EGU25-8702, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-8702
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Thursday, 01 May, 08:30–10:15 (CEST), Display time Thursday, 01 May, 08:30–12:30
 
Hall X4, X4.166
Influence of sensor noise levels on magnetometer calibration parameters
Gerlinde Timmermann, Patrick Kolhey, Hans-Ulrich Auster, Ingo Richter, and Ferdinand Plaschke
Gerlinde Timmermann et al.
  • TU Braunschweig, Institute of Geophysics and Extraterrestrial Physics, Faculty of Electrical Engineering, Information Technology, Physics, Germany

Magnetometers are prime instruments of scientific spacecraft targeting the space plasma environments of solar system bodies. Despite extensive ground calibration efforts, regular inflight calibration activities of these magnetometers have shown to be crucial to maintain necessary data quality levels over time. Classically, 12 parameters influence the calibration: 3 gain values, 6 angles defining magnetic sensor orientations, and 3 zero level offsets that correspond to instrument outputs in vanishing ambient fields. Particularly in low fields, accurate choice of offset levels are of utmost importance. To achieve this, measurements of Alfvénic fluctuations in the solar wind are typically used. We investigate the influence of sensor noise levels on the accuracy of different calibration parameters, particularly on the offsets, using THEMIS/ARTEMIS magnetic field measurements. 

How to cite: Timmermann, G., Kolhey, P., Auster, H.-U., Richter, I., and Plaschke, F.: Influence of sensor noise levels on magnetometer calibration parameters, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8702, https://doi.org/10.5194/egusphere-egu25-8702, 2025.