Virtual European Solar & Planetary Access (VESPA): A Planetary Science Virtual Observatory Cornerstone

0539650 - ÚFA 2021 RIV FR eng J - Journal Article
Erard, S. - Cecconi, B. - Le Sidaner, P. - Chauvin, C. - Rossi, A. P. - Minin, M. - Capria, M.T. - Ivanovski, S. - Schmitt, B. - Génot, V. - André, N. - Marmo, C. - Vandaele, A. C. - Trompet, L. - Scherf, M. - Hueso, R. - Määttänen, A. - Carry, B. - Achilleos, N. - Souček, Jan - Píša, David - Benson, K. - Fernique, P. - Millour, E.
Virtual European Solar & Planetary Access (VESPA): A Planetary Science Virtual Observatory Cornerstone.
Data Science Journal. Roč. 19, č. 1 (2020), s. 1-10, č. článku 22. E-ISSN 1683-1470
EU Projects: European Commission(XE) 654208 - EPN2020-RI; European Commission(XE) 871149 - EPN-2024-RI
Institutional support: RVO:68378289
Keywords : gis * Solar System * Virtual Observatory
OECD category: Astronomy (including astrophysics,space science)
Method of publishing: Open access
https://datascience.codata.org/articles/10.5334/dsj-2020-022/

The Europlanet-2020 programme, which ended on Aug 31st, 2019, included an activity called VESPA (Virtual European Solar and Planetary Access), which focused on adapting Virtual Observatory (VO) techniques to handle Planetary Science data. This paper describes some aspects of VESPA at the end of this 4-years development phase and at the onset of the newly selected Europlanet-2024 programme starting in 2020. The main objectives of VESPA are to facilitate searches both in big archives and in small databases, to enable data analysis by providing simple data access and online visualization functions, and to allow research teams to publish derived data in an interoperable environment as easily as possible. VESPA encompasses a wide scope, including surfaces, atmospheres, magnetospheres and planetary plasmas, small bodies, heliophysics, exoplanets, and spectroscopy in solid phase. This system relies in particular on standards and tools developed for the Astronomy VO (IVOA) and extends them where required to handle specificities of Solar System studies. It also aims at making the VO compatible with tools and protocols developed in different contexts, for instance GIS for planetary surfaces, or time series tools for plasma-related measurements. An essential part of the activity is to publish a significant amount of high-quality data in this system, with a focus on derived products resulting from data analysis or simulations.
Permanent Link: http://hdl.handle.net/11104/0317353