EGU26-20732, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-20732
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Tuesday, 05 May, 08:30–10:15 (CEST), Display time Tuesday, 05 May, 08:30–12:30
 
Hall X4, X4.136
The DPU BOX-P flight software of Plasma Observatory, a LIRA contribution
Léa Griton1, Philippe Plasson1, Karine Issautier1, Milan Maksimovic1, Thibault Peccoux1, Pierre-Vincent Gouel1, Matthieu Berthomier2, Cécile Fiachetti3, Hanna Rothkaehl4, Grzegorz Ptasinski4, Raffaella D'Amicis5, Maria Marcucci5, and Alessandro Retino2
Léa Griton et al.
  • 1LIRA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Cité, 5 place Jules Janssen, 92195 Meudon, France
  • 2Laboratoire de Physique des Plasmas (LPP-CNRS/UMR7648), France
  • 3Centre national d'Etudes spatiales (CNES), France
  • 4Centrum Badań Kosmicznych PAN, Space Research Centre PAS, Poland
  • 5INAF - Institute for Space Astrophysics and Planetology (IAPS), Italy

Plasma Observatory is one of the three candidates currently being evaluated by ESA as the future M7 mission. Its objectives are to determine how particles are energized, identify the main processes that transport energy in space plasma, and understand the interactions between the different regions of the Earth's magnetosphere with multi-scale measurements in situ. To achieve these scientific objectives, Plasma Observatory (PMO) is deseigned as seven identical sister spacecrafts (SSCs) in a two nested tetrahedra configuration.

The Laboratory for Instrumentation and Research in Astrophysics (LIRA) of the Observatory of Paris is responsible for the DPU-P application software for the BOX-P instrument. The LIRA contribution includes the specification, design, implementation and testing, verification and validation, product assurance, and development of the test platform. The DPU BOX-P flight software transforms the raw data produced by the instruments into scientific products of L0 level that can be used on the ground (precise dating, synchronisation, filtering, reduction, compression), which means that a significant part of the scientific value of each instrument is directly produced by the software. Responsibility for the flight software places LIRA at the heart of defining scientific products (content, format and cadence of L0s), optimizing on-board processing and science/resource trade-offs, in direct interaction with the instrument teams and mission constraints. The LIRA team has recognized expertise in complex scientific flight software, demonstrated on missions such as PLATO and Solar Orbiter.

Here we present the DPU-P software and we discuss its contribution to the science of Plasma Observatory.

How to cite: Griton, L., Plasson, P., Issautier, K., Maksimovic, M., Peccoux, T., Gouel, P.-V., Berthomier, M., Fiachetti, C., Rothkaehl, H., Ptasinski, G., D'Amicis, R., Marcucci, M., and Retino, A.: The DPU BOX-P flight software of Plasma Observatory, a LIRA contribution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20732, https://doi.org/10.5194/egusphere-egu26-20732, 2026.