Balance

 

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Line-length and area-balance work with DepthCon2000

 

Let's look first at line-length checks for compressional structures. This of course is the standard method of drawing pins either side of the zone of interest and simply measuring the lengths of beds between those pins. 

Here's a depth-converted seismic section across the Burnt Timber Thrust, also in Alberta, with some of the eroded geology re-drawn, and a line-length balance has been made. (The Burnt Timber Thrust is the pale blue surface in centre of the image). Unfortunately the profile is not long enough to show the cut-off of the Turner Valley Formation (blue) in the footwall of the Burnt Timber Thrust, so we don't see the ramp which climbs through the carbonates and without that information we can't restore the fault at dark blue level. In the Mesozoics there has been substantial erosion to remove yellow and green line length and likewise restoration on those markers is not possible either. Nevertheless, to show how line-length balance might be attempted with this software, here is a template drawn between the two pins marked in red:

 

burnttimberdepthtemplate.jpg (229558 bytes)

 

This example is one of the download demo models, and is fully described in the program help and FAQ notes. We hope you'll be interested to try working with it. For line-length balance checks between pins, this is an excellent tool. Line segments are drawn in order from the fixed pin and define the pre-deformation fault pattern. If the line lengths are more or less correct, the fault trajectories will look sensible whereas if bed length is locally wrong, the sketched faults will assume impossible shapes. There is a large literature on this topic, see for example Boyer and Elliott (1982), Thrust Systems, AAPG 66 (9), 1196-1230, their Fig. 17 shows a template restoration of the Mount Crandell Thrust. DepthCon2000 is well able to handle that kind of job. 

 
Shear (Area-balanced) Restoration

Here are two examples of simple shear restorations using seismic:

Turner Valley

Returning to the Turner Valley model which we have depth converted we should need to see a much longer line than we have here, to comment usefully on plausible restoration.  Looking at the footwall, clearly there are a number of important ramps on which the structure has been displaced eastwards by significant amounts, and to build the fold we should have to go looking for a big ramp off-section well to the west. But we can do some local modelling, even though its out of sequence, to show that the pick of the pale blue backthrust of the pop-up is probably on the right lines:

Here is what happens when we draw it and slip the hangingwall rightwards some 400 metres:

 

TVRestore-1.jpg (133800 bytes)

 

And then a 600 metres leftwards move on the red fault, puts the pop-up back into its back limb position, with some local distortions of course which we could try to resolve if it was important to do so. To restore the right side of the pop-up, rejoin the blue to blue on this red fault:

 

TVRestore-2.jpg (134744 bytes)

 

Interestingly, the displacements on the pop-up margins are about the same order of magnitude, in a sense we can get rid of it by pulling a wedge of rock sideways out of the profile. Its reasonable to draw the red fault in the way we have, through the leftward part of the image: although the fault isn't clearly imaged on seismic the limb of the fold is pervasively cut by left-vergent slices; and the traces found by TraceInterpreter are consistent with what we've done.

And that leaves a relatively simple thrust fold with three or four major ramps in its footwall, on which the slips are probably a kilometre or so apiece, and the compensating backthrusts will be found climbing westwards above the structure, in the Cretaceous sequence. So I would interpret Turner Valley as being built in an intercutaneous wedge, and there's no need to model it as a fault-propagation fold.

 

A complex gas field:

Here's a restoration of a North Sea sequence including several salt/anhydrite horizons, extended by Cretaceous faulting and inverted during regional Alpine compression. The strong event is a carbonate, folded and then axially ruptured so that the limbs are overlapping. Between the two "T" shaped rafts of dolomite the Rotliegendes reservoir is thrusted rightwards onto the carbonates, the normal stratigraphic sequence is seen just to the left of this thrust juxtaposition.

 

raftrestore1.jpg (115410 bytes)

 

We can restore this, firstly by rejoining the severed ends of the carbonate using the pale blue fault, and at the same time removing the Rotliegendes from the end of the raft; then slipping back to the left on the dark blue fault to unfold the right-hand end of the profile:

 

raftrestore2.jpg (122189 bytes)

 

and then we can see the old extensional surface (orange) which separates the Rotliegendes blocks, and on restoring this we can sketch the top of the Rotliegendes in yellow, solving the correlation problem. This is a difficult license to review, without restoration of seismic.

 

raftrestore3.jpg (104999 bytes)

 

 

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This site is maintained by John Nicholson. All photography is copyright.    İHighland Geology Limited 2004