EGU21-13999, updated on 04 Mar 2021
https://doi.org/10.5194/egusphere-egu21-13999
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Determining OBS clock drift using ambient seismic noise 

David Naranjo1,2,3, Laura Parisi1, Philippe Jousset2, Cornelis Weemstra3,4, and Sigurjón Jónsson1
David Naranjo et al.
  • 1King Abdullah University of Science and Technology, Physical Science and Engineering Division, Thuwal, Saudi Arabia
  • 2Helmholtz Center Potsdam, GFZ German Research Centre for Geosciences, Germany
  • 3Department of Geoscience and Engineering, Delft University of Technology, Delft, The Netherlands
  • 4Royal Netherlands Meteorological Institute, De Bilt, The Netherlands

Accurate timing of seismic records is essential for almost all applications in seismology. Wrong timing of the waveforms may result in incorrect Earth models and/or inaccurate earthquake locations. As such, it may render interpretations of underground processes incorrect. Ocean bottom seismometers (OBSs) experience clock drifts due to their inability to synchronize with a GNSS signal (with the correct reference time), since electromagnetic signals are unable to propagate efficiently in water. As OBSs generally operate in relatively stable ambient temperature, the timing deviation is usually assumed to be linear. Therefore, the time corrections can be estimated through GPS synchronization before deployment and after recovery of the instrument. However, if the instrument has run out of power prior to recovery (i.e., due to the battery being dead at the time of recovery), the timing error at the end of the deployment cannot be determined. In addition, the drift may not be linear, e.g., due to rapid temperature drop while the OBS sinks to the seabed. Here we present an algorithm that recovers the linear clock drift, as well as a potential timing error at the onset.

The algorithm presented in this study exploits seismic interferometry (SI). Specifically, time-lapse (averaged) cross-correlations of ambient seismic noise are computed. As such, virtual-source responses, which are generally dominated by the recorded surface waves, are retrieved. These interferometric responses generate two virtual sources: a causal wave (arriving at a positive time) and an acausal wave (arriving at a negative time). Under favorable conditions, both interferometric responses approach the surface-wave part of the medium's Green's function. Therefore, it is possible to calculate the clock drift for each station by exploiting the time-symmetry between the causal and acausal waves. For this purpose, the clock drift is calculated by measuring the differential arrival times of the causal and acausal waves for a large number of receiver-receiver pairs and computing the drift by carrying-out a least-squares inversion. The methodology described is applied to time-lapse cross-correlations of ambient seismic noise recorded on and around the Reykjanes peninsula, SW Iceland. The stations used for the analysis were deployed in the context of IMAGE (Integrated Methods for Advanced Geothermal Exploration) and consisted of 30 on-land stations and 24 ocean bottom seismometers (OBSs).  The seismic activity was recorded from spring 2014 until August 2015 on an area of around 100 km in diameter (from the tip of the Reykjanes peninsula).

How to cite: Naranjo, D., Parisi, L., Jousset, P., Weemstra, C., and Jónsson, S.: Determining OBS clock drift using ambient seismic noise , EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-13999, https://doi.org/10.5194/egusphere-egu21-13999, 2021.

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