Lowe sequence

Layers S1-S3 in a high-density turbidite exposed near Talara, Peru.

The Lowe sequence describes a set of sedimentary structures in turbidite sandstone beds that are deposited by high-density turbidity currents. It is intended to complement, not replace, the better known Bouma sequence, which applies primarily to turbidites deposited by low-density (i.e., low-sand concentration) turbidity currents.

Description

The Lowe sequence adds three layers labelled S1 through S3 to Bouma's terminology, with S1 being at the bottom and S3 at the top of a sandy turbidite bed. As with the Bouma sequence, each layer has a specific set of sedimentary structures and lithology. And like the Bouma sequence, the layers become finer grained from bottom to top.[1][2]

The layers are described as follows.[2]

As previously mentioned, the Lowe sequence is intended to complement, not replace the Bouma sequence. Fine-grained turbidites resulting from low-density turbidity currents, in which the Bouma A through Bouma E terminology applies, are referred to in the Lowe classification as Ta through Te, in which the T acronym derives from "Traction". By contrast, because the S1-S3 terminology describes sand-rich turbidites deposited by high-density turbidity currents, the S acronym derives from "Sandstone". Lastly, R1-R3, which uses the same descriptive criteria as S1-S3, applies to conglomerates, wherein the R acronym derives from "Rubble". In practice, the S1-S3 terminology is widely used, Ta-Te, is used sometimes, and R1-R3 is seldom used.

Processes

Initially grains, pebbles and large clasts in a high-density turbidity current (i.e., a high-sand concentration flow), are moved by traction (rolling and sliding) to generate a coarse-grained to conglomeratic, parallel-laminated to cross-laminated S1 layer. However, as grains settle out and move closer together, grain-to-grain collisions begin to generate dispersive pressures that help prevent further settling. This results in smaller grains moving between larger grains and preferentially settling out beneath them. Thus, an inverse graded layer develops that is called a traction carpet, since it is thought to move as a single unit. At some point, the grains move close enough together that collisions no longer generate enough energy to keep the grains in suspension, and the entire layer freezes to create an S2 layer. This process can then repeat to create additional traction carpets.[2]

When grains move closer together and settle out, the water between them is displaced so that it can move upward into the flow, helping to keep grains above the traction carpets in suspension. Because the flow is in motion, this upward movement of fluid quickly becomes turbulent. When the energy of the flow drops low enough that it can no longer sustain turbulence, then the entire flow freezes to create the massive to normally graded S3 layer. Subsequent reworking of the top of this new deposit by overlying remnant currents, or by new currents unrelated to the original flow can create laminations that resemble the Bouma B layer. When reworking stops, suspension settling may deposit massive mudstone (Bouma E) directly on top of the laminated layer. Alternatively, if new sediment is introduced during this reworking phase, or if sediment is sufficiently remobilized and transported, then a more complete Bouma sequence may develop on top of the S3 layer.[2]

References

  1. Bouma, Arnold H. (1962). Sedimentology of some Flysch deposits: A graphic approach to facies interpretation. Elsevier. p. 168.
  2. 1 2 3 4 Lowe, D.R. (1982). "Sediment gravity flows: II. Depositional models with special reference to the deposits of high-density turbidity currents". Journal of Sedimentology, Society of Economic Paleontologists and Mineralogists: v. 52, p. 279–297.

See also

This article is issued from Wikipedia - version of the Monday, January 05, 2015. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.