EGU25-17894, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-17894
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Tuesday, 29 Apr, 08:30–10:15 (CEST), Display time Tuesday, 29 Apr, 08:30–12:30
 
Hall X4, X4.78
The MAG-M magnetometer onboard Plasma Observatory
Lorenzo Matteini, Patrick Brown, Madeleine Tomes, and John Hodgkins
Lorenzo Matteini et al.
  • Imperial College London, Physics Dept., London, United Kingdom of Great Britain – England, Scotland, Wales (l.matteini@imperial.ac.uk)

Plasma Observatory (PO) is an ESA mission proposal to study for the first time plasma transport and energization in the near-Earth environment simultaneously at both fluid and ion scales, with a constellation of 7 spacecraft: 1 mother and 6 daughters. 
In the PO mission framework, MAG-M is the proposed fluxgate magnetometer onboard the Mothercraft, to be built at Imperial College London.
It is a dual-sensor instrument mounted on a rigid boom dedicated to high-resolution measurements of the DC magnetic field, with strong design heritage from previous missions. In this presentation we review MAG-M main characteristics and its development stage. 
We also discuss the key role of magnetic field measurements in the goals of the mission and how MAG-M will contribute, both with single-point and multi-point measurements, to the investigation of the nature of waves and structures in the plasma at both fluid and kinetic scales, their vector anisotropies, the 3-dimensional shapes of eddies and boundaries in the plasma as well as to the determination of the flows of energy acting between particles and fields in the near-Earth environment.

How to cite: Matteini, L., Brown, P., Tomes, M., and Hodgkins, J.: The MAG-M magnetometer onboard Plasma Observatory, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17894, https://doi.org/10.5194/egusphere-egu25-17894, 2025.