MATISSE Multi-purpose Advanced Tool for Instruments for the Solar System Exploration Angelo Zinzi1,2, M. T. Capria3,1, E. Palomba3,1, L. A. Antonelli1,2 1) ASDC; 2) INAF – OAR; 3) INAF-IAPS [email protected] ASI Science Data Center (ASDC) 1996 BeppoSAX Science Data Center founded PV 2013 | ESA ESRIN | 4-6 November 2013 ASDC major partner for the ASI missions of observation of Universe (Swift, AGILE, Fermi, NuSTAR, AMS, …) October 2012 The Solar System Exploration group is born ASDC staff Science ASI IT PV 2013 | ESA ESRIN | 4-6 November 2013 • INAF • INFN • Senior Scientists • ASI • Telespazio HERSCHEL PLANCK Beppo FERMI SAX SWIFT AGILE Data Explorer PV 2013 | ESA ESRIN | 4-6 November 2013 NUSTAR Sky Explorer Gaia SED Builder Data (points) + fit (lines) PV 2013 | ESA ESRIN | 4-6 November 2013 Problems in using planetary exploration data In order to work with data from an instruments you need to know their format and the best analysis techniques Code writing to perform the research PV 2013 | ESA ESRIN | 4-6 November 2013 IT IS REALLY HARD TO MAKE SCIENCE WITH DATA IF YOU ARE NOT PART OF THE TEAM! PV 2013 | ESA ESRIN | 4-6 November 2013 It is therefore impossible to exploit the “data fusion”, i.e. … SYSTEMATIC ANALYSIS OF DIFFERENT PHYSICAL QUANTITIES OBSERVED BY DIFFERENT INSTRUMENTS By means of data fusion it is possible to expand the scientific capabilities of an instrument PV 2013 | ESA ESRIN | 4-6 November 2013 MATISSE MATISSE aims to apply to planetary exploration data the huge experience of ASDC in developing tools to support the astrophysics community By means of a VO-like approach it will allow to: • • • • Find multimission data Produce different maps and figures Visualize data on 2D maps or 3D shape models Download only the requested products and not a large dataset PV 2013 | ESA ESRIN | 4-6 November 2013 Intelligent archive To have a really powerful instrument an Intelligent Archive must be developed, i.e., Searchable by specific input parameter, as: Apply DATAsuch MINING to Solar • • • • Planetocentric coordinates Time Surface/atmospheric features Instrument type System Exploration archives PV 2013 | ESA ESRIN | 4-6 November 2013 MATISSE and the “VO-like” approach MATISSE No file format knowledge needed Scientific Higher WWWorder informations from dataoutput query Different instruments data different instruments Analysis tools Reduced time to write codeVisualization PV 2013 | ESA ESRIN | 4-6 November 2013 MATISSE and the Data Fusion This will expand the scientific objectives of every mission, helping in raising scientific production ESA Rosetta mission • VIRTIS & OSIRIS nucleus + coma • GIADA coma + dust particles By fusing their data it will be possible to study dust particles and active regions PV 2013 | ESA ESRIN | 4-6 November 2013 MATISSE for Rosetta • The first year of the project has been mainly dedicated to ESA Rosetta mission, in particular to OSIRIS, VIRTIS and GIADA • The main aim of this first year was to have a stable version of the SW, so that teams can use it for visualization and simple analysis tasks PV 2013 | ESA ESRIN | 4-6 November 2013 MATISSE current version The version now available online is the 0.5 and allows to: • Overlay data from a single observation on the shape model of Lutetia or ChuryumovGerasimenko • Perform ratio and averaging (mosaic) over multiple ROSETTA observations and show the result on the shape model of the selected target PV 2013 | ESA ESRIN | 4-6 November 2013 MATISSE current version No DB Few data available Few scientific capabilities Still in demo/prototype version Complete version after DB and collaboration with scientific teams PV 2013 | ESA ESRIN | 4-6 November 2013 Target, mission, instrument selection Spatial + Time parameters Color control Observation selection (Differentiated access based on user permissions) PV 2013 | ESA ESRIN | 4-6 November 2013 Surface analysis PV 2013 | ESA ESRIN | 4-6 November 2013 Coma/dust analysis PV 2013 | ESA ESRIN | 4-6 November 2013 MATISSE and the teams Indicate scientific Teams priorities ASDC SSE group PV 2013 | ESA ESRIN | 4-6 November 2013 Allows the use of fused data Database issue • Big wealth of data (in the future) • Definition of the granule: whole file/single pixel? • Very different data • • • • • Spectrometers (imaging/non imaging) Cameras Radars Dust analysers … PV 2013 | ESA ESRIN | 4-6 November 2013 Database issue SQL NoSQL + EPN-TAP compliant Geospatial management (see D’Amore et al.,LPSC 2013) Ideal for Big Data Suitable for instruments with different characteristics Not fully scalable No EPN-TAP compliant PV 2013 | ESA ESRIN | 4-6 November 2013 Future developments VESTA PV 2013 | ESA ESRIN | 4-6 November 2013 CERES PV 2013 | ESA ESRIN | 4-6 November 2013 Conclusions • Thanks to MATISSE planetary data could be better and faster analysed • Scientific production would be improved • New and old data could be fused together to have a more complete look PV 2013 | ESA ESRIN | 4-6 November 2013 For info or suggestions please contact me [email protected] THANK YOU PV 2013 | ESA ESRIN | 4-6 November 2013
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