A Compilation of Radiocarbon Dates from Disko Bugt,Central West Greenland/Meteorological Observations in 1996 at the Arctic Station,Qeqertarsuaq (Godhavn), Central West Greenland/A Discussion on Pingos in Mellemfjord,Disko, Central West Greenland/Open System Pingos in Mellemfjord,Disko, Central West Greenland: A Reply to Gurney and Worsley     

Morten Rasch  Birger Hansen  Ole Humlum  Niels Nielsen  Peter Funch  Stephen D. Gurney 《Geografisk tidskrift / udgivet af Bestyrelsen for Det Kongelige danske geografiske selskab》2013,113(1):143-159

188 new and previously published radiocarbon dates on Holocene material from Disko Bugt, central West Greenland, are presented together with relevant informations (laboratory number, place name, dated material, geografic coordinates, altitude and δ¹³C-value) about the dates.

In October 1990 an automatic weather station was established at the Arctic station (65 °15′N,53 °31′W), Qeqertarsuaq (Godhavn), Central West Greenland. The Station register parameters each 20 min., and the parameters have been described in an earlier paper in this journal by Nielsen et al. (1995). The present paper summarises main points of the climate during 1996.

Open system, or more correctly, hydraulic pingos, are genetically poorly understood. A continuing problem concerns their need for a perennial groundwater supply (intra- or sub-permafrost). This has to be maintained despite the existence of continuous permafrost in many areas where they are located. Recent work on Disko Island has suggested a new type of hydraulic pingo developing only in a “marsh environment”. It is argued that the marsh setting is not relevant to the formation of these features and that they are simply hydraulic pingos.

Abstract

A group of marsh initiated open system pingo remnants from the Iterdlagssûp kûgssua valley mouth, in Mellemfjord, Disko Island, Central West Greenland was described in Christiansen (1995). Gurney and Worsley (1997) state that the location of this group of pingo remnants in the Iterdlagssûp kûgssua valley mouth is of no relevance to their genesis, and that they presumably were the result of an assumed late Holocene sea level regression, causing permafrost to be established in the valley bottom. In this reply the arguments by Gurney and Worsley (1997) on the Iterdlagssûp kûgssua valley pingos are commented, and it is argued by way of sea level information, frost penetration and water supply that the special setting must indeed have caused pingo initiation and growth. Furthermore, the area has experienced a relative sea level rise during the late Holocene.  相似文献   

Meteorological Observations 2002 at the Arctic Station,Qeqertarsuaq (69°15'N), Central West Greenland     

Birger Ulf Hansen  Ole Humlum  Niels Nielsen  Dorte P. Lundqvist  Ditte L. Jansen  Christian Christiansen 《Geografisk tidskrift / udgivet af Bestyrelsen for Det Kongelige danske geografiske selskab》2013,113(2):93-109

An automatic meteorological station has been operating at the Arctic Station (69°15'N, 53°31'W) in West Greenland since 1990. This paper summarises meteorological parameters during 2002, including snow cover, ground temperatures and active layer development, and air temperatures at the Station during the last 12 years are compared to large scale trends during the last century.

A compilation of 93 sedimentation rate determinations based on ²¹⁰Pb dating has been carried out for the North Sea-Baltic Sea transition area from a database containing 165 determinations carried out by Danish institutions. In the depositional parts of the area sedimentation rates generally range 25–6403 g m^?2 y^?1. An extreme rate of 13351 g m^?2 y^?1 is observed on a station in the Skagerrak. Sedimentation rates significantly increase with depth indicating that the Skagerrak and northern parts of the Kattegat as well as the deep basins in the Baltic Sea act as depocentres for fine-grained sediments. Apparently, sedimentation rates have increased in recent years.  相似文献   

Mutual validation of GNSS height measurements and high-precision geometric-astronomical leveling     

Christian Hirt  Martin Schmitz  Uwe Feldmann-Westendorff  Gerhard Wübbena  Cord-Hinrich Jahn  Günter Seeber 《GPS Solutions》2011,15(2):149-159

The method of geometric-astronomical leveling is presented as a suited technique for the validation of GNSS (Global Navigation Satellite System) heights. In geometric-astronomical leveling, the ellipsoidal height differences are obtained by combining conventional spirit leveling and astronomical leveling. Astronomical leveling with recently developed digital zenith camera systems is capable of providing the geometry of equipotential surfaces of the gravity field accurate to a few 0.1 mm per km. This is comparable to the accuracy of spirit leveling. Consequently, geometric-astronomical leveling yields accurate ellipsoidal height differences that may serve as an independent check on GNSS height measurements at local scales. A test was performed in a local geodetic network near Hanover. GPS observations were simultaneously carried out at five stations over a time span of 48 h and processed considering state-of-the-art techniques and sophisticated new approaches to reduce station-dependent errors. The comparison of GPS height differences with those from geometric-astronomical leveling shows a promising agreement of some millimeters. The experiment indicates the currently achievable accuracy level of GPS height measurements and demonstrates the practical applicability of the proposed approach for the validation of GNSS height measurements as well as the evaluation of GNSS height processing strategies.  相似文献   

Response of xenotime to prograde metamorphism     

Birger Rasmussen  Ian R. Fletcher  Janet R. Muhling 《Contributions to Mineralogy and Petrology》2011,162(6):1259-1277

Xenotime is a widespread accessory mineral in lower greenschist to upper amphibolite facies metasedimentary rocks from the Palaeoproterozoic Mount Barren Group, southwestern Australia. Xenotime is closely associated with detrital zircon, commonly forming syntaxial outgrowths, in samples of sandstone, micaceous quartzite, slate, phyllite, garnet-bearing semi-pelites, and in kyanite-, garnet-, and staurolite-bearing mica schists. In situ geochronology of xenotime from lower greenschist sandstones has previously yielded multiple U–Pb ages with peaks at ~2.0, ~1.7, and ~1.65 Ga, interpreted to represent the age of detritus, early diagenesis, and a later thermal event, respectively. New U–Pb dating of xenotime in slate yields a major population at ~1.7 Ga with a minor population at ~1.2 Ga, reflecting diagenetic and metamorphic growth, respectively, whereas xenotime in phyllite forms a minor age population at ~1.7 Ga and a main peak at ~1.2 Ga. Mid-greenschist facies semi-pelitic schists (quartz-muscovite-garnet) contain xenotime that formed before 1.8 Ga and at 1.2 Ga, representing detrital and peak metamorphic ages, respectively. Xenotime in samples of amphibolite facies schist (650°C and ~8 kbars) yields U–Pb ages of ~1.2 Ga, coinciding with the time of peak metamorphism. A single analysis of a xenotime core from an amphibolite facies schist gave an age of ~1.8 Ga, consistent with the presence of detrital xenotime. Our results suggest that detrital xenotime may be preserved under greenschist facies conditions, but is largely replaced during upper amphibolite facies conditions. Detrital xenotime is replaced through dissolution–reprecipitation reactions forming compositionally distinct rims during greenschist and amphibolite facies metamorphism at 1.2 Ga. Diagenetic xenotime is present in lower greenschist facies samples, but was not observed in metasedimentary rocks that had experienced temperatures above mid-greenschist facies metamorphism (450°C). The apparent disappearance of detrital and diagenetic xenotime and appearance of metamorphic xenotime during prograde metamorphism indicates that some of the yttrium, heavy rare earth elements, and phosphorus needed for metamorphic xenotime growth are probably derived from the replacement of detrital and diagenetic xenotime.  相似文献   

Pb/Pb geochronology, petrography and chemistry of Zr-rich accessory minerals (zirconolite, tranquillityite and baddeleyite) in mare basalt 10047     

Birger Rasmussen  Ian R. Fletcher 《Geochimica et cosmochimica acta》2008,72(23):5799-5818

In situ U-Pb isotopic measurements were carried out by ion microprobe on the Zr-rich accessory minerals zirconolite [CaZrTi₂O₇], tranquillityite [Fe₈²⁺(ZrY)₂Ti₃Si₃O₂₄] and baddeleyite [ZrO₂] in low-K, high-Ti mare basalt 10047 collected during the Apollo 11 mission. The analysed minerals are concentrated in pockets of late-stage mesostasis that comprises an intergrowth of silica, barian K-feldspar and Si-Al-K glass, from a phaneritic, subophitic, basalt comprising mainly pyroxene, plagioclase, ilmenite, cristobalite and troilite. Most Zr-rich minerals are unaltered, however, some tranquillityite is replaced by a complex intergrowth of zirconolite, baddeleyite, ilmenite and fayalite, suggesting that the mineral became unstable during crystallization. Several baddeleyite crystals have also undergone alteration to secondary zircon. Zirconolite was analysed in thin section 10047,11 and tranquillityite and baddeleyite in 10047,227, using a ∼6 μm primary ion beam. Both zirconolite and tranquillityite have significant U and low initial Pb contents, and are highly suitable for Pb/Pb dating. Fifteen analyses of zirconolite give a ²⁰⁷Pb/²⁰⁶Pb age of 3708 ± 7 Ma (²⁰⁷Pb/²⁰⁶Pb:²⁰⁴Pb/²⁰⁶Pb isochron; 95% confidence, including renormalisation of ratios) and twenty-five analyses of tranquillityite give 3710 ± 6 Ma. The ²⁰⁷Pb/²⁰⁶Pb dates are consistent with each other and refine results from an earlier study. Baddeleyite data were less precise, mainly due to lower secondary ionisation efficiency. Our results show that zirconolite and tranquillityite can provide precise isotopic dates and, given their presence in other samples, they represent important U-Pb chronometers for refining lunar geology.  相似文献   

Zirconolite,zircon and monazite-(Ce) U-Th-Pb age constraints on the emplacement,deformation and alteration history of the Cummins Range Carbonatite Complex,Halls Creek Orogen,Kimberley region,Western Australia   总被引：1，自引：0，他引：1  

Peter J. Downes  Daniel J. Dunkley  Ian R. Fletcher  Neal J. McNaughton  Birger Rasmussen  A. Lynton Jaques  Michael Verrall  Marcus T. Sweetapple 《Mineralogy and Petrology》2016,110(2-3):199-222

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Zu den beziehungen für den fluktuativen und mittleren Wassertransport in der Atmosphäre     

H. P. Schmitz 《Pure and Applied Geophysics》1963,55(1):217-238

Zusammenfassung Die Gleichungen für den mikro- und makroturbulenten Austausch und Transport von Wasser in gasförmiger, flüssiger und fester Form werden unter Benutzung abgewogener Augenblicks- und Mittelwerte des Geschwindigkeitsvektors dargestellt. Fragwürdigkeiten bei der Behandlung des bodennahen Wasserdampfaustausches nach dem Vorgang vonWilh. Schmidt und einige Probleme bei der Ermittlung von Verdunstung minus Niederschlag größerer Gebiete aus dem atmosphärischen Wassertransport werden erörtet.

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Summary The equations concerning the micro- and macroturbulent «austausch» and transport of water in its three phases are represented by using weighted vectors of instantaneous and average velocities. Usual defects in treating the eddy diffusion of water vapour next to the bottom by applying the theory ofWilhelm Schmidt are discussed as well as some problems in the estimation of evaporation minus precipitation of large areas from the transport of water in the atmosphere.

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Foraminiferal and δ13C isotopic event‐stratigraphy across the Danian–Selandian transition at Zumaya (northern Spain): chronostratigraphic implications     

I. Arenillas  E. Molina  S. Ortiz  B. Schmitz 《地学学报》2008,20(1):38-44

The Zumaya section, northern Spain, is a suitable candidate to define the Global Stratotype Section and Point for the base of the Selandian Stage (Palaeocene) because of its excellent accessibility, exposure and stratigraphic continuity. Uncertainties exist, however, with regard to the stratigraphic horizon where to place the Danian/Selandian (D/S) boundary. Five potential stratigraphic horizons (HDS1 to HDS5) to define the D/S boundary have been identified at Zumaya, based on integrated stratigraphic studies that include quantitative planktic and benthic foraminiferal results, as well as δ¹³C isotopic and lithological data. Two of these horizons (HDS2 and HDS4) placed in Zone C26r appear to have particularly good potential for serving as the D/S boundary marker, because they may represent significant global palaeoceanographic, palaeoclimatic and eustatic events.  相似文献   

Impact structures and events - a Nordic perspective     

Henning Dypvik Jueri Plado Claus Heinberg Eckart Hakansson Lauri J. Pesonen Birger Schmitz Selen Raiskila 《《幕》》2008,31(1):107-114

Impact cratering is one of the fundamental processes in the formation of the Earth and our planetary system, as reflected, for example in the surfaces of Mars and the Moon. The Earth has been covered by a comparable number of impact scars, but due to active geological processes, weathering, sea floor spreading etc, the number of preserved and recognized impact craters on the Earth are limited. The study of impact structures is consequently of great importance in our understanding of the formation of the Earth and the planets, and one way we directly, on the Earth, can study planetary geology.
The Nordic-Baltic area have about thirty confirmed impact structures which makes it one of the most densely crater-populated terrains on Earth. The high density of identified craters is due to the level of research activity, coupled with a deterministic view of what we look for. In spite of these results, many Nordic structures are poorly understood due to the lack of 3D-geophysical interpretations, isotopeor other dating efforts and better knowledge of the amount of erosion and subsequent tectonic modifications.
The Nordic and Baltic impact community is closely collaborating in several impact-related projects and the many researchers （about forty） and PhD students （some seventeen） promise that this level will continue for many more years. The main topics of research include geological, geophysical and geochemical studies in combination with modeling and impact experiments. Moreover, the Nordic and Baltic crust contains some hundred suspect structures which call for detailed analysis to define their origin.
New advanced methods of analyzing geophysical information in combination with detailed geochemical analyses and numerical modeling will be the future basic occupation of the impact scientists of the region. The unique Cretaceous/Tertiary boundary （K-T） occurrences in Denmark form an important source of information in explaining one of the major mass extinctions on Earth.  相似文献   

Erweiterte Grundgleichungen zur Bestimmung der Verdunstung auf dem Meer aus dem klein- und großräumigen Feuchteaustausch     

H. P. Schmitz 《Ocean Dynamics》1963,16(3):105-136

Zusammenfassung Es wird eine anwendbare Verallgemeinerung der Konzeptionen angestrebt, nachdenen man die Verdunstung auf dem Meere aus dem atmosphärischen Wasseraustausch bestimmt. Dabei ergeben sich einige Hinweise auf mehrere übliche aber kaum erkannte Vernachlässigungen. Unteranderem werden die Effekte der Druckänderungen sowie — durch Anwendung abgewogener Mittelwerte — die Wirkung des fluktuativen Massentransports in Rechnung gestellt. Jene werden meist in Makroturbulenzbetrachtungen, diese in Mikroturbulenzbetrachtungen zum Feuchteaustausch vernachlässigt, obgleich sie die Größenordnung der berechneten Verdunstungswerte erreichen und beispielsweise zur Erklärung der bei labiler Schichtung beobachteten deutlichen Verschiedenheit der gebräuchlichen Austauschkoeffizienten für Wasserdampf und Wärme beitragen können.

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Extended basic equations concerning the estimation of evaporation on the ocean from small- and large-scale exchange of moisture

Summary This paper aims at an applicable generalisation of the conceptions adapted to the estimation of evaporation on the ocean from theaustausch of water in the atmosphere. It gives some hints to several common but scarcely known neglects. Among others, the effects of the variation of pressure, and — by applying weighted means — those of the fluctuative transport of mass are taken into account. Usually the first effects are neglected in considerations on large-scale exchange of atmospheric water, the second ones in small-scale considerations although they may be of the same order of magnitude as the computed evaporation and may be able, for instance, to support an interpretation of the distinct inequalities of the usual eddy transfer coefficients of water vapour and heat observed in unstable lapse conditions.

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Equations fondamentales étendues pour dériver du flux micro- et macroturbulent de l'humidité l'évaporation à la surface de la mer

Résumé Le but de ce travail est de trouver une généralisation applicable des conceptions employées à dériver de l'échange atmosphérique de l'eau l'évaporation à la surface de la mer. Au cours de ces recherches on rencontre plusieurs indications de diverses négligences en usage qui, cependant, ne sont guère reconnues. Entre autre, on tient compte des effets dus aux variations de la pression atmosphérique et — en appliquant des moyennes pondérées — on considère également l'action du transport fluctuatif de la masse. Conventionnellement, le premier effet est négligé dans des considérations à base macroturbulente pendant que le deuxième effet est laissé de côté en cas de la diffusion microturbulente, bien que ces deux effets puissent atteindre la même ordre de grandeur que l'évaporation calculée et qu'ils puissent, par exemple, aider à expliquer les diversités distinctes des coefficients d'échange de l'humidité et de la chaleur observées quand la répartition des masses suivant la verticale est instable.

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Für Anregungen und die Möglichkeit zur Bearbeitung der diskutierten Fragen ist der Verfasser Herrn Professor Dr. Hermann Flohn zu Dank verpflichtet.  相似文献