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71.
Dipl.-Ing. Uwe Hammerschmidt 《Ocean Dynamics》1968,21(1):1-14
Zusammenfassung Das Hi-Fix-Verfahren ist ein funktechnisches Hilfsmittel zur Ortsbestimmung auf der Grundlage der Hyperbelnavigation, das in küstennahen Seegebieten eingesetzt wird. Es werden das Prinzip, die Technik und die Anwendung dieses Verfahrens behandelt. Über die im praktischen Einsatz gesammelten Erfahrungen, sowie über die Aufgabenstellung für die Auswertung zahlreichen Registriermaterials, das während des Großversuches einiger Bundesbehörden in den Jahren 1964 und 1965 anfiel, wird berichtet. Es soll dabei untersucht werden, welchen Einfluß geophysikalische Größen, wie z. B. die Bodenleitfähigkeit und atmosphärische Störungen (Gewitter) sowie Sekundärstrahlungen von metallischen Gebilden in Empfängernähe auf die Anzeigegenauigkeit der Hi-Fix-Geräte ausüben.
Nach einem Vortrag, gehalten auf der Meteorologen-Geophysiker-Tagung am 4. 4. 1968 in Hamburg.
Hi-Fix ist eine Abkürzung für High Accuracy Position Fixing, es wird ebensowenig aufgelöst wie z. B. Radar. Die Redaktion. 相似文献
Hi-Fix — a new tool of position fixing in near-coastal sea areas
Summary Hi-Fix is a new tool of position fixing on the basis of hyperbolic navigation that is used in near-coastal sea areas. Principle, technique, and application of this system are treated. A report is given of the experience gained from field work as well as of the objects of the evaluation of the numerous recordings obtained from a large-scale experiment conducted by several federal agencies in the years 1964 and 1965. The effect of geophysical quantities, such as soil conductivity and atmospherics (thunderstorm) as well as secondary radiation from metallic bodies in the vicinity of the receiver on the indication accuracy of the Hi-Fix devices shall be studied.
Hi-Fix — un nouveau procédé de localisation en mer à proximité de la côle
Résumé Le procédé Hi-Fix apporte une nouvelle contribution au problème de la localisation; il est basé sur le système hyperbolique et utilisé dans les eaux côtières. Il est rendu compte des expériences réalisées pratiquement ainsi que de la tâche qu'imposait, à quelques autorités fédérales, l'exploitation des nombreuses informations recueillies au cours des essais à grande échelle des années 1964 et 1965. A cette occasion on cherche à mesurer l'influence qu'exercent sur la précision fournie par les appareils Hi-Fix, des grandeurs atmosphériques (orages) ainsi que les rayonnements secondaires de formations métalliques au voisinage du récepteur.
Nach einem Vortrag, gehalten auf der Meteorologen-Geophysiker-Tagung am 4. 4. 1968 in Hamburg.
Hi-Fix ist eine Abkürzung für High Accuracy Position Fixing, es wird ebensowenig aufgelöst wie z. B. Radar. Die Redaktion. 相似文献
72.
Michael A. Feierberg Harold P. Larson Uwe Fink Howard A. Smith 《Geochimica et cosmochimica acta》1980,44(3):513-524
A Fourier spectrometer was used to obtain IR spectra of asteroids 349 Dembowska and 4 Vesta (0.8–2.5μm; 25cm ?1 resolution). The spectrum of Dembowska shows olivine and pyroxene (Fs24 ± 8) with an olivine/pyroxene abundance ratio greater than 2, and possibly as high as 10. This is probably an unsampled achondritic composition, similar to the unique achondrite ALHA 77005. Similar olivine-rich compositions have also been proposed for the mantles of basaltic achondrite parent bodies. Dembowska's mineralogy therefore appears related in some way to the achondrites. but a direct link cannot as yet be made. Our IR observations of Vesta have more complete spectral coverage than those first obtained by Larson and Fink (1975b). Pyroxene (Fs50 ± 5) and plagioclase feldspar are both seen, with a pyroxene/feldspar abundance ratio between 1.5 and 2.0. Vesta's mineralogy is consistent with a mixture of eucrites and howardites on its surface. Time-resolved observations over one-half of the rotation period show no spectral variations at the 2% level, indicating compositional homogeneity. Both 349 Dembowska and 4 Vesta can be considered as candidates for the parent bodies of igneous meteorites. 相似文献
73.
Uwe Walzer 《Physics of the Earth and Planetary Interiors》1982,30(1):62-83
A new equation of state for metals is developed. The starting point for this development is a realistic expression for the free energy, allowance being made not only for the lattice energy but also for the Fermi energy, the exchange and correlation energies of the electrons. This expression is extended by means of three free parameters. The equation of state is successfully transformed in such a way that only macrophysical material parameters occur in it. In this way, the equation can be applied both to experimental high-pressure physics and to geophysics, its advantage resting in the fact that the bonding structure has been taken into account better than in other equations of state.The new equation, along with two other well-proven equations of state, was tried out on isothermal and Hugoniot data of 40 materials. Good agreement with the measured data was found not only for metallic elements, but also for halides and some oxides of geophysical importance. This agreement even proved to be better for most of the materials than that obtained with the other two equations of state. 相似文献
74.
Uwe Walzer 《Pure and Applied Geophysics》1971,87(1):73-92
Summary A system of simple principles concerning the kinematics of the convection currents in the Earth's mantle was postulated as the starting point. The mantle is supposed to become more and more homogeneous downward. Here it is essential, for the reason of symmetry, that the current system has a degree of regularity as high as possible and is modified only in the upper part, mainly due to the distribution of continents and oceans. The adequate system is chosen by the help of the theory of point groups. Evaluating the distribution to be expected of the coefficients of the spherical harmonic development of the Earth's theoretical topography by means of electronic computers, accordance is found for the extrema to the 31 st order, i.e. as far as they have been determined until now. — The system yields the seismic discontinuities of the Earth's mantle as a secondary product. That does not mean that the system explains them, but it is absolutely consistent with them. That seems to be aquantitative proof of the system regarded as probable on the strength of group-theoretic considerations.Report No. 74, lectured in Potsdam, May 7, 1970. 相似文献
75.
76.
Manuela A. Fehr Mark Rehkämper Alex N. Halliday Uwe Wiechert Detlef Günther Jennifer L. Eigenbrode Douglas Rumble III 《Geochimica et cosmochimica acta》2005,69(21):5099-5112
New precise Te isotope data acquired by multiple collector inductively coupled plasma mass spectrometry (MC-ICPMS) are presented for selected extraterrestrial and terrestrial materials. Bulk samples of carbonaceous, ordinary and enstatite chondrites as well as the metal and sulfide phases of iron meteorites were analyzed to search for nucleosynthetic isotope anomalies and to find evidence of formerly live 126Sn, which decays to 126Te with a half-life of 234,500 yr. None of the meteorites show evidence of mass dependent Te isotope fractionations larger than 2‰ for δ126/128Te. Following internal normalization of the data to 125Te/128Te, the Te isotope ratios of all analyzed meteorites were found to be identical to a terrestrial standard, within uncertainties. This provides evidence that the regions of the solar disk that were sampled during accretion of the meteorite parent bodies were well mixed and homogeneous on a large scale, with respect to Te isotopes. The data acquired for bulk carbonaceous chondrites indicate that the initial 126Sn/118Sn ratio of the solar system was <4 × 10−5, but this is dependent on the assumption that no redistribution of Sn and Te occurred since the start of the solar system. Five Archean sedimentary sulfides that display both mass dependent and mass-independent isotope effects for S yield internally normalized Te isotope data, which indicate that mass-independent Te isotope effects are absent. The mass dependent fractionations in these samples are constrained to be less than ∼1‰ for δ126/128Te. 相似文献
77.
Moraines southwest of Lake Yashilkul, Pamir, Tajikistan, were dated using 10Be exposure ages of boulder surfaces. We found evidence for (1) an extensive glaciation ∼60,000 yr ago; (2) a less extensive glacial advance, which deposited a characteristic hummocky moraine lobe with exposure ages ranging from ∼11,000 to 47,000 yr, probably deposited at or before 47,000 yr ago; and (3) lateral moraines with exposure ages of ∼40,000 yr, 27,000 yr and 19,000 yr, respectively. Increasing aridity in the Pamir is most likely responsible for the progressively limited extent of the glaciers during the Late Pleistocene. 相似文献
78.
In-situ Measurements of Tropospheric Hydroxyl Radicals by Folded Long-Path Laser Absorption During the Field Campaign POPCORN 总被引:1,自引:0,他引:1
Uwe Brandenburger Theo Brauers Hans-Peter Dorn Martin Hausmann Dieter H. Ehhalt 《Journal of Atmospheric Chemistry》1998,31(1-2):181-204
Absolutely calibrated in-situ measurements of tropospheric hydroxyl radicals, formaldehyde, sulfur dioxide, and naphthalene (C10H8) were performed by long-path laser absorption spectroscopy during the field campaign POPCORN. The absorption light path was folded into an open optical multiple reflection cell with a mirror separation of 38.5 m. Using a light path length of 1848 m and an integration time of 200 s, the average 1-detection limits of OH, HCHO, SO2 and C10H8 during POPCORN were 8.7 · 105 cm–3, 8.3 · 109 cm–3, 2.4 · 109 cm–3, 1.5 · 108 cm–3, respectively. In total, 392 identifications of OH in air spectra were made in a rural environment between August 5 and August 23, 1994. We present and discuss OH absorption spectra and diurnal OH concentration profiles of three days which are representative for measurements under different pollution conditions during POPCORN. The observed maximum and median OH radical concentrations are 1.3 · 107 OH/cm3 and 4.0 · 106 OH/cm3, respectively. The measured diurnal variation of the OH concentration shows a good correlation with the primary formation reaction of OH radicals which is the photolysis of ambient ozone. Deviations from this correlation in the morning and evening hours, when the OH concentration is higher than expected from the ozone photolysis, demonstrate the importance of other photochemical HOx production pathways during POPCORN. 相似文献
79.
A numerical scheme is described for the calculation of effective albedo values of long city street canyons. The method is based on a generalization of the radiation model for inclined surfaces recently presented by Brühl and Zdunkowski (1983). Calculated albedo values are compared with Aida's (1982) experimentally determined results. It is found that experiment and theory are in reasonable and in some cases in excellent agreement. Additional results obtained by varying the geometry of the street canyon as well as the surface reflectivities are shown to demonstrate the versatility of the calculation scheme. 相似文献
80.
Thomas Neumann Uwe HeiserMarkus A Leosson Michael Kersten 《Geochimica et cosmochimica acta》2002,66(5):867-879
The formation of authigenic Ca-rich rhodochrosite (ACR) in sapropelic sediments of the Gotland Basin, Baltic Sea, is governed by deepwater renewal processes whereby saline water from the North Atlantic flushes the brackish anoxic Baltic Deeps. The carbon and oxygen isotopic compositions of these Mn-carbonates suggest that ACR formation takes place just below the sediment surface and that dissolved compounds from the deepwater column, such as water and bicarbonate molecules, were incorporated in ACR during authigenesis. Porewaters near the sediment surface display δ18O values of −5.4‰ (VSMOW) and are generally depleted in 18O, compared to the oxygen isotopic composition of water in equilibrium with Mn-carbonate solid solutions (ACR δ18O values are −4.6‰). This suggests that early burial diagenetic processes significantly modify the initial isotopic composition of water during Mn-carbonate formation. The reduction of sulfate having δ18O values of +8.4‰ accounts for a permanent enrichment of porewater 18O and observed δ18O values at depth equal to −4.6‰. However, this process does not explain the observed disequilibrium in the oxygen isotopic composition between water and ACR close to the sediment surface where Mn-carbonate formation takes place. Based on isotopic mass balance calculations, we suggest that MnO2 with δ18O values of +8.9‰ released oxygen enriched in 18O into the anoxic porewaters close below the sediment surface. This process should occur after oxygenation events during deepwater renewal when MnO2 accumulates at the surface of anoxic sediments. Manganese carbonates formed in these waters display δ18O values of ∼1.0‰ heavier than values expected solely from the initial deepwater composition. This quantitatively explains the discrepancy between paleosalinities calculated from ACR δ18O based on Mn-carbonate/water isotopic equilibrium fractionation and direct observations for the same period. Our results emphasize the important role of microbial MnO2 reduction during rhodochrosite authigenesis and suggest that Mn(II) activity, rather than alkalinity, is the limiting component for sedimentary Mn-carbonate formation. 相似文献