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Single-Station Back-Azimuth Determination with the Receiver Function Rotation Technique Validated by the Locations of Earthquakes, Impacts, and Explosions

dc.contributor.authorSun, Weijiaen
dc.contributor.authorTkalčić, Hrvojeen
dc.contributor.authorTang, Qingyaen
dc.date.accessioned2025-05-31T07:31:42Z
dc.date.available2025-05-31T07:31:42Z
dc.date.issued2024-06-10en
dc.description.abstractThe success of seismometer installations on the ocean floor, polar regions, remote continental areas, and even other planets’ surfaces has sparked renewed interest in determining the location via the azimuthal direction of a seismic event recorded by a single station, also known as the back azimuth (BAZ). However, classical algorithms for the BAZ estimate, like principal component and polarization analyses based on P-wave particle motions, are prone to ambiguities of 180°. Motivated by the sensor orientation correction techniques used for ocean-bottom seismometers and land stations for known event locations, we explore a receiver function rotation (RFR) method to determine the BAZ for events recorded by a single station. It is a parameter search over a range of horizontal component rotation angles from 0° to 360°. The fundamental feature of the method is that the direct P wave in the radial receiver function (RF) will have the maximum amplitude when the rotation from the ZNE system (vertical, north–south, and east–west) to ZRT (vertical, radial, and tangential) is aligned with the BAZ of the incoming P wave. Hence, the largest amplitude at zero time of the ensemble of RFs computed for different horizontal component rotations shows the optimal BAZ, which is consequently free of the 180° ambiguities. The technique’s performance is validated using the well-documented location of the 2017 Democratic People’s Republic of Korea nuclear explosion and over 1200 cataloged earthquakes on the two permanent stations in Australia. We further benchmark the RFR algorithm by the locations of two ground-truth Martian impact events documented by the orbital camera and recorded by InSight’s seismometer. Our method helps enhance the reliability of BAZ estimation as a complementary scheme to other methods. It can be used in remote areas on Earth and on the future missions to the Moon and other planets.en
dc.description.sponsorshipThe authors thank the editor and two anonymous reviewers for their valuable comments. The authors acknowledge NASA, Centre Nationale d\u2019Etudes Spatiale (French Space Agency [CNES]), their partner agencies, and institutions (United Kingdom Space Agency [UKSA], Swiss Space Office [SSO], Deutsches Zentrum f\u00FCr Luft- und Raumfahrt [German Aerospace Center, DLR], Jet Propulsion Laboratory [JPL], Institute de Physique du Globe de Paris-Centre National de la Recherche Scientifique [IPGP-CNRS], Eidgen\u00F6ssische Technische Hochschule Z\u00FCrich [ETHZ], Imperial College [IC], and Max Planck Institute for Solar System ResearchMax Planck Gesellschaft [MPS-MPG]), the flight operations team at JPL, SEIS on Mars Operations Center (SISMOC), Mars SEIS Data Service (MSDS), Incorporated Research Institutions for Seismology Data Management Center (IRIS-DMC), and Planetary Data Service (PDS) for providing Standard for the Exchange of Earthquake Data (SEED) The Seismic Experiment for Interior Structure (SEIS) data. This work is supported by the National Key R&D Program of China Grant Number 2022YFF0503203, Youth Innovation Promotion Association of Chinese Academy of Sciences (CAS), and State Key Laboratory of Lunar and Planetary Science, Macau University of Science and Technology Grant Number SKL-LPS(MUST)-2021-2023. Propulsion Laboratory [JPL], Institute de Physique du Globe de Paris-Centre National de la Recherche Scientifique [IPGP-CNRS], Eidgen\u00F6ssische Technische Hochschule Z\u00FCrich [ETHZ], Imperial College [IC], and Max Planck Institute for Solar System ResearchMax Planck Gesellschaft [MPS-MPG]), the flight operations team at JPL, SEIS on Mars Operations Center (SISMOC), Mars SEIS Data Service (MSDS), Incorporated Research Institutions for Seismology Data Management Center (IRIS-DMC), and Planetary Data Service (PDS) for providing Standard for the Exchange of Earthquake Data (SEED) The Seismic Experiment for Interior Structure (SEIS) data. This work is supported by the National Key R&D Program of China Grant Number 2022YFF0503203, Youth Innovation Promotion Association of Chinese Academy of Sciences (CAS), and State Key Laboratory of Lunar and Planetary Science, Macau University of Science and Technology Grant Number SKL-LPS(MUST)-2021-2023.en
dc.description.statusPeer-revieweden
dc.format.extent14en
dc.identifier.issn0895-0695en
dc.identifier.otherORCID:/0000-0001-7072-490X/work/183511747en
dc.identifier.scopus85205347581en
dc.identifier.urihttp://www.scopus.com/inward/record.url?scp=85205347581&partnerID=8YFLogxKen
dc.identifier.urihttps://hdl.handle.net/1885/733756235
dc.language.isoenen
dc.rightsPublisher Copyright: © Seismological Society of America.en
dc.sourceSeismological Research Lettersen
dc.titleSingle-Station Back-Azimuth Determination with the Receiver Function Rotation Technique Validated by the Locations of Earthquakes, Impacts, and Explosionsen
dc.typeJournal articleen
dspace.entity.typePublicationen
local.bibliographicCitation.lastpage2938en
local.bibliographicCitation.startpage2925en
local.contributor.affiliationSun, Weijia; CAS - Institute of Geology and Geophysicsen
local.contributor.affiliationTkalčić, Hrvoje; Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationTang, Qingya; CAS - Institute of Geology and Geophysicsen
local.identifier.citationvolume95en
local.identifier.doi10.1785/0220240117en
local.identifier.puref8e5aa32-ce79-46c9-acdf-4f163d707e57en
local.identifier.urlhttps://www.scopus.com/pages/publications/85205347581en
local.type.statusPublisheden

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