Mutual radio occultation experiment between ExoMars Trace Gas Orbiter and Mars Express: algorithms testing
- 1The Abdus Salam International Centre for Theoretical Physics, Trieste, Italy
- 2Department of Physics, University of New Brunswick, Fredericton, New Brunswick, Canada
- 3School of Physics and Astronomy, University of Leicester, Leicester, UK
- 4European Space Agency, ESA/ESTEC, Directorate of Science, Noordwijk, Netherlands
- 5Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
Radio Occultation (RO) is a very powerful technique to probe a planetary atmosphere, in providing vertical density profiles of the neutral atmosphere and ionosphere. The standard method uses a radio link between a spacecraft and an Earth ground station. Nevertheless, the possibility to obtain information about the Martian atmosphere with mutual RO events, using data from NASA Mars Odyssey and Mars Reconnaissance Orbiters (MRO), has been demonstrated by Ao et al. (2015).
Taking advantage of two European spacecraft in orbit around Mars, the European Space Agency is currently preparing experiments of mutual RO between Mars Express (MEX) and the ExoMars Trace Gas Orbiter (TGO). In preparation of MEX and TGO data inversion and analysis, a simulation-based strategy has been adopted and an algorithm able to retrieve vertical electron density profiles from Doppler shift measurements has been implemented and validated. Subsequently, in order to test the mentioned algorithm with experimental data, the same three RO events considered in the paper by Ao et al. (2015) have been processed. In particular, for each RO event, having the information about the satellites’ orbit, the (excess) Doppler shift values corresponding to the Mars Odyssey-MRO ray-paths have been converted to bending angles as a function of impact parameter. Then, assuming a spherical symmetry (Fjeldbo et al., 1971) for the ionosphere electron density, the bending angles have been transformed (through Abel integral) to a vertical refractivity profile, which, in turn, has been converted to an ionospheric electron density profile.
In this work, the results obtained by the application of the mentioned inversion algorithm to experimental data will be presented, with particular focus on the retrieval of the ionospheric electron density profiles.
References
Ao, C. O., C. D. Edwards Jr., D. S. Kahan, X. Pi, S. W. Asmar, and A. J. Mannucci (2015), A first demonstration of Mars crosslink occultation measurements, Radio Sci., 50, 997–1007, doi:10.1002/2015RS005750.
Fjeldbo, G., A. J. Kliore, and V. R. Eshleman (1971), The neutral atmosphere of Venus as studied with the Mariner V radio occultation
experiments, Astron. J., 76, 123–140.
How to cite: Nava, B., Migoya-Orue, Y., Kashcheyev, A., Sánchez-Cano, B., Witasse, O., Svedhem, H., Parrott, J., Titov, D., Toni, A., and Ao, C.: Mutual radio occultation experiment between ExoMars Trace Gas Orbiter and Mars Express: algorithms testing, European Planetary Science Congress 2021, online, 13–24 Sep 2021, EPSC2021-605, https://doi.org/10.5194/epsc2021-605, 2021.
