerspat. Dichte Schwerspat-Lagen treten da auf, wo die Flint-Lagen sehr dünn sind oder fehlen. Solche Erscheinungen treten normalerweise sehr häufig in Sedimenten auf. Diese und andere erwähnte Beobachtungen geben Anlaß zur Annahme, daß es sich hier um synsedimentäre Lagerstätten handelt.

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Results of deep seismic soundings along international profile VII in Czechoslovakia and poland     

Břetislav Beránek  Milica Mayerová  Milada Zounková  Alexander Guterch  Rufin Materzok  Jan Pajchel  Reviewer J. Vaněk 《Studia Geophysica et Geodaetica》1973,17(3):205-217

Summary The paper deals with the results of DSS measurements along international profile VII, carried out by Czechoslovak and Polish geophysicists in 1970 – 71. The profile situation is shown in Fig. 1. By 1971 part of the profile in the region of the Bohemian Massif between points 1 and 3 and in Poland between points 5 and 7 had been surveyed (Fig. 2). The seismograms were used to construct the travel-time curves of the fundamental types of waves P^K, P^M, P_n (Fig. 4). The mean velocities were computed from the travel-time curves of the reflected waves (P^M and P^K) and the refracted waves (P_g). Isolines of the mean velocities could be constructed for the region of the Bohemian Massif (Fig. 6). The velocity data found were used for the depth interpretation of the travel-time curves of the principal types of waves and to construct a seismic section (Fig. 8). In the region of the Pre-Sudeten block the thickness of the crust was found to be 34–37 km, and in the Sudeten it increased to 40 km. Towards the south the thickness of the crust gradually reduces to 30 km in the system of the Luice faults. In the Bohemian Cretaceous the thickness of the crust is about 30 km. Further to the south, in the region of the Moldanubicum, the thickness of the Earth's crust increases rapidly, and at the southern border of the Central Bohemian pluton it reaches values of about 42 km.  相似文献   

Constructing the Coronal Magnetic Field By Correlating Parameterized Magnetic Field Lines With Observed Coronal Plasma Structures     

Gary  G. Allen  Alexander  David 《Solar physics》1999,186(1-2):123-139

A method is presented for constructing the coronal magnetic field from photospheric magnetograms and observed coronal loops. A set of magnetic field lines generated from magnetogram data is parameterized and then deformed by varying the parameterized values. The coronal flux tubes associated with this field are adjusted until the correlation between the field lines and the observed coronal loops is maximized. A mathematical formulation is described which ensures that (i) the normal component of the photospheric field remains unchanged, (ii) the field is given in the entire corona over an active region, (iii) the field remains divergence-free, and (iv) electric currents are introduced into the field. It is demonstrated that a parameterization of a potential field, comprising a radial stretching of the field, can provide a match for a simple bipolar active region, AR 7999, which crossed the central meridian on 1996 November 26. The result is a non-force-free magnetic field with the Lorentz force being of the order of 10^–5.5 g cm s^–2 resulting from an electric current density of 0.079 A m^–2. Calculations show that the plasma beta becomes larger than unity at a relatively low height of 0.25 r supporting the non-force-free conclusion. The presence of such strong non-radial currents requires large transverse pressure gradients to maintain a magnetostatic atmosphere, required by the relatively persistent nature of the coronal structures observed in AR 7999. This scheme is an important tool in generating a magnetic field solution consistent with the coronal flux tube observations and the observed photospheric magnetic field.  相似文献   

A potentiometric study of Eu complexation with acetate ligand from 25 to 170°C at P_sat     

Alexander V Zotov  Boris R Tagirov  Igor I Diakonov  K.Vala Ragnarsdottir 《Geochimica et cosmochimica acta》2002,66(20):3599-3613

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NOAA AR 8210: EVOLUTION AND FLARES FROM MULTIBAND DIAGNOSTICS     

Warmuth  Alexander  Hanslmeier  Arnold  Messerotti  Mauro  Cacciani  Alessandro  Moretti  Pier Francesco  Otruba  Wolfgang 《Solar physics》2000,194(1):103-120

NOAA 8210 has been a region showing a remarkable level of activity well before solar maximum. Dominated by a large, rapidly rotating spot, it produced several intense flares during its disk passage at the end of April–beginning of May 1998. We examine the development of AR 8210 in H and white light (WL) and study the evolution of its complex magnetic topology. While the other principal flares are briefly reviewed, the great X1.1/3B flare of 2 May, which was observed at Kanzelhöhe Solar Observatory during a SOHO/UVCS ground support campaign, is studied in detail. This event has been documented in full-disk H and Na-D intensitygrams, Dopplergrams, and magnetograms, with a time cadence of one minute each. The flare was associated with a CME and produced significant geomagnetic effects. Furthermore, we point out the perspectives for our planned Flare Monitoring and Alerting System, since the two new instruments (Magneto-Optical Filter and Digital H camera), which made their first operational run with the campaign, are crucial components for this program.  相似文献   

Structure of a Large low-Latitude Coronal Hole     

Bromage  B.J.J.  Alexander  D.  Breen  A.  Clegg  J.R.  Del Zanna  G.  DeForest  C.  Dobrzycka  D.  Gopalswamy  N.  Thompson  B.  Browning  P.K. 《Solar physics》2000,193(1-2):181-193

Coronal holes on the Sun are the source of high-speed solar wind streams that produce magnetic disturbances at the Earth. A series of multi-wavelength, multi-instrument observations obtained during the 1996 Whole Sun Month campaign examined a large coronal hole in greater detail than ever before. It appeared on the Sun in August, and extended from the north pole to a large active region in the southern hemisphere. Its physical and magnetic structure and subsequent evolution are described.  相似文献   

Salt transport on islands in the Okavango Delta: Numerical investigations     

S. Zimmermann  P. Bauer  R. Held  W. Kinzelbach  J.H. Walther 《Advances in water resources》2006

This study uses a numerical model to investigate the groundwater flow and salt transport mechanisms below islands in the Okavango Delta. Continuous evapotranspiration on the islands results in accumulation of solutes and the formation of a saline boundary layer, which may eventually become unstable. A novel Lagrangian method is employed in this study and compared to other numerical methods. The numerical results support the geophysical observations of density fingering on Thata Island. However, the process is slow and it takes some hundreds of years until density fingering is triggered. The results are sensitive to changes of the hydraulic gradient and the evapotranspiration rate. Small changes may lead to different plume developments. Results further demonstrate that density effects may be entirely overridden by lateral flow on islands embedded in a sufficiently high regional hydraulic gradient.  相似文献   

Seismic Moment Tensor Resolution on a Local Scale: Simulated Rockburst and Mine-induced Seismic Events in the Kopanang Gold Mine, South Africa   总被引：2，自引：0，他引：2  

Jan Šílený  Alexander Milev 《Pure and Applied Geophysics》2006,163(8):1495-1513

Seismic records contain information about the effect of the source as well as the effect of wave propagation through the rock mass. The effect of wave propagation is usually not well known as only simplified models of geological structures are available. Therefore, the information about the source retrieved by inverting seismograms may include errors due to incomplete knowledge of the rock mass along the propagation path, which in turn cause a distortion in the calculated moment tensor (MT). The distortion of the MT on a local scale was observed by inverting records of a simulated rockburst conducted at the Kopanang gold mine in South Africa. A dominant isotropic component of the explosive characteristics was found from the inversion. The deviatoric components retrieved from the blast are spurious. A test of their stability indicated that they are not significant, assuming an uncertainty above 5% for velocities and 10% for attenuation within the homogeneous model available for the mine. Thus, the retrieval of the MT from records of local networks in mines using a homogeneous model of the rock mass seems to be feasible. However, the homogeneous model of the rock mass can only be applied to close stations, within a few kilometers of the source. The seismic records from distant stations were too complex to be modelled by a homogeneous rock mass. Records of six mine-induced seismic events recorded at the Kopanang gold mine were also inverted. A vertical linear dipole along the pressure (P) axis was found for three of the events, suggesting a pillar burst. The mechanism of two events contains an isotropic implosion together with a nearly vertical dip-slip, and seems to indicate a combination of a cavity collapse with a down dip-slip along a nearly vertical fault. One event corresponds to a dipole along the tensional (T) axis. However, it is vertical, thus its association with tensile faulting of the hangingwall is uncertain.  相似文献