EGU24-20446, updated on 11 Mar 2024
https://doi.org/10.5194/egusphere-egu24-20446
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

M-Matisse Crosslink experiment MaCro: an intersatellite radio link for the sounding of the Martian atmosphere

Martin Pätzold1, Tom Andert2, Takeshi Imamura3, Hiroki Ando4, Antonio Genova5, Matthias Hahn1, Katsuyuki Noguchi5, Janusz Oschlisniok1, Kerstin Peter1, and Silvia Tellmann1
Martin Pätzold et al.
  • 1Rheinisches Institut für Umweltforschung an der Universität zu Köln, Abteilung Planetenforschung, Köln, Germany
  • 2Institut für Raumfahrttechnik und Weltraumnutzung, Universität der Bundeswehr München, Neubiberg, Germany
  • 3Graduate School of Frontier Sciences, The University of Tokyo, Tokyo, Japan
  • 4Kyoto Sangyo University, Kyoto, Japan
  • 5Department of Mechanical and Aerospace Enginnering, Universita di Roma, Rome, Italy

The "Mars Magnetosphere ATmosphere Ionosphere and Space-weather SciencE (M-MATISSE)" mission, currently in Phase A study by the European Space Agency (ESA), is a Medium-class (M7) candidate. M-MATISSE aims to unravel the intricate and dynamic couplings of the Martian magnetosphere, ionosphere, and thermosphere (MIT coupling) in relation to the solar wind (i.e., space weather) and the lower atmosphere. This two-spacecraft mission involves both spacecraft carrying an identical payload suite, each following different orbits with an apocenter at 3,000 km and 10,000 km altitude, and a pericenter at 250 km altitude. The intersatellite radio link, MaCro, operates at two frequencies to probe the ionosphere and atmosphere of Mars during occultation, as one spacecraft disappears behind the planetary disk as seen from the other spacecraft. The instrumentation comprises two transceivers at UHF and S-band, stabilized by an ultrastable oscillator on both spacecraft each. The observables include the shift of the carrier frequencies caused by the bending of the radio ray path in the atmosphere/ionosphere. Onboard data pre-processing precedes the transmission of telemetry to Earth. The orbits allow about eight occultations events (ingress or egress) on average per day starting at an altitude of 1000 km.

How to cite: Pätzold, M., Andert, T., Imamura, T., Ando, H., Genova, A., Hahn, M., Noguchi, K., Oschlisniok, J., Peter, K., and Tellmann, S.: M-Matisse Crosslink experiment MaCro: an intersatellite radio link for the sounding of the Martian atmosphere, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-20446, https://doi.org/10.5194/egusphere-egu24-20446, 2024.