In-Orbit Performance of the GRACE Accelerometers and Microwave Ranging Instrument

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

Autoren

  • Michael Murböck
  • Petro Abrykosov
  • Christoph Dahle
  • Markus Hauk
  • Roland Pail
  • Frank Flechtner

Organisationseinheiten

Externe Organisationen

  • Technische Universität Berlin
  • Technische Universität München (TUM)
  • Helmholtz-Zentrum Potsdam Deutsches GeoForschungsZentrum (GFZ)
  • Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR)
  • Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut)
Forschungs-netzwerk anzeigen

Details

OriginalspracheEnglisch
Aufsatznummer563
FachzeitschriftRemote sensing
Jahrgang15
Ausgabenummer3
PublikationsstatusVeröffentlicht - 17 Jan. 2023

Abstract

The Gravity Recovery and Climate Experiment (GRACE) satellite mission has provided global long-term observations of mass transport in the Earth system with applications in numerous geophysical fields. In this paper, we targeted the in-orbit performance of the GRACE key instruments, the ACCelerometers (ACC) and the MicroWave ranging Instrument (MWI). For the ACC data, we followed a transplant approach analyzing the residual accelerations from transplanted accelerations of one of the two satellites to the other. For the MWI data, we analyzed the post-fit residuals of the monthly GFZ GRACE RL06 solutions with a focus on stationarity. Based on the analyses for the two test years 2007 and 2014, we derived stochastic models for the two instruments and a combined ACC+MWI stochastic model. While all three ACC axes showed worse performance than their preflight specifications, in 2007, a better ACC performance than in 2014 was observed by a factor of 3.6 due to switched-off satellite thermal control. The GRACE MWI noise showed white noise behavior for frequencies above 10 mHz around the level of (Formula presented.). In the combined ACC+MWI noise model, the ACC part dominated the frequencies below 10 mHz, while the MWI part dominated above 10 mHz. We applied the combined ACC+MWI stochastic models for 2007 and 2014 to the monthly GFZ GRACE RL06 processing. This improved the formal errors and resulted in a comparable noise level of the estimated gravity field parameters. Furthermore, the need for co-estimating empirical parameters was reduced.

ASJC Scopus Sachgebiete

Zitieren

In-Orbit Performance of the GRACE Accelerometers and Microwave Ranging Instrument. / Murböck, Michael; Abrykosov, Petro; Dahle, Christoph et al.
in: Remote sensing, Jahrgang 15, Nr. 3, 563, 17.01.2023.

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

Murböck, M, Abrykosov, P, Dahle, C, Hauk, M, Pail, R & Flechtner, F 2023, 'In-Orbit Performance of the GRACE Accelerometers and Microwave Ranging Instrument', Remote sensing, Jg. 15, Nr. 3, 563. https://doi.org/10.3390/rs15030563
Murböck, M., Abrykosov, P., Dahle, C., Hauk, M., Pail, R., & Flechtner, F. (2023). In-Orbit Performance of the GRACE Accelerometers and Microwave Ranging Instrument. Remote sensing, 15(3), Artikel 563. https://doi.org/10.3390/rs15030563
Murböck M, Abrykosov P, Dahle C, Hauk M, Pail R, Flechtner F. In-Orbit Performance of the GRACE Accelerometers and Microwave Ranging Instrument. Remote sensing. 2023 Jan 17;15(3):563. doi: 10.3390/rs15030563
Murböck, Michael ; Abrykosov, Petro ; Dahle, Christoph et al. / In-Orbit Performance of the GRACE Accelerometers and Microwave Ranging Instrument. in: Remote sensing. 2023 ; Jahrgang 15, Nr. 3.
Download
@article{eb32151f9809490c8dfa02a925ec1f9b,
title = "In-Orbit Performance of the GRACE Accelerometers and Microwave Ranging Instrument",
abstract = "The Gravity Recovery and Climate Experiment (GRACE) satellite mission has provided global long-term observations of mass transport in the Earth system with applications in numerous geophysical fields. In this paper, we targeted the in-orbit performance of the GRACE key instruments, the ACCelerometers (ACC) and the MicroWave ranging Instrument (MWI). For the ACC data, we followed a transplant approach analyzing the residual accelerations from transplanted accelerations of one of the two satellites to the other. For the MWI data, we analyzed the post-fit residuals of the monthly GFZ GRACE RL06 solutions with a focus on stationarity. Based on the analyses for the two test years 2007 and 2014, we derived stochastic models for the two instruments and a combined ACC+MWI stochastic model. While all three ACC axes showed worse performance than their preflight specifications, in 2007, a better ACC performance than in 2014 was observed by a factor of 3.6 due to switched-off satellite thermal control. The GRACE MWI noise showed white noise behavior for frequencies above 10 mHz around the level of (Formula presented.). In the combined ACC+MWI noise model, the ACC part dominated the frequencies below 10 mHz, while the MWI part dominated above 10 mHz. We applied the combined ACC+MWI stochastic models for 2007 and 2014 to the monthly GFZ GRACE RL06 processing. This improved the formal errors and resulted in a comparable noise level of the estimated gravity field parameters. Furthermore, the need for co-estimating empirical parameters was reduced.",
keywords = "accelerometer transplant, empirical parameters, GRACE, microwave ranging instrument post-fit residuals, monthly gravity field determination, stochastic modeling",
author = "Michael Murb{\"o}ck and Petro Abrykosov and Christoph Dahle and Markus Hauk and Roland Pail and Frank Flechtner",
note = "Funding Information: This work is funded by the Deutsche Forschungsgemeinschaft (DFG) within the research unit New Refined Observations of Climate Change from Spaceborne Gravity Missions (NEROGRAV, DFG Research Unit 2736). The mentioned aspects of future research are part of the second phase of this research unit. ",
year = "2023",
month = jan,
day = "17",
doi = "10.3390/rs15030563",
language = "English",
volume = "15",
journal = "Remote sensing",
issn = "2072-4292",
publisher = "Multidisciplinary Digital Publishing Institute",
number = "3",

}

Download

TY - JOUR

T1 - In-Orbit Performance of the GRACE Accelerometers and Microwave Ranging Instrument

AU - Murböck, Michael

AU - Abrykosov, Petro

AU - Dahle, Christoph

AU - Hauk, Markus

AU - Pail, Roland

AU - Flechtner, Frank

N1 - Funding Information: This work is funded by the Deutsche Forschungsgemeinschaft (DFG) within the research unit New Refined Observations of Climate Change from Spaceborne Gravity Missions (NEROGRAV, DFG Research Unit 2736). The mentioned aspects of future research are part of the second phase of this research unit.

PY - 2023/1/17

Y1 - 2023/1/17

N2 - The Gravity Recovery and Climate Experiment (GRACE) satellite mission has provided global long-term observations of mass transport in the Earth system with applications in numerous geophysical fields. In this paper, we targeted the in-orbit performance of the GRACE key instruments, the ACCelerometers (ACC) and the MicroWave ranging Instrument (MWI). For the ACC data, we followed a transplant approach analyzing the residual accelerations from transplanted accelerations of one of the two satellites to the other. For the MWI data, we analyzed the post-fit residuals of the monthly GFZ GRACE RL06 solutions with a focus on stationarity. Based on the analyses for the two test years 2007 and 2014, we derived stochastic models for the two instruments and a combined ACC+MWI stochastic model. While all three ACC axes showed worse performance than their preflight specifications, in 2007, a better ACC performance than in 2014 was observed by a factor of 3.6 due to switched-off satellite thermal control. The GRACE MWI noise showed white noise behavior for frequencies above 10 mHz around the level of (Formula presented.). In the combined ACC+MWI noise model, the ACC part dominated the frequencies below 10 mHz, while the MWI part dominated above 10 mHz. We applied the combined ACC+MWI stochastic models for 2007 and 2014 to the monthly GFZ GRACE RL06 processing. This improved the formal errors and resulted in a comparable noise level of the estimated gravity field parameters. Furthermore, the need for co-estimating empirical parameters was reduced.

AB - The Gravity Recovery and Climate Experiment (GRACE) satellite mission has provided global long-term observations of mass transport in the Earth system with applications in numerous geophysical fields. In this paper, we targeted the in-orbit performance of the GRACE key instruments, the ACCelerometers (ACC) and the MicroWave ranging Instrument (MWI). For the ACC data, we followed a transplant approach analyzing the residual accelerations from transplanted accelerations of one of the two satellites to the other. For the MWI data, we analyzed the post-fit residuals of the monthly GFZ GRACE RL06 solutions with a focus on stationarity. Based on the analyses for the two test years 2007 and 2014, we derived stochastic models for the two instruments and a combined ACC+MWI stochastic model. While all three ACC axes showed worse performance than their preflight specifications, in 2007, a better ACC performance than in 2014 was observed by a factor of 3.6 due to switched-off satellite thermal control. The GRACE MWI noise showed white noise behavior for frequencies above 10 mHz around the level of (Formula presented.). In the combined ACC+MWI noise model, the ACC part dominated the frequencies below 10 mHz, while the MWI part dominated above 10 mHz. We applied the combined ACC+MWI stochastic models for 2007 and 2014 to the monthly GFZ GRACE RL06 processing. This improved the formal errors and resulted in a comparable noise level of the estimated gravity field parameters. Furthermore, the need for co-estimating empirical parameters was reduced.

KW - accelerometer transplant

KW - empirical parameters

KW - GRACE

KW - microwave ranging instrument post-fit residuals

KW - monthly gravity field determination

KW - stochastic modeling

UR - http://www.scopus.com/inward/record.url?scp=85147858024&partnerID=8YFLogxK

U2 - 10.3390/rs15030563

DO - 10.3390/rs15030563

M3 - Article

AN - SCOPUS:85147858024

VL - 15

JO - Remote sensing

JF - Remote sensing

SN - 2072-4292

IS - 3

M1 - 563

ER -