Draft:SPIS

Spacecraft Plasma Interaction Software (SPIS)
Developer(s)	Artenum SARL ONERA CNES ESA Airbus Defence and Space
Stable release	6.1.2 (January 2024)
Written in	Java
Operating system	Linux/Windows/Unix-like
License	GPL-2.0-only
Website	www.spis.org/software/spis/

Submission declined on 25 April 2024 by Utopes (talk).

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Declined by Utopes 6 days ago. Last edited by Utopes 6 days ago. Reviewer: Inform author.

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Comment: Requires significant coverage from independent sources, per Wikipedia's notability guidelines. Utopes _{(talk / cont)} 23:57, 25 April 2024 (UTC)

Spacecraft Plasma Interaction Software (SPIS) is a multi-platform open source (GPL-2.0-only) scientific computing software for spacecraft-plasma interactions modelling in 3D. It is used in the assessment of platform-level risks to spacecraft from differential surface charging and internal charging in space, the diagnosis and assessment of scientific (plasma) instrumentation and electrical thrusters, and the study of charging phenomena on dust, moons and other airless bodies.^[1]

SPIS includes a 3D electrostatic plasma solver developped in Java based on an unstructured mesh to model detailed (sheath) structures around complex and realistic geometries. Integrating several models (PIC, fluid ,backtracking, others), SPIS is able to handle a large scale of plasma conditions, materials and physics.

With years, SPIS became the de facto European reference tool for spacecraft charging analysis.^[2], with a long list of peer-reviewed journal articles associated with it ^[3]^[4]^[5]

References[edit]

^ "SPIS Website". SPIS. Retrieved 23 April 2024.
^ "ESA Space environment and effects section". ESA. Retrieved 23 April 2024.
^ "Publications – SPINE". Retrieved 24 April 2024.
^ Roussel, J.-F.; Rogier, F.; Dufour, G.; Mateo-Velez, J.-C.; Forest, J.; Hilgers, A.; Rodgers, D.; Girard, L.; Payan, D. (October 2008). "SPIS Open-Source Code: Methods, Capabilities, Achievements, and Prospects". IEEE Transactions on Plasma Science. 36 (5): 2360–2368. Bibcode:2008ITPS...36.2360R. doi:10.1109/TPS.2008.2002327.
^ Johansson, F. L.; Eriksson, A. I.; Gilet, N.; Henri, P.; Wattieaux, G.; Taylor, M. G. G. T.; Imhof, C.; Cipriani, F. (1 October 2020). "A charging model for the Rosetta spacecraft". Astronomy & Astrophysics. 642: A43. arXiv:2008.09456. Bibcode:2020A&A...642A..43J. doi:10.1051/0004-6361/202038592.

[1] "SPIS Website". SPIS. Retrieved 23 April 2024.

[2] "ESA Space environment and effects section". ESA. Retrieved 23 April 2024.

[3] "Publications – SPINE". Retrieved 24 April 2024.

[4] Roussel, J.-F.; Rogier, F.; Dufour, G.; Mateo-Velez, J.-C.; Forest, J.; Hilgers, A.; Rodgers, D.; Girard, L.; Payan, D. (October 2008). "SPIS Open-Source Code: Methods, Capabilities, Achievements, and Prospects". IEEE Transactions on Plasma Science. 36 (5): 2360–2368. Bibcode:2008ITPS...36.2360R. doi:10.1109/TPS.2008.2002327.

[5] Johansson, F. L.; Eriksson, A. I.; Gilet, N.; Henri, P.; Wattieaux, G.; Taylor, M. G. G. T.; Imhof, C.; Cipriani, F. (1 October 2020). "A charging model for the Rosetta spacecraft". Astronomy & Astrophysics. 642: A43. arXiv:2008.09456. Bibcode:2020A&A...642A..43J. doi:10.1051/0004-6361/202038592.

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