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oa Can full waveform refraction imaging overcome the century-long impasse at the first breaks?
- Australian Society of Exploration Geophysicists
- Source: ASEG Extended Abstracts, Volume 2019, Issue 2nd Australasian Exploration Geoscience Conference: Data to Discovery, Dec 2019, p. 1 - 4
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- 01 Dec 2019
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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