On the inner-outer core density contrast from PKiKP/PcP amplitude ratios and uncertainties caused by seismic noise
| dc.contributor.author | Tkalčić, Hrvoje | en |
| dc.contributor.author | Kennett, Brian L.N. | en |
| dc.contributor.author | Cormier, Vernon F. | en |
| dc.date.accessioned | 2025-03-17T02:34:50Z | |
| dc.date.available | 2025-03-17T02:34:50Z | |
| dc.date.issued | 2009 | en |
| dc.description.abstract | The inner core boundary (ICB) of the earth is characterized by a discontinuous change in elastic properties between the liquid outer and solid inner core. In the ray theory approximation, a measure of the density contrast at the ICB is given by the amplitude ratio of P waves reflected from the core-mantle boundary (CMB; PcP waves) and the ICB (PKiKP waves), since that ratio conveniently appears in an explicit form in the transmission/reflection coefficient equations. The results for inner-outer core density contrast derived from direct amplitude picks of these waves in the time domain have varied significantly among different authors.The transmission/reflection coefficients on the liquid-solid and solid-liquid boundaries derived from ground displacements enable a direct comparison between the amplitude measurements on displacement seismograms in the time domain and theoretical values. A new approach is proposed and applied to integrate effects of microseismic and signal-generated noise with the amplitude measurements, thus providing a direct maximal uncertainty measure. To suppress the effects of varying radiation pattern and distinctively different ray paths at longer epicentral distances, this new method was applied to high-quality arrivals of PcP and PKiKP waves from a nuclear explosion observed at epicentral distances 10°-20° from recording stations. The resulting uncertainties are high precluding precise estimates of the ICB density contrast, but provide a robust estimate of an upper bound from body waves of about 1100 kg m-3. Median values of two amplitude ratios observed around 17° epicentral distance indicate a small density contrast of 200-300 kg m-3 and suggest the existence of zones of suppressed density contrast between the inner and the outer core, a density contrast stronger than 5000 kg m-3 at the CMB, or a combination of both. | en |
| dc.description.status | true | en |
| dc.format.extent | 19 | en |
| dc.identifier.other | researchoutputwizard:u9503261xPUB306 | en |
| dc.identifier.other | Scopus:70349979952 | en |
| dc.identifier.other | WOS:269736600031 | en |
| dc.identifier.uri | https://dspace-test.anu.edu.au/handle/1885/733720135 | |
| dc.identifier.url | http://www.scopus.com/inward/record.url?scp=70349979952&partnerID=8YFLogxK | en |
| dc.language.iso | English | en |
| dc.source | Geophysical Journal International | en |
| dc.subject | Body waves | en |
| dc.subject | Composition of the core | en |
| dc.subject | Time-series analysis | en |
| dc.subject | Wave propagation | en |
| dc.title | On the inner-outer core density contrast from PKiKP/PcP amplitude ratios and uncertainties caused by seismic noise | en |
| dc.type | Article | en |
| local.bibliographicCitation.lastpage | 443 | en |
| local.bibliographicCitation.startpage | 425 | en |
| local.contributor.affiliation | Tkalčić, Hrvoje; RSES Salaries, Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National University | en |
| local.contributor.affiliation | Kennett, Brian L.N.; RSES Salaries, Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National University | en |
| local.contributor.affiliation | Cormier, Vernon F.; University of Connecticut | en |
| local.identifier.citationvolume | 179 | en |
| local.identifier.doi | 10.1111/j.1365-246X.2009.04294.x | en |
| local.identifier.pure | b4f4e887-aa5a-4460-934c-b89ba1fd93dc | en |
| local.type.status | Published | en |