985 resultados para XML Metadata Interchange
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Lecture 3: DOM and XPath Lecture slides and exercises for using DOM and XPath to access material within an XML database or document.
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Lecture 5: XLink and XPointer Lecture slides and exercises for using XLink and XPointer to link to and control material within an XML database or document.
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In this class, we will discuss metadata as well as current phenomena such as tagging and folksonomies. Readings: Ontologies Are Us: A Unified Model of Social Networks and Semantics, P. Mika, International Semantic Web Conference, 522-536, 2005. [Web link] Optional: Folksonomies: power to the people, E. Quintarelli, ISKO Italy-UniMIB Meeting, (2005)
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Discussions around the kind of decisions that people should make in their exam questions
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Lecture 1: Basic XML & HTML5 Lecture slides and exercises for reading and writing basic XML and HTML
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El artículo está incluido en un número monográfico especial con los trabajos del I Simposio Pluridisciplinar sobre Diseño, Evaluación y Descripción de Contenidos Educativos Reutilizables (Guadalajara, Octubre 2004).Resumen tomado de la publicación
Extensión y uso de KML para la anotación, georreferenciación y distribución de recursos de tipo MIME
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En el actual contexto de la Web 2.0 y de la futura Web Geográfica o simplemente GeoWeb la información georreferenciada cobra cada día más importancia. Desde hace años distintas técnicas han sido desarrolladas para dar solución al problema de la georreferenciación de recursos de distinta índole. Sin embargo ninguna de estas técnicas está exenta de problemas y restricciones. En este estudio presentamos una nueva aproximación que intenta facilitar la georreferenciación y distribución de recursos de tipos contemplados como Multipurpose Internet Mail Extensions (MIME). El elemento básico para la anotación, georreferenciación y también representación del recurso es el Keyhole Markup Language (KML). Este lenguaje permite la anotación y visualización de elementos, así como su extensión para aumentar su funcionalidad. Esta última propiedad se ha utilizado en nuestra aproximación para crear nuevos elementos que permitan la anotación de cualquier tipo de recurso MIME sobre KML obteniendo así la extensión KML MIMEXT. Esta extensión permite describir y georreferenciar tipos de recursos no habituales en el entorno SIG. La encapsulación del propio recurso junto con sus metadatos (incluyendo la georreferenciación) y otros recursos relacionados se realiza mediante la compresión de todos ellos en un único archivo KMZ facilitando así su distribución y mantenimiento. De forma similar a la interpretación de etiquetas HTML5 como video por los navegadores Web, el uso de la extensión MIMEXT podría ser implementado por visores basados en globos virtuales para visualizar o reproducir nuevos tipos de recursos. Para ejemplificar dicho comportamiento se ha implementado un prototipo de aplicación Java basado en el SDK World Wind Java
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An update of Owens et al. (2008) shows that the relationship between the coronal mass ejection (CME) rate and the heliospheric magnetic field strength predicts a field floor of less than 4 nT at 1 AU. This implies that the record low values measured during this solar minimum do not necessarily contradict the idea that open flux is conserved. The results are consistent with the hypothesis that CMEs add flux to the heliosphere and interchange reconnection between open flux and closed CME loops subtracts flux. An existing model embracing this hypothesis, however, overestimates flux during the current minimum, even though the CME rate has been low. The discrepancy calls for reasonable changes in model assumptions.
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Motivation: There is a frequent need to apply a large range of local or remote prediction and annotation tools to one or more sequences. We have created a tool able to dispatch one or more sequences to assorted services by defining a consistent XML format for data and annotations. Results: By analyzing annotation tools, we have determined that annotations can be described using one or more of the six forms of data: numeric or textual annotation of residues, domains (residue ranges) or whole sequences. With this in mind, XML DTDs have been designed to store the input and output of any server. Plug-in wrappers to a number of services have been written which are called from a master script. The resulting APATML is then formatted for display in HTML. Alternatively further tools may be written to perform post-analysis.
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We outline a method to determine the direction of solar open flux transport that results from the opening of magnetic clouds (MCs) by interchange reconnection at the Sun based solely on in-situ observations. This method uses established findings about i) the locations and magnetic polarities of emerging MC footpoints, ii) the hemispheric dependence of the helicity of MCs, and iii) the occurrence of interchange reconnection at the Sun being signaled by uni-directional suprathermal electrons inside MCs. Combining those observational facts in a statistical analysis of MCs during solar cycle 23 (period 1995 – 2007), we show that the time of disappearance of the northern polar coronal hole (1998 – 1999), permeated by an outward-pointing magnetic field, is associated with a peak in the number of MCs originating from the northern hemisphere and connected to the Sun by outward-pointing magnetic field lines. A similar peak is observed in the number of MCs originating from the southern hemisphere and connected to the Sun by inward-pointing magnetic field lines. This pattern is interpreted as the result of interchange reconnection occurring between MCs and the open field lines of nearby polar coronal holes. This reconnection process closes down polar coronal hole open field lines and transports these open field lines equatorward, thus contributing to the global coronal magnetic field reversal process. These results will be further constrainable with the rising phase of solar cycle 24.
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Interchange reconnection at the Sun, that is, reconnection between a doubly-connected field loop and singly-connected or open field line that extends to infinity, has important implications for the heliospheric magnetic flux budget. Recent work on the topic is reviewed, with emphasis on two aspects. The first is a possible heliospheric signature of interchange reconnection at the coronal hole boundary, where open fields meet closed loops. The second aspect concerns the means by which the heliospheric magnetic field strength reached record-lows during the recent solar minimum period. A new implication of this work is that interchange reconnection may be responsible for the puzzling, occasional coincidence of the heliospheric current sheet and the interface between fast and slow flow in the solar wind.