A Chandra X-ray survey of nearby dwarf starburst galaxies – II. Starburst properties and outflows     

Jürgen Ott †  Fabian Walter  Elias Brinks † 《Monthly notices of the Royal Astronomical Society》2005,358(4):1453-1471

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Endel Varep, 1915–1988     

Ott Kurs 《GeoJournal》1995,35(4):561-561

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Growth and Production in Posidonia Oceanica (L.) Delile*     

Jrg A. Ott 《Marine Ecology》1980,1(1):47-64

Abstract. In situ investigations of growth and production in a stand of Posidonia oceanica (L.) DELILE at a depth of 4 m at Ischia (Gulf of Naples) were carried out over two growing seasons. Posidonia starts to grow in August and an average bundle produces ten leaves in increasing time intervals until May. Growth curves for the leaves are given. Maximum leaf standing crop is in May with 1300 g dry weight per m^-2, leaf area index at this time reaches 22 m² m^-2. Leaf net productivity is highest in March with 12 g dry weight per m² per day. Annual leaf production is estimated as 3110 g dry weight per m², “underground” production as 115 g dry weight per m². About half the leaf production is exported from the system. Adaptive strategies of the growth and production pattern are discussed.  相似文献   

Editorial     

Jörg Ott Editor-in-Chief 《Marine Ecology》2003,24(2):81-81

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Preface     

Jörg Ott 《Marine Ecology》2007,28(S1):1-2

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Marine Ecology: Processes, Systems and Impacts.     

Jörg Ott 《Marine Ecology》2007,28(2):339-339

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The Vigny limestones: a record of Palaeocene (Danian) tectonic-sedimentary events in the Paris Basin     

Christian Montenat  Pascal Barrier  Philippe Ott D'Estevou 《Sedimentology》2002,49(3):421-440

Danian marine sedimentation in the Paris Basin occurred between two major erosional phases. The earlier was responsible for the stripping of presumably deposited Maastrichtian sediments and of a variable thickness of Campanian chalk. The later occurred during the late Palaeocene and resulted in the erosion of almost all Danian deposits, which are now limited to small and scattered outcrops. One of these outcrops corresponds to reefal and peri‐reefal limestones of middle to late Danian age, exposed in the quarries of Vigny (NW of Paris). Danian deposits here show intricate relations with the surrounding Campanian chalk. Danian sedimentation was contemporaneous with faulting, which generated signifiant sea‐floor relief and resulted in contrasting depositional areas: topographic highs with coralgal reefs, and depressions where calcirudite channel fill accumulated. Normal faulting occurred along WNW–ESE master faults. The generation of submarine fault scarps gave rise to various types of gravity‐driven phenomena, including the sliding and slumping of large blocks of reefal limestone and the deposition of carbonate debris flows. Along with the redeposition of the Danian carbonates, flows of fluidized and reworked Campanian chalk resulted from the peculiar physical properties of the undercompacted chalks. Erosion and faulting occurred predominantly during the Palaeocene and represent a major episode in the physiographic evolution of the Paris Basin.  相似文献   

Implanted radiogenic and other noble gases in crustal diamonds from Northern Kazakhstan     

A.B. Verchovsky  U. Ott  F. Begemann 《Earth and Planetary Science Letters》1993,120(3-4):87-102

Noble gases were extracted in steps from grain size fractions of microdiamonds ( < 100 μm) from the Kokchetav Massif, Northern Kazakhstan, by pyrolysis and combustion. The concentration of ⁴He in the diamonds proper (liberated by combustion) shows a 1/r dependence on grain size. For grain diameters > 15 μm the concentration also decreases with the combustion step. Both results are clear evidence that ⁴He has been implanted into the diamonds from -decaying elements in the surrounding matrix. The saturation concentration of ⁴He(5.6 × 10⁻⁴ cm³ STP/g) is among the very highest observed in any terrestrial diamonds. Fission xenon from the spontaneous fission of ²³⁸U accompanies the radiogenic ⁴He; the ¹³⁶Xe_f/⁴He ratio of (2.5 ± 0.3) × 10⁻⁹ agrees well with the production ratio of 2.3 × 10⁻⁹ expected in a reservoir where Th/U 3.3. Radiogenic ⁴⁰Ar is predominantly ( > 90%) set free upon combustion; it also resides in the diamonds and appears to have been incorporated into the diamonds upon their formation.

³He, on the other hand is mainly released during pyrolysis and hence is apparently carried by ‘contaminants’. The concentration in the diamonds proper is of the order of 4 × 10⁻¹² cm³ STP/g, with a ³He/⁴He ratio of 1 × 10⁻⁸. Excess ²¹Ne, similarly, appears to be present in contaminants as well as in diamonds proper. These two nuclides in the contaminants must have a nucleogenic origin, but it is difficult to explain their high concentrations.  相似文献   

Ein stratiformes Fluoritvorkommen im Zechsteindolomit bei Eschwege und Sontra in Hessen     

Dr. Heinz Ziehr  Klaus Matzke  Dr Gert Ott  Dr. Vassilios Vouttsidis 《International Journal of Earth Sciences》1980,69(2):325-348

Zusammenfassung Im Hauptdolomit (Ca₂) und im Plattendolomit (Ca₃) des mittleren Zechsteins bei Eschwege und Sontra in Hessen wurde 1974 erstmals Fluorit entdeckt. Durch Bohrungen, chemische und geochemische Untersuchungen konnte nachgewiesen werden, daß im Hauptdolomit der Fluorit schichtgebunden, gelegentlich in dunklen Lagen und Linsen bis 0,5 m mächtig, makroskopisch sichtbar auftritt. Häufiger kommt er in 18–20 m mächtigen Zonen vor, die aber wegen des geringen Fluoritgehaltes von unter 10 % CaF₂ sich von dem grauweißen Dolomit ohne Fluorit nicht unterscheiden.In den dunklen bis schwarz gefärbten Lagen schwanken die Fluoritgehalte zwischen 10 und 50 % CaF₂. Einzelproben enthalten bis 80 % CaF₂. Die Dunkelfärbung ist teils durch den Gehalt von violettem Fluorit, mehr noch durch Bitumen bedingt.Fluorit wurde ferner im stratigraphisch höher gelegenen Plattendolomit (Ca₃) der Leine-Serie Z3 gefunden. In Aufschlüssen und Steinbrüchen in der Nähe von Sontra enthält der Plattendolomit lokal 1–4 % CaF₂.Die makro- und mikroskopisch sichtbare Wechsellagerung von Fluorit und Dolomit mit einem deutlichen Lagengefüge und das Fehlen von hydrothermalem Fluorit und anderen Mineralien auf Gängen und Klüften sind Beweise für eine synsedimentäre Bildung des Fluorites im Hauptdolomit (Ca₂) und Plattendolomit (Ca₃) in Hessen. Für den Hauptdolomit wird angenommen, daß er spätdiagenetisch entstanden ist. Dies dürfte auch für den Fluorit zutreffen. Als Bildungsbereich werden flache Lagunen mit salinärer Fazies angenommen. Das Fluor stammt aus dem normalen Gehalt des Meerwassers. Es muß aber angenommen werden, daß der Fluorgehalt des Meerwassers durch Zufuhr von Fluor aus dem Festlande, z. B. aus den fluorreichen Graniten des Harzes merklich erhöht wurde. Nur so sind die großen Fluoritmengen im Zechsteindolomit in Hessen zu erklären. Sie werden auf 5–7·10⁶ + CaF₂ geschätzt.

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In 1974, fluorite was detected for the first time in the Hauptdolomit (Ca₂) and in the Plattendolomit (Ca₃) of the Middle Zechsteinformation near Eschwege and Sontra, Hessia. It was confirmed by means of drilling, chemical and geochemical investigations that the fluorite in the Hauptdolomit is stratabound. It occurs both locally in the form of macroscopic dark layers and lenses of up to 0,5 m thickness and moreoften, as zones up to 18–20 m thick which cannot macroscopically be distinguished from the greyish white dolomite without fluorite because of the low CaF₂ content (less than 10 %).The fluorite contents vary between 10 an 50 % CaF₂ in the dark black layers. Special samples may contain up to 80 % CaF₂. The dark colour derives partly from the lilac fluorite but to a greater degree from bitumous material.Fluorite has also been detected in the stratigraphically higher Plattendolomit (Ca₃) of the Leine-Series Z 3. Outcrops and quarries near Sontra have local contents of 1–4 % CaF₂.The macroscopic and microscopic interstratification of fluorite and dolomite with clear layer textures and the absence of hydrothermal fluorite and other minerals in veins of fissures are evidence for a synsedimentary formation of the fluorite in the Hauptdolomit (Ca₂) and the Plattendolomit (Ca₃). The Hauptdolomit is thought to have developed during late diagenesis. This should be valid for the fluorite, too. Shallow lagoons of a salinar facies are thought to have been the depositional environment. The fluorite precipitated from the sea waters, which were apparently enriched in fluorine by erosion at the fluorine rich granites of the Harz mountains. This is the only obvious explanation of the large amounts of fluorine in the Zechstein dolomite, estimated at 5–7×10⁶ tonnes CaF₂.

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Résumé En 1974, de la fluorine fut découverte dans la dolomie dite »Hauptdolomit« (Ca₂) et dans la dolomie dite »Plattendolomit» (Ca₃) du Zechstein moyen, près d'Eschwege et de Sontra, en Hesse. Les sondages effectués ainsi que les analyses chimiques et géochimiques ont montré que la fluorine se rencontre de façon stratiforme dans la »Hauptdolomit«, quelquefois en couches et lentilles foncées d'une épaisseur maximale de 0,5 m, ou elle est visible macroscopiquement. La fluorine est souvent présente en faibles teneurs (moins de 10% de CaF₂) dans des couches de 18 à 20 m d'épaisseur; de ce fait, ces dernières ne se distinguent pas de la dolomie gris-blanche exempte de fluorine.La teneur en fluorine varie de 10 % à 50% de CaF₂ dans les couches foncées à noires. Certains échantillons renferment jusqu'à 80% de CaF₂. La coloration foncée est due en partie à la fluorine violette, mais plus encore à la présence de bitume.De la fluorine fut également localisée dans la »Plattendolomit« (Ca₃) de la »LeineSerie Z 3«, qui est située à un niveau stratigraphique supérieur. Cette »Plattendolomit« telle qu'on la rencontre dans les affleurements et carrières des environs de Sontra, contient de 1–4% de CaF₂.L'alternance de fluorine et de dolomie qui, avec sa structure en couches nettement développées, est visible tant macroscopiquement que microscopiquement, ainsi que l'absence de fluorine hydrothermale et d'autres minéraux dans les filons et cassures, sont considérées comme preuves de la formation syn-sédimentaire de la fluorine dans la »Hauptdolomit« (Ca₂) et dans la »Plattendolomit« (Ca₃) de la Hesse. On suppose que la formation de la »Hauptdolomit« est diagénétique tardive. Cette hypothèse devrait également s'appliquer à la fluorine. Il est probable que ce processus a eu lieu dans les lagunes peu profondes à faciès salin. Le fluor provient de l'eau de mer à teneur normale. On peut cependant supposer que la teneur en fluor de l'eau de mer s'est accrue suite à l'apport de fluor provenant du continent, p.ex. à partir de granites riches en fluor du Harz. C'est seulement ainsi que peuvent s'expliquer les grandes quantités de fluorine de la dolomie du Zechstein, en Hesse. Elles sont évaluées entre 5 et 7 · 10⁶ de CaF₂.

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(Ca₂) (Ca₃) . , , , 0,5 . 18–20 , - — CaF₂ 10% — , . 10 50% CaF₂. 80% CaF₂. , . (Ca₃). 1–4% CaF₂. , , ; , . , Ca₂ . . , . . , ., , . . 5–7 × 10⁶ CaF₂.

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Unserem Lehrer, Herrn Professor Dr. Georg Fischer, München, zum 80. Geburtstag gewidmet.  相似文献   

Noble gases in mineral separates from three shergottites: Shergotty,Zagami, and EETA79001     

Susanne P. Schwenzer  Siegfried Herrmann  Ratan K. Mohapatra  Ulrich Ott 《Meteoritics & planetary science》2007,42(3):387-412

Abstract— This study provides a complete data set of all five noble gases for bulk samples and mineral separates from three Martian shergottites: Shergotty (bulk, pyroxene, maskelynite), Zagami (bulk, pyroxene, maskelynite), and Elephant Moraine (EET) A79001, lithology A (bulk, pyroxene). We also give a compilation of all noble gas and nitrogen studies performed on these meteorites. Our mean values for cosmic‐ray exposure ages from ³He, ²¹Ne, and ³⁸Ar are 2.48 Myr for Shergotty, 2.73 Myr for Zagami, and 0.65 Myr for EETA79001 lith. A. Serious loss of radiogenic ⁴He due to shock is observed. Cosmogenic neon results for bulk samples from 13 Martian meteorites (new data and literature data) are used in addition to the mineral separates of this study in a new approach to explore evidence of solar cosmic‐ray effects. While a contribution of this low‐energy irradiation is strongly indicated for all of the shergottites, spallation Ne in Chassigny, Allan Hills (ALH) 84001, and the nakhlites is fully explained by galactic cosmic‐ray spallation. Implanted Martian atmospheric gases are present in all mineral separates and the thermal release indicates a near‐surface siting. We derive an estimate for the ⁴⁰Ar/³⁶Ar ratio of the Martian interior component by subtracting from measured Ar in the (K‐poor) pyroxenes the (small) radiogenic component as well as the implanted atmospheric component as indicated from ¹²⁹Xe, * excesses. Unless compromised by the presence of additional components, a high ratio of ～2000 is indicated for Martian interior argon, similar to that in the Martian atmosphere. Since much lower ratios have been inferred for Chassigny and ALH 84001, the result may indicate spatial and/or temporal variations of ⁴⁰Ar/³⁶Ar in the Martian mantle.  相似文献