1887
2nd Australasian Exploration Geoscience Conference: Data to Discovery
  • ISSN: 2202-0586
  • E-ISSN:

Abstract

Summary

The signal-to-noise ratios (SNR) of the first arrivals are a function of the source-to-receiver distance and the head wave coefficient (HWC), the refraction analogue of the reflection coefficient. In turn, the precision of the first break traveltimes is a function of the SNR.

Stacking with the refraction convolution section (RCS) can significantly reduce the effects of geometrical spreading. However, the effects of the HWC still remain.

The time models of the base of the weathering computed with the common reciprocal method are comparable to those computed with the RCS. However, only the RCS is able to detect small thrusts within the Fresnel zone.

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/content/journals/10.1080/22020586.2019.12072942
2019-12-01
2026-01-14
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References

  1. Brown, A. R., 2011, Interpretation of three-dimensional seismic data; SEG Investigations in Geophysics, No. 9, 7th edition, Society of Exploration Geophysicists, Tulsa, 646p.
  2. Cox, M. J. G., 1999, Static corrections for seismic reflection surveys. Society of Exploration Geophysicists, Tulsa.
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  5. Palmer, D, 2001, Imaging refractors with the convolution section, Geophysics 66, 1582-1589.
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  7. Palmer, D., 2013, Resolving complex structure in near-surface refraction seismology with common offset gathers: The Leading Edge, 32, 680-690.
  8. Palmer, D., 2015a, Is accuracy more important than precision in near surface refraction seismology? Near Surface Geophysics, 13, 1-18.
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  • Article Type: Research Article
Keyword(s): first breaks; precision; RCS; signal-to-noise
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