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Published January 19, 2023 | Published
Journal Article Open

Morphodynamic Preservation of Fluvial Channel Belts

  • 1. ROR icon California Institute of Technology
  • 2. ROR icon Colorado School of Mines

Abstract

The fluvial sedimentary record is largely composed of deposits from relatively common flow events, rather than more catastrophic scour-and-fill events. At the scales of bedforms, such deposits are preserved within the stratigraphic record because they rapidly accumulate within, and are protected by, morphodynamic topographic depressions that occur naturally in the fluvial system as a result of feedbacks between flow, sediment transport, and topography. Examples include the preservation of ripples in front of dunes, dunes in front of bars, and bars within channels. Here, we used 3D seismic data that images preserved channel belts to test the hypothesis that alluvial-ridge basins, morphodynamic depressions formed between raised channel beds due to decreasing sedimentation rates away from channels in alluvial settings, are a source of topography driving channel-belt-scale preservation. Using the 3D seismic data, we measured the stratigraphic positions of channel belts, as well as their lengths, widths, sinuosities, and centerline orientations in the 3D seismic dataset. Results are consistent with well-preserved channel belts steered by alluvial-ridge-basin topography. Further, the thickness of the channel-belt interval exceeds the relief of any one alluvial-ridge basin, suggesting the volume records the filling of multiple alluvial-ridge basins and that the process is common. Characterizing the stratigraphic signature of alluvial-ridge basins is necessary for understanding contrasting fluvial architectures where external forcings prevented their formation.

Copyright and License

This is an open-access article distribute d under the terms of the Creative Commons Attribution 4.0 International License (CC-BY4.0).

Acknowledgement

We thank Editor Jenn Pickering for handling our manuscript, and Tian Dong and an anonymous reviewer for their helpful comments. We thank Jay Dickson at Caltech's Bruce Murray Lab for Planetary Visualization for technical support (http://murray-lab.caltech.edu/). We acknowledge Schlumberger for providing Petrel licenses to Caltech and Penn State, and the USGS for maintaining the NAMSS. Eric Prokocki is thanked for helpful discussions early in the preparation of this manuscript. Tables with belt edge and centerline coordinates, geometric measurements, python scripts used for analysis, and the seismic volume in numpy formation are available for download (Cardenas, 2022). Cardenas was funded by National Science Foundation Earth Sciences Postdoctoral Fellowship #2052912.

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Additional details

Created:
December 7, 2023
Modified:
December 7, 2023