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dc.contributor.authorKarakostas, F.
dc.contributor.authorRakoto, V.
dc.contributor.authorLognonne, P.
dc.contributor.authorLarmat, C.
dc.contributor.authorDaubar, I.
dc.contributor.authorMiljković, Katarina
dc.identifier.citationKarakostas, F. and Rakoto, V. and Lognonne, P. and Larmat, C. and Daubar, I. and Miljkovic, K. 2018. Inversion of Meteor Rayleigh Waves on Earth and Modeling of Air Coupled Rayleigh Waves on Mars. Space Science Reviews. 214 (8): 127.

Meteor impacts and/or meteor events generate body and surface seismic waves on the surface of a planet. When meteoroids burst in the atmosphere, they generate shock waves that subsequently convert into acoustic waves in the atmosphere and seismic waves in the ground. This effect can be modeled as the amplitude of Rayleigh and other Spheroidal modes excitation, due to atmospheric/ground coupling effects. First, an inversion of the seismic source of Chelyabinsk superbolide is performed. We develop an approach in order to model a line source in the atmosphere, corresponding to the consecutive generation of shock waves by the interaction with the atmosphere. The model is based on the known trajectory. We calculate the synthetic seismograms of Rayleigh waves associated with the event by the summation of normal modes of a model of the solid part and the atmosphere of the planet. Through an inversion technique based on singular value decomposition, we perform a full Rayleigh wave inversion and we provide solutions for the moment magnitude. SEIS will likely detect seismic waves generated by impacts and the later might be further located by remote sensing differential processing. In the case of Mars, we use the same method to obtain waveforms associated with impacts on the planetary surface or in low altitudes in the Martian atmosphere. We show that the contribution of the fundamental spheroidal solid mode is dominating the waveforms, compared to that of the first two overtones. We perform an amplitude comparison and we show that small impactors (diameter of 0.5 to 2 m), can be detected by the SEIS VBB seismometer of InSight mission, even in short epicentral distances, in the higher frequencies of the Rayleigh waves. We perform an analysis based on impact rate estimations and we calculate the number of detectable events of 1 meter diameter meteor impacts to be 6.7 to 13.4 per 1 Martian year for a Q= 500.

dc.publisherSpringer Nature
dc.subjectScience & Technology
dc.subjectPhysical Sciences
dc.subjectAstronomy & Astrophysics
dc.subjectRayleigh waves
dc.subjectMeteor impacts
dc.subjectNormal modes
dc.titleInversion of Meteor Rayleigh Waves on Earth and Modeling of Air Coupled Rayleigh Waves on Mars
dc.typeJournal Article
dcterms.source.titleSpace Science Reviews

This is a post-peer-review, pre-copyedit version of an article published in Space Science Reviews. The final authenticated version is available online at:

curtin.departmentSchool of Earth and Planetary Sciences (EPS)
curtin.accessStatusOpen access
curtin.facultyFaculty of Science and Engineering
curtin.contributor.orcidMiljković, Katarina [0000-0001-8644-8903]
curtin.contributor.researcheridMiljković, Katarina [D-4844-2013]
curtin.contributor.scopusauthoridMiljković, Katarina [35219281700]

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