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Deformation Bands

Deformation bands are thin, tabular bands of localized deformation (Figure 1), also referred to as Luders bands or granulation seams in earlier literature. Following Aydin (1978) we will use the former because it includes a wider variety of structures; Luders bands are thought to have no shear offset and granulation is associated with only certain types of bands. Single deformation bands are about a few mm to a few cm thick, and their lengths rarely exceed one hundred meters. See 'Geometry, Statistics, and Scaling of Deformation Bands' and under the link, 'Properties of Deformation Bands.' The strain accommodated by single deformation bands is also relatively small. In spite of such small dimensions and small strain magnitude, even single deformation bands are easily recognized in the field, thanks to their commonly positive relief and the color difference between band materials and the surrounding parent rock.

Diagram showing deformation bands with three basic kinematic types: predominantly shear, compactive, and dilatant, each of which is illustrated by a pair of arrows.Figure 1. Diagram showing deformation bands with three basic kinematic types: predominantly shear, compactive, and dilatant, each of which is illustrated by a pair of arrows.

Recent studies have documented a rich variability in their overall kinematics (Aydin et al., 2006, Fossen et al., 2007). Among these are shear bands and volumetric bands, which can also be divided into compaction bands and dilation bands (see various kinematics represented by a pair of arrows in Figure 1). The first type mentioned above has predominantly shear deformation across which the sense of motion is primarily parallel to the overall structure, while the last two are structures with predominantly volumetric deformation across which the sense of motion is towards or away from the structures. However, these appear to be the end members of deformation bands of a broad kinematic spectrum as mentioned above. For example, shear bands with compaction or dilation commonly occur, as do volumetric bands with some component of shear.

Deformation bands are known to occur in a wide variety of natural and man-made materials. Deformation bands in steels and aluminum alloys have been known for a long time in the engineering literature. Figure 2 shows adiabatic shear bands in aluminum alloy from Leach (1985). Figure 3(a) shows a sheet of polycarbonate hexagonal honeycombs of 0.0057 inches thick subjected to axial compression in both laboratory and numerical experiments by Papka and Kyriakides (1998). Predominantly compactive deformation bands were formed by collapsing of cells of honeycombs (Figure 3b). One of the least expected materials to have deformation bands is ice on the basis of its highly brittle nature in common familiar environments on earth. Yet, satellite images of the surface of Jupiter's icy moon, Europa, display astonishing arrays of lineaments (http://galileo.jpl.nasa.gov), some of which have been interpreted as faults (Kattenhorn, 2004) and deformation bands (Aydin, 2006). Figure 4 is a satellite image showing the Androgeos Linea (the diagonal lineament from upper right to lower left) and the surrounding features from the Bright Plains area of Europa. Some of these lineaments including the Androgeos Linea were proposed to be deformation bands produced by the transformation of one form of crystalline structure of ice to another (Aydin, 2006).

Adiabatic shear bands in aluminum alloy. From Leach (1985). Note the scale bar on the bottom left.Figure 2. Adiabatic shear bands in aluminum alloy. From Leach (1985). Note the scale bar on the bottom left.
A sheet of poly carbonate hexagonal honeycombs of a thickness of 0.0057 inches subjected to uniaxial compression (a) in both laboratory and numerical experiments producing collapsed strings of honeycomb cells (b) as localized deformation of predominantly compactive nature. From Papka and Kyriakides (1998).Figure 3. A sheet of poly carbonate hexagonal honeycombs of a thickness of 0.0057 inches subjected to uniaxial compression (a) in both laboratory and numerical experiments producing collapsed strings of honeycomb cells (b) as localized deformation of predominantly compactive nature. From Papka and Kyriakides (1998).
Satellite image of the Bright Plains area of Jupiter's moon Europa showing astonishing arrays of lineaments, some of which have been interpreted as faults (Kattenhorn, 2004) and deformation bands (Aydin, 2006). The image focuses on the Androgeos Linea which crosses the image from lower left to upper right. From Aydin (2006) and http://galileo.jpl.nasa.gov.Figure 4. Satellite image of the Bright Plains area of Jupiter's moon Europa showing astonishing arrays of lineaments, some of which have been interpreted as faults (Kattenhorn, 2004) and deformation bands (Aydin, 2006). The image focuses on the Androgeos Linea which crosses the image from lower left to upper right. From Aydin (2006) and http://galileo.jpl.nasa.gov.

Loose sand grains (Viggiani et al., 2008) and poorly consolidated sediments (Cashman and Cashman, 2000; Aydin et al., 2006) including mud (Karig and Lundberg, 1990), carbonate grain stones (Tondi et al., 2006), and sandstones of various types (for example aeolian sandstone in Figure 5) make up a wide spectrum of granular materials in which deformation bands have been known to occur. These will be described in details later in this Knowledgebase.

Network of deformation bands as ribs in Aztec Sandstone exposed at Valley of Fire State Park, southeast Nevada. Jian Zhong in the background is for scale.Figure 5. Network of deformation bands as ribs in Aztec Sandstone exposed at Valley of Fire State Park, southeast Nevada. Jian Zhong in the background is for scale.
Types of Deformation Bands:
Volumetric BandsShear Bands
Splay Deformation BandsEchelon Deformation BandsComposite Deformation Bands
Hybrid Deformation Bands
Reference:

Aydin, A., Borja, R., Eichhubl, P., 2006. Geological and mathematical framework for failure modes in granular rock. Journal of Structural Geology 28 (1): 83-98.

Aydin, A., 2006. Failure modes of the lineaments on Jupiter's moon, Europa: Implications for the evolution of its icy crust. Journal of Structural Geology 28: 2222-2236, doi:10.1016/j.jsg.2006.08.003.

Cashman, S., Cashman, K., 2000. Cataclasis and deformation-band formation in unconsolidated marine terrace sand, Humboldt County, California. Geology 28: 111-114.

Fossen, H., Schultz, R.A., Shipton, Z.K., Mair, K., 2007. Deformation bands in sandstone: a review. Journal of the Geological Society 164: 755-769.

Karig, D.E., Lundberg, N., 1990. Deformation bands from the toe of the Nankai accretionary prism. Journal of Geophysical Research 95: doi: 10.1029/89JB01389.

Kattenhorn, S., 2004. Strike-slip fault evolution on Europa: evidence from tailcrack geometries. Icarus 172, 582-602. doi:10.1016/j.

Leach, P.W., 1985. Observation of adiabatic shear band formation in 7039 Aluminum alloy. Metallurgical Transections A 16A: 1900-1903.

Papka, S.D., Kyriakides, S., 1998. Experiments and Full-Scale Numerical Simulations of In-Plane Crushing of a Honeycomb. Acta Materialia 46(8): 2765-2776,​ ​http://dx.doi.org/10.1016/S1359-6454(97)00453-9.

Tondi, E., Antonellini, M., Aydin, A., Marchegiani, L., Cello, G., 2006. The role of deformation bands, stylolites and sheared stylolites in fault development in carbonate grainstones of Majella Mountain, Italy. Journal of Structural Geology 28 (3): 376-391.

Viggiani, G., Kuntz, M., Desrues, J., 2008. An experimental investigation of the relationships between grain size distribution and shear banding in sand, 111-127: In: P.A. Vermeer, S. Diebels, W. Ehlers, H.J. Herrmann, S. Luding, E. Ramm (Eds.), Continuous and Discontinuous Modelling of Cohesive-Frictional Materials. Springer, 310p.



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