Ship hull drag reduction using bottom air injection

The idea of bottom air injection to reduce ship hull resistance is not new. Early patents envisioned planing hull applications. Recent planing hull tests speed realized an increase of 7–12 knots. River barges and ship fitted with an air injection system results are presented to show a 10–15% reduction in the frictional resistance. Graphs for making initial estimates for displacement hulls with bottom air injection are presented. It is clear from these results that improvements in high speed planing catamarans and full form hull resistance can be realized by using bottom air injection.     

La constante solar

Zusammenfassung Aus der Temperatur der Sonnenoberfläche und der Entfernung Sonne-Erde ergiebt sich die Solarkonstante 2.4 in Uebereinstimmung mit dem rohen Wert, der die Instrument-Temperatur berücksichtigt. Da an den meisten Observatorien die mittägliche Sonnenhöhe nicht ausreicht für eine genaue Bestimmung der Solarkonstante, wird 2.4 als rohe vorläufige Solarkonstante vorgeschlagen, bis im Laufe der nächsten 2 Jahre eine genauere Bestimmung vorliegt. Vermutlich ist auch die Strahlungskonstante von dem Temperaturfehler beeinflusst.     

The atmospheric tide as a continuous spectrum: Lunar semidiurnal tide in surface pressure

Summary The standard equations for the theory of atmospheric tides are solved here by an integral representation on the continuous spectrum of free oscillations. The model profile of back-ground temperature is that of the U.S. Standard Atmosphere in the lower and middle atmosphere, and in the lower thermosphere, above which an isothermal top extends to arbitrarily great heights. The top is warm enough to bring both the Lamb and the Pekeris modes into the continuous spectrum.Computations are made for semidiurnal lunar tidal pressure at sea level at the equator, and the contributions are partitioned according to vertical as well as horizontal structure. Almost all the response is taken up by the Lamb and Pekeris modes of the slowest westward-propagating gravity wave. At sea level, the Lamb-mode response is direct and is relatively insensitive to details of the temperature profile. The Pekeris mode at sea level has an indirect response-in competition with the Lamb mode-and, as has been known since the time of its discovery, it is quite sensitive to the temperature profile, in particular to stratopause temperature. In the standard atmosphere the Lamb mode contributes about +0.078 mb to tidal surface pressure at the equator and the Pekeris mode about –0.048 mb.The aim of this investigation is to illustrate some consequences of representing the tide in terms of the structures of free oscillations. To simplify that task as much as possible, all modifying influences were omitted, such as background wind and ocean or earth tide. Perhaps the main defect of this paper's implementation of the free-oscillation spectrum is that, in contrast to the conventional expansion in the structures of forced oscillations, it does not include dissipation, either implicity or explicity, and thus does not satisfy causality. Dissipation could be added implicity by means of an impedance condition, for example, which would cause up-going energy flux to exceed downgoing flux at the base of the isothermal top layer. To achieve complete causality, however, the dissipation must be modeled explicity. Nevertheless, since the Lamb and Pekeris modes are strongly trapped in the lower and middle atmosphere, where dissipation is rather weak (except possibly in the surface boundary layer), more realistic modeling is not likely to change the broad features of the present results.Symbols a earth's mean radius; expansion coefficient in (5.3) - b recursion variable in (7.4); proximity to resonance in (9.2) - c sound speed in (2.2); specific heatc _p in (2.2) - f Coriolis parameter 2sin in (2.2) - g standard surface gravity - h equivalent depth - i ; discretization index in (7.3) - j index for horizontal structure - k index for horizontal structure; upward unit vectork in (2.2) - m wave number in longitude - n spherical-harmonic degree; number of grid layers in a model layer - p tidal pressure perturbation; background pressurep ₀ - q heating function (energy per mass per time) - r tidal state vector in (2.1) - s tidal entropy perturbation; background entropys ₀ - t time - u tidal horizontal velocityu - w tidal vertical component of velocity - x excitation vector defined in (2.3); vertical coordinate lnp _*/p ₀ [except in (3.8), where it is lnp /p ₀] - y vertical-structure function in (7.1) - z geopotential height - A constant defined in (6.2) - C spherical-harmonic expansion coefficient in (3.6) - D vertical cross section defined in (5.6) and (5.9) - E eigenstate vector - F vertical-structure function for eigenstate pressure in (3.2) [re-defined with WKB scaling in (7.2)] - G vertical-structure function for eigenstate vertical velocity in (3.2) [re-defined with WKB scaling in (7.2)] - H pressure-scale height - I mode intensity defined in (8.1) - K quadratic form defined in (4.4) - L quadratic form defined in (4.4); horizontal-structure magnification factor defined in (5.11) - M vertical-structure magnification factor defined in (4.6) - P eigenstate pressure in (3.2); tidal pressure in (6.2) - R tidal state vector in (5.1) - S eigenstate entropy in (3.2); spherical surface area, in differential dS - T background molecular-scale (NOAA, 1976) absolute temperatureT ₀ - U eigenstate horizontal velocityU in (3.2); coefficient in (7.3) - V horizontal-structure functionV for eigenstate horizontal velocity in (3.2); recursion variable in (7.3) - W eigenstate vertical velocity in (3.2) - X excitation vector in (5.1) - Y surface spherical harmonic in (3.7) - Z Hough function defined in (3.6) - +dH/dz - (1––)/2 - Kronecker delta; Dirac delta; correction operator in (7.6) - equilibrium tide elevation - (square-root of Hough-function eigenvalue) - ratio of specific gas constant to specific heat for air=2/7 - longitude - - - background density ₀ - eigenstate frequency in (3.1) - proxy for heating functionq =c _P/t - latitude - tide frequency - operator for the limitz - horizontal-structure function for eigenstate pressure in (3.2) - Hough function defined in (6.2) - earth's rotation speed - horizontal gradient operator - ()₀ background variable - ()_* surface value of background variable - () value at base of isothermal top layer - Õ state vector with zerow-component - , energy product defined in (2.4) - | | energy norm - ()^* complex conjugate With 10 Figures     

Klastische und pyroklastische Sedimente des Südharzer Rotliegenden

Ohne Zusammenfassung     

Über stratigraphische Untersuchungsmethoden in rezenten Tiefseesedimenten

Zusammenfassung Durch Bestimmung der Foraminiferenanzahl in I g Sediment wird die biostratigraphische Untersuchungsmethode, die mittels einer qualitativen und quantitativen Erfassung der Foraminiferenfauna in den Tiefseekernen der deutschen Meteor-Expedition und schwedischen Albatroß-Expedition durchgeführt werden ist, auf ihre Richtigkeit hin geprüft. Die Untersuchung hat die Anwendbarkeit dieser stratigraphischen Methode bestätigt. Sie hat daneben wiederum gezeigt, daß die Verbreitung und Entwicklung der einzelnen Foraminiferenarten vor allem von der Temperatur des Meerwassers abhängig sind; andere Faktoren wie Phosphatgehalt des Wassers usw. scheinen in dieser Hinsicht eine mehr untergeordnete Rolle zu spielen. Unter gewissen Voraussetzungen können Tiefseekerne durch Bestimmung der Foraminiferenanzahl je 1 g Sediment in groben Zügen stratigraphisch gegliedert werden; auch kann die Individuenanzahl der einzelnen Foraminiferenarten aus der Foraminiferenanzahl in 1 g Sediment und aus der prozentualen Zusammensetzung der Gesamtfauna errechnet werden. Mit den hier gewonnenen Erkenntnissen wird versucht, die engen Bezichungen zwischen dem prozentualen Anteil der Warmwasserforaminiferen in der Gesamtfauna und dem CO₂-Gehalt des Sedimentes, dieOvey im Kern 241 der schwedischen Albatroß-Expedition beobachtet hat, zu deuten.Herrn Professor Dr.Carl W. Correns zum 60. Geburtstag gewidmet.     

Changes in the water regime of the caspian sea

The article deals with issues of structure and dynamics of the Caspian Sea water balance. On the base of historical, paleogeomorphological and other data the evolution history of the Caspian Sea and its basin has been observed for different time intervals down to 400 thous. years ago. Presented are computerized data on water balance components in the current centenary obtained from instrumental observations, revealed are causes of the sea-level fluctuations within that time interval and anthropogenic factor contribution to this process. Based on the analysis of this material, an attempt has been undertaken to present a scenarion of a possible sea-level position of the Caspian Sea with the expected versions of climatic changes at the end of the XX and beginning of the XXI centuries.     

Orthogneisses due to irrotational extension,a case from the Sudetes,Bohemian massif

Orthogneisses occurring in the core of the Orlica-Kodzko dome, NE part of the Bohemian massif, exibit a penetrative, N-S stretching lineation defined by mostly ductile elongation of quartz and dilation of K-feldspar crystals of the former granite, now turned into quartz rods and variously elongated K-feldspar porphyroclasts. N-S stretching of the granite seems to be inconsistent with W-E tectonic transport shown by major folds and thrusts developing concurrently in its schistose envelope. The two major lithologies of the dome, differing in their fabrics and rheological properties, offered a drastically different response to an overall shortening. It is interpreted that folds due to buckling evolved in the mantle rocks and after a certain definite range of incremental shortening suffered extension parallel to their hinges. At that time the statistically isotropic granite body was subjected to the same N-S extension and was deformed in common with its schistose mantle under conditions of irrotational strain which represents an early but significant part of the protracted deformation history related to the granite-gneiss transformation.

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Zusammenfassung Die Orthogneise, die im NE-Teil der Böhmischen Masse den Kern der Adlergebirge-Kodzko-Kuppel bilden, zeigen eine N-S-ausgerichtete Streckungslineation. Die Streckungsfaser ist an plastisch gedehnten Quarz-Aggregaten zu erkennen sowie an Klastenzügen von Kalifeldspat. Große Falten und Überschiebungen in der Schieferhülle des Granits hingegen geben eine W-E Richtung des tektonischen Transports an. Diese entspricht nicht der Längung des Granits.Zur Deutung werden die unterschiedlichen rheologischen Eigenschaften des Granits und seiner Hüllgesteine herangezogen, die auf Unterschieden der Zusammensetzung und des Gefüges beruhen. Diese Unterschiede bewirken, daß die Hüllgesteine zunächst Biegefaltung erleben bis weitere Einengung durch Faltung unmöglich wird. Daraufhin werden die Hüllgesteine parallel zur Faltenachse in N-S-Richtung gedehnt. Diese Dehnungsrichtung ist allein und von Anfang an den isotropen Graniten überprägt.Die Deformation erfolgte irrotational und nahezu als achsialsymmetrische Streckung. Sie stellt ein frühes, aber wichtiges Stadium der Umwandlung dieses Granits zu Gneisen dar.

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Résumé Les orthogneiss qui constituent le coeur du dôme d'Orlica-kodzko (région nord-est du massif de Bohème) présentent une linéation d'étirement pénétrative orientée nordsud. Cette linéation est exprimée principalement par l'allongement ductile en bâtonnets d'agrégats de quartz et par l'alignement de porphyroclastes de feldspath potassique. D'autre part, dans l'encaissant schisteux du granite, les grands plis et les charriages indiquent une direction ouest-est du transport tectonique, ce qui ne semble donc pas correspondre à la structure de l'orthogneiss central.Ce contraste est interprété par la différence entre les propriétés rhéologiques des deux ensembles lithologiques, qui ont répondu de manières différentes au processus de raccourcissement régional. Dans les roches de l'enveloppe, se sont formés d'abord des plis de courbure, jusqu'à un certain degré de raccourcissement, après quoi, ce processus n'étant plus possible, elles ont subi un étirement parallèle aux axes de ces plis. Le corps granitique isotrope, au contraire, a réagi dès le début par une extension nord-sud. Ces conditions de déformation irrotationnelle, à symétrie quasi-axiale, représentent un stade précoce, mais significatif de la transformation du granite en orthogneiss.

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