This paper presents the project Comprehensive spAce wEather Studies for the ASPIS prototype Realization (CAESAR), which aims to tackle the relevant aspects of Space Weather (SWE) science and develop a prototype of the scientific data centre for Space Weather of the Italian Space Agency (ASI) called ASPIS (ASI SPace Weather InfraStructure). To this end, CAESAR involves the majority of the SWE Italian community, bringing together 10 Italian institutions as partners, and a total of 92 researchers. The CAESAR approach encompasses the whole chain of phenomena from the Sun to Earth up to planetary environments in a multidisciplinary, comprehensive, and unprecedented way. Detailed and integrated studies are being performed on a number of well-observed “target SWE events”, which exhibit noticeable SWE characteristics from several SWE perspectives. CAESAR investigations synergistically exploit a great variety of different products (datasets, codes, models), both long-standing and novel, that will be made available in the ASPIS prototype: this will consist of a relational database (DB), an interface, and a wiki-like documentation structure. The DB will be accessed through both a Web graphical interface and the ASPIS.py module, i.e., a library of functions in Python, which will be available for download and installation. The ASPIS prototype will unify multiple SWE resources through a flexible and adaptable architecture, and will integrate currently available international SWE assets to foster scientific studies and advance forecasting capabilities.

The CAESAR Project for the ASI Space Weather Infrastructure

Vigorito C.;
2023-01-01

Abstract

This paper presents the project Comprehensive spAce wEather Studies for the ASPIS prototype Realization (CAESAR), which aims to tackle the relevant aspects of Space Weather (SWE) science and develop a prototype of the scientific data centre for Space Weather of the Italian Space Agency (ASI) called ASPIS (ASI SPace Weather InfraStructure). To this end, CAESAR involves the majority of the SWE Italian community, bringing together 10 Italian institutions as partners, and a total of 92 researchers. The CAESAR approach encompasses the whole chain of phenomena from the Sun to Earth up to planetary environments in a multidisciplinary, comprehensive, and unprecedented way. Detailed and integrated studies are being performed on a number of well-observed “target SWE events”, which exhibit noticeable SWE characteristics from several SWE perspectives. CAESAR investigations synergistically exploit a great variety of different products (datasets, codes, models), both long-standing and novel, that will be made available in the ASPIS prototype: this will consist of a relational database (DB), an interface, and a wiki-like documentation structure. The DB will be accessed through both a Web graphical interface and the ASPIS.py module, i.e., a library of functions in Python, which will be available for download and installation. The ASPIS prototype will unify multiple SWE resources through a flexible and adaptable architecture, and will integrate currently available international SWE assets to foster scientific studies and advance forecasting capabilities.
2023
15
2
1
22
https://www.mdpi.com/2072-4292/15/2/346
earth’s ionosphere; earth’s magnetosphere; earth’s plasmasphere; galactic cosmic rays; planetary space weather; solar activity; solar chromosphere; solar corona; solar energetic particles; solar photosphere; solar wind; space weather
Laurenza M.; Del Moro D.; Alberti T.; Battiston R.; Benella S.; Benvenuto F.; Berrilli F.; Bertello I.; Bertucci B.; Biasiotti L.; Campi C.; Carbone V.; Casolino M.; Cecchi Pestellini C.; Chiappetta F.; Coco I.; Colombo S.; Consolini G.; D'Amicis R.; De Gasperis G.; De Marco R.; Del Corpo A.; Diego P.; Di Felice V.; Di Fino L.; Di Geronimo C.; Faldi F.; Ferrente F.; Feruglio C.; Fiandrini E.; Fiore F.; Foldes R.; Formato V.; Francisco G.; Giannattasio F.; Giardino M.; Giobbi P.; Giovannelli L.; Giusti M.; Gorgi A.; Heilig B.; Iafrate G.; Ivanovski S.L.; Jerse G.; Korsos M.B.; Lepreti F.; Locci D.; Magnafico C.; Mangano V.; Marcucci M.F.; Martucci M.; Massetti S.; Micela G.; Milillo A.; Miteva R.; Molinaro M.; Mugatwala R.; Mura A.; Napoletano G.; Narici L.; Neubuser C.; Nistico G.; Pauluzzi M.; Perfetti A.; Perri S.; Petralia A.; Pezzopane M.; Piersanti M.; Pietropaolo E.; Pignalberi A.; Plainaki C.; Polenta G.; Primavera L.; Romoli G.; Rossi M.; Santarelli L.; Santi Amantini G.; Siciliano F.; Sindoni G.; Spadoni S.; Sparvoli R.; Stumpo M.; Tomassetti N.; Tozzi R.; Vagelli V.; Vasantharaju N.; Vecchio A.; Vellante M.; Vernetto S.; Vigorito C.; West M.J.; Zimbardo G.; Zucca P.; Zuccarello F.; Zuccon P.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2318/1946609
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