On the wave field generated by a variable wind

Abstract

By using an empirical expression relating the rate of increase in wave energy to the local wind speed, an equation for the phase speed at the peak of the wave spectrum is derived. The solution of the equation is determined for some simple wind fields. In particular, the wave field caused by a localised storm moving steadily over an unbounded ocean is considered. It is also shown that only a small fraction of the momentum transferred from the wind into the water propagates away from a local storm area in the form of wave momentum.     

Comparison of the Brunhes epoch geomagnetic secular variation recorded in the volcanic and sedimentary rocks

The results of numerical modeling of the geomagnetic secular variation by the method of the Giant Gaussian Process (GGP) are presented and compared with the information derived from the presentday databases for paleointensity. The variances of the positions of the virtual geomagnetic pole (VGP) calculated from the synthetic and experimental data (Brunhes epoch, effusive rocks) are nearly similar, which supports the validity of the theoretical model. The average value of the virtual axial geomagnetic dipole (VADM) calculated from the PINT world database on paleointensity and the Sint-2000 model is lower than VADM calculated by the GGP model; at the same time, the estimates based on the archaeomagnetic data give the VADM value slightly above the model prediction. The largest difference is observed in the variances of VADM, which is for all the three databases noticeably higher than the value calculated from the GGP model. Most probably, this is due to the contribution of the neglected measurement errors of VADM.     

Geodynamics and underlying bedrock of the magnetically active crust layer of the Lut block,Eastern Iran

The Curie point depth map of Eastern Iran was constituted from spectral analysis of the aeromagnetic data. The reduction to pole (RTP) was applied to the magnetic anomaly data. The Curie point depth values from 165 overlapping blocks, 100 × 100 km in size, have been estimated. The Curie point depth method provides a relationship between the 2-D FFT power spectrum of the magnetic anomalies and the depth of magnetic sources by transforming the spatial data into the frequency domain. The centroid and top depth of the magnetic sources (respectively Z₀ and Z_t) is calculated from radially averaged log power spectrum for each block. Finally, the Curie point depth of Eastern Iran is obtained by Z_b = 2Z₀–Z_t. The highest value of 24 km is located in eastern and western boundaries of the Lut block, and the lowest value of 12 km is located at north of study area. The shallow depths in the Curie-point depth map are well correlated with the young volcanic areas and geothermal potential fields. Geothermal gradient ranging from 24 to 45°C/km. The deduced thermal structure in eastern Iran has a relationship with orogenic collapse associated with delamination of thickened lithospheric root between the Lut and Afghan continental blocks.     

Some comments on the Oort cloud

The arguments used by Lyttleton to prove the nonexistence of the Oort cloud are reviewed, and it is shown that Oort's hypothesis remains consistent with observation. The 1950 model of the cloud cannot be correct and, by use of the results from a number of more recent papers, an improved model is described and compared with observations. It is emphasized that comparison of the predictions of theory with observations should concentrate on thea-distribution, as the 1/a-distribution masks much of the detailed structure of the theory. An order of magnitude argument is given which shows that 20% of so-called new comets have passed through the planetary system before, and the implications of this to the statistics of near-parabolic comet orbits are briefly investigated.     

The transition from passive to active margin tectonics: a case study from the zone of Samedan (eastern Switzerland)

The Zone of Samedan is part of a fossil, early Mesozoic rift system originally situated in the distal, Lower Austro-Alpine domain of the Adriatic passive continental margin. An early Mesozoic configuration of asymmetrical rift basins bounded by relative structural highs compartmentalized Late Cretaceous active margin tectonics; Jurassic half-grabens were folded into arcuate synclines, whereas relative structural highs engendered thin, imbricated thrust sheets. West-directed thrusting and folding initiated at the surface and continued to depths favoring mylonitization under lower greenschist-facies conditions. At this time Liguria-Piemontese ophiolites were accreted to Lower Austro-Alpine units directly underlying the Zone of Samedan. Late Cretaceous orogenic collapse of the Adriatic active margin involved the reactivation of west-directed thrusts as low-angle, top-to-the-east, normal faults. These faults accommodated extensional uplift of Liguria-Piemontese ophiolites and Lower Austro-Alpine units beneath and within the Zone of Samedan. During Paleogene collision, some Late Cretaceous faults in the Zone of Samedan were reactivated under lower anchizonal conditions as north-directed thrusts. The latter stages of this early Tertiary thickening were transitional to brittle, high-angle normal faulting associated with top-to-the-east extension and spreading above the warm, uplifting Lepontine dome.     

Osmium Isotopic Evidence for Crust-Mantle Interaction in the Genesis of Continental Intraplate Basalts from the Newer Volcanics Province, Southeastern Australia

Basalts from the Quaternary Newer Volcanics Province in southeasternAustralia have a large diversity in their chemical and Nd, Srand Os isotopic compositions. Plains series olivine tholeiitesand Cones series nepheline hawaiites have distinctive isotopiccompositions and are clearly not related to each other by asimple genetic process. The Cones series nepheline hawaiiteshave trace element abundances and Nd (     

Die Entstehung einiger tektonischer Grundbegriffe. Ein Beitrag zur Geschichte der Geologie

Zusammenfassung Die ersten tektonischen Vorstellungen legte 1669Nic. Steno in seinem Prodromus nieder. Seine Beobachtungen an horizontalen und geneigten Schichten führten später zu dem Begriffe der orogenetischen Diskordanzen. L.Élie de Beaumont ist sein direkter Nachfolger geworden, während J.Hutton ganz unabhängig von beiden den Diskordanzbegriff entwickelte. Die neptunistische Lehre von A. G.Werner ging von einem primären, von Wasserfluten geschaffenen Relief der Erdoberfläche aus, das überschichtet wurde. Doch auchWerner dachte daneben ebenfalls an große Höhlen, deren Decken einbrechen würden. Die neptunistischen Schwierigkeiten ergaben sich aus der Unmöglichkeit einer vertikalen Sedimentation von primär senkrecht gestellten Schichten. Die Anfänge der Erforschung der Tektonik des Rheingrabens werden dargelegt, und es wird besonders gezeigt, daßÉlie de Beaumont, der 1836 von einem eingebrochenen Gewölbe sprach, schon vorher Kenntnis eines eingebrochenen Gewölbes von Island und eines Schichtgewölbes von Württemberg über Schwarz wald — Vogesen nach Lothringen hatte. Die Zeit des Einbruches legteÉ. de Beaumont irrtümlich in die Zeit des Buntsandsteins.Theorien der Gebirgsbildung wurden mit L. v.Buch's Erhebungstheorie und geognostischen Gebirgssystemen um zwei weitere Ideen 1824–1835 erweitert.Élie de Beaumont baute diese Theorie sehr aus und sprach von Revolutionen der Erdkruste (1829). Die Faltengebirge fanden in J.Thurmann (1832) ihren ersten gründlichen Bearbeiter, der am Beispiel des Faltenjuras nachwies, daß doch nur Horizontalkräfte am Werke gewesen sein können und die Erhebungstheorie L. v.Buch's für diese Gebirgsarten keine Erklärung bringe. Zum Schlusse wird die Geschichte des Geologenkompasses gebracht.

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Nic. Steno was the first who developed tectonic ideas in his Prodromus in 1669. His observations in the surroundings of Firenze (Italy) led him to the notion what nowadays is called a discordance by orogeny. He was followed by the French L.Élie de Beaumont, while the Scotchman J.Hutton developed this term of tectonic discordance quite independently of both.The neptunic theory of A. G.Werner in Freiberg (Saxony) started from the idea that the primary relief of the surface of the earth was formed by floods and covered with sediments. Furtheron he assumed large caves, the tops of them having broken down, explaining in this manner very inclined strata. The difficulties in this neptunic theory resulted from the fact that it was impossible to account for a sedimentation in a vertical line as seen in vertical layers.The author gives a survey of the first researches in the tectonics of the Rhinegraben and shows thatÉlie de Beaumont, who in 1836 mentioned the breakdown of the central ridge of a vault, so forming the rift-valley, had already some information of such a pressure arch in Iceland and of a second one stretching from Würtemberg via Black Forest—Vosges to Lorraine.Élie de Beaumont misdated the collapse of this large vault, stating erroneously the time of Buntsandstein (=New Red Sandstone).Between 1824 and 1835 L. v.Buch developed two further theories on orogenesis, that of the elevation-crater hypothesis and that of the geognostic systems of mountains. É.de Beaumont completedBuch's theory and in 1829 he spoke of revolutions of the earth's crust.The first who thoroughly researched the Swiss Jura was J.Thurmann. Quoting the folded strata of this region as an example he proved that only horizontal stresses could have been responsible for the formation of these mountains and that the elevation-crater hypothesis of L. v.Buch acting only with vertical forces could not give any explanation for it.Finally the author recapitulates the history of the geologist's compass.

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Résumé Les premières conceptions tectoniques ont été exposées en 1669 par N.Steno dans son « Prodrome ». Ses observations sur des strates horizontales ou inclinées ont conduit ultérieurement à la notion de discordances orogéniques. L.Élie de Beaumont fut son successeur direct, cependant que J.Hutton, tout à fait indépendamment des deux premiers développa la notion de discordance. La théorie neptuniste de A. G.Werner se basait sur l'existence préalable d'un relief terrestre créé par les flots et qui aurait été noyé sous les strates des dépôts ultérieurs. Pourtant, dans un autre ordre d'idées,Werner pensait aussi à l'existence d'immenses grottes dont les toits s'effondreraient. Les neptunistes éprouvèrent des difficultés résultant de l'impossibilité d'expliquer des couches redressées par une sédimentation verticale. L'auteur expose les débuts des recherches sur la tectonique du fossé rhénan et montre en particulier qu'Élie de Beaumont, qui parla en 1836 d'une voûte effondrée avait déjà auparavant eu connaissance d'une voûte effondrée en Islande et d'une voûter structurale allant du Wurttemberg en Lorraine par-dessus la Forêt-Noire et les Vosges. Par erreur,É de Beaumont plaça le moment de cet effondrement à l'époque du grès bigarré.Avec la théorie des soulèvements et des orogènes géognostiques L. v.Buch enrichit de 1824–1835 les théories orogéniques de deux concepts supplémentaires.Élie de Beaumont les développa et parla de révolution de la croûte terrestre (1829). Les premières recherches approfondies sur les chaînes plissées sont dues à J.Thurmann (1832) qui, d'après l'exemple du Jura plissé, démontra que seules des forces horizontales ont pu avoir été à l'oeuvre et que la théorie des soulèvements de L.von Buch n'apportait pas d'explication pour les chaînes de ce type.Pour terminer, l'auteur expose l'histoire de la boussole du géologue.

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