The Erbisberg drilling 2011: Implications for the structure and postimpact evolution of the inner ring of the Ries impact crater     

Gernot Arp  Andreas Reimer  Klaus Simon  Sebastian Sturm  Jakob Wilk  Corina Kruppa  Lutz Hecht  Bent T. Hansen  Jean Pohl  Wolf Uwe Reimold  Thomas Kenkmann  Dietmar Jung 《Meteoritics & planetary science》2019,54(10):2448-2482

The 26 km diameter Nördlinger Ries is a complex impact structure with a ring structure that resembles a peak ring. A first research drilling through this “inner crystalline ring” of the Ries was performed at the Erbisberg hill (SW Ries) to better understand the internal structure and lithology of this feature, and possibly reveal impact‐induced hydrothermal alteration. The drill core intersected the slope of a 22 m thick postimpact travertine mound, before entering 42 m of blocks and breccias of crystalline rocks excavated from the Variscan basement at >500 m depth. Weakly shocked gneiss blocks that show that shock pressure did not exceed 5 GPa occur above polymict lithic breccias of shock stage Ia (10–20 GPa), with planar fractures and planar deformation features (PDFs) in quartz. Only a narrow zone at 49.20–50.00 m core depth exhibits strong mosaicism in feldspar and {102} PDFs in quartz, which are indicative of shock stage Ib (20–35 GPa). Finally, 2 m of brecciated Keuper sediments at the base of the section point to an inverse layering of strata. While reverse grading of clast sizes in lithic breccias and gneiss blocks is consistent with lateral transport, the absence of diaplectic glass and melt products argues against dynamic overthrusting of material from a collapsing central peak, as seen in the much larger Chicxulub structure. Indeed, weakly shocked gneiss blocks are rather of local provenance (i.e., the transient crater wall), whereas moderately shocked polymict lithic breccias with geochemical composition and ⁸⁷Sr/⁸⁶Sr signature similar to Ries suevite were derived from a position closer to the impact center. Thus, the inner ring of the Ries is formed by moderately shocked polymict lithic breccias likely injected into the transient crater wall during the excavation stage and weakly shocked gneiss blocks of the collapsing transient crater wall that were emplaced during the modification stage. While the presence of an overturned flap is not evident from the Erbisberg drilling, a survey of all drillings at or near the inner ring point to inverted strata throughout its outer limb. Whether the central ring of the Ries represents remains of a collapsed central peak remains to be shown. Postimpact hydrothermal alteration along the Erbisberg section comprises chloritization, sulfide veinlets, and strong carbonatization. In addition, a narrow zone in the lower parts of the polymict lithic breccia sequence shows a positive Eu anomaly in its carbonate phase. The surface expression of this hydrothermal activity, i.e., the travertine mound, comprises subaerial as well as subaquatic growth phases. Intercalated lake sediments equivalent to the early parts of the evolution of the central crater basin succession confirm a persistent impact‐generated hydrothermal activity, although for less time than previously suggested.  相似文献   

Multicriteria assessment of water dynamics reveals subcatchment variability in a seemingly homogeneous tropical cloud forest catchment          下载免费PDF全文

Edison Timbe  Jan Feyen  Luis Timbe  Patricio Crespo  Rolando Célleri  David Windhorst  Hans‐Georg Frede  Lutz Breuer 《水文研究》2017,31(7):1456-1468

  相似文献   

Continuous versus event‐based sampling: how many samples are required for deriving general hydrological understanding on Ecuador's páramo region?          下载免费PDF全文

Alicia Correa  David Windhorst  Patricio Crespo  Rolando Célleri  Jan Feyen  Lutz Breuer 《水文研究》2016,30(22):4059-4073

As a consequence of the remote location of the Andean páramo, knowledge on their hydrologic functioning is limited; notwithstanding, these alpine tundra ecosystems act as water towers for a large fraction of the society. Given the harsh environmental conditions in this region, year‐round monitoring is cumbersome, and it would be beneficial if the monitoring needed for the understanding of the rainfall–runoff response could be limited in time. To identify the hydrological response and the effect of temporal monitoring, a nested (n = 7) hydrological monitoring network was set up in the Zhurucay catchment (7.53 km²), south Ecuador. The research questions were as follows: (1) Can event sampling provide similar information in comparison with continuous monitoring, and (2) if so, how many events are needed to achieve a similar degree of information? A subset of 34 rainfall–runoff events was compared with monthly values derived from a continuous monitoring scheme from December 2010 to November 2013. Land cover and physiographic characteristics were correlated with 11 hydrological indices. Results show that despite some distinct differences between event and continuous sampling, both data sets reveal similar information; more in particular, the monitoring of a single event in the rainy season provides the same information as continuous monitoring, while during the dry season, ten events ought to be monitored. Copyright © 2016 John Wiley & Sons, Ltd.  相似文献   

Preliminary evaluation of the runoff processes in a remote montane cloud forest basin using Mixing Model Analysis and Mean Transit Time     

Patricio Crespo  Amelie Bücker  Jan Feyen  Kellie B. Vaché  Hans‐Georg Frede  Lutz Breuer 《水文研究》2012,26(25):3896-3910

In this study, the Mean Transit Time and Mixing Model Analysis methods are combined to unravel the runoff generation process of the San Francisco River basin (73.5 km²) situated on the Amazonian side of the Cordillera Real in the southernmost Andes of Ecuador. The montane basin is covered with cloud forest, sub‐páramo, pasture and ferns. Nested sampling was applied for the collection of streamwater samples and discharge measurements in the main tributaries and outlet of the basin, and for the collection of soil and rock water samples. Weekly to biweekly water grab samples were taken at all stations in the period April 2007–November 2008. Hydrometric data, Mean Transit Time and Mixing Model Analysis allowed preliminary evaluation of the processes controlling the runoff in the San Francisco River basin. Results suggest that flow during dry conditions mainly consists of lateral flow through the C‐horizon and cracks in the top weathered bedrock layer, and that all subcatchments have an important contribution of this deep water to runoff, no matter whether pristine or deforested. During normal to low precipitation intensities, when antecedent soil moisture conditions favour water infiltration, vertical flow paths to deeper soil horizons with subsequent lateral subsurface flow contribute most to streamflow. Under wet conditions in forested catchments, streamflow is controlled by near surface lateral flow through the organic horizon. Exceptionally, saturation excess overland flow occurs. By absence of the litter layer in pasture, streamflow under wet conditions originates from the A horizon, and overland flow. Copyright © 2011 John Wiley & Sons, Ltd.  相似文献   

CODE’s new solar radiation pressure model for GNSS orbit determination   总被引：10，自引：8，他引：2  

D. Arnold  M. Meindl  G. Beutler  R. Dach  S. Schaer  S. Lutz  L. Prange  K. Sośnica  L. Mervart  A. Jäggi 《Journal of Geodesy》2015,89(8):775-791

  相似文献   

STAGES: the Space Telescope A901/2 Galaxy Evolution Survey     

Meghan E. Gray  Christian Wolf  Marco Barden  Chien Y. Peng  Boris Häußler  Eric F. Bell  Daniel H. McIntosh  Yicheng Guo  John A. R. Caldwell  David Bacon  Michael Balogh  Fabio D. Barazza  Asmus Böhm  Catherine Heymans  Knud Jahnke  Shardha Jogee  Eelco van Kampen  Kyle Lane  Klaus Meisenheimer  Sebastian F. Sánchez  y Taylor  Lutz Wisotzki  Xianzhong Zheng  David A. Green  R. J. Beswick  D. J. Saikia  Rachel Gilmour  Benjamin D. Johnson  Casey Papovich 《Monthly notices of the Royal Astronomical Society》2009,393(4):1275-1301

We present an overview of the Space Telescope A901/2 Galaxy Evolution Survey (STAGES). STAGES is a multiwavelength project designed to probe physical drivers of galaxy evolution across a wide range of environments and luminosity. A complex multicluster system at   z ∼ 0.165  has been the subject of an 80-orbit F606W Hubble Space Telescope (HST) /Advanced Camera for Surveys (ACS) mosaic covering the full     span of the supercluster. Extensive multiwavelength observations with XMM–Newton , GALEX, Spitzer , 2dF, Giant Metrewave Radio Telescope and the 17-band COMBO-17 photometric redshift survey complement the HST imaging. Our survey goals include simultaneously linking galaxy morphology with other observables such as age, star formation rate, nuclear activity and stellar mass. In addition, with the multiwavelength data set and new high-resolution mass maps from gravitational lensing, we are able to disentangle the large-scale structure of the system. By examining all aspects of an environment we will be able to evaluate the relative importance of the dark matter haloes, the local galaxy density and the hot X-ray gas in driving galaxy transformation. This paper describes the HST imaging, data reduction and creation of a master catalogue. We perform the Sérsic fitting on the HST images and conduct associated simulations to quantify completeness. In addition, we present the COMBO-17 photometric redshift catalogue and estimates of stellar masses and star formation rates for this field. We define galaxy and cluster sample selection criteria, which will be the basis for forthcoming science analyses, and present a compilation of notable objects in the field. Finally, we describe the further multiwavelength observations and announce public access to the data and catalogues.  相似文献   

Identifying Controls on Water Chemistry of Tropical Cloud Forest Catchments: Combining Descriptive Approaches and Multivariate Analysis     

Amelie Bücker  Patricio Crespo  Hans-Georg Frede  Kellie Vaché  Felipe Cisneros  Lutz Breuer 《Aquatic Geochemistry》2010,16(1):127-149

We investigated controls on the water chemistry of a South Ecuadorian cloud forest catchment which is partly pristine, and partly converted to extensive pasture. From April 2007 to May 2008 water samples were taken weekly to biweekly at nine different subcatchments, and were screened for differences in electric conductivity, pH, anion, as well as element composition. A principal component analysis was conducted to reduce dimensionality of the data set and define major factors explaining variation in the data. Three main factors were isolated by a subset of 10 elements (Ca²⁺, Ce, Gd, K⁺, Mg²⁺, Na⁺, Nd, Rb, Sr, Y), explaining around 90% of the data variation. Land-use was the major factor controlling and changing water chemistry of the subcatchments. A second factor was associated with the concentration of rare earth elements in water, presumably highlighting other anthropogenic influences such as gravel excavation or road construction. Around 12% of the variation was explained by the third component, which was defined by the occurrence of Rb and K and represents the influence of vegetation dynamics on element accumulation and wash-out. Comparison of base- and fast flow concentrations led to the assumption that a significant portion of soil water from around 30 cm depth contributes to storm flow, as revealed by increased rare earth element concentrations in fast flow samples. Our findings demonstrate the utility of multi-tracer principal component analysis to study tropical headwater streams, and emphasize the need for effective land management in cloud forest catchments.  相似文献   

ISO Spectroscopy of Ultraluminous Infrared Galaxies     

D. Lutz  R. Genzel  D. Kunze  D. Rigopoulou  H.W.W. Spoon  E. Sturm  D. Tran  A.F.M. Moorwood 《Astrophysics and Space Science》1999,266(1-2):85-90

Spectroscopy from the Infrared Space Observatory ISO has for the first timeprovided the sensitivity to exploit the diagnostic power ofmid-infrared fine structure lines and PAH features for the study ofultraluminous infrared galaxies (L_IR >10¹² L ). We report on observations obtainedwith SWS, ISOPHOT-S, and the CVF option of ISOCAM. From both fine structure lines and PAH features, we find that the majority of ULIRGs is predominantlypowered by star formation. Our total sample of about 75 ULIRGs allows tosearch for trends within the class of ULIRGs: The fraction of AGNs increaseswith luminosity above 3 × 10¹²L but there is no obvioustrend for ULIRGs to be more AGN-like with more advanced merger phase.  相似文献   

Der Brechungsindexgradient für elektromagnetische Wellen (Cm-bis M-Band) in der maritimen Grenzschicht der Atmosphäre     

Karl Brocks  Lutz Hasse 《Ocean Dynamics》1956,9(5):217-221

Zusammenfassung Für ein in der Abhandlung von K. Brocks [1955] abgeleitetes Verfahren der Berechnung von Brechungsindex-Profilen unmittelbar über dem Meer werden weitere Hilfsmittel angegeben, insbesondere eine graphische Psychrometertafel (Tafel 8), aus der der Dampfdruck der Luft [in mb] als Funktion der Temperatur des feuchten und trockenen Thermometers entnommen werden kann, und ein Diagramm des Wasserdampfdrucks und des Sättigungsdampfdruckes der Luft sowie der relativen Luftfeuchtigkeit als Funktion der Lufttemperatur (Tafel 9).Es wird ferner ein Kurzverfahren mitgeteilt, das eine schnelle Berechnung des Brechungsindexprofils über dem Meer ermöglicht aus Messungen der Lufttemperatur, Luftfeuchtigkeit, Windgeschwindigkeit und Wassertemperatur. Hierfür wird ein Diagramm gegeben (Tafel 10), das den BrechungswertN=(n–1) 10^–6 als Funktion der Temperatur des trockenen und des feuchten Thermometers bzw. der Wassertemperatur enthält.

---

On the gradient of the refractive index of electro-magnetic waves (centimetre-to metre-waves) in the maritime boundary layer of the atmosphere. 2^nd article

Summary The present paper adds further aids to the method developed by K. Brocks [1955] for the computation of the curves of the refractive index occurring immediately above the sea surface. These aids, before all, consist in a graphical psychrometer plate (plate 8) and a diagramme (plate 9). Plate 8 permits to derive from it the vapour pressure of the air [in mb] as a function of temperature to be read from dry bulb and a wet bulb thermometres. Plate 9 represents the water vapour pressure and the saturation pressure of the air as well as relative humidity of the air as a function of air temperature.Besides, an abbreviated method is discussed permitting a time-saving computation of the curves of the refractive index above sea surface from measurements of air temperature, atmospheric moisture, wind velocity, and water temperature. This computation is carried out with the aid of a diagram (plate 10), giving the refractive valueN=(n–1) 10^–6 as a function of the temperature, measured with a dry bulb and a wet bulb thermometre, or as a function of the water temperature, respectively.

---

Sur le gradient de l'indice de réfraction des ondes électromagnétiques (de 0,1 m à 1m), présentes dans la couche limite maritime de l'atmosphère. 2^e article

Résumé Le travail actuel ajoute à la méthode développée par K. Brocks [1955] d'autres moyens pour le calcul des courbures du gradient de l'indice de réfraction se présentant immédiatement au-dessus de la surface de la mer. Ces moyens se composent surtout d'une représentation graphique des valeurs psychométriques (planche 8) et d'un diagramme (planche 9). La planche 8 permet d'en tirer la pression de vapeur de l'air [en mb] en fonction de températures indiquées sur de thermomètres mouillés ou sur de thermomètres secs. La planche 9 montre la pression de vapeur d'eau et la tension de vapeur saturante de l'air ainsi que l'humidité relative de l'air en fonction de la température de l'air.De plus, une méthode abbréviée est présentée qui permet de calculer, sans perdre beaucoup de temps, au moyen des mesures de la température de l'air et de l'eau, de l'humidité de l'air et de la vitesse du vent, la courbure de l'indice de réfraction au-dessus de la mer. Ce calcul se fait à l'aide d'un diagramme (planche 10) qui donne la valeur de réfractionN=(n}-1) 10^–6 en fonction de la température du thermomètre sec et du thermomètre mouillé ou la représente respectivement en fonction de la température de l'eau.

  相似文献   

Hydrogen bonding in basic copper salts: a spectroscopic study of malachite,Cu2(OH)2CO3, and brochantite,Cu4(OH)6SO4     

M. Schmidt  H. D. Lutz 《Physics and Chemistry of Minerals》1993,20(1):27-32

Infrared and Raman spectra of the basic copper salts malachite, Cu₂(OH)₂CO₃, and brochantite, Cu₄(OH)₆SO₄, as well as of deuterated and ¹³C substituted samples are presented and discussed in terms of group theory and the hydrogen bonds present. The main results are that (i) the hydrogen donor strengths of the OH^? ions are strongly increased due to the very great synergetic effect of the copper ions, (ii) the acceptor strengths of the H-bond acceptor groups (SO₄ ^2-, CO₃ ^2-, and OH^? ions) are significantly modified by the linkage and coordination of the acceptor atoms — this complicates true assignment of the OH bands observed to the two and six different OH^? ions present in malachite and brochantite, respectively -, and (iii) the Cu — O stretching modes at 430–590 cm^?1 and 420–520 cm^?1 for malachite and brochantite, respectively, exhibit strong, partially covalent Cu — O bonding.  相似文献