GOCE-Derived Coseismic Gravity Gradient Changes Caused by the 2011 Tohoku-Oki Earthquake

In contrast to most of the coseismic gravity change studies, which are generally based on data from the Gravity field Recovery and Climate Experiment (GRACE) satellite mission, we use observations from the Gravity field and steady-state Ocean Circulation Explorer (GOCE) Satellite Gravity Gradient (S...

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Main Authors: Xinyu Xu, Hao Ding, Yongqi Zhao, Jin Li, Minzhang Hu
Format: Article
Language:English
Published: MDPI AG 2019-05-01
Series:Remote Sensing
Subjects:
Online Access:https://www.mdpi.com/2072-4292/11/11/1295
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spelling doaj-42de0eb2d6284536a1fe31953edcef502020-11-25T01:12:18ZengMDPI AGRemote Sensing2072-42922019-05-011111129510.3390/rs11111295rs11111295GOCE-Derived Coseismic Gravity Gradient Changes Caused by the 2011 Tohoku-Oki EarthquakeXinyu Xu0Hao Ding1Yongqi Zhao2Jin Li3Minzhang Hu4School of Geodesy and Geomatics, Wuhan University, Wuhan 430079, ChinaSchool of Geodesy and Geomatics, Wuhan University, Wuhan 430079, ChinaSchool of Geodesy and Geomatics, Wuhan University, Wuhan 430079, ChinaShanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, ChinaKey Laboratory of Earthquake Geodesy, Institute of Seismology, China Earthquake Administration, 40 Hongshan Celu, Wuhan 430071, ChinaIn contrast to most of the coseismic gravity change studies, which are generally based on data from the Gravity field Recovery and Climate Experiment (GRACE) satellite mission, we use observations from the Gravity field and steady-state Ocean Circulation Explorer (GOCE) Satellite Gravity Gradient (SGG) mission to estimate the coseismic gravity and gravity gradient changes caused by the 2011 Tohoku-Oki Mw 9.0 earthquake. We first construct two global gravity field models up to degree and order 220, before and after the earthquake, based on the least-squares method, with a bandpass Auto Regression Moving Average (ARMA) filter applied to the SGG data along the orbit. In addition, to reduce the influences of colored noise in the SGG data and the polar gap problem on the recovered model, we propose a tailored spherical harmonic (TSH) approach, which only uses the spherical harmonic (SH) coefficients with the degree range 30&#8722;95 to compute the coseismic gravity changes in the spatial domain. Then, both the results from the GOCE observations and the GRACE temporal gravity field models (with the same TSH degrees and orders) are simultaneously compared with the forward-modeled signals that are estimated based on the fault slip model of the earthquake event. Although there are considerable misfits between GOCE-derived and modeled gravity gradient changes (&#916;<i>V<sub>xx</sub></i>, &#916;<i>V<sub>yy</sub></i>, &#916;<i>V<sub>zz</sub></i>, and &#916;<i>V<sub>xz</sub></i>), we find analogous spatial patterns and a significant change (greater than 3<i>&#963;</i>) in gravity gradients before and after the earthquake. Moreover, we estimate the radial gravity gradient changes from the GOCE-derived monthly time-variable gravity field models before and after the earthquake, whose amplitudes are at a level over three times that of their corresponding uncertainties, and are thus significant. Additionally, the results show that the recovered coseismic gravity signals in the west-to-east direction from GOCE are closer to the modeled signals than those from GRACE in the TSH degree range 30&#8722;95. This indicates that the GOCE-derived gravity models might be used as additional observations to infer/explain some time-variable geophysical signals of interest.https://www.mdpi.com/2072-4292/11/11/1295coseismic gravity gradient changesgravity field modelGOCEGRACE
collection DOAJ
language English
format Article
sources DOAJ
author Xinyu Xu
Hao Ding
Yongqi Zhao
Jin Li
Minzhang Hu
spellingShingle Xinyu Xu
Hao Ding
Yongqi Zhao
Jin Li
Minzhang Hu
GOCE-Derived Coseismic Gravity Gradient Changes Caused by the 2011 Tohoku-Oki Earthquake
Remote Sensing
coseismic gravity gradient changes
gravity field model
GOCE
GRACE
author_facet Xinyu Xu
Hao Ding
Yongqi Zhao
Jin Li
Minzhang Hu
author_sort Xinyu Xu
title GOCE-Derived Coseismic Gravity Gradient Changes Caused by the 2011 Tohoku-Oki Earthquake
title_short GOCE-Derived Coseismic Gravity Gradient Changes Caused by the 2011 Tohoku-Oki Earthquake
title_full GOCE-Derived Coseismic Gravity Gradient Changes Caused by the 2011 Tohoku-Oki Earthquake
title_fullStr GOCE-Derived Coseismic Gravity Gradient Changes Caused by the 2011 Tohoku-Oki Earthquake
title_full_unstemmed GOCE-Derived Coseismic Gravity Gradient Changes Caused by the 2011 Tohoku-Oki Earthquake
title_sort goce-derived coseismic gravity gradient changes caused by the 2011 tohoku-oki earthquake
publisher MDPI AG
series Remote Sensing
issn 2072-4292
publishDate 2019-05-01
description In contrast to most of the coseismic gravity change studies, which are generally based on data from the Gravity field Recovery and Climate Experiment (GRACE) satellite mission, we use observations from the Gravity field and steady-state Ocean Circulation Explorer (GOCE) Satellite Gravity Gradient (SGG) mission to estimate the coseismic gravity and gravity gradient changes caused by the 2011 Tohoku-Oki Mw 9.0 earthquake. We first construct two global gravity field models up to degree and order 220, before and after the earthquake, based on the least-squares method, with a bandpass Auto Regression Moving Average (ARMA) filter applied to the SGG data along the orbit. In addition, to reduce the influences of colored noise in the SGG data and the polar gap problem on the recovered model, we propose a tailored spherical harmonic (TSH) approach, which only uses the spherical harmonic (SH) coefficients with the degree range 30&#8722;95 to compute the coseismic gravity changes in the spatial domain. Then, both the results from the GOCE observations and the GRACE temporal gravity field models (with the same TSH degrees and orders) are simultaneously compared with the forward-modeled signals that are estimated based on the fault slip model of the earthquake event. Although there are considerable misfits between GOCE-derived and modeled gravity gradient changes (&#916;<i>V<sub>xx</sub></i>, &#916;<i>V<sub>yy</sub></i>, &#916;<i>V<sub>zz</sub></i>, and &#916;<i>V<sub>xz</sub></i>), we find analogous spatial patterns and a significant change (greater than 3<i>&#963;</i>) in gravity gradients before and after the earthquake. Moreover, we estimate the radial gravity gradient changes from the GOCE-derived monthly time-variable gravity field models before and after the earthquake, whose amplitudes are at a level over three times that of their corresponding uncertainties, and are thus significant. Additionally, the results show that the recovered coseismic gravity signals in the west-to-east direction from GOCE are closer to the modeled signals than those from GRACE in the TSH degree range 30&#8722;95. This indicates that the GOCE-derived gravity models might be used as additional observations to infer/explain some time-variable geophysical signals of interest.
topic coseismic gravity gradient changes
gravity field model
GOCE
GRACE
url https://www.mdpi.com/2072-4292/11/11/1295
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