Precursory quiescence before the August 1982 Stone Canyon,San Andreas fault,earthquakes     

Max Wyss  R. E. Habermann 《Pure and Applied Geophysics》1988,126(2-4):333-356

The Stone Canyon earthquake sequence started during August 1982 and lasted for about four months. It contained four mainshocks withM _L 4, each with an aftershock zone about 4 km long. These mainshocks, progressing from southeast to northwest, ruptured a segment of the fault approximately 20 km long leaving two gaps, which were later filled by theM _L =4.6 mainshocks of January 14, and May 31, 1986. The equivalent magnitude of the sequence isM _L =5.0.Precursory seismic quiescence could be identified in: (1) the northernmost 10 km of the aftershock zone which contained three of the mainshocks; and (2) the southern gap in the aftershock zone. The fault segment containing the first mainshock and its aftershocks did not show quiescence. This pattern of precursory quiescence is very similar to two cases in Hawaii where the rupture initiation points of the mainshocks (M _S =7.2 and 6.6, respectively) were located in volumes of constant seismicity rate, surrounded by volumes with pronounced precursory quiescence.The precursory quiescence before the August 1982 Stone Canyon earthquakes lasted for 76 weeks, amounted to a reduction in rate of about 60%, and could be recognized without any false alarms. That is, the anomaly was unique within the 60 km study segment of the fault and in the years 1975 through August 1982. Eighteen foreshocks occurred between July 27 and August 7, 1982. We conclude that the August 1982 mainshocks could have been predicted, based on seismic quiescence and foreshocks.  相似文献   

A model for the emission spectrum of Active Galactic Nuclei     

Thierry J. -L. Courvoisier  Max Camenzind 《Astrophysics and Space Science》1983,93(2):277-280

The overall spectrum of Active Galactic Nuclei is discussed in terms of a wind and shock model. The central object of the active galactic nuclei is the source of a strong supercritical wind. The interaction of the wind with the surrounding medium generates the non-thermal radiation observed in active galactic nuclei. The spectrum predicted by the wind and shock model is compared with the observations of the quasar 3C 273.  相似文献   

Stochastic and dynamic temperature changes in the interplanetary gas     

Max K. Wallis  M.H.A. Hassan 《Planetary and Space Science》1978,26(2):111-120

Exact solutions have been found to the Fokker-Planck equations, incorporating stochastic velocity changes and modelling particles moving in an inverse square central force field under an inverse square collision frequency. The solutions for the velocity distribution contain a combination of collisional and dynamical (reversible) heating. At a general position, there are two populations each with three distinct temperatures, one normal to the orbital plane and the others closely parallel and perpendicular to the mean orbit. Collisional heating is strong and most readily detected in the secondary component of gas which reaches upstream directions along indirect orbits (attractive central force). For interplanetary helium gas reaching 1 a.u., the collisional heating ranges from effective transverse increase of 200 K and radial increase of 1500 K in the downstream wake, to several thousand K increase in radial temperature of the secondary component transverse to the initial gas stream. In interpreting 584 Å sky background radiation observations, the dynamical changes in the velocity spread have to be taken into account for helium gas that is initially hot, when Doppler shifts relative to the solar emission line are significant; the present solutions being the thermal approximations to the distribution function reveal the appropriate radial temperature as a function of space.  相似文献   

Book review     

Max Wyss 《Pure and Applied Geophysics》1976,114(4):741-741

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Editors' Introduction     

Carlos Nunes Silva  Max Barlow 《GeoJournal》2002,58(1):1-2

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Using Ontologies for Integrated Geographic Information Systems   总被引：13，自引：0，他引：13  

Frederico T. Fonseca  Max J. Egenhofer  Peggy Agouris  & Gilberto Câmara 《Transactions in GIS》2002,6(3):231-257

Today, there is a huge amount of data gathered about the Earth, not only from new spatial information systems, but also from new and more sophisticated data collection technologies. This scenario leads to a number of interesting research challenges, such as how to integrate geographic information of different kinds. The basic motivation of this paper is to introduce a GIS architecture that can enable geographic information integration in a seamless and flexible way based on its semantic value and regardless of its representation. The proposed solution is an ontology-driven geographic information system that acts as a system integrator. In this system, an ontology is a component, such as the database, cooperating to fulfill the system's objectives. By browsing through ontologies the users can be provided with information about the embedded knowledge of the system. Special emphasis is given to the case of remote sensing systems and geographic information systems. The levels of ontologies can be used to guide processes for the extraction of more general or more detailed information. The use of multiple ontologies allows the extraction of information in different stages of classification. The semantic integration of aerial images and GIS is a crucial step towards better geospatial modeling.  相似文献   

The Guiana and the West African Shield Palaeoproterozoic grouping: new palaeomagnetic data for French Guiana and the Ivory Coast     

Sébastien Nomade  Yan Chen  ré Pouclet  Gilbert Féraud  Hervé Théveniaut  Bertin Yao Daouda  Max Vidal  Cécile Rigolet 《Geophysical Journal International》2003,154(3):677-694

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Snow research in Svalbard–an overview     

Jan-Gunnar Winther  Oddbjørn Bruland  Knut Sand  Sebastian Gerland  David Marechal  Boris Ivanov  Piotr Gøowacki  Max König 《Polar research》2003,22(2):125-144

This paper summarizes the most significant snow-related research that has been conducted in Svalbard. Most of the research has been performed during the 1990s and includes investigations of snow distribution, snow-melt, snow pack characteristics, remote sensing of snow and biological studies where snow conditions play an important role. For example, studies have shown regional trends with about 50% higher amounts of snow accumulation at the east coast of Spitsbergen compared to the west coast. Further, the accumulation rates are about twice as high in the south compared to the north. On average, the increase in accumulation with elevation is 97 mm water equivalents per 100 m increase in elevation. Several researchers reported melt rates, which are primarily driven by incoming short-wave radiation, in the range of 10-20 mm/day during spring. Maximum melt rates close to 70 mm/day have been measured. In addition to presenting an overview of research activities, we discuss new, unpublished results in areas where considerable progress is being made. These are i) modelling of snow distribution, ii) modelling of snowmelt runoff and iii) monitoring of snow coverage by satellite imagery. We also identify some weaknesses in current research activities. They are lacks of i) integration between various studies, ii) comparative studies with other Arctic regions, iii) applying local field studies in models that can be used to study larger areas of Svalbard and, finally, iv) using satellite remote sensing data for operational monitoring purposes.  相似文献   

Spatial‐Scene Similarity Queries     

Konstantinos A Nedas  Max J Egenhofer 《Transactions in GIS》2008,12(6):661-681

Assessing spatial scenes for similarity is difficult from a cognitive and computational perspective. Solutions to spatial‐scene similarity assessments are sensible only if corresponding elements in the compared scenes are identified correctly. This matching process becomes increasingly complex and error‐prone for large spatial scenes as it is questionable how to choose one set of associations over another or how to account quantitatively for unmatched elements. We develop a comprehensive methodology for similarity queries over spatial scenes that incorporates cognitively motivated approaches about scene comparisons, together with explicit domain knowledge about spatial objects and their relations for the relaxation of spatial query constraints. Along with a sound graph‐theoretical methodology, this approach provides the foundation for plausible reasoning about spatial‐scene similarity queries.  相似文献   

The clustering of luminous red galaxies in the Sloan Digital Sky Survey imaging data     

Nikhil Padmanabhan  David J. Schlegel  Uro&#; Seljak  Alexey Makarov  Neta A. Bahcall  Michael R. Blanton  Jonathan Brinkmann  Daniel J. Eisenstein  Douglas P. Finkbeiner  James E. Gunn  David W. Hogg  &#;eljko Ivezi&#;  Gillian R. Knapp  Jon Loveday  Robert H. Lupton  Robert C. Nichol  Donald P. Schneider  Michael A. Strauss  Max Tegmark  Donald G. York 《Monthly notices of the Royal Astronomical Society》2007,378(3):852-872

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