Integrated Access to Solar Observations With EGSO

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7594 Instruments And Techniques, 9805 Instruments Useful In Three Or More Fields, 9810 New Fields (Not Classifiable Under Other Headings), 9820 Techniques Applicable In Three Or More Fields

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{\b Co-Authors}: J.Aboudarham (2), E.Antonucci (3), R.D.Bentely (4), L.Ciminiera (5), A.Finkelstein (4), J.B.Gurman(6), F.Hill (7), D.Pike (8), I.Scholl (9), V.Zharkova and the EGSO development team {\b Institutions}: (2) Observatoire de Paris-Meudon (France); (3) INAF - Istituto Nazionale di Astrofisica (Italy); (4) University College London (U.K.); (5) Politecnico di Torino (Italy), (6) NASA Goddard Space Flight Center (USA); (7) National Solar Observatory (USA); (8) Rutherford Appleton Lab. (U.K.); (9) Institut d'Astrophysique Spatial, Universite de Paris-Sud (France) ; (10) University of Bradford (U.K) {\b Abstract}: The European Grid of Solar Observations is the European contribution to the deployment of a virtual solar observatory. The project is funded under the Information Society Technologies (IST) thematic programme of the European Commission's Fifth Framework. EGSO started in March 2002 and will last until March 2005. The project is categorized as a computer science effort. Evidently, a fair amount of issues it addresses are general to grid projects. Nevertheless, EGSO is also of benefit to the application domains, including solar physics, space weather, climate physics and astrophysics. With EGSO, researchers as well as the general public can access and combine solar data from distributed archives in an integrated virtual solar resource. Users express queries based on various search parameters. The search possibilities of EGSO extend the search possibilities of traditional data access systems. For instance, users can formulate a query to search for simultaneous observations of a specific solar event in a given number of wavelengths. In other words, users can search for observations on the basis of events and phenomena, rather than just time and location. The software architecture consists of three collaborating components: a consumer, a broker and a provider. The first component, the consumer, organizes the end user interaction and controls requests submitted to the grid. The consumer is thus in charge of tasks such as request handling, request composition, data visualization and data caching. The second component, the provider, is dedicated to data providing and processing. It links the grid to individual data providers and data centers. The third component, the broker, collects information about providers and allows consumers to perform the searches on the grid. Each component can exist in multiple instances. This follows a basic grid concept: The failure or unavailability of a single component will not generate a failure of the whole system, as other systems will take over the processing of requests. The architecture relies on a global data model for the semantics. The data model is in some way the brains of the grid. It provides a description of the information entities available within the grid, as well as a description of their relationships. EGSO is now in the development phase. A demonstration (www.egso.org/demo) is provided to get an idea about how the system will function once the project is completed. The demonstration focuses on retrieving data needed to determine the energy released in the solar atmosphere during the impulsive phase of flares. It allows finding simultaneous observations in the visible, UV, Soft X-rays, hard X-rays, gamma-rays, and radio. The types of observations that can be specified are images at high space and time resolutions as well as integrated emission and spectra from a yet limited set of instruments, including the NASA spacecraft TRACE, SOHO, RHESSI, and the ground-based observatories Phoenix-2 in Switzerland and Meudon Observatory in France

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