EGU23-124, updated on 22 Feb 2023
https://doi.org/10.5194/egusphere-egu23-124
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

The impact of isolated noise sources on correlation wavefields

Sven Schippkus1, Roel Snieder2, Mahsa Safarkhani1, and Céline Hadziioannou1
Sven Schippkus et al.
  • 1Institute of Geophysics, Centre for Earth System Research and Sustainability (CEN), University of Hamburg, Hamburg, Germany (sven.schippkus@uni-hamburg.de)
  • 2Center for Wave Phenomena, Colorado School of Mines, Boulder, CO, USA

Seismic interferometry gives rise to a correlation wavefield that is closely related to the Green’s function under the condition of uniformly distributed noise sources. Asymmetric correlation wavefields result from the violation of this condition and are commonly observed in field data. In the presence of an additional isolated noise source a second contribution to the correlation wavefield is introduced that emerges from the isolated source location at negative lapse time. The two wavefield contributions interfere, resulting in biased surface wave dispersion measurements. Isolated noise sources that act continuously, such as machinery or ocean microseisms, further have significant impact on the coda of the correlation wavefield. The coda can be dominated by direct waves propagating from the isolated noise source, not by multiply scattered waves originating from the master station. This fundamentally challenges the current understanding of how velocity changes detected in the coda can be measured and interpreted.

How to cite: Schippkus, S., Snieder, R., Safarkhani, M., and Hadziioannou, C.: The impact of isolated noise sources on correlation wavefields, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-124, https://doi.org/10.5194/egusphere-egu23-124, 2023.