A multiphysics and multiscale software environment for modeling astrophysical systems     

Simon Portegies Zwart  Steve McMillan  Stefan Harfst  Derek Groen  Michiko Fujii  Breanndán Ó Nualláin  Evert Glebbeek  Douglas Heggie  James Lombardi  Piet Hut  Vangelis Angelou  Sambaran Banerjee  Houria Belkus  Tassos Fragos  John Fregeau  Evghenii Gaburov  Rob Izzard  Mario Jurić  Stephen Justham  Andrea Sottoriva  Marcel Zemp 《New Astronomy》2009,14(4):369-378

We present MUSE, a software framework for combining existing computational tools for different astrophysical domains into a single multiphysics, multiscale application. MUSE facilitates the coupling of existing codes written in different languages by providing inter-language tools and by specifying an interface between each module and the framework that represents a balance between generality and computational efficiency. This approach allows scientists to use combinations of codes to solve highly coupled problems without the need to write new codes for other domains or significantly alter their existing codes. MUSE currently incorporates the domains of stellar dynamics, stellar evolution and stellar hydrodynamics for studying generalized stellar systems. We have now reached a “Noah’s Ark” milestone, with (at least) two available numerical solvers for each domain. MUSE can treat multiscale and multiphysics systems in which the time- and size-scales are well separated, like simulating the evolution of planetary systems, small stellar associations, dense stellar clusters, galaxies and galactic nuclei. In this paper we describe three examples calculated using MUSE: the merger of two galaxies, the merger of two evolving stars, and a hybrid N-body simulation. In addition, we demonstrate an implementation of MUSE on a distributed computer which may also include special-purpose hardware, such as GRAPEs or GPUs, to accelerate computations. The current MUSE code base is publicly available as open source at http://muse.li.  相似文献   

Fluidization of buried mass-wasting deposits in lake sediments and its relevance for paleoseismology: Results from a reflection seismic study of lakes Villarrica and Calafquén (South-Central Chile)     

Jasper Moernaut  Marc De Batist  Katrien Heirman  Maarten Van Daele  Mario Pino  Robert Brümmer  Roberto Urrutia 《Sedimentary Geology》2009,213(3-4):121-135

A dense grid of very-high resolution seismic profiles on Lake Villarrica provides a quasi-3D view on intercalated lenses of low-amplitude reflections, which are connected by acoustic wipe-out patches and fractures to an underlying voluminous mass-wasting deposit. The lenses are interpreted as being created by earthquake-triggered liquefaction in this buried mass-wasting deposit and subsequent sediment fluidization and extrusion at the paleo-lake bottom. These sediment volcanoes are mapped in detail. They have a rather uniform circular geometry and show a linear relationship between apparent width and maximum thickness on a seismic section. The largest sediment volcanoes are up to 80 m wide and 1.9 m thick. Their slope angles designate a syn- to post-depositional sagging of most sediment volcanoes. Sediment volcano detection and mapping from nearby Lake Calafquén further strengthen the revealed geometrical relationships. Locally, some of the sediment/fluid escape structures extend to a higher position in the stratigraphy, which points to a polyphase escape process associated with multiple multi-century spaced strong earthquakes. Thickness and morphology of the source layer seem to exert a dominant control in the production of sediment/fluid extrusions. This study shows that reflection seismic profiling allowed recognizing 4 different seismic events in the studied stratigraphic interval, which are evidenced by mass-wasting deposits and/or fluidization features.  相似文献   

Gravitation astrometric measurement experiment     

Mario Gai  Alberto Vecchiato  Sebastiano Ligori  Alessandro Sozzetti  Mario G. Lattanzi 《Experimental Astronomy》2012,34(2):165-180

The Gravitation Astrometric Measurement Experiment (GAME) is a mission concept based on astronomical techniques (astrometry and coronagraphy) for Fundamental Physics measurements, namely the ?? and ?? parameters of the Parametrized Post-Newtonian formulation of gravitation theories extending the General Relativity. The science case also addresses cosmology, extra-solar planets, Solar System objects and fundamental stellar parameters. The mission concept is described, including the measurement approach and the instrument design.  相似文献   

An exact solution to the relativistic advance of perihelion: correcting the Einstein approximation     

Jose Mario Saca 《Astrophysics and Space Science》2008,315(1-4):365-365

New calculations of the main term of the advance of perihelion for the asteroid Icarus and planet Mercury are discussed. With the help of this author’s previously published formula for the advance, results are then compared to the values given by Einstein’s approximation.  相似文献   

Mechanism of generation of the emission bands in the dynamic spectrum of the Crab pulsar     

Houshang Ardavan  ArzhangArdavan  John Singleton  Mario R. Perez 《Monthly notices of the Royal Astronomical Society》2008,388(2):873-883

We show that the proportionately spaced emission bands in the dynamic spectrum of the Crab pulsar fit the oscillations of the square of a Bessel function whose argument exceeds its order. This function has already been encountered in the analysis of the emission from a polarization current with a superluminal distribution pattern: a current whose distribution pattern rotates (with an angular frequency ω) and oscillates (with a frequency  Ω > ω  differing from an integral multiple of ω) at the same time. Using the results of our earlier analysis, we find that the dependence on frequency of the spacing and width of the observed emission bands can be quantitatively accounted for by an appropriate choice of the value of the single free parameter  Ω/ω  . In addition, the value of this parameter, thus implied by Hankins & Eilek's data, places the last peak in the amplitude of the oscillating Bessel function in question at a frequency  (∼Ω³/ω²)  that agrees with the position of the observed ultraviolet peak in the spectrum of the Crab pulsar. We also show how the suppression of the emission bands by the interference of the contributions from differing polarizations can account for the differences in the time and frequency signatures of the interpulse and the main pulse in the Crab pulsar. Finally, we put the emission bands in the context of the observed continuum spectrum of the Crab pulsar by fitting this broad-band spectrum (over 16 orders of magnitude of frequency) with that generated by an electric current with a superluminally rotating distribution pattern.  相似文献   

A digital earth platform for sustainability   总被引：1，自引：1，他引：0  

Mario Hernandez 《International Journal of Digital Earth》2017,10(4):342-355

ABSTRACT

Based on the experience of the International Society for Digital Earth (ISDE), this paper describes some challenges foreseen in order to develop a Digital Earth platform that can support the implementation of the Sustainable Development Goals. The use of ready-to-use derived geospatial information is essential. Future Earth’s methodology of ‘co-design’ aims to bring together natural, social scientists and decision makers to plan and carry out research for sustainability. Sustainability implies transdisciplinary research, but in order for scientists of different disciplines to work together, they will need to be able to share, access and use common data. This is by far not simple! While the good will to share data might exist, the associated technological, ethical and privacy issues are difficult to solve. An adequate e-infrastructure will be required. ISDE could consider to use the SDGs is the basis to develop the desired Digital Earth platform. This paper, by no means, covers everything for a Digital Earth platform, it aims to trigger research discussions and to have a good view about a starting point.  相似文献   

Sur les perturbations magnétiques à Mogadiscio     

Mario Bossolasco 《Pure and Applied Geophysics》1951,20(1):46-49

Summary The comparison of the geomagneticK-indices for Mogadiscio with the correspondingK _p for the whole earth, during the 2.nd Intern. Polar Year 1932–33, allows to deduce some features of the equatorial geomagnetic activity. Furthermore, evidence is adduced indicating that the geomagnetic disturbance at Mogadiscio is normal inH andD, while it appears slightly abnormal inZ.

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Communication presentée à l'Association Internationale de Magnétisme et Electricité Terrestres, IXe Assemblée Générale de l'UGGI, Bruxelles, Séance du 28 Août 1951.  相似文献   

Variazioni del moto polare della Terra e loro correlazioni meteorologiche     

Mario Bossolasco 《Pure and Applied Geophysics》1949,14(3-4):197-202

Riassunto Vengono documentate ed illustrate alcune correlazioni fra le alterazioni del moto di rotazione terrestre iniziatesi nel 1923 con gli eventi meteorologici; in particolare si discutono e si spiegano in tal modo le forti anomalie della pressione osservate a Genova nel periodo 1924–32.

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Zusammenfassung Störungen in der Bewegung des Erdkörpers und Verschiebungen seiner Rotaktionsachse rufen Wirkungen hervor, welcke mit der Anpassung der Luftmassen an den neuen Bewegungen und an den neuen Lagen der Rotaktionsachse sich ausdrucken. Das führt zu Veränderungen der Luftströmungen, der Luftdruckverteilungen und daher der Grossewetterlagen. Einige meteorologischen Korrelationen dieser Art werden für die bedeutende Störung der Polarbewegung des 1923 gezeigt. Nachher werden damit besonders die starken Luftdruckanomalien erklärt, welche in Genua in der Periode 1924–32 beobachtet worden sind.

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Sulle correnti telluriche nelle regioni equatoriali     

Mario Bossolasco 《Pure and Applied Geophysics》1947,10(1-2):41-53

Riassunto Si espongono i risultati delle osservazioni sulle correnti telluriche eseguite a Mogadiscio nel 1933 con misure delle due componenti NS ed EW, traendone alcune deduzioni che permettono di precisarne le caratteristiche, specie nei confronti del relativo andamento diurno.

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Summary The paper deals with the results of the earth-current-observations made at Mogadiscio during 1933. The analysis reveal elements for a new picture of the distribution of the earth-currents in the equatorial regions, particularly concerning the daily variation.

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Zusammenfassung Die Ergebnisse des Erdstrom-Beobachtungen durchgeführt in einigen Monaten des Jahres 1933 in Modagiscio sind angegeben. Aus des Diskussion folgen einige Elemente die eine Neubearbeitung des Darstellung des Erdstrom-Verteilung in dem äquatorialem Gürtel nötig machen und dazu dienen werden sollen. besonders in Beziehung auf den täglichen Gang.

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Sullo spostamento dei cicloni nel Mediterraneo     

Mario Bossolasco 《Pure and Applied Geophysics》1952,22(3-4):255-261

Riassunto Vengono esaminati due esempi di spostamento retrogrado di depressioni nel Mediterraneo, illustrandone le cause. Per uno di essi si calcolano gli elementi energetici, dimostrando come il rapportoK/P fra l'energia cinetica e quella potenziale della depressione costituisca un indice della sua capacità di proseguire il moto lungo la rotta precedente.

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Summary Two examples of retrograde displacement of depressions in the Mediterranean are being examined, explaining their causes. For one of them the energetic elements are calculated showing how the ratioK/P between the kinetic and the potential energy of the depression constitutes an index of its capacity to continue the motion along the preceding course.

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Zusammenfassung Es werden zwei Fälle rückläufiger Bewegungen, von Mittelmeerdepressionen untersucht und die Ursachen derselben erläutert. Für einen dieser Fälle werden die Grössen der Energie berechnet: und es wird gezeigt, dass das VerhältnisK/P zwischen kinetischer und potentieller Energie massgebend ist für die Fähigkeit der Depression, ihre Bewegung in der ursprünglichen Richtung fortzusetzen.

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