ALBERT

All Library Books, journals and Electronic Records Telegrafenberg

feed icon rss

Your email was sent successfully. Check your inbox.

An error occurred while sending the email. Please try again.

Proceed reservation?

Export
Filter
  • Other Sources  (24)
  • 1
    Publication Date: 2023-01-15
    Description: The dynamics of the Alps and surrounding regions is still not completely understood, partly because of a non‐unique interpretation of its upper‐mantle architecture. In particular, it is unclear if interpreted slabs are consistent with the observed surface deformation and topography. We derive three end‐member scenarios of lithospheric thickness and slab geometries by clustering available shear‐wave tomography models into a statistical ensemble. We use these scenarios as input for geodynamic simulations and compare modeled topography, surface velocities and mantle flow to observations. We found that a slab detached beneath the Alps, but attached beneath the Northern Apennines captures first‐order patterns in topography and vertical surface velocities and can provide a causative explanation for the observed seismicity.
    Description: Plain Language Summary: Present‐day surface deformation, including earthquakes, plate motion, and mass (re)distribution, results from processes operating at the surface and in the interior of the Earth. Understanding these processes and their coupling is of utmost importance in light of the hazard they pose to society. The Alps provide an excellent natural laboratory to understand such coupling. Here, we use seismic tomography models to constrain its upper‐mantle architecture. We further use these models to quantify forces originating from the resolved architecture and their effects on the present‐day surface deformation. The models can reproduce first‐order patterns in the observed topography and vertical surface motions. We found a causative correlation between the presence of a shallow slab attached to the overlying lithosphere in the Northern Apennines and the seismicity in the region. Our results allow us to better understand the transfer of internal forces to the surface, thereby helping to quantify the present‐day mechanical setup of the area.
    Description: Key Points: Statistical ensemble of S‐wave tomography models is used to infer the Lithosphere‐Asthenosphere Boundary configuration and slab geometries in the Alps. The 3‐D upper‐mantle architecture from the statistics reproduce first‐order patterns in observed topography and Global Navigation Satellite Systems vertical velocities. A shallow/attached slab in the Northern Apennines is consistent with the mantle depth seismicity observed in this region.
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: https://doi.org/10.5880/GFZ.4.5.2019.004
    Description: https://gfzpublic.gfz-potsdam.de/pubman/item/item_238001
    Description: http://ds.iris.edu/ds/products/emc-earthmodels/
    Description: https://doi.org/10.5281/zenodo.7071571
    Description: https://doi.org/10.5281/zenodo.6538257
    Keywords: ddc:551.1 ; Alps ; Apennines ; lithospheric architecture ; slabs ; seismicity
    Language: English
    Type: doc-type:article
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 2
    Publication Date: 2024-04-25
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉In this contribution we report the first systematic study of zircon U‐Pb geochronology and δ〈sup〉18〈/sup〉O‐〈italic〉ε〈/italic〉Hf〈sub〉(〈italic〉t〈/italic〉)〈/sub〉 isotope geochemistry from 10 islands of the hot‐spot related Galapagos Archipelago. The data extracted from the zircons allow them to be grouped into three types: (a) young zircons (0–∼4 Ma) with 〈italic〉ε〈/italic〉Hf〈sub〉(〈italic〉t〈/italic〉)〈/sub〉 (∼5–13) and δ〈sup〉18〈/sup〉O (∼4–7) isotopic mantle signature with crystallization ages dating the islands, (b) zircons with 〈italic〉ε〈/italic〉Hf〈sub〉(〈italic〉t〈/italic〉)〈/sub〉 (∼5–13) and δ〈sup〉18〈/sup〉O (∼5–7) isotopic mantle signature (∼4–164 Ma) which are interpreted to date the time of plume activity below the islands (∼164 Ma is the minimum time of impingement of the plume below the lithosphere), and (c) very old zircons (∼213–3,000 Ma) with mostly continental (but also juvenile) 〈italic〉ε〈/italic〉Hf〈sub〉(〈italic〉t〈/italic〉)〈/sub〉 (∼−28–8) and δ〈sup〉18〈/sup〉O (∼5–11) isotopic values documenting potential contamination from a number of sources. The first two types with similar isotopic mantle signature define what we call the Galápagos Plume Array (GPA). Given lithospheric plate motion, this result implies that GPA zircon predating the Galápagos lithosphere (i.e., >14–164 Ma) formed and were stored at sublithospheric depths for extended periods of time. In order to explain these observations, we performed 2D and 3D thermo‐mechanical numerical experiments of plume‐lithosphere interaction which show that dynamic plume activity gives rise to complex asthenospheric flow patterns and results in distinct long‐lasting mantle domains beneath a moving lithosphere. This demonstrates that it is physically plausible that old plume‐derived zircons survive at asthenospheric depths below ocean islands.〈/p〉
    Description: Key Points: 〈list list-type="bullet"〉 〈list-item〉 〈p xml:lang="en"〉Our data define the Galápagos Plume Array defined by mantle 〈italic〉ε〈/italic〉Hf〈sub〉(〈italic〉t〈/italic〉)〈/sub〉 and δ18O values in the range ∼0–164 Ma〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉This finding allows dating back plume activity to, at least, early Middle Jurassic (∼164 Ma)〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉Numerical experiments confirm it is plausible that old Plume‐derived zircons survive in the asthenosphere for extended periods of time〈/p〉〈/list-item〉 〈/list〉 〈/p〉
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: Ministerio de Asuntos Económicos y Transformación Digital, Gobierno de España http://dx.doi.org/10.13039/501100010198
    Description: Ministerio de Ciencia e Innovación http://dx.doi.org/10.13039/501100004837
    Description: European Research Council http://dx.doi.org/10.13039/501100000781
    Description: https://doi.org/10.5281/zenodo.7047729
    Description: https://doi.org/10.5281/zenodo.6967187
    Keywords: ddc:551.9 ; mantle plume ; galapagos zircon ages ; asthenospheric zircon ; oceanic islands ; thermo‐mechanical numerical experiments
    Language: English
    Type: doc-type:article
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 3
    facet.materialart.
    Unknown
    In:  Geophys. Res. Lett., Amsterdam, Univ. Tokyo, vol. 33, no. 14, pp. 16,341-16,358, pp. L14309, (ISSN: 1340-4202)
    Publication Date: 2006
    Keywords: Three dimensional ; Finite Element Method ; Modelling ; Stress ; Crustal deformation (cf. Earthquake precursor: deformation or strain) ; Tectonics ; GRL ; 3215 ; Mathematical ; Geophysics: ; Instability ; analysis ; 8005 ; Structural ; Geology: ; Folds ; and ; folding ; 8020 ; Mechanics, ; theory ; and ; modeling ; 8109 ; Tectonophysics: ; Continental ; tectonics: ; extensional ; (0905)
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 4
    facet.materialart.
    Unknown
    In:  J. Geophys. Res., Amsterdam, Univ. Tokyo, vol. 111, no. B4, pp. 16,341-16,358, pp. B04412, (ISSN: 1340-4202)
    Publication Date: 2006
    Keywords: Rheology ; Fracture ; Modelling ; Rock mechanics ; Inelastic ; JGR ; shear ; localization ; numerical ; mathematical ; modeling ; 8118 ; Tectonophysics: ; Dynamics ; and ; mechanics ; of ; faulting ; (8004) ; 8120 ; Dynamics ; of ; lithosphere ; and ; mantle: ; general ; (1213) ; 8149 ; Planetary ; tectonics ; (5475) ; 8164 ; Stresses: ; crust ; and ; lithosphere ; 8163 ; Rheology ; and ; friction ; of ; fault ; zones ; (8034)
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 5
    facet.materialart.
    Unknown
    In:  Nature, Luxembourg, Conseil de l'Europe, vol. 427, no. 6976, pp. 724-727, pp. 2182, (ISSN: 1340-4202)
    Publication Date: 2004
    Keywords: Aftershocks ; Fluids ; Stress ; triggering ; SPAROLAI ; noksp
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 6
    Publication Date: 2011-08-19
    Description: Emerging magnetic flux plays an important role in the development of active regions on the sun and, perhaps, in the subsequent activation of flares. However, the energy input that produces preflare brightenings and flares probably does not come from the flux emergence itself but from one or more associated energy-releasing processes - likely candidates include magnetic reconnection and various current-driven plasma micro-instabilities. Here the interplay between the changing physical characteristics of an emerging magnetic-flux tube and the onset and evolution of a representative 'bump-on-tail' plasma current-driven instability is investigated. The microinstability heats the ambient material, thus changing the macroscopic characteristics of the plasma in which the model and current-driven instability occurs.
    Keywords: SOLAR PHYSICS
    Type: Astrophysical Journal, Part 1 (ISSN 0004-637X); 307; 826-837
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 7
    Publication Date: 2011-08-19
    Description: In virtue of adding one elliptic equation that must be implicitly solved, the 'barely implicit correction' method presented removes the stringent sidestep limit imposed by sound speed in the explicit methods. The barely implicit method is presently combined with a flux-corrected transport algorithm, which has been rendered fourth-order by the appropriate subtraction of corrected fluxes, in order to accurately represent the sharp gradients in subsonic flows. The multigrid MGRID technique (DeVore, 1984) is used to efficiently solve the elliptic pressure equation.
    Keywords: FLUID MECHANICS AND HEAT TRANSFER
    Type: Journal of Computational Physics (ISSN 0021-9991); 71; 1-20
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 8
    Publication Date: 2011-08-19
    Description: According to the approach employed in this investigation, particularly important simple configurations of magnetic field and plasma are identified, and it is attempted to achieve an understanding of the large-scale dynamic processes and transformations which these systems can undergo. Fundamental concepts are discussed, taking into account aspects of magnetic energy generation, ideal MHD theory, non-MHD properties, the concept of 'anomalous' resistivity, and global electrodynamic coupling. Questions of magnetically controlled energy conversion are examined, giving attention to magnetic modifications of plasma transport, the transition region structure and flows, channeling and acceleration of plasma, channeling and dissipation of MHD waves, and anomalous dissipation of field-aligned currents. A description of the characteristics of magnetohydrodynamic energy conversion is also provided, and outstanding questions are discussed.
    Keywords: SOLAR PHYSICS
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 9
    Publication Date: 2011-08-19
    Description: Coronal bullets are small ejecta of cool, dense plasma observed to accelerate through the solar atmosphere from 20 to 450 km/s. The NRL Dynamic Flux Tube Model has been used to simulate the evolving physical properties of these dynamic events. The present calculations utilize an adaptive-gridding technique to resolve the fine structure within and around the bullets. In this work, an identification was made of a component of shocked plasma which piles up ahead of the bullet and eventually dominates both the dynamics and heating of the original bullet mass. The observational consequences of this shocked component are discussed in terms of the available HRTS EUV data, and suggestions are made for optimizing future observations of this phenomenon. An investigation has also been conducted of the structure of the bullet material visible in EUV spectral lines and the observable characteristics of the EUV-emitting plasma. Finally, the most likely mechanisms for accelerating the bullets, as well as favorable sites of origin are evaluated.
    Keywords: SOLAR PHYSICS
    Type: Astrophysical Journal, Part 1 (ISSN 0004-637X); 287; 396-403
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 10
    facet.materialart.
    Unknown
    In:  Other Sources
    Publication Date: 2011-08-18
    Description: The study of stellar atmospheres and the determination of specific physical mechanisms, geometries, and magnetic structures by which coronae are maintained is examined. Ultraviolet and soft X-ray components observed in the radiative output of cool stars and the Sun require counterentropic temperature gradients for their explanation. The existence of a hot corona is recognized as a result of mechanical or fluid dynamic effects and the importance of the magnetic field in the heating is accepted. Magnetohydrodynamic energy release associated with the emergence of magnetic flux through the chromosphere and its dynamic readjustment in the corona are major counterentropic phenomena which are considered as primary candidates for corona heating. Systematic plows in coronal flux tubes result from asymmetric heating and systematic flows can exist without substantial chromospheric pressure differences.
    Keywords: SOLAR PHYSICS
    Type: Smithsonian Astrophysics Observatory 2nd Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, Vol. 1; p 53-58
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
Close ⊗
This website uses cookies and the analysis tool Matomo. More information can be found here...