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Wöske, Florian, Huckfeldt, Moritz, and Rievers, Benny, 2024. Tailored accelerometer calibration by POD for thermospheric density retrieval with GRACE and GRACE-FO. Advances in Space Research, 74(10):4517–4542, doi:10.1016/j.asr.2024.09.021.
• from the NASA Astrophysics Data System • by the DOI System •
@ARTICLE{2024AdSpR..74.4517W,
author = {{W{\"o}ske}, Florian and {Huckfeldt}, Moritz and {Rievers}, Benny},
title = "{Tailored accelerometer calibration by POD for thermospheric density retrieval with GRACE and GRACE-FO}",
journal = {Advances in Space Research},
keywords = {Precise Orbit Determination (POD), GRACE/-FO, Accelerometer, Thermospheric density, Non-gravitational forces},
year = 2024,
month = nov,
volume = {74},
number = {10},
pages = {4517-4542},
abstract = "{The density of the upper atmosphere can be determined by orbit and
accelerometer data from low Earth orbit satellites as insitu
measurements along the orbit. One main challenge therein is the
estimation of physical accelerometer calibration parameters,
meaning that these parameters should not absorb other effects
and model deficiencies in the Precise Orbit Determination (POD)
process. The accelerometers of all geodetic satellites like
GRACE and GRACE-FO are affected by time dependent bias and scale
factors. Therefore a calibration of the data is indispensable. A
dynamic POD based physical accelerometer calibration is
developed for the complete GRACE and GRACE-FO missions. We
investigate different parametrization strategies and utilize
different observation data, as the accurate inter-satellite
ranging additionally to GPS orbit data. For the estimation
parameters we distinguish between offset and scale, furthermore,
cross-track and radial directions are significantly less
sensitive than along-track and require a different evaluation.
For the offset, constant and time dependent parameters are
investigated. Furthermore, a continuous offset calibration over
arc boundaries is implemented and tested. The sensitivity of the
scale factor is lower, although, in contrast to the offset, it
increases with higher total accelerations. This means that it
needs to be estimated over longer time periods. We investigate
periods between three hours and one month as well as results
from Gravity Field Recovery (GFR). Monthly scale factors give
valuable results, at least for x-axis and when the Solar
activity is not very low. Nevertheless, we also estimate
weighted constant scale factors from the monthly results and use
these in a subsequent POD, giving more realistic offset results
for most periods and cross-track and radial directions. From the
used background models in the POD, Earth's gravitational model
has a noticeable influence on the estimated calibration
parameters, especially the scale factors. We utilized several
different models. Results with monthly ITSG solutions are
distinctly better than the ones with the time dependent GOCO06s
model. We show that the validation with usual metrics, like
post-fit POD residuals, is not able to reflect the quality of
the different estimated calibration parameters. For a
quantitative validation we introduce an approach based on the
modeled non-gravitational accelerations. Therefore, the
uncertainty of the models is evaluated first. The influence of
main error sources in the models is assessed and propagated to
the results. We compare our scale parameters to available
references and the complete calibration to TU Delft's latest
results. Finally we show the effect of different calibration
options on the retrieved density. The estimated calibration
parameters and non-gravitational accelerations for the whole
GRACE and GRACE-FO missions are available on our data server
www.zarm.uni-bremen.de/zarm\_daten.}",
doi = {10.1016/j.asr.2024.09.021},
adsurl = {https://ui.adsabs.harvard.edu/abs/2024AdSpR..74.4517W},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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