Signal Apparition
date
Dec 31, 2021
slug
10050
status
Published
tags
SeismicExploration
summary
type
Post

以传统三震源为例,
一源按照
(..., 1, 1, 1, 1, 1, 1, ...)
激发,周期为1二源按照
(..., 1, A, 1, A, 1, A, ...)
激发,周期为2三源按照
(..., 1, 1, A, 1, 1, A, ...)
激发,周期为3“Wavefield signal apparition” is a new method to sample time-discrete signals that allows for the separation of interfering signals from multiple sources. The theory of wavefield signal apparition is discussed in detail in a companion paper (Robertsson et al., 2016, submitted to EAGE). Essentially, by changing a well-sampled conventional source sequence
(…,1,1,1,1,1,…)
, where the wavefield in the spectral fk-domain is present in a cone around the spatial wavenumber 𝑘 = 0, to the source sequence (…,1,A,1,A,1,…)
where A is any function independent of spatial positions, the wavefield in the spectral 𝑓𝑘-domain will be present in two cones: one around 𝑘 = 0 and the other around the Nyquist wavenumber . Then, in simultaneous shooting, where the combined source sequences (…,1,1,1,1,1,…)
and (…,1,A,1,A,1,…)
are used, the data from the (…,1,A,1,A,1,…)
sequence will be solely apparent and isolated in the cone around the Nyquist wavenumber. The data from the two source sequences thus can be separated in the fk-domain.
A 25Hz Ricker wavelet is used to simulate data at a receiver station. The data are acquired sufficiently densely to avoid spatial aliasing according to the geometry shown in Figure 1. The simultaneous source data with the apex to the left were generated by source ‘A’ shooting regularly (with source sequence
(…,1,1,1,1,1,…)
). The data with the apex to the right were generated by source ‘B’ shooting with the periodic sequence (…,1,A,1,A,1,…)
where A represents a time delay: ; we have selected T=10ms which gives on every second recording a somewhat “fuzzy” appearance of this part of the data. The data are transformed to the fk-domain, where the data generated from source ‘B’ are solely present in the cone around the Nyquist number . These data are isolated and properly scaled (with a function depending on the function A) before inverse Fourier transforming the source ‘B’ data to time-space domain. Here, they are subtracted from the originally acquired simultaneous source data, recovering the source ‘A’ data. As seen in Figure 1, the result is excellent and, apart from limited numerical artifacts at the top and bottom (related to windowing of data before the temporal Fourier transform), no signal leakage from source ‘B’ is visible.
reference: Wavefield signal apparition, Part II: Applications