Triple-Pair Constellation Configurations for Temporal Gravity Field Retrieval

The goal of next-generation gravity missions (NGGM) is to improve the monitoring of mass transport in the Earth system by an increased space-time sampling capability as well as higher accuracies of a new generation of instrumentation, but also to continue the monitoring time series obtained by past...

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Main Authors: Anna F. Purkhauser, Roland Pail
Format: Article
Language:English
Published: MDPI AG 2020-03-01
Series:Remote Sensing
Subjects:
Online Access:https://www.mdpi.com/2072-4292/12/5/831
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spelling doaj-4d70414bc7b843cb82dcb952be9c9e5a2020-11-25T02:09:30ZengMDPI AGRemote Sensing2072-42922020-03-0112583110.3390/rs12050831rs12050831Triple-Pair Constellation Configurations for Temporal Gravity Field RetrievalAnna F. Purkhauser0Roland Pail1Chair of Astronomical and Physical Geodesy, Technical University of Munich, Arcisstraße 21, 80333 Munich, GermanyChair of Astronomical and Physical Geodesy, Technical University of Munich, Arcisstraße 21, 80333 Munich, GermanyThe goal of next-generation gravity missions (NGGM) is to improve the monitoring of mass transport in the Earth system by an increased space-time sampling capability as well as higher accuracies of a new generation of instrumentation, but also to continue the monitoring time series obtained by past and current missions such as GRACE and GRACE Follow-On. As the likelihood of three satellite pairs being simultaneously in orbit in the mid-term future increased, we have performed a closed-loop simulation to investigate the impact of a third pair in either polar or inclined orbit as an addition to a Bender-type constellation with NGGM instrumentation. For the additional pair, GRACE-like as well as NGGM instrumentation was tested. The analysis showed that the third pair mainly increases the redundancy of the monitoring system but does not significantly improve de-aliasing capabilities. The best-performing triple-pair scenario comprises a third inclined pair with NGGM sensors. Starting with a Bender-type constellation of a polar and an inclined satellite pair, simulation results indicate an average improvement of 11% in case of adding the third pair in a near-polar orbit, and of 21% for the third pair placed in an inclined orbit. The most important advantage of a multi-pair constellation, however, is the possibility to recover daily gravity fields with higher spatial resolution. In the case of the investigated triple-pair scenarios, a meaningful daily resolution with a maximum spherical harmonic degree of 26 can be achieved, while a higher daily parametrization up to degree 40 results in spatial aliasing and thus would need additional constraints or prior information.https://www.mdpi.com/2072-4292/12/5/831future gravity missionstime variable gravitynear-real timenumerical simulationspherical harmonics
collection DOAJ
language English
format Article
sources DOAJ
author Anna F. Purkhauser
Roland Pail
spellingShingle Anna F. Purkhauser
Roland Pail
Triple-Pair Constellation Configurations for Temporal Gravity Field Retrieval
Remote Sensing
future gravity missions
time variable gravity
near-real time
numerical simulation
spherical harmonics
author_facet Anna F. Purkhauser
Roland Pail
author_sort Anna F. Purkhauser
title Triple-Pair Constellation Configurations for Temporal Gravity Field Retrieval
title_short Triple-Pair Constellation Configurations for Temporal Gravity Field Retrieval
title_full Triple-Pair Constellation Configurations for Temporal Gravity Field Retrieval
title_fullStr Triple-Pair Constellation Configurations for Temporal Gravity Field Retrieval
title_full_unstemmed Triple-Pair Constellation Configurations for Temporal Gravity Field Retrieval
title_sort triple-pair constellation configurations for temporal gravity field retrieval
publisher MDPI AG
series Remote Sensing
issn 2072-4292
publishDate 2020-03-01
description The goal of next-generation gravity missions (NGGM) is to improve the monitoring of mass transport in the Earth system by an increased space-time sampling capability as well as higher accuracies of a new generation of instrumentation, but also to continue the monitoring time series obtained by past and current missions such as GRACE and GRACE Follow-On. As the likelihood of three satellite pairs being simultaneously in orbit in the mid-term future increased, we have performed a closed-loop simulation to investigate the impact of a third pair in either polar or inclined orbit as an addition to a Bender-type constellation with NGGM instrumentation. For the additional pair, GRACE-like as well as NGGM instrumentation was tested. The analysis showed that the third pair mainly increases the redundancy of the monitoring system but does not significantly improve de-aliasing capabilities. The best-performing triple-pair scenario comprises a third inclined pair with NGGM sensors. Starting with a Bender-type constellation of a polar and an inclined satellite pair, simulation results indicate an average improvement of 11% in case of adding the third pair in a near-polar orbit, and of 21% for the third pair placed in an inclined orbit. The most important advantage of a multi-pair constellation, however, is the possibility to recover daily gravity fields with higher spatial resolution. In the case of the investigated triple-pair scenarios, a meaningful daily resolution with a maximum spherical harmonic degree of 26 can be achieved, while a higher daily parametrization up to degree 40 results in spatial aliasing and thus would need additional constraints or prior information.
topic future gravity missions
time variable gravity
near-real time
numerical simulation
spherical harmonics
url https://www.mdpi.com/2072-4292/12/5/831
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