Least squares restoration of tertiary thrust sheets in map view, Tajik depression, central Asia

Research areas:

• Environnement, Paléo-Environnement et Bio-Indicateurs (2011 - 2016)

Year:

1997

Authors:

• Olivier Bourgeois
• PR Cobbold
• D Rouby
• JC Thomas
• V Shein

Journal:

JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH

Volume:

102

Number:

B12

Pages:

27553-27573

Month:

DEC 10

ISSN:

0148-0227

BibTex:

@article{WOS:A1997YL14500020, author = "Olivier Bourgeois and PR Cobbold and D Rouby and JC Thomas and V Shein", abstract = "The Tajik depression, located west of the Pamirs and south of the Tien Shan, is a compressional intermontane basin, bounded by basement overthrusts and filled with Mesozoic and Cenozoic sediments. The internal structure is typical of a thin-skinned fold and thrust belt. Kinematic data available in the literature suggest that indentation of the Pamirs into Asia during the Cenozoic collision of India and Asia has been accommodated in various ways within the depression, including westward extrusion, thickening combined with wrenching along N-S folds and thrusts, and counterclockwise rotations. These various deformation processes can be analyzed and quantified by reconstruction of the predeformed state of the depression. However, the combination ol thrusting, wrenching and block rotations implies a nonplane deformation: which cannot be restored propel ly using balanced cross sections alone. We have therefore developed a numerical method for restoration of stratigraphic surfaces, designed for regions of nonplane compressional tectonics. The deformed region is represented in map view as a mosaic of fault-bounded blocks, overlapping each other along the faults. Blocks are separately unfolded and then numerically packed together by least squares minimization of overlaps, yielding fields of finite horizontal translations and rotations about vertical axes. To analyze the deformation postdating the collision of India and Asia, we have restored a stratigraphic surface at the base of the Cenozoic. First, in order to test the numerical method, we restored a map that had previously been restored by a purely manual method. Restoration of a second map, drawn from newly available subsurface data; leads to geometrical inconsistencies: overlaps and gaps, which cannot be reduced, remain in the restored slate. After-correction of these inconsistencies, restoration yields a complex mode of deformation for the depression. Individual thrust slices have undergone counter-clockwise rotations about vertical axes, the magnitudies increasing from west to east, up to a maximum of 40 degrees neat the Pamirs. Horizontal shortening is 150 km (35\%) in the center of the depression and 240 km (85\%) in the northeastern part, between the Pamirs and the Tien Shan. Strike slip motions, commonly not revealed by balancing cross sections, are associated with thrusting on faults striking N-S. Independent paleomagnetic data and slip directions on small-scale faults pl provide positive checks on the results of our restoration.", doi = "10.1029/97JB02477", extra = "PICL", issn = "0148-0227", journal = "JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH", month = "DEC 10", number = "B12", pages = "27553-27573", title = "{L}east squares restoration of tertiary thrust sheets in map view, {T}ajik depression, central {A}sia", volume = "102", year = "1997", }

Abstract:

The Tajik depression, located west of the Pamirs and south of the Tien
Shan, is a compressional intermontane basin, bounded by basement
overthrusts and filled with Mesozoic and Cenozoic sediments. The
internal structure is typical of a thin-skinned fold and thrust belt.
Kinematic data available in the literature suggest that indentation of
the Pamirs into Asia during the Cenozoic collision of India and Asia has
been accommodated in various ways within the depression, including
westward extrusion, thickening combined with wrenching along N-S folds
and thrusts, and counterclockwise rotations. These various deformation
processes can be analyzed and quantified by reconstruction of the
predeformed state of the depression. However, the combination ol
thrusting, wrenching and block rotations implies a nonplane deformation:
which cannot be restored propel ly using balanced cross sections alone.
We have therefore developed a numerical method for restoration of
stratigraphic surfaces, designed for regions of nonplane compressional
tectonics. The deformed region is represented in map view as a mosaic of
fault-bounded blocks, overlapping each other along the faults. Blocks
are separately unfolded and then numerically packed together by least
squares minimization of overlaps, yielding fields of finite horizontal
translations and rotations about vertical axes. To analyze the
deformation postdating the collision of India and Asia, we have restored
a stratigraphic surface at the base of the Cenozoic. First, in order to
test the numerical method, we restored a map that had previously been
restored by a purely manual method. Restoration of a second map, drawn
from newly available subsurface data; leads to geometrical
inconsistencies: overlaps and gaps, which cannot be reduced, remain in
the restored slate. After-correction of these inconsistencies,
restoration yields a complex mode of deformation for the depression.
Individual thrust slices have undergone counter-clockwise rotations
about vertical axes, the magnitudies increasing from west to east, up to
a maximum of 40 degrees neat the Pamirs. Horizontal shortening is 150 km
(35\%) in the center of the depression and 240 km (85\%) in the
northeastern part, between the Pamirs and the Tien Shan. Strike slip
motions, commonly not revealed by balancing cross sections, are
associated with thrusting on faults striking N-S. Independent
paleomagnetic data and slip directions on small-scale faults pl provide
positive checks on the results of our restoration.