EGU26-3438, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-3438
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, X4.129
Fluxgate Magnetic Field Instrument for Seven Small Plasma Observatory Spacecraft
Evgeny V. Panov1, Ferdinand Plaschke2, Lorenzo Matteini3, David Fischer1, Gerlinde Timmermann2, Patrick Brown3, Hans Ulrich Auster2, Emanuele Cupido3, Werner Magnes1, Rumi Nakamura1, Yasuhito Narita4, Ingo Richter2, Adriana Settino1, Zoltan Vörös1, and Owen Roberts5
Evgeny V. Panov et al.
  • 1Space Research Institute, Austrian Academy of Sciences, Graz, Austria
  • 2Institute of Geophysics and Extraterrestrial Physics, Technical University of Braunschweig, Braunschweig, Germany
  • 3Imperial College London, London, United Kingdom
  • 4Institute of Theoretical Physics, Technical University of Braunschweig, Braunschweig, Germany
  • 5Department of Physics, Aberystwyth University, Aberystwyth, United Kingdom

The fluxgate magnetic field instrument (MAG) onboard seven small Plasma Observatory (PO) spacecraft is a collaborative effort between the Space Research Institute in Graz (AT), the Technical University of Braunschweig (DE) and the Imperial College London (UK). MAG is a dual-sensor fluxgate magnetometer that measures the vector of the magnetic field in space. The science objective of MAG is to provide the magnetic field measurements that are crucial for analyzing plasma processes in six key science regions of Plasma Observatory: foreshock, bowshock, magnetosheath, magnetopause, transition region and tail current sheet. MAG measures the background magnetic field in the near-Earth space in the range ± 10,000 nT with frequencies up to 256 Hz, a noise floor of less than 10 pT/√Hz at 1Hz and an error of less than ±0.5 nT.  The targeted value range in terms of static and variational field for PMO is in the order of 100 nT. The maximum sampling frequency of 256 Hz allows for a sufficient overlap with concurrent Search Coil Magnetometer measurements. The poster gives an overview over the magnetometer design as well as its scientific goals.

How to cite: Panov, E. V., Plaschke, F., Matteini, L., Fischer, D., Timmermann, G., Brown, P., Auster, H. U., Cupido, E., Magnes, W., Nakamura, R., Narita, Y., Richter, I., Settino, A., Vörös, Z., and Roberts, O.: Fluxgate Magnetic Field Instrument for Seven Small Plasma Observatory Spacecraft, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3438, https://doi.org/10.5194/egusphere-egu26-3438, 2026.