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Analysis of The Itsg-Grace Daily Models in The Determination of Polar Motion Excitation Function Cover

Analysis of The Itsg-Grace Daily Models in The Determination of Polar Motion Excitation Function

Open Access
|Oct 2023

Figures & Tables

Figure 1.

Methodology flowchart, which shows all the calculation steps
Methodology flowchart, which shows all the calculation steps

Figure 2.

Comparison of the (a) χ1 and (b) χ2 components of nonseasonal series of GAO, HAM + SLAM, and HAM obtained from ITSG 2016 and ITSG 2018
Comparison of the (a) χ1 and (b) χ2 components of nonseasonal series of GAO, HAM + SLAM, and HAM obtained from ITSG 2016 and ITSG 2018

Figure 3.

Comparison of (a) χ1 and (b) χ2 amplitude spectra series of GAO, HAM + SLAM, and HAM obtained from ITSG 2016 and ITSG 2018 from 20 to 120 days
Comparison of (a) χ1 and (b) χ2 amplitude spectra series of GAO, HAM + SLAM, and HAM obtained from ITSG 2016 and ITSG 2018 from 20 to 120 days

Figure 4.

Comparison of (a) χ1 and (b) χ2 amplitude spectra series of GAO, HAM + SLAM, and HAM obtained from ITSG 2016 and ITSG 2018 from 2 to 20 days
Comparison of (a) χ1 and (b) χ2 amplitude spectra series of GAO, HAM + SLAM, and HAM obtained from ITSG 2016 and ITSG 2018 from 2 to 20 days

Figure 5.

RMSEs of ITSG 2016-based series, ITSG 2018-based series, and HAM + SLAM calculated using GAO as the reference series. The exact RMSE values are given above the bars for each series.
RMSEs of ITSG 2016-based series, ITSG 2018-based series, and HAM + SLAM calculated using GAO as the reference series. The exact RMSE values are given above the bars for each series.

Figure 6.

Varexp of ITSG 2016-based series, ITSG 2018-based series, and HAM + SLAM calculated using GAO as the reference series. The exact explained variance values are given above the bars for each series.
Varexp of ITSG 2016-based series, ITSG 2018-based series, and HAM + SLAM calculated using GAO as the reference series. The exact explained variance values are given above the bars for each series.

Figure 7.

Correlations between ITSG 2016-based series, ITSG 2018-based series, GAO, and HAM + SLAM in (a) χ1 and (b) χ2
Correlations between ITSG 2016-based series, ITSG 2018-based series, GAO, and HAM + SLAM in (a) χ1 and (b) χ2

Figure A1.

Comparison of (a) χ1 and (b) χ2 amplitude spectra series of HAM + SLAM and HAM obtained from ITSG 2016 and ITSG 2018 from 2 to 120 days
Comparison of (a) χ1 and (b) χ2 amplitude spectra series of HAM + SLAM and HAM obtained from ITSG 2016 and ITSG 2018 from 2 to 120 days

Figure A2.

Comparison of (a) χ1 and (b) χ2 amplitude spectra series of HAM + SLAM and HAM obtained from ITSG 2016 and ITSG 2018 from 2 to 20 days
Comparison of (a) χ1 and (b) χ2 amplitude spectra series of HAM + SLAM and HAM obtained from ITSG 2016 and ITSG 2018 from 2 to 20 days

Models used to produce the ITSG 2016 and ITSG 2018 series

ITSG 2016ITSG 2018
Earth rotationIERS 2010IERS 2010
Moon, sun, and planets ephemeridesJPL DE421JPL DE421
Earth tideIERS 2010IERS 2010
Ocean tideEOT11aFES2014b, co-estimated
Pole tideIERS 2010 (constant mean pole)IERS 2010 (linear mean pole)
Ocean pole tideDesai 2004 (IERS 2010)Desai 2004 (IERS 2010, linear mean pole)
Atmospheric tides (S1, S2)van Dam, Ray (2010)AOD1B RL06
Atmosphere and ocean dealiasingAOD1B RL05AOD1B RL06
Relativistic correctionsIERS 2010IERS 2010
Permanent tidal deformationIncluded (zero tide)Included (zero tide)

Correlation coefficients between GAO and ITSG-based HAM series computed from ITSG 2016, ITSG 2018, ITSG 2016 with changed AOD1B data (AOD1B RL06 instead of RL05), and ITSG 2018 with changed AOD1B data (AOD1B RL05 instead of RL06)

ITSG 2016ITSG 2016 RL06ITSG 2018ITSG 2018 RL05
χ10.350.310.350.32
χ20.510.300.410.56

Comparison of STD, min, and max values from χ1 and χ2 nonseasonal series of GAO, HAM + SLAM, and HAM obtained from ITSG 2016 and ITSG 2018

STD [mas]Min [mas]Max [mas]
Seriesχ1χ2χ1χ2χ1χ2
ITSG 20165.487.28−15.91−23.1519.4624.25
ITSG 20183.905.05−12.04−14.1114.0317.84
GAO13.7121.76−67.01−76.1842.9076.10
HAM + SLAM1.992.24−6.65−7.386.687.18
DOI: https://doi.org/10.2478/arsa-2023-0008 | Journal eISSN: 2083-6104 | Journal ISSN: 1509-3859
Language: English
Page range: 105 - 121
Submitted on: Mar 13, 2023
Accepted on: Jul 10, 2023
Published on: Oct 10, 2023
Published by: Polish Academy of Sciences, Space Research Centre
In partnership with: Paradigm Publishing Services
Publication frequency: 4 issues per year

© 2023 Aleksander Partyka, Jolanta Nastula, Justyna Śliwińska, Tomasz Kur, Malgorzata Wińska, published by Polish Academy of Sciences, Space Research Centre
This work is licensed under the Creative Commons Attribution 4.0 License.