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H. U. Roll  Fr. Model  K. Kalle 《Ocean Dynamics》1955,8(1):42-46

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Hydrographische Bibliographie     

Fr. Model 《Ocean Dynamics》1961,14(2):68-80

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Properties of dusty tori in active galactic nuclei – II. Type 2 AGN     

E. Hatziminaoglou  J. Fritz  T. H. Jarrett 《Monthly notices of the Royal Astronomical Society》2009,399(3):1206-1222

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Erosion-driven uplift of the modern Central Alps   总被引：2，自引：0，他引：2  

Jean-Daniel Champagnac  Fritz Schlunegger  Kevin Norton  Friedhelm von Blanckenburg  Luca M. Abbühl  Marco Schwab 《Tectonophysics》2009,474(1-2):236

We present a compilation of data of modern tectono-geomorphic processes in the Central European Alps which suggest that observed rock uplift is a response to climate-driven denudation. This interpretation is predominantly based on the recent quantification of basin-averaged Late Holocene denudation rates that are so similar to the pattern and rates of rock uplift rates as determined by geodetic leveling. Furthermore, a GPS data-based synthesis of Adriatic microplate kinematics suggests that the Central Alps are currently not in a state of active convergence. Finally, we illustrate that the Central Alps have acted as a closed system for Holocene redistribution of sediment in which the peri-Alpine lakes have operated as a sink for the erosional products of the inner Central Alps.While various hypotheses have been put forward to explain Central Alpine rock uplift (e.g. lithospheric forcing by convergence, mantle processes, or ice melting) we show with an elastic model of lithospheric deformation, that the correlation between erosion and rock uplift rates reflects a positive feedback between denudation and the associated isostatic response to unloading. Thus, erosion does not passively respond to advection of crustal material as might be the case in actively converging orogens. Rather, we suggest that the geomorphic response of the Alpine topography to glacial and fluvial erosion and the resulting disequilibrium for modern channelized and associated hillslope processes explains much of the pattern of modern denudation and hence rock uplift. Therefore, in a non-convergent orogen such as the Central European Alps, the observed vertical rock uplift is primarily a consequence of passive unloading due to erosion.  相似文献   

Biological and Physical Clogging in Infiltration Wells: Effects of Well Diameter and Gravel Pack     

Fritz Kalwa  Martin Binder  Falk Händel  Luzie Grüneberg  Rudolf Liedl 《Ground water》2021,59(6):819-828

Gravity-driven infiltration into the shallow subsurface via small-diameter wells (SDWs), i.e., wells with an inner diameter smaller than 7.5 cm (3 inches) and no gravel pack) has proven to be a cost-efficient and flexible tool for managed aquifer recharge (MAR), as it provides relatively high recharge rates with minimal construction effort. SDWs have a significantly smaller open filter area than larger diameter wells with gravel pack, making the infiltration of low-quality waters through these wells more at risk clogging. To investigate their susceptibility for biological and physical clogging, 24 physical models with different well setups were evaluated by infiltrating either nutrient-poor but turbid water or nutrient-rich but clear water. The experiments showed that smaller diameters and the lack of a gravel pack increase the well's susceptibility to both kinds of clogging. However, this effect was observed to be much more pronounced for physical than for biological clogging. Our conclusion is that SDWs show severe disadvantages with respect to the infiltration of highly turbid waters in comparison to large diameter wells with a gravel pack. Nevertheless, this disadvantage is much less severe when it comes to the infiltration of clear but nutrient-rich waters (e.g., treated wastewater). Depending on the economic and geological circumstances of a MAR-project, this disadvantage could be outweighed by the significantly lower construction costs of SDWs.  相似文献   

Properties of dusty tori in active galactic nuclei – I. The case of SWIRE/SDSS quasars     

E. Hatziminaoglou  J. Fritz  A. Franceschini  A. Afonso-Luis  A. Hernán-Caballero  I. Pérez-Fournon  S. Serjeant  C. Lonsdale  S. Oliver  M. Rowan-Robinson  D. Shupe  H. E. Smith  J. Surace 《Monthly notices of the Royal Astronomical Society》2008,386(3):1252-1264

We derive the properties of dusty tori in active galactic nuclei from the comparison of observed spectral energy distributions (SEDs) of SDSS quasars and a precomputed grid of torus models. The observed SEDs comprise SDSS photometry, Two-Micron All-Sky Survey J , H and K data, whenever available, and mid-infrared (mid-IR) data from the Spitzer Wide-area InfraRed Extragalactic Survey. The adopted model is that of Fritz, Franceschini & Hatziminaoglou. The fit is performed by standard  χ²  -minimization; the model, however, can be a multicomponent comprising a stellar and a starburst component, whenever necessary. Models with low equatorial optical depth, τ_9.7, were allowed as well as 'traditional' models with  τ_9.7≥ 1.0  , corresponding to   A _V≥ 22  and the results were compared. Fits using high optical depth tori models only produced dust more compactly distributed than in the configuration where all τ_9.7 models were permitted. Tori with decreasing dust density with the distance from the centre were favoured while there was no clear preference for models with or without angular variation of the dust density. The computed outer radii of the tori are of some tens of parsecs large but can reach, in a few cases, a few hundreds of parsecs. The mass of dust, M _Dust, and IR luminosity, L _IR, integrated in the wavelength range between 1 and 1000 μm, do not show significant variations with redshift, once the observational biases are taken into account. Objects with 70-μm detections, representing 25 per cent of the sample, are studied separately and the starburst contribution (whenever present) to the IR luminosity can reach, in the most extreme but very few cases, 80 per cent.  相似文献   

Messungen der erdmagnetischen Vertikalintensität auf See auf mehrfach befahrenen Profilen zur Prüfung der mit einem geschleppten Rotationsgerät erreichbaren Meβgenauigkeit     

Fritz Errulat 《Ocean Dynamics》1950,3(3-4):249-255

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Der Chlorophyllgehalt im See und seine photosynthetische Valenz als geophysikalisches Problem     

Fritz Gessner 《Aquatic Sciences - Research Across Boundaries》1949,11(3-4):378-410

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Klimaänderung oder Beobachtungsfehler?     

Fritz Model 《Ocean Dynamics》1948,1(5-6):220-221

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POLAR spacecraft observations of helium ion angular anisotropy in the Earth’s radiation belts     

W. N. Spjeldvik  T. A. Fritz  J. Chen  R. B. Sheldon 《Annales Geophysicae》1999,17(6):723-733

New observations of energetic helium ion fluxes in the Earth’s radiation belts have been obtained with the CAMMICE/HIT instrument on the ISTP/GGS POLAR spacecraft during the extended geomagnetically low activity period April through October 1996. POLAR executes a high inclination trajectory that crosses over both polar cap regions and passes over the geomagnetic equator in the heart of the radiation belts. The latter attribute makes possible direct observations of nearly the full equatorial helium ion pitch angle distributions in the heart of the Earth’s radiation belt region. Additionally, the spacecraft often re-encounters the same geomagnetic flux tube at a substantially off-equatorial location within a few tens of minutes prior to or after the equatorial crossing. This makes both the equatorial pitch angle distribution and an expanded view of the local off-equatorial pitch angle distribution observable. The orbit of POLAR also permitted observations to be made in conjugate magnetic local time sectors over the course of the same day, and this afforded direct comparison of observations on diametrically opposite locations in the Earth’s radiation belt region at closely spaced times. Results from four helium ion data channels covering ion kinetic energies from 520 to 8200 KeV show that the distributions display trapped particle characteristics with angular flux peaks for equatorially mirroring particles as one might reasonably expect. However, the helium ion pitch angle distributions generally flattened out for equatorial pitch angles below about 45°. Significant and systematic helium ion anisotropy difference at conjugate magnetic local time were also observed, and we report quiet time azimuthal variations of the anisotropy index.  相似文献