Control strategies for the Clam Wave Energy Device   总被引：1，自引：0，他引：1  

Martin Greenhow  Jay H. Rosen  Mark Reed 《Applied Ocean Research》1984,6(4):197-206

A promising wave energy device being currently investigated is the ‘clam’. The clam extracts energy by pumping air through a specially designed (Wells) turbine. Although operation of the Wells turbine does not require a rectified air flow, some additional control will be necessary to optimize the phase of the clam motion for good efficiencies. An examination of the equation of motion in the time domain suggests the possibility of phase control by mechanical, power take-off, or pneumatic latching. Latching can be shown to increase the efficiency of the device in the longer wavelengths of the wave spectrum, i.e. those of high incident wave power. Equivalently latching could be used to keep the device efficiency high while reducing its size, possibly resulting in cheaper power extraction.  相似文献   

Salmon lice, Lepeophtheirus salmonis (Kroyer), infestation in sympatric populations of Arctic char, Salvelinus alpinus (L.), and sea trout, Salmo trutta (L.), in areas near and distant from salmon farms     

Bjorn  Pal Arne; Finstad  Bengt 《ICES Journal of Marine Science》2002,59(1):131-139

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Solar limb brightening at the extreme limb from photoelectric eclipse observations     

Warren A. Rosen  Howard L. Poss 《Solar physics》1982,78(1):17-27

Photoelectric observations of the light intensity from the solar crescent before and after totality were made during the eclipses of 7 March, 1970 and 26 February, 1979. Effective wavelengths were determined by interference filters of 20 nm bandwidth. To obtain the limb darkening function, the resulting intensity curves were analyzed by an extension of the method of Julius in which we take into account the actual lunar limb profile. The limb darkening function at 433 nm was obtained for the region 0.937 < sin < 0.9999. Our results are in good agreement with existing center-to-limb measurements in the region of overlap which extends to sin = 0.99. Additional data were obtained at 600 nm for 0.994 < sin < 0.9999. The curves at both wavelengths show a distinctive limb brightening effect at sin = 0.999.  相似文献   

Reflectance spectra for sodium and potassium doped ammonia frosts: Implications for Io's surface     

M.D.A. Rosen  F.M. Pipkin 《Icarus》1978,35(2):252-262

This paper reports measurements of the reflection spectra of sodium and potassium doped ammonia frosts as a function of alkali metal concentration which cover the wavelength range 0.35–2.5 μm. The purpose of the measurements was to determine whether or not the reflection spectra for such a solid was compatible with the spectral albedo of Io. The data show that with a sufficiently large alkali metal concentration, the reflection spectra of the doped ammonia frost do not display the characteristic ammonia features at 2.0 and 2.25 μm. The high reflectance of the more concentrated samples and the character of the observed reflection spectrum make it difficult to rule out sodium doped ammonia frost as a surface constituent on Io on the basis of existing data.  相似文献   

Contamination of Silurian volcanic rocks in the Tagil synform by Precambrian zircon     

V. N. Puchkov  O. M. Rosen  D. Z. Zhuravlev  E. V. Bibikova 《Doklady Earth Sciences》2006,411(2):1381-1384

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Paleoproterozoic accretion in the Northeast Siberian craton: Isotopic dating of the Anabar collision system   总被引：1，自引：0，他引：1  

O. M. Rosen  L. K. Levskii  D. Z. Zhuravlev  A. Ya. Rotman  Z. V. Spetsius  A. F. Makeev  N. N. Zinchuk  A. V. Manakov  V. P. Serenko 《Stratigraphy and Geological Correlation》2006,14(6):581-601

Geochronological database considered in the work and characterizing the Anabar collision system in the Northeast Siberian craton includes coordinated results of Sm-Nd and Rb-Sr dating of samples from crustal xenoliths in kimberlites, deep drill holes, and bedrock outcrops. As is inferred, collision developed in three stages dated at 2200–2100, 1940–1760, and 1710–1630 Ma. The age of 2000–1960 Ma is established for substratum of mafic rocks, which probably originated during the lower crust interaction with asthenosphere due to the local collapse of the collision prism. Comparison of Sm-Nd and Rb-Sr isochron dates shows that the system cooling from ≈700 to ≈300°C lasted approximately 300 m.y. with a substantial lag relative to collision metamorphism and granite formation. It is assumed that accretion of the Siberian craton resulted in formation of a giant collision mountainous structure of the Himalayan type that was eroded by 1.65 Ga ago, when accumulation of gently dipping Meso-to Neoproterozoic (Riphean) platform cover commenced.  相似文献   

The Quantitative Mineral Composition of Sedimentary Rocks: Calculation from Chemical Analyses and Assessment of Adequacy (MINLITH Computer Program)     

Rosen  O. M.  Abbyasov  A. A. 《Lithology and Mineral Resources》2003,38(3):252-264

The MINLITH program provides for calculating the first approximation mineral composition of sedimentary rocks and their metamorphic counterparts from the bulk chemical compositions. The method is universal and can be applied to most types of clastic, pelitic, and carbonate sedimentary rocks based on a limited set of minerals and their simplified compositions. The program comprises a great number of arithmetic operations making up an algorithm. Each operation solves the equations allocating the major oxides to possible (expected) normative minerals. The operation sequence is determined from empirical relationships based on the study of numerous reference samples. The accuracy of MINLITH calculations was statistically estimated from comparison with results of the high-precision study of modal mineral compositions. Uncertainty is commonly within a range of 5–15 rel % and attains 60–70 rel % if the mineral content is below 5 wt %. It is evident that the program is a rather simple, convenient, and useful tool for the approximate estimation of mineral compositions of sedimentary rocks for lithological purposes.  相似文献   

High-precision stellar abundances of the elements: methods and applications     

Poul Erik Nissen  Bengt Gustafsson 《Astronomy and Astrophysics Review》2018,26(1):6

Efficient spectrographs at large telescopes have made it possible to obtain high-resolution spectra of stars with high signal-to-noise ratio and advances in model atmosphere analyses have enabled estimates of high-precision differential abundances of the elements from these spectra, i.e. with errors in the range 0.01–0.03 dex for F, G, and K stars. Methods to determine such high-precision abundances together with precise values of effective temperatures and surface gravities from equivalent widths of spectral lines or by spectrum synthesis techniques are outlined, and effects on abundance determinations from using a 3D non-LTE analysis instead of a classical 1D LTE analysis are considered. The determination of high-precision stellar abundances of the elements has led to the discovery of unexpected phenomena and relations with important bearings on the astrophysics of galaxies, stars, and planets, i.e. (i) Existence of discrete stellar populations within each of the main Galactic components (disk, halo, and bulge) providing new constraints on models for the formation of the Milky Way. (ii) Differences in the relation between abundances and elemental condensation temperature for the Sun and solar twins suggesting dust-cleansing effects in proto-planetary disks and/or engulfment of planets by stars; (iii) Differences in chemical composition between binary star components and between members of open or globular clusters showing that star- and cluster-formation processes are more complicated than previously thought; (iv) Tight relations between some abundance ratios and age for solar-like stars providing new constraints on nucleosynthesis and Galactic chemical evolution models as well as the composition of terrestrial exoplanets. We conclude that if stellar abundances with precisions of 0.01–0.03 dex can be achieved in studies of more distant stars and stars on the giant and supergiant branches, many more interesting future applications, of great relevance to stellar and galaxy evolution, are probable. Hence, in planning abundance surveys, it is important to carefully balance the need for large samples of stars against the spectral resolution and signal-to-noise ratio needed to obtain high-precision abundances. Furthermore, it is an advantage to work differentially on stars with similar atmospheric parameters, because then a simple 1D LTE analysis of stellar spectra may be sufficient. However, when determining high-precision absolute abundances or differential abundance between stars having more widely different parameters, e.g. metal-poor stars compared to the Sun or giants to dwarfs, then 3D non-LTE effects must be taken into account.  相似文献   

Retention of U and Pb in zircons from shocked granite in the Siljan impact structure,Sweden     

Göran berg  Bengt Bollmark 《Earth and Planetary Science Letters》1985,74(4):347-349

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Geodynamics of the Early Precambrian,Part 1: Volcanism and associated mantle processes     

O. M. Rosen  A. A. Shchipansky 《Stratigraphy and Geological Correlation》2007,15(5):449-469

The work is dedicated to most important abiotic processes of the Early Precambrian, effect of which is recorded in continental crust, and to complementary processes in subcontinental mantle. We intend to figure out when a certain process was triggered first in the past and what indications suggest its further activity, evolution and possible cessation in subsequent geological history. Considerations are based on described natural objects characterizing particular geological events and enabling the cause-and-effect interpretation in order to understand different viewpoints known from publications. Considered in the work are the early Precambrian greenstone belts and ophiolites, island-arc systems and ecologites, magmatism unconnected with subduction zones (rifting-related, plateau basalts, dykes, kimberlites) and anorthosites representing a group of heterochronous intrusions of complicated genesis. Main considerations are premised with a brief review of the earliest geodynamic phenomena associated with meteorite impacts by termination of the planetary accretion.  相似文献