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INSIGHT-II



Interactions of Low-orbiting Satellites with the Surrounding Ionosphere and Thermosphere Part II

Accelerometer measurements are used in two major topics in Earth observations, namely gravity field recovery and thermosphere studies. We have shown that the thermospheric signatures in the GOCE gravity gradients are due to an unexpected quadratic response of the instruments to the accelerations acting on the satellite. A hypothesis has been worked out, implying the fact that the quadratic factor and other disturbances seen on the accelerometers are coupled together. This hypothesis will be evaluated further, strengthened in experiments and the impact on gravity field recovery as well as thermosphere and ionosphere studied. For gravity field this means an improvement of the GOCE satellite only gravity field by reducing the noise in the gradients and recalibrating the gradiometer. For the Swarm satellite mission, this means an enhancement of the scientific outcome of the accelerometer data by studying high amplitude signals in times of ionospheric storms. An elaborated data processing schema is necessary to make use of these instruments, so an uncertainty estimation procedure will we established evaluating the quality of the retrieved neutral density. Assimilating the neutral density into a physical based ionosphere-thermosphere coupling model the dynamics in the ionosphere at times of storms can be studied. As validation is very important a validation concept is worked out. Therefore, an empirical ionosphere model is enlarged further.

The DLR institute of Communications and Navigation (KN) contributes to this project with enhancement and analysis of the Coupled Thermosphere Ionosphere Electrodynamics (CTIPe) model. KN targets the following objectives:

  1. Validation of CTIPe reconstructions with Swarm, CHAMP, GRACE data and comparing them to thermosphere models. 
  2. Investigation of the dynamics driving mid-latitude ionospheric storms, resulting from different solar wind input like coronal mass ejection (CME), high speed solar wind stream (HSS), magnetic cloud (MC) and co-rotating interaction region (CIR)
  3. Develop a new approach for approximating Swarm neutral density uncertainties

Duration

Sep. 2018 – Aug. 2021

Funded by

Partners

Technische Universität München
Universität Hannover
Deutsches Geodätisches Forschungsinstitut


Contact
Dr. Claudia Borries
Group Leader

German Aerospace Center

Institute of Communications and Navigation
, Navigation
Neustrelitz

Tel.: +49 3981 480-215

Fax: +49 3981 480-123


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