EGU2020-15238, updated on 12 Jun 2020
https://doi.org/10.5194/egusphere-egu2020-15238
EGU General Assembly 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Calculation of temporally high-resolution scaling factors for the thermospheric density from SLR observations

Lea Zeitler, Michael Schmidt, Mathis Bloßfeld, and Sergei Rudenko
Lea Zeitler et al.
  • Technische Universität München, Deutsches Geodätisches Forschungsinstitut (DGFI-TUM), Munich, Germany (lea.zeitler@tum.de)

The motion of a satellite depends on gravitational and non-gravitational accelerations. A major problem in precise orbit determination (POD) of low-Earth orbiting (LEO) satellites is modelling the thermospheric drag. It is the largest non-gravitational acceleration acting on satellites with altitudes lower than 1000 km and decelerates them. In case of the Swarm satellites with an altitude of around 460 km not considering the drag within a POD would cause an error of around 3 meters per revolution in the along-track direction.

In this study, we present results of DGFI-TUM in the context of the project TIPOD (Development of High-Precision Thermosphere Models for Improving Precise Orbit Determination of Low-Earth-Orbiting Satellites) funded by DFG in the frame of the SPP 1788 ‘Dynamic Earth’. One aim of this project is the computation of scaling factors for the thermospheric density from different satellite observation techniques, such as SLR, DORIS, GNSS or accelerometry. For a joint estimation of thermospheric model parameters the spatial, temporal and spectral content of the different scaling factors have to be analysed and interpreted. For example, accelerometer measurements along the satellite orbit provide scaling factors as point values. In this study we derive scaling factors from SLR measurements which could be interpreted as quasi-point values.

For the POD of LEO satellites, DGFI-TUM’s software package DOGS (DGFI-TUM Orbit and Geodetic parameter estimation Software) is used. It is characterized by the ability to process observations of different space geodetic techniques and to combine their linear parameter estimation systems within a joint Gauss-Markov model.

Here, we estimate scaling factors for the thermospheric density with a time resolution much higher than in our previous studies. Therefore, we use information of short passages from selected spherical satellites above SLR ground stations. Different temporal resolutions for the scaling factors varying from 6 hours down to 5 minutes will be tested and discussed in terms of reliability.

How to cite: Zeitler, L., Schmidt, M., Bloßfeld, M., and Rudenko, S.: Calculation of temporally high-resolution scaling factors for the thermospheric density from SLR observations, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-15238, https://doi.org/10.5194/egusphere-egu2020-15238, 2020

This abstract will not be presented.