TY - JOUR
T1 - Seismic velocity structure of the upper inner core in the north polar region
AU - Ohtaki, Toshiki
AU - Tanaka, Satoru
AU - Kaneshima, Satoshi
AU - Siripunvaraporn, Weerachai
AU - Boonchaisuk, Songkhun
AU - Noisagool, Sutthipong
AU - Kawai, Kenji
AU - Kim, Taewoon
AU - Suzuki, Yuki
AU - Ishihara, Yasushi
AU - Miyakawa, Koji
AU - Takeuchi, Nozomu
N1 - Funding Information:
We are grateful to all involved with TSAR in Thailand for their assistance and to K. Yokoyama at the Earthquake Research Institute of the University of Tokyo for operating and maintaining the TSAR data center. We also thank T. Tsuchiya and S. Takehiro for helpful discussions and R. Iritani for providing their models. Constructive comments by two anonymous reviewers improved this paper. We used the Generic Mapping Tools (GMT) (Wessel and Smith, 1998) to make figures, the TauP Toolkit (Crotwell et al. 1999) to calculate raypaths, the Seismic Analysis Code (SAC) (Goldstein et al. 2003) to process data and make figures, and the Direct Solution Method (DSM) (Takeuchi et al. 1996) to calculate synthetic waveforms. Data at the surrounding broadband stations used in this study were collected from networks GE, IC, IU, MM, RM, and TM via the Data Management Center of IRIS (Incorporated Research Institutions for Seismology, http://ds.iris.edu/). Data were also collected from F-net by the National Research Institute for Earth Science and Disaster Resilience, Japan (NIED) (DOI:10.17598/nied.0005, http://www.fnet.bosai.go.jp/). This research was supported by JSPS KAKENHI (grant JP15H05832). We thank Esther Posner, PhD, from Liwen Bianji, Edanz Editing China (www.liwenbianji.cn/ac), for editing the English text of a draft of this manuscript.
Funding Information:
We are grateful to all involved with TSAR in Thailand for their assistance and to K. Yokoyama at the Earthquake Research Institute of the University of Tokyo for operating and maintaining the TSAR data center. We also thank T. Tsuchiya and S. Takehiro for helpful discussions and R. Iritani for providing their models. Constructive comments by two anonymous reviewers improved this paper. We used the Generic Mapping Tools (GMT) ( Wessel and Smith, 1998 ) to make figures, the TauP Toolkit ( Crotwell et al., 1999 ) to calculate raypaths, the Seismic Analysis Code (SAC) ( Goldstein et al., 2003 ) to process data and make figures, and the Direct Solution Method (DSM) ( Takeuchi et al., 1996 ) to calculate synthetic waveforms. Data at the surrounding broadband stations used in this study were collected from networks GE, IC, IU, MM, RM, and TM via the Data Management Center of IRIS (Incorporated Research Institutions for Seismology, http://ds.iris.edu/ ). Data were also collected from F-net by the National Research Institute for Earth Science and Disaster Resilience, Japan (NIED) (DOI: 10.17598/nied.0005 , http://www.fnet.bosai.go.jp/ ). This research was supported by JSPS KAKENHI (grant JP15H05832 ). We thank Esther Posner, PhD, from Liwen Bianji, Edanz Editing China ( www.liwenbianji.cn/ac ), for editing the English text of a draft of this manuscript.
Publisher Copyright:
© 2020 Elsevier B.V.
PY - 2021/2
Y1 - 2021/2
N2 - The Earth's upper inner core has a quasi-hemispherical velocity structure. One of the two quasi-hemispheres has a high-velocity region centered beneath Southeast Asia and is referred to as “East”. The remaining low-velocity region is referred to as “West”. The boundary positions between the quasi-hemispheres are rather scattered but well estimated at low- and mid-latitudes, whereas discrepancies between seismological hemisphere models increase at high latitudes. However, the boundary position at high latitudes is important when considering the origin of the quasi hemisphericity. Recent deployment of a temporary broadband seismic array in Thailand (Thai Seismic Array; TSAR) provides a means to analyze the inner core structure in the north polar region because rays from Central American earthquakes to the network are transmitted through the inner core and have their turning points approximately 150–400 km beneath the north polar region of the inner core boundary. We measured the differential traveltimes of earthquake waveforms between a seismic phase transmitted through the inner core (PKIKP, DF) and a phase that turns in the lower outer core (PKPbc, BC). The observed differential times are approximately 0.2–0.3 s smaller than theoretical estimates predicted by the Preliminary Reference Earth Model (PREM) over the observed distance range and 0.3–0.5 s smaller than those of AK135 at larger distances, which suggests lower velocities in the analyzed region of the upper inner core. Our analyses show that models with velocities ~0.03 km/s lower than those of PREM in the upper 300 km of the inner core, with a velocity about midway between PREM and AK135 in the F layer, sufficiently fit the observed differential times. This low-velocity feature in the upper inner core is characteristic of the “West”. The observations are also largely explained by the model obtained for the structure beneath the northeast Pacific in mid-latitudes classified as “West”. Our previous study also shows that the south polar region of the upper inner core has “West” characteristics. Our results thus suggest that the north and south polar regions of the upper inner core have a “West” structure and that the Earth's upper inner core has an eyeball-shaped high-velocity anomaly called the “East”. The shape of the hemispheric boundary is possibly an ellipse shortened in the north-south direction rather than a circle.
AB - The Earth's upper inner core has a quasi-hemispherical velocity structure. One of the two quasi-hemispheres has a high-velocity region centered beneath Southeast Asia and is referred to as “East”. The remaining low-velocity region is referred to as “West”. The boundary positions between the quasi-hemispheres are rather scattered but well estimated at low- and mid-latitudes, whereas discrepancies between seismological hemisphere models increase at high latitudes. However, the boundary position at high latitudes is important when considering the origin of the quasi hemisphericity. Recent deployment of a temporary broadband seismic array in Thailand (Thai Seismic Array; TSAR) provides a means to analyze the inner core structure in the north polar region because rays from Central American earthquakes to the network are transmitted through the inner core and have their turning points approximately 150–400 km beneath the north polar region of the inner core boundary. We measured the differential traveltimes of earthquake waveforms between a seismic phase transmitted through the inner core (PKIKP, DF) and a phase that turns in the lower outer core (PKPbc, BC). The observed differential times are approximately 0.2–0.3 s smaller than theoretical estimates predicted by the Preliminary Reference Earth Model (PREM) over the observed distance range and 0.3–0.5 s smaller than those of AK135 at larger distances, which suggests lower velocities in the analyzed region of the upper inner core. Our analyses show that models with velocities ~0.03 km/s lower than those of PREM in the upper 300 km of the inner core, with a velocity about midway between PREM and AK135 in the F layer, sufficiently fit the observed differential times. This low-velocity feature in the upper inner core is characteristic of the “West”. The observations are also largely explained by the model obtained for the structure beneath the northeast Pacific in mid-latitudes classified as “West”. Our previous study also shows that the south polar region of the upper inner core has “West” characteristics. Our results thus suggest that the north and south polar regions of the upper inner core have a “West” structure and that the Earth's upper inner core has an eyeball-shaped high-velocity anomaly called the “East”. The shape of the hemispheric boundary is possibly an ellipse shortened in the north-south direction rather than a circle.
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U2 - 10.1016/j.pepi.2020.106636
DO - 10.1016/j.pepi.2020.106636
M3 - Article
AN - SCOPUS:85099274334
SN - 0031-9201
VL - 311
JO - Physics of the Earth and Planetary Interiors
JF - Physics of the Earth and Planetary Interiors
M1 - 106636
ER -