EGU21-12027
https://doi.org/10.5194/egusphere-egu21-12027
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Assessment of COSMIC-2 reduced-dynamic and kinematic orbit determination

Adrian Jaeggi1, Daniel Arnold1, Jan Weiss2, and Doug Hunt2
Adrian Jaeggi et al.
  • 1University of Bern, Astronomical Institute, Berne, Switzerland (adrian.jaeggi@aiub.unibe.ch)
  • 2University Corporation for Atmospheric Research, COSMIC Program, Boulder, Colorado

The Constellation Observing System for Meteorology, Ionosphere, and Climate 2 (COSMIC-2) mission was launched on June 25, 2019 into six evenly spaced circular orbital planes of 24° inclination with initial altitudes of 725 km. By February 2021 the COSMIC-2 satellites will be lowered to an operational altitude of about 520 km. The satellites carry an advanced Tri‐GNSS (Global Navigation Satellite System) Radio-occultation System (TGRS) instrument to provide high vertical resolution profiles of atmospheric bending angle and refractivity, as well as measurements of ionospheric total electron content, electron density, and scintillation. The TGRS payload tracks GPS and GLONASS signals on two upward looking antennas used for precise orbit determination (POD). We compute one- and two-antenna GPS and GPS+GLONASS POD solutions at both orbit altitudes and assess the orbit quality and systematic orbit errors using different metrics. In particular, we also use different POD setups to compute kinematic solutions employing single-receiver ambiguity fixing and test their contribution to selected months of gravity field recovery based on Swarm GPS data.

How to cite: Jaeggi, A., Arnold, D., Weiss, J., and Hunt, D.: Assessment of COSMIC-2 reduced-dynamic and kinematic orbit determination, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-12027, https://doi.org/10.5194/egusphere-egu21-12027, 2021.

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