AIUB-GRACE gravity field solutions for G3P: processing strategies and instrument parameterization
<p>This paper discusses strategies to improve the Gravity Recovery And Climate Experiment (GRACE) monthly solutions computed at the Astronomical Institute of the University of Bern (AIUB) which are contributing to the Horizon 2020 project G3P – Global Gravity-based Groundwater Product. To impr...
| Main Authors: | , , , , |
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| Format: | Article |
| Language: | English |
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Copernicus Publications
2024-03-01
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| Series: | Earth System Science Data |
| Online Access: | https://essd.copernicus.org/articles/16/1589/2024/essd-16-1589-2024.pdf |
| _version_ | 1797246107419410432 |
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| author | N. Darbeheshti M. Lasser U. Meyer D. Arnold A. Jäggi |
| author_facet | N. Darbeheshti M. Lasser U. Meyer D. Arnold A. Jäggi |
| author_sort | N. Darbeheshti |
| collection | DOAJ |
| description | <p>This paper discusses strategies to improve the Gravity Recovery And Climate Experiment (GRACE) monthly solutions computed at the Astronomical Institute of the University of Bern (AIUB) which are contributing to the Horizon 2020 project G3P – Global Gravity-based Groundwater Product. To improve the AIUB-GRACE gravity field solutions, we updated the use of the Level-1B observations, adapted the background models, and improved the processing strategies in terms of instrument screening and parameterization. We used the Release 3 K-band product (KBR) and star camera data (L1B RL03), and we adopted Release 6 of the Atmospheric and Ocean De-aliasing (AOD1B RL06) product. For the accelerometer parameterization, we used arc-wise full scale factor matrix and arc-wise third-order polynomial biases. The new accelerometer parameterization is effective in reducing noise over the oceans in gravity field solutions, especially for the late years of the GRACE mission when the thermal control was switched off. In this paper, we show that the outliers in the KBR antenna offset correction (AOC) are projected into the range rate residuals; therefore, we used the KBR AOC as the main source for outlier detection and eliminated the AOC above a threshold for all data before the gravity field processing. The full time series of GRACE AIUB-G3P gravity field solutions (Darbeheshti et al., 2023b) is available at <a href="https://doi.org/10.5880/ICGEM.2023.001">https://doi.org/10.5880/ICGEM.2023.001</a>.</p> |
| first_indexed | 2024-04-24T19:37:32Z |
| format | Article |
| id | doaj.art-6fe18e74561a4551ba59cbf291fe4698 |
| institution | Directory Open Access Journal |
| issn | 1866-3508 1866-3516 |
| language | English |
| last_indexed | 2024-04-24T19:37:32Z |
| publishDate | 2024-03-01 |
| publisher | Copernicus Publications |
| record_format | Article |
| series | Earth System Science Data |
| spelling | doaj.art-6fe18e74561a4551ba59cbf291fe46982024-03-25T12:05:18ZengCopernicus PublicationsEarth System Science Data1866-35081866-35162024-03-01161589159910.5194/essd-16-1589-2024AIUB-GRACE gravity field solutions for G3P: processing strategies and instrument parameterizationN. DarbeheshtiM. LasserU. MeyerD. ArnoldA. Jäggi<p>This paper discusses strategies to improve the Gravity Recovery And Climate Experiment (GRACE) monthly solutions computed at the Astronomical Institute of the University of Bern (AIUB) which are contributing to the Horizon 2020 project G3P – Global Gravity-based Groundwater Product. To improve the AIUB-GRACE gravity field solutions, we updated the use of the Level-1B observations, adapted the background models, and improved the processing strategies in terms of instrument screening and parameterization. We used the Release 3 K-band product (KBR) and star camera data (L1B RL03), and we adopted Release 6 of the Atmospheric and Ocean De-aliasing (AOD1B RL06) product. For the accelerometer parameterization, we used arc-wise full scale factor matrix and arc-wise third-order polynomial biases. The new accelerometer parameterization is effective in reducing noise over the oceans in gravity field solutions, especially for the late years of the GRACE mission when the thermal control was switched off. In this paper, we show that the outliers in the KBR antenna offset correction (AOC) are projected into the range rate residuals; therefore, we used the KBR AOC as the main source for outlier detection and eliminated the AOC above a threshold for all data before the gravity field processing. The full time series of GRACE AIUB-G3P gravity field solutions (Darbeheshti et al., 2023b) is available at <a href="https://doi.org/10.5880/ICGEM.2023.001">https://doi.org/10.5880/ICGEM.2023.001</a>.</p>https://essd.copernicus.org/articles/16/1589/2024/essd-16-1589-2024.pdf |
| spellingShingle | N. Darbeheshti M. Lasser U. Meyer D. Arnold A. Jäggi AIUB-GRACE gravity field solutions for G3P: processing strategies and instrument parameterization Earth System Science Data |
| title | AIUB-GRACE gravity field solutions for G3P: processing strategies and instrument parameterization |
| title_full | AIUB-GRACE gravity field solutions for G3P: processing strategies and instrument parameterization |
| title_fullStr | AIUB-GRACE gravity field solutions for G3P: processing strategies and instrument parameterization |
| title_full_unstemmed | AIUB-GRACE gravity field solutions for G3P: processing strategies and instrument parameterization |
| title_short | AIUB-GRACE gravity field solutions for G3P: processing strategies and instrument parameterization |
| title_sort | aiub grace gravity field solutions for g3p processing strategies and instrument parameterization |
| url | https://essd.copernicus.org/articles/16/1589/2024/essd-16-1589-2024.pdf |
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