14 research outputs found

    Connecting the CDPP/AMDA service to planetary plasma data: Venus, Earth, Mars, Saturn (Jupiter and comets)

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    International audienceThese last years, CDPP has developed a new service, AMDA (Automated Multi-Dataset Analysis), which is a web-based facility for on line analysis of space physics data (magnetospheric, heliospheric, planetary plasmas) coming from either its local database or distant ones. This tool allows the user to perform on line classical manipulations such as data visualization, parameter computation or data extraction. AMDA also offers innovative functionalities such as event search on the content of the data in either visual or automated way. AMDA has been recently integrated as a service to the scientific community for the Plasma Physics thematic node of the EuroPlaNet IDIS (Integrated and Distributed Information Service) activities. We will present the service AMDA and the planetary plasma data accessible via the service. We will then illustrate some of its applications (boundary identification and planetary space weather) for the comparative analysis of the planetary ionized environments. We will finally discuss future developments under study at CDPP to integrate with AMDA new datasets (Jupiter, comets) and new (astronomical) tools

    Space Weather applications with CDPP/AMDA

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    International audienceAMDA (Automated Multi-Dataset Analysis), a new data analysis service, recently opened at the French Plasma Physics Data Center (CDPP). AMDA is developed according to the Virtual Observatory paradigm: it is a web-based facility for on-line analyses of space physics. Data may come from its own local database as well as remote ones. This tool allows the user to perform classical manipulations such as data visualization, parameter computation and data extraction. AMDA also offers innovative functionalities such as event searches on the content of the data in either visual or automated ways, generation, use and management of time tables (event lists). The general functionalities of AMDA are presented in the context of Space Weather with example scientific use cases

    HST auroral campaign observations of Jupiter and Saturn enabled by the CDPP/AMDA and IVOA/Aladin tools

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    International audienceThe Plasma Physics thematic node of IDIS (http://europlanet-plasmanode.oeaw.ac.at/) is established in close cooperation between the IWF Graz (http://www.iwf.oeaw.ac.at/) and CDPP Toulouse (http://cdpp.cesr.fr/). These last years, CDPP has developed a new service, AMDA (Automated Multi-Dataset Analysis, http://cdpp-amda.cesr.fr/), which is a web-based facility for on line analysis of space physics data (heliosphere, magnetospheres, planetary environments) coming from either its local database or distant ones, such as the Cassini/MAPSKP, VEX/MAG at IWF/Graz or the CDAWeb (http://cdaweb.gsfc.nasa.gov/). These last years, a large campaignof remote high resolution imaging of Jupiter and Saturn aurorae has been undertaken using the Hubble Space Telescope, in association with in situ measurements of local solar wind and magnetospheric plasma conditions using several different spacecraft (including Galileo, Cassini and New Horizons). The coordinated scientific exploitation of all these data is a major technical challenge, since it requires accessing heterogeneous data from diverse origins to perform an integrated study combining different software tools appropriate for the analysis of the solar wind, magnetospheric, ionospheric and atmospheric phenomena observed.In the context of our IDIS activities, we will detail our prototype service connecting the CDPP/AMDA service with the IVOA (http://www.ivoa.net/) tool Aladin (http://aladin.u-strasbg.fr/), which is an interactive software that enable the user to visualize digitized astronomical images of Jupiter and Saturn aurorae in combination with solar wind and magnetospheric data reachable via AMDA

    AMDA, Automated Multi-Dataset Analysis: A web-based service provided by the CDPP.

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    For in depth studies of plasma objects such as the Earth's magnetosphere or the solar wind, it is necessary to analyse multi-points and multiinstruments measurements. In practice, that means that researchers have to exploit together data coming from many sources which can initially be heterogeneous in their internal organisation, their description or their codhal-00455456
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