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Teleseismic Pn arrivals: Influence of mantle velocity gradient and crustal scattering

  • L. Nielsen
  • , H. Thybo
  • , I.B. Morozov
  • , S.B. Smithson
  • , L. Solodilov

Research output: Contribution to journalArticleResearchpeer-review

18 Citations (Scopus)

Abstract

Teleseismic Pn phases with a long, high-amplitude coda, are observed to offsets >3000 km along the Peaceful Nuclear Explosion seismic profiles Quartz and Ruby. For the high-frequency (>5 Hz) part of the Quartz data, which is shown here, coda lengths of more than 10 s can be visually observed in the seismic sections. We interpret the teleseismic Pn arrivals as multiple sub-Moho refractions (whispering-gallery phases), which travel over large distances due to a positive upper-mantle velocity gradient. The coda of these arrivals is explained by lower crustal scattering of the whispering-gallery phases from the mantle. The modelling is based on calculation of reflectivity and 2-D visco-elastic finite-difference synthetic seismograms. Our models are in agreement with other deep seismic data from continental areas, which typically show a reflective lower crust and an almost transparent uppermost mantle. The lower crustal heterogeneity is described by von Karman distribution with a standard deviation of 0.5 km s-1 for the P-wave velocity and correlation lengths of 2.4 km (horizontally) and 0.6 km (vertically). The positive vertical upper-mantle velocity gradient of ∼0.004 km s-1 km-1, which is characteristic for profile Quartz, forms a waveguide which gives rise to the teleseismic Pn. It is not necessary to include upper-mantle heterogeneity in order to explain the characteristics of this arrival.

Original languageEnglish
Pages (from-to)F1-F7
Number of pages7
JournalGeophysical Journal International
Volume152
Issue number2
DOIs
Publication statusPublished - Feb 2003
Externally publishedYes

Keywords

  • Crust
  • Nuclear explosions
  • Refraction seismology
  • Scattering
  • Seismic-wave propagation
  • Upper-mantle

Programme Area

  • Programme Area 3: Energy Resources

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