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Structural description of sections
The Rubjerg Knude Glaciotectonic Complex is differ-
entiated into 13 structural sections, which are named after the localities recorded in the geological cross- section of Lønstrup Klint by Jessen (1918). The sec- tions can be grouped into three zones within the com- plex: a distal zone (three sections farthest to the south), a central zone (seven sections in the middle part of the complex), and a proximal zone (three sections farth-
est to the north). They are named, from south (near
Nørre Lyngby) to north (at Lønstrup): Ulstrup, Stens- næs, Martørv Bakker, Kramrende, Brede Rende, Sand- rende, Stenstue Rende, Grønne Rende, Rubjerg Knude
Fyr, Stortorn, Moserende, Mårup Kirke and Ribjerg
Sections. Three criteria were used for defining the sections: (1) the sections had to be bordered by marked footwall ramps, (2) each section should be character - ised by uniform structural architecture, and (3) the sections had to be descriptively and geographically delimited. A good example of the first criteria is the steep thrust fault separating the Sandrende Section from the Stenstue Rende Section. As an example of a uniform architecture, the Grønne Rende Section can be mentioned, and finally the Mårup Kirke Section includes the long barren stretch from the Mårup church to Ribjerg at Lønstrup where the lack of geographical markers as well as characteristic footwall ramps is sig- nificant.
Each section is described separately, a general phys-
iographic introduction being followed by four parts:
(1) tectonic architecture, (2) sedimentary units, (3) struc-
tures, and (4) interpretation of structural development.
The first descriptive part provides a general descrip- tion of the macro-structures. The second part presents the sedimentary deposits, and although to some de- gree it repeats the lithostratigraphic descriptions of the formations (see above), the detailed observations of syntectonic sedimentation are relevant to an ap- pr eciation of the structural development in the indi- vidual sections. The third part concerns the descrip- tion of meso- and mini-structures (thrust faults, folds, faults, shear zones, joints, fractures, breccias, polydia- pirs etc.). The description of each section is conclud- ed with an interpretation of the formation of the struc- tures. This interpr etation should not be confused with the overall interpretation of the dynamic development of the progressive thrust-fault deformation that fol- lows the systematic descriptions of the sections. The
organisation of the section descriptions follows the
general systematics of structural geology: the descrip- tion of geometry, the kinematic investigation, inter- pretation of the dynamics and finally the analysis can be concluded by a tectonic synthesis (Dennis 1972).
The reader should note that the structural elements
are numbered from distal to proximal. This is a conse-
quence of the systematic analysis; in order to obtain an overview, the reader can compare the structural de-
scription given for each section with the dynamic de-
velopment presented in the latter part of this bulletin.
Ulstrup Section
The southern frontal edge of the Rubjerg Knude Gla-
ciotectonic Complex is positioned in the Ulstrup Sec- tion where the undeformed foreland is exposed be- low the hanging-wall flat of the last displaced and most distal thrust sheet (UL01, see Plate 2). One of the most interesting problems addressed in the analy- sis of this complex is the presence of two long thin thrust sheets that were translated southwards for about 500 m from their ramps to their present positions with- out complete internal disruption. The Ulstrup Section represents the foreland margin of the thrust-fault com- plex, and the two flat-lying thrust sheets extend from the southern edge of the thrust front at Tvonnet Rende to the steep ramp thrust separating the Ulstrup and Stensnæs Sections (Plate 1). The Stensnæs ramp thrust was initially regarded as the foreland thrust (Peder- sen 1987), but new outcrops of the southern Ulstrup thrust exposed in 1996 and 1997 clearly demonstra- ted additional details of the frontal thrusting. Conse- quently, the long cliff section showing horizontal bed- ding that had previously been regarded as a primary, undeformed sedimentary unit (Fig. 42) is now inter- preted as a displaced thrust sheet (UL01).
The Ulstrup Section is truncated by a broadly hori-
zontal glaciotectonic and erosional unconformity
above which aeolian sand was deposited, either as sheet sands or as small dunes, up to 10 m high.
61
Tectonic architecture
The Ulstrup Section comprises the two flat-lying thrust
sheets, UL01 and UL02. The tip line of the hanging- wall ramp (the edge of the frontal thrust) is situated on the northern side of Tvonnet Rende (for location, see Plate 1). Unfortunately, the precise position is obscured by late, syntectonic erosion and sedimenta- tion at the front of the thrust-fault complex, as well as by sand scree covering the outcrops at Tvonnet Rende. The northern boundary of the section is the footwall ramp and flat of the UL02 thrust sheet, which forms a transitional zone of imbricate thrusting related to the frontal part of the Stensnæs Section.
The frontal part of the UL01 thrust sheet was dis-
placed from the upper footwall ramp (Fig. 43) along
an upper footwall flat on the top surface of the fore- land. At the tip of the thrust sheet, the thrust fault dips
gently towards the foreland, and a small foreland-dip-
ping ramp is also located at point 6040 m in the cross- section (Plate 1, see Fig. 50). The ramps probably formed
due to erosion in front of the propagating thrust-fault
edge. In the central part of the UL01 thrust sheet, a synform structure is associated with a chaotic breccia, interpreted as the collapse of a frost mound or sand-
mud diapir below the thrust fault; the synformal de-
pression is referred to hereafter as Ulstrup Rende (for location, see Plate 1). The trailing end of the thrust sheet starts at the upper footwall ramp of the foreland from where the hanging-wall flat is inferred to contin- ue along the footwall flat to the footwall ramp at its trailing end. The total length of the thrust sheet is about 750 m and the displacement is estimated at 350 m, which is the distance from the footwall ramp at point 5800 m in the cross-section to the frontal termi- nation in Tvonnet Rende (Plate 1). The thickness of the thrust sheet varies from 10 to 20 m, decreasing towards the tip to the south, and increasing in thick- ness where syntectonic deposits fill the piggyback basin on the back of the thrust sheet. The thickness of the Lønstrup Klint Formation is only 6 m in the souther n part of the piggyback basin due to erosion related to elevation during thrust faulting.
The UL02 thrust sheet is 600 m long, with the fron-
tal edge situated on the northern side of the UL01
piggyback basin at point 5900 m, and the trailing end disappearing into the décollement zone at point 5300 m. The thrust fault consists of a more than 400 m long footwall flat on top of UL01 extending from the foot- wall ramp hinge at point 5360 m southwards to the
Fig. 42. The steep sandy cliff of the Ulstrup Section displays horizontal bedding of an apparently undisturbed deposit. However,
structural analysis of thrust-fault relationships to the south indicates that it is a long flat thrust sheet displaced more than 500 m
towards the foreland to the south. The cliff section is 25 m high and the view is towards the south. Photograph: June 1984.
62
gently dipping frontal bend at point 5780 m in the
cross-section (Plate 1). The frontal bend corresponds to the hinterland-dipping limb of the flat-topped hang- ing-wall anticline of UL01. This hanging-wall anticline compares well with the structure of the thrust-fault model in Fig. 6, and the southernmost c. 100 m of UL02 can be regarded to have been emplaced piggy- back on UL01 during the translation over the frontal footwall ramp. The UL02 thrust sheet is only 5-6 m thick above the flat-topped anticline, whereas the thick- ness increases to 20 m at the trailing-end ramp. The displacement along the northern thrust fault is 550 m, with an uncertainty of 10-25 m depending on the in- terpretation of the shape of the trailing-end ramp and the amount of erosion of the frontal part at the piggy- back basin at Ulstrup Rende.
Sedimentary units
The sedimentary units in the Ulstrup Section comprise
the upper part of the Lønstrup Klint Formation, ero- sional remnants of the lower part of the Rubjerg Knu- de Formation, and a variety of intercalations of the Rubjerg Knude Formation distinguished here as the
Ulstrup beds. The L/R-unconformity between the Løn-
strup Klint and Rubjerg Knude Formations can be traced along the upper part of the UL01 thrust sheet in which it also forms the base of the piggyback ba- sin. A few younger erosional unconformities, below and above the Ulstrup beds, are of only local signifi- cance within the Ulstrup Section.
Lønstrup Klint Formation
The mud-dominated Lønstrup Klint Formation forms
the main part of the thrust sheets in the Ulstrup Sec- tion, and has an average thickness of about 10 m (Fig. 19). In the southern thrust sheet, the fine-grained sand beds are thin and only small-scale current ripples have been observed. A combination of load structures (ball- and-pillow) and water-escape structures (convolution and small-scale diapirs) are developed at certain hori- zons. Above the hanging-wall flat, a zone about 2 m thick takes the form of a mobilised mud breccia, which can be characterised as a sole thrust zone. This brec- cia is superimposed by beds affected by a brittle type of brecciation, for ming cracks and joints in an up to 4 m thick zone in the lower part of the thrust sheet.
Fig. 43. The upper footwall ramp of the foreland (Foreland FWR) along which the UL01 thrust fault propagated (
UL01HWF
: Ulstrup
thrust sheet 01 hanging-wall flat), and from where it continued for more than 300 m over the footwall flat of the foreland. The cliff
section is 25 m high and south is to the right. Photograph: May 1998.
63
The northern thrust sheet (UL02) displays a more
sandy part of the Lønstrup Klint Formation (Fig. 25).
Here the sand beds are up to 1 m thick and water- escape structures, convolute bedding and flame struc- tures commonly disturb the primary bedding. Ball- and-pillow structures are more common towards the trailing end of the thrust sheets.
Rubjerg Knude Formation
In the Ulstrup Section, the Rubjerg Knude Formation
comprises three different depositional units: the main 'background' sedimentation of outwash sand, the gla- ciolacustrine Ulstrup beds (Fig. 25), and the coarse- grained glaciofluvial Ulstrup beds (Fig. 20).
The main depositional unit is fine- to medium-
grained meltwater sand represented in the footwall
block of the foreland (Fig. 43). Small-scale current rip- ples occur in the parallel bedded sand, which is inter- layered with c. 0.5 m thick trough cross-stratified beds.
The
glaciolacustrine Ulstrup beds
for m a 3-5 m thick
unit that is only found on the back of the UL02 thrust
sheet (Fig. 25). This unit consists of dark bluish grey, laminated clayey mud interlayered with a few sandy beds up to 0.5 m in thickness. The unit was deposited on a bedding-parallel unconformity, which is only discordantly developed in the northernmost trailing part of thrust sheet UL02. The unit thins out towards the south, and disappears near the hinterland-dipping limb of the flat-topped hanging-wall anticline formed above the footwall ramp of the foreland. Intraforma-
Fig. 44. The mud-mobilised thrust-zone
breccia consists of structureless mud
with scattered clasts floating in the
matrix. Dilation cracks filled with sand
are superimposed on the mud-mobilised
brecciation fabric. This reflects two
phase of cataclastic deformation: a first
phase of water-over-pressured breccia-
tion (hydrodynamic brecciation), and a
second phase of brittle fracturing when
the mud was consolidated, dehydrated
or perhaps frozen. Handle of spade is
12 cm. Photograph: June 1997.
tional hydrodynamic brecciation, including small-scale
diapirs and slump-like features, deformed the clayey mud; such deformation is not seen in the Lønstrup Klint Formation below the unit.
The
glaciofluvial Ulstrup beds
occur in the Ulstrup
Rende depression between points 5900 and 6000 m
in the cross-section (Plate 1). This unit is a c. 8 m thick succession of meltwater gravel fining up into coarse-grained sand (Fig. 20). Large-scale trough cross- bedding dominates the succession and clasts up to boulder size occur in the lowermost 2 m (Fig. 28). Lithologically, the clasts are dominated by flint, but clasts of fossil frozen sand are abundant (Fig. 29).
The glaciofluvial Ulstrup beds are overlain by
c.
5
m of medium- to coarse-grained sand of the Rubjerg
Knude Formation. On the north side of the Ulstrup Rende depression, between points 5900 and 6000 m, slump-folded sand beds and sedimentary breccias occur in the upper part of this succession, suggesting gravity gliding down the steep slope of the depres- sion (piggyback basin of UL01).
Structures and breccias
The most important structures related to the thrust
faults in the Ulstrup Section are the breccias occurring in the thrust zones above the thrust-fault surfaces. They appear to have formed by collapse of the thrust sheet during translation. The low-angle anastomosing faults that developed in the most distal part of the thrust- fault complex originated similarly during translation
64
and are associated with southerly dipping normal
faults. A significant collapse structure that formed be-
neath the Ulstrup Rende depression is also worthy of
note.
Thrust-zone breccias
The thrust-zone breccias occur above the hanging-
wall flat of the UL01 and UL02 thrust sheets, where they affect the mud-dominated Lønstrup Klint For ma- tion. The thrust zone is up to 4 m thick in the most distal part of the thrust-fault system (souther n part of UL01), and decr eases in thickness to 1 m northwards; it can be traced along the hanging-wall flat of UL02
for a considerable distance. The thrust-zone breccia
consists of mobilised mud with irregular clasts of mud scattered throughout (Fig. 44). Some patches may be more sandy and others more clayey, and lenses and layers of sand may be present. The mobilisation was apparently initiated as sandy mud-fluid that developed at the thrust-fault surface and extended up into the sedimentary unit (Fig. 45). In many cases, the initial hydrodynamic brecciation of the thrust zone left seg- ments along the displacement surface of the thrust fault, which were modified and developed into elon- gated cataclasts along the sole of the breccia zone. Convolute bedding and small-scale diapirism are also present.
The mobilised mud was subsequently transected
by dilation cracks and sand-filled fissures (Fig. 46).
The dilation cracks form an irregular network and the sand-fill was injected into consolidated mud (Figs 44, 46, 47). More or less horizontal sand-filled cracks have been observed in the frontal part of the UL01 thrust sheet, where they are up to 15 cm thick and appear up to 1 m above the hanging-wall flat. The sand in the cracks shows planar horizontal lamination and small-scale current ripples and a few vertical sand- filled pipes extend upwards from the cracks (Fig. 48).
Towards the frontal tip of the UL01 thrust sheet, an
increasing number of bedding parallel or low-angle
anastomosing fractures and small-scale faults appear to be related to an increased rate of inter nal gliding. This is an indication of how close the thrust sheet was to disintegration and a loss of cohesion. Zones 0.2-0.5 m thick, grading into mobilised mud, occur in between the anastomosing fractures, resulting in the destruction of bedding (Fig. 49).
Foreland-dipping hanging-wall flat faults
In the frontal part of the UL01 thrust zone, foreland-
dipping faults become increasingly common. These faults are either foreland-dipping (20-30°S) ramps formed by the hanging-wall flat scouring into the foot- wall flat (Fig. 50), or sets of 50°S dipping normal faults with displacements of about 10 cm. These structures are considered to be the result of partial collapse of the tip of the foreland-dipping limb of the hanging- wall ramp above a low-angle hanging-wall ramp trans- lated along the footwall flat of the foreland.
Intrusive contact
Thrust-fault surface
Fig. 45. Mud mobilisation along the hanging-wall flat of the
UL02 thrust sheet. From the thrust-fault sur face, a sandy mud
fluid intruded along fractures and up into the lower part of the
thrust sheet where it formed a mud-intrusion. During the initial
hydrodynamic brecciation of the thrust zone, small relict seg-
ments remained at the thrust plane where they were modified
and developed into elongate cataclasts in the sole of the thrust
breccia zone. Photograph: July 1998; matchbox for scale.
65
Fig. 46. Subsequent to mud mobilisation, the thrust zone was transected by dilation cracks and fissures, which form an irregular
network into which sand was 'injected'. The mobilised mud had clearly become consolidated before the sand-filled cracks formed.
The close-up inset illustrates the 'reverse' drag of the sand-fill (
arrowed
) indicating an upward direction of flow in the fissure.
Photograph: May 1998.
66
Collapse structure in the Ulstrup Rende
Structures in the central part of Ulstrup Rende (Figs
51, 52) are interpreted to represent a collapsed diapir. The early phase structures include thinning of the Løn-
strup Klint Formation in the thrust sheet, and forma-
tion of concave troughs in its surface. Vertically or steeply dipping sand breccias with upward directed flow structures cross-cut the thrust-zone breccia. The appearance of structureless sand pockets indicates sand-
fill of mobilised sediment from an over-pressured zone
in the subsurface. The complex of breccias and re- orientated bedding is interpreted as a collapse struc- ture; it is considered to be responsible for the forma- tion of the Ulstrup Rende depression, and the disrup- tion of the thrust sheet along steeply dipping frac- tures. In the breccia zone, steeply dipping sand-filled cracks and normal faults formed prior to the contin- ued deposition of the Rubjerg Knude Formation in the depression.
On the southern side of the Ulstrup Rende depres-
sion, the muddy part of the thrust sheet is displaced
by steeply dipping normal faults. Downthrow is to the
south, synthetic towards the depression, and the faults
are thought to be related to the collapse of the diapir structure.
Interpretation of structural development
There are two reasons why the Ulstrup Section de-
serves special attention. The first is that it represents a foreland thrust section with long lateral transport of thin thrust sheets, the nature of which has not previ- ously been documented. Secondly, it demonstrates the likely development of the initial stages of defor- mation, which the remainder of the thin-skinned thrust faulting in the Rubjerg Knude Glaciotectonic Com- plex also experienced before the upper most part was eroded. Thus the first phase of thrust-fault deforma- tion is preserved her e whereas it is almost never re- presented in the thrust-fault sections that have been
Fig. 47. The formation of thrust-zone breccias in the distal part of the thrust-fault complex is here illustrated in four stages of
development. ( 1 ) The initial undeformed sediment (Lønstrup Klint Formation) comprises clayey mud interlayered with thin sand
beds. (
2
) A mud-fluid is formed above the thrust-fault surface (line with
open triangles
) from where it is injected up into the layers
above (see Fig. 45). ( 3 ) Increasing mud-mobilisation results in the formation of a structureless matrix with dispersed matrix-
supported clasts of the primary sediment (see Fig. 44). Note the small normal faults indicating an on-going process of collapse. (
4
)
The mobilised mud becomes consolidated and the thrust-zone breccia develops into a more brittle stage; dilation cracks form into
which water-saturated sand is injected (see Fig. 46).
67
more intensely deformed. The interpretation of the
structural development can be summarised in the fol- lowing nine stages.
1. Initial thrust-fault fracturing and thrust-fault propa-
gation took place during mobilisation of mud along
the hanging-wall flat. At this stage, the thrust-zone breccia was formed due to high pore-water pres- sure in an unfrozen stage.
2. The UL01 and UL02 thrust sheets probably started
to move along the décollement zone as one coher-
ent thrust sheet, and first separated into two thrust
sheets after the frontal part of the sheet had passed
the most distal foreland footwall ramp.
3. The ramping up of the northern UL02 thrust sheet
probably increased the pore-water pressure, and
when this increase also affected the frontal part of UL01, diapirism was initiated under the central part of the southern thrust sheet.
4. The diapiric uplift and erosion took place in the
elevated surface. This erosion extended through the
Rubjerg Knude Formation to locally intersect the L/R-unconformity. The residual coarse clastic gravel
Fig. 48. A subhorizontal sand-filled
fracture occurring in the frontal part of
the UL01 thrust sheet. The sand-filled
fracture appears about 1 m above the
hanging-wall flat; the sand shows planar
horizontal lamination and current ripple
cross-lamination. The sand-filled fracture
is interpreted to have formed during
ground-frozen conditions, whereas the
vertical sand-filled pipe probably reflects
loading of the thrust sheet when it
ultimately lost its carrying pore-water
pressure and settled on its hanging-wall
flat. Photograph: June 1997.
Fig. 49. Subhorizontal anastomosing
faulting (centre left) with mud-mobilisa-
tion developed in domains between
fault fractures in the frontal part of the
UL01 thrust sheet. Photograph: June
1997.
68
Fig. 50.
A
: Foreland-dipping ramping of hanging-wall flat
formed by scouring-erosion of the footwall flat into the
top surface of the foreland. Note in the close-up (
B
) that
some hydrodynamic brecciation occurred in the footwall
ramp just below the thrust zone. Photograph: June 1997.
on the footwall flat at the surface of the foreland
in the Ulstrup Section.
7. The consequence of the diapir collapse was the
formation of the depression in Ulstrup Rende.
Redeposited coarse-grained clastic material filled the depression, generating the glaciofluvial Ul- strup beds. The occurrence of fossil frozen-sand clasts implies that part of the surface, the Ru- bjerg Knude Formation, was ground-frozen - probably that part of the thrust sheet that had been elevated due to the propagation up over the central ramp. The ground-frozen condition was probably also responsible for freezing of the mobilised mud in the thrust zone and the subsequent development of sand-filled dilation cracks (Fig. 47)
bed on the unconformity surface was probably the orig-
inal source for the large amount of coarse-grained ma- terial in the Ulstrup Rende depression.
5. The mud-sand volcano broke through to the surface, and
the mobilised mud and sand were extruded with the
release of the high pore-water pressure.
6. The surface of the diapir collapsed and gravel and sand
filled the fractured structure. The collapse was probably
contemporaneous with the loss of pore pressure through-
out the thrust zone. The release of over-pressure in the thrust zone resulted in the final settling of the thrust sheet
69
8. The depression was ultimately filled by the sand of
the upper unit of the Rubjerg Knude Formation.
The frontal edge of the northern thrust sheet prop- agated towards the northern side of Ulstrup Rende and parts of its leading tip slumped down the steep slope of the depression. This indicates the sequen- tial and later movement of the northern thrust sheet. The depression can be interpreted in part as a pig- gyback basin that formed according to the model demonstrated in Fig. 7.
9. Finally, the upper most sediments of the Rubjerg
Knude Formation covered the section before the
glacier advanced across the area. The uppermost metre of sand was transformed into a glaciofluvial- sand-glacitectonite.
Fig. 51. The Ulstrup Rende depression is interpreted to represent a combination of a piggyback basin (according to the model in
Fig. 7) and the collapse of an underlying mud diapir or frost-mound feature. Note the steep normal fault on the left side of the
depression (to the north). Photograph: June 1997; spade (lower centre) for scale.
Fig. 52. Chaotic sand/gravel breccia in the centre of the Ulstrup
Rende depression, which is interpreted as the result of the col-
lapse of the diapiric structure created in the subsurface below
the UL01 thrust sheet. Photograph: May 1998.
70
Stensnæs Section
The Stensnæs Section is named after Stensnæs, which
is a minor point (Danish: sten = stone; næs (pynt) = point) at a gentle bend in the cliff section. Stones and erratic blocks, probably derived from the up to 2 m thick sandy till and the erosional unconformity below the Vendsyssel Formation, were formerly abundant on this part of the beach. The sandy till thins out south- wards where a glaciotectonic unconformity truncates the section.
The Stensnæs Section displays the most spectacu-
lar folds in the Rubjerg Knude Glaciotectonic Com-
plex (Fig. 53). The folds are situated at the transition from the flat-lying beds to the south (the Ulstrup Sec- tion) and the main thrust-fault imbrications to the north. The fold complex is truncated by an erosional unconformity forming a depression in which slump slides and sedimentary breccias derived from the tip of the thrust sheet were deposited after collapse and gravity gliding. In general, the fold complex is well exposed, whereas the transition further southwards is often covered by sand scree. During the years of study of the Rubjerg Knude Glaciotectonic Complex by the author, variations in the degree of exposure of the Stensnæs Section have contributed to a fuller under -
standing of the structural development of the section
that represents the foreland margin of the thrust-fault complex.
Tectonic architecture
The Stensnæs Section comprises four thrust sheets
(SN01, SN02, SN03 and SN04, Plate 2). The southern boundary of the section is defined by the footwall ramp of UL02, although the trailing end of UL02 is here included in the description of the imbricate du- plex that hosts the fold complex. The northern boun- dary is the hanging-wall ramp of MB01/MB02, that is thrust up along the footwall block of SN04. The thrust sheets comprise the uppermost part of the Lønstrup Klint Formation and a relatively thin cover of the over- lying Rubjerg Knude Formation sediments. Two dis- crete piggyback basins (early and late) were formed above the SN01 and SN02 thrust sheets.
The SN01 thrust sheet is about 30 m thick, and al-
though the thrust sheet includes a number of small
duplex imbricates it can be subdivided into upper and lower segments. The lower segment is thrust onto the UL02 footwall block with a displacement of about 30 m.
The displacement of the upper segment is partitioned
Fig. 53. The fold complex developed in the transitional imbricate zone between Ulstrup and Stensnæs Sections. Note that the thrust
faults acting as flexural slip surfaces in the folding continue into the bedding-parallel thrust-fault flats to the south (right). Photo-
graph: July 2000.
71
into a series of minor differential displacements rang-
ing from minor flexural slips along bedding surfaces in
the fold structures to imbricate offsets of about 1-3 m.
In the frontal part of the SN02 thrust sheet, the Løn-
strup Klint Formation is only a few metres thick, and
is overlain by 10 m of sediments of the Rubjerg Knu- de Formation r esting on the L/R-unconformity. At the trailing end of the thrust sheet, the Lønstrup Klint For- mation is more than 15 m thick, whereas the Rubjerg Knude Formation is cut off by the footwall ramp of SN02 (corresponding to the hanging-wall thrust fault
for the imbricates of SN03). The accumulated displace-
ment of SN02 amounts to 88 m, including 15 m up over the footwall ramp and 73 m along the footwall flat of SN01.
The SN03 thrust sheet may be divided into four
imbricate segments thrust onto the footwall ramp of
SN02. The displacement along the hanging-wall thrust fault is 45 m, but it was also carried piggyback on SN02 during the translation along the décollement zone, which gives an accumulated displacement of 163 m for the SN03 thrust sheet.
Fig. 54. Ball-and-pillow structures in the
Lønstrup Klint Formation in the Stens-
næs Section. Note that the size of the
structures reflects the thickness of the
sand beds involved. Photograph: July
2000; staff divisions are 20 cm.
Fig. 55. Dish-and-pillar structures
developed in the lowermost sandy bed
above the hanging-wall flat of the SN2
thrust sheet in the Stensnæs Section.
This type of water-escape structure is
interpreted to have formed during the
thrust-fault translation along a hanging-
wall flat due to the high water pressure
released from the sole of the thrust
sheet. Photograph: July 1998.
72
The SN04 thrust sheet is about 20 m thick, includ-
ing an up to 8 m thick unit of the Rubjerg Knude
Formation resting on the L/R-unconformity above the Lønstrup Klint Formation; this unit increases in thick- ness to about 15 m towards the trailing end of SN04. Total displacement is about 45 m, including a hang- ing-wall ramp-and-flat propagation along the footwall ramp of SN03.
Sedimentary units
The sedimentary units that crop out in the Stensnæs
Section are dominated by the upper sandy parts of the Lønstrup Klint Formation. A lens of a glaciolacust- rine diamictite is preserved as an imbricate thrust sheet, c. 3.5 m thick and 22 m long, and is tentatively inter- preted to form part of the Rubjerg Knude Formation. The latter is mainly represented by a 6-8 m thick suc- cession including the residual gravel deposited on the uneven sur face of the L/R-unconformity. An upper unconformity truncates the SN01 and SN02 thrust sheets, and coarse gravel beds as well as olistoliths of the Lønstrup Klint Formation were deposited in a late piggyback basin (SnstRu in Plate 2).
Lønstrup Klint Formation
The sedimentology of the Lønstrup Klint Formation
in the Stensnæs Section is similar to that described for the Ulstrup Section. The maximum thickness of the formation is about 15 m, and lithologies are dominated
by 0.2-0.8 m thick fine-grained sand beds with climb-
ing ripple lamination. Thin laminae of mud and small amounts of detrital organic material commonly drape the ripples. The sand beds are interlayered with thin
laminated dark grey mud beds; micro-faulting is evi-
dent in this facies. Ball-and-pillow and convolute struc- tures are abundant (Fig. 54). In the uppermost 4 m of the formation, the sandy beds become thinner and the uppermost part is dominated by mud. In sand beds inferred to be situated above the hanging-wall flat, dish-and-pillar structures have been observed (Fig. 55) that are interpreted to have formed by water-escape processes related to the thrusting.
Cheel & Rust (1986) provided a model for the de-
velopment of water-escape structures in glacial out-
wash deposits from Ottawa, Canada. In their model, a sequential development from simple load structures through detached ball-and-pillow structures to dish structures is demonstrated. The model predicts a stra-
Fig. 56. The piggyback basin situated above the erosional truncation of thrust sheet UL02 and SN01 in the Stensnæs Section (SNstRu
in Plate 2). Note that normal listric faults ( arr ow ) may be traced to the trailing end of the large olistoliths ( green ) deposited in the
meltwater sand and gravel. This is interpreted as the result of gravity gliding of the tip of a thrust sheet, which during propagation
from the north collapsed subsequent to thrust faulting up above the mean level of sedimentation. Photograph: July 2000; thrusts
indicated in
red
, unconformity indicated in
purple
.
73
tified distribution with convolute stratification at the
base of a bed, ball-and-pillow structures dominating the main part, and dish structures formed in the up- permost part of the bed (or unit) resulting from ex- cess pore-water fluid pressure. The observed water- escape structures in the Stensnæs Section as well as in the sections further to the north compare well with the model of Cheel & Rust (1986) (Figs 54, 55; see also fig. 77), although they suggested the triggering mechanism to be earthquakes or movements due to melting of dead-ice.
Rubjerg Knude Formation
In the Stensnæs Section, two units of the Rubjerg
Knude Formation are distinguished: (1) a lower unit dominated by fine- to medium-grained glaciofluvial sand, and (2) an upper unit of varied sedimentary breccias and coarse-grained clastic deposits that in- fills the piggyback basin on top of the truncated thrust sheets in the section (Fig. 56). The sand deposited in the lower unit may be planar parallel stratified, or exhibit large-scale trough cross-bedding with shallow troughs, only 0.5 m deep. The lower unit of the Ru- bjerg Knude Formation is estimated to be 6-8 m thick, and although strongly affected by hydrodynamic bre- cciation, the unit compares well with the description of the lower part of the formation provided by Sado- lin et al. (1997).
The upper unit was deposited on the erosional
unconformity truncating the back of the UL02 thrust
sheet, the fold and imbricate complex of SN01, and the tip of the SN02 thrust sheet (SnstRu in Plate 2). The central part of the basin is about 7 m thick, de- creasing towards both the north and south forming a relatively narrow trough. The sediments in the basin consist of large-scale irregularly trough cross-bedded glaciofluvial sand and gravel. Blocks of sandy mud, which can be identified as derived from the Lønstrup Klint Formation, were deposited as sedimentary brec- cias in the basin. The clasts are up to 1 × 5 m in size; blocks and clasts less than one metre in size were commonly rotated during redeposition. Normal listric faults in the northern part of the basin relate to the deposition of the largest olistoliths (Fig. 56). The south- ern part of the basin was tilted subsequent to deposi- tion due to the fault-bend folding of the hanging-wall flat of UL02 when it propagated along the footwall flat during the latest phase of thrust faulting. Thus the upper unit of the Rubjerg Knude Formation in the
Stensnæs Section is interpreted to have been deposit-
ed in a piggyback basin in which thrust-sheet tips thrust up from the north collapsed and gravity-glided out into the basin.
Structures
Two types of structures in the Stensnæs Section are
related to thrust faulting: (1) the folding related to duplex imbricates, and (2) extensional faults related to push-from-the-rear in the trailing end of a thrust sheet.
Imbricate duplex folding
The folds in the Stensnæs Section can be described as
flexural slip folds, and have amplitudes of 1-3 m and wavelengths of 2-5 m (Figs 53, 57, 58). The folds ar e very irregular in shape, however, and cannot be ex- plained in terms of simple compression. Analysis of the flexural slip surfaces shows that the folded layers were separated into segments and that discordant re- lationships exist between beds in neighbouring seg- ments. By defining the segments as small imbricate thrust sheets in a duplex, thrust-fault terminology can be applied and hanging-wall and footwall thrusts of the individual duplex segments defined. In Fig. 57 this has been done by identifying the footwall ramps (FWR), thus distinguishing five imbricate thrust sheets about 1 m in thickness. The folds in the imbricate duplex segments include both hanging-wall anticlines and footwall synclines. As documented by the refold- ing of the upper hanging-wall anticline in Fig. 57, the folds are superimposed by sequential phases of fold- ing and thus also phases of imbricate thrusting. Fig- ures 58 and 59 illustrate the sequential development of imbricate thrusting; the imbrication steps forward towards the footwall ramp of UL02 to the south. Note also that the hanging-wall flat of each imbricate con- tinues into an intraformational bedding-parallel thrust fault. This can be difficult to recognise in an isolated exposure, where the flats cannot be traced back to the ramp structures in the imbricate duplex (Fig. 53).
Extensional faults
In the trailing part of the SN03 thrust sheet, listric ex-
tensional faults have been observed (Fig. 60). Dis- placements along the faults are up to 0.5 m and the
74
Fig. 57. Flexural slip folding in the sandy beds of the Lønstrup
Klint Formation in the Stensnæs Section. Numbers ( 1 - 4 ) refer
to the sequential development of the thrust faults in the duplex
structure, which probably formed during the collapse of the
footwall ramp to the south (UL02FWR). Note that the ramp
thrust faults propagate into bedding-parallel flats. Photograph:
May 1996.
Fig. 58. Detail of the fold structures formed by superimposed
ramp propagation (see Fig. 57). The thrust-fault segments in
the imbricate duplex are marked by black lines and the
recognised footwall ramps are annotated
FWR
. Hanging-wall
anticlines are dominant, but footwall synclines also add to the
fold framework. Photograph: May 1996.
75
Fig. 59. Simplified model of superimposed folding formed by sequential imbrication in a duplex complex.
Step 1
shows the
undeformed beds with the ramps bordering the segments indicated. The numbers refer to the sequentially propagating hanging-
wall ramps.
Step 2
shows the first hanging-wall anticline to be formed by the progressive collapse of the trailing end of the footwall
block (footwall ramp collapse). Step 3 illustrates the formation of an antiformal stack during the progressive superimposed defor-
mation.
Step 4
demonstrates the developed stage of superimposed fault-bend folding comparable to the structures illustrated in Figs
57, 58.
76
Fig. 60. Low-angle listric extensional faults in the SN03 thrust sheet, in the central part of the Stensnæs Complex.
A
: An overview of
the macr oscopic structure, where the SN04 thrust sheet ramps up along the footwall flat of SN03 and pushes it laterally in the back.
The resultant extensional fault imbricates form a boudinage-like network.
B
: Detail of the listric extensional faults (
arrows
) inter-
preted to have been formed by push-from-the-rear. Photograph: July 1996; staff divisions are 20 cm.
77
Fig. 61. Illustration of the difference between the mild deformation affecting the top of the footwall block and the strong defor-
mation of the hanging-wall block. Only a 20 cm thick zone below the shear-laminated thrust-fault surface was affected by low-angle
extensional faulting grading down into a minor normal fault network. It is thus evident that the elevated water pressures supporting
the thrust sheet were transmitted to the hanging-wall flat, where intense hydrodynamic brecciation took place. Photograph: July
1998.
78
spacing between the faults is 0.2-0.6 m, which creates
a boudinage-like network. The structures are interpre-
ted to have been formed by push and loading of a thrust
sheet ramping the formerly monoclinal fault-bend-fold-
ed thrust sheet, which responded to the gravity spread- ing by displacements along the extensional faults.
Similar mini-scale extensional normal faults are rec-
ognised in the footwall block below the hanging-wall
flat of SN03 (Fig. 61). It is remarkable that the thrust- fault deformation only weakly affects the top of the footwall block, while the hanging-wall block is strongly affected by hydr odynamic brecciation. A zone only 20 cm thick below the shear-laminated thrust-fault sur face is affected by low-angle extensional faulting, and grades down into a minor normal fault network (Fig. 61). Isoclinal folding has been observed in the narrow shear-laminated thrust-fault zone, adding to the impr ession of high strain along the thrust fault. However, it is clear that the elevated water pressures supporting the thrust sheet were located in the hang- ing-wall flat.
Interpretation of structural development
The formation of the imbricate duplex fold complex
in the Stensnæs Section is evidently related to ramp pr opagation. Two footwall ramps are significant: the footwall ramp of UL01, which can be regarded as re- pr esenting the footwall ramp of the foreland, and the footwall ramp of the trailing end of UL02. The UL01 footwall ramp acted as a stopping block for the for - ward push of the imbricate thrust sheets, and the pro- pagation of this ramp was responsible for the general gentle northerly tilt of the structures. The UL02 foot- wall ramp was subjected to successive thrust-fault splay formation, and consequently imbrication and super- imposed folding, which can be viewed as the col- lapse of the trailing end of the UL02 thrust sheet.
The imbricate duplex fold complex of the Stensnæs
Section can be readily compared to the model for
connecting splay duplexes of the Sevier thrust belt in the Cordilleran Fold Belt (Mitra & Sussmann 1997). There is a close similarity with respect to the growth of the duplex by successive connecting splays of the thrust fault and the creation of folds by thrust-fault propagation. Moreover, the analysis of the imbricate duplex fold complex implies that the imbrication start- ed at the footwall ramp in the trailing end of the sys- tem and propagated towards the foreland. It can there- fore be argued that the process was one of footwall
ramp collapse. A simplified model for the growth of
duplexes in a connecting splay duplex system is illus- trated in Fig. 59.
With respect to the thrust-fault displacement, an ac-
tive and a passive stage of translation need to be dis-
tinguished. The active translation is the amount of dis-
placement of the thrust sheet arising from propaga-
tion along its hanging-wall thrust fault. The passive translation is the amount of transport arising from the displacement of the underlying thrust sheet which carries it piggyback fashion. During this latter transla- tion, the underlying thrust sheet may propagate foot- wall ramps, which will fold the actively translating thrust
sheet as well as the piggyback thrust sheets into hang-
ing-wall anticlines. This type of deformation will cre- ate an antiformal stack. The Stensnæs imbricate du- plex fold complex may thus also be viewed as a meso- to macroscopic-scale antiformal stack (Fig. 59).
A roof thrust, which is 110 m long and about 8-12
m thick covers the SN01-SN02 duplex. The accumu-
lated length of the three duplex segments is 175 m; c. 65 m is thus missing in the balance calculation of the southern half of the Stensnæs Section. It is most likely that part of the initial thrust sheet has been eroded away, but up to c. 45 m of it might have been incor- porated in a foreland-dipping frontal thrust structure preserved in the chaotic imbricate fold complex.
Martørv Bakker Section
The name Martørv Bakker is derived from the peat
exposed in the coastal cliff (Danish: mar = sea; tørv = peat; bakker = hills), which is covered by aeolian sand dunes above the northern end of the section. In the southern part of the section, the Vendsyssel Forma- tion forms the top unit in the cliff. The Vendsyssel Formation was deposited on an erosional unconfor m- ity above the glaciotectonic complex. All the post- tectonic deposits are prone to cliff erosion and the resultant scr ee partly obscures the structures in the Martørv Bakker Section. In addition, the unconformi- ty at the base of the planar-bedded Vendsyssel For- mation is a focus for groundwater seep which also conceals details in the exposures. However, two im- portant architectural elements have been recognised: (1) the common appearance of minor duplexes in the southern part of the section, and (2) the occurrence of southerly dipping normal faults in the northern part.
The southern boundary of the section is the foot-
wall ramp of SN04 in the trailing end of the Stensnæs
79
Section. The northern boundary is not defined by a
simple reference point in the cross-section, but by the trailing end of the MB04 thrust sheet which is a com- bination of footwall ramp and footwall flat below the leading-edge thrust fault of the Kramrende Section.
Tectonic architecture
The Martørv Bakker Section is subdivided into four
thrust sheets (MB01-MB04). The thrust sheets in the southern part of the section are subdivided into up- per and lower duplex segments of which only the lower duplex segments are distinguished by separate annotations (MB02u1-MB02u3, Plate 2). In the front- al part of the section, smaller imbricate duplexes are associated with syntectonically formed hydrodynam- ic breccias and ball-and-pillow structures.
The MB01 thrust sheet is up to 20 m thick and com-
prises the upper part of the Lønstrup Klint Formation.
The frontal hanging-wall ramp was thrust up along the 15° dipping footwall ramp of SN04, and displace- ment is estimated at about 55 m. The bedding be- comes steeper in the trailing end of the thrust sheet, probably due to the relatively steep dip of the ramp in the subsurface from the 20 m to the 10 m flat level.
The MB02 thrust sheet is long and flat-lying and
occupies more than 400 m of the section. The frontal
part is only 10-15 m thick and was displaced along its upper hanging-wall flat along the footwall flat of MB01 for a distance of about 180 m. The trailing part of the MB02 thrust sheet is 20 m thick, but as indicated in the balanced cross-section it roots down to the 30 m décollement level (Plate 2). The thrust sheet is dis- placed by a prominent normal fault in the central part of the Martørv Bakker Section (Fig. 62). Above the Lønstrup Klint Formation, a marked basin developed in the hanging-wall block of the normal fault. The
Fig. 62. The normal fault developed in the central part of the Martørv Bakker Section. In the hanging-wall block to the south, the
fluvial sands of the lower part of the Rubjerg Knude Formation are preserved in a 'fault trap' along the fault plane. Diamict
sediments were deposited above the sand in a piggyback basin that developed during the thrust faulting of the MB02 thrust sheet.
Note that the thickness of the Lønstrup Klint Formation in the footwall block decreases downwards along the normal fault drag. This
is interpreted as a foreland-dipping limb related to a hanging-wall anticline formed prior to offset by the normal faulting. The
formation of the normal fault is interpreted to be related to a foreland-dipping limb of a hanging-wall anticline at the tip of a
subsurface thrust-sheet segment (MB02u3 in Plate 2). Photograph: June 1993.
80
sediments in this basin were described as moraine
sand by Jessen (1918, 1931).
The MB03 thrust sheet is 30 m thick and made up
of the Lønstrup Klint Formation, which is here strong-
ly deformed by hydrodynamic brecciation and disloca-
ted by a number of bedding-parallel minor thrust faults.
The frontal part is flat-lying, whereas the dip of the bed-
ding increases to 25-30° at the trailing end indicating
a bend over an upper hinge on top of the footwall ramp of MB02. In the exposed part of the section, the MB03 thrust sheet is only about 120 m long, and it is inferred that the foreland-dipping structures in the fr ontal part reflect re-orientation due to hanging-wall ramp propagation along the footwall flat of MB02.
The MB04 thrust sheet forms a flat-topped hang-
ing-wall anticline above the footwall ramp of MB03.
The thrust sheet is displaced along a normal fault par-
allel to the foreland-dipping bend in the top of the frontal part of MB03. The normal fault does not dis- place the footwall flat of MB02, and is therefore re- garded as a structure related only to the framework of MB03 and MB04. The structural framework in this part of the section may be characterised as an antiformal stack, including thrust sheets MB03 below and KR01 above MB04.
Sedimentary units
The Martørv Bakker Section is dominated by the Løn-
strup Klint Formation. However, the most important sedimentological feature in the section is related to
Fig. 63. Hydrodynamic brecciation in the
Lønstrup Klint Formation in the north-
ern part of the Martørv Bakker Section.
Photograph: June 1993.
Fig. 64. Slump-fold structures formed in
the thin-bedded sand layers enveloped
in dark muds of the diamict sediments
in the piggyback basin in the Martørv
Bakker Section. Photograph: October
1998.
81
the basin developed at the top of the hanging-wall
block connected to the normal fault displacing the MB02 thrust sheet (Fig. 62). The deposits in this basin are regarded as an exotic part of the Rubjerg Knude For-
mation, and are described under this heading below.
The southern part of the Martørv Bakker Section is
unconformably overlain by the Vendsyssel Formation,
the initially glaciotectonic truncation being superim-
posed by a post-glacial erosional unconformity. A Holo-
cene erosional unconformity truncates the Vendsys-
sel Formation as well as the glaciotectonic unconform-
ity, and the peat deposited on this unconformity is up
to 2 m thick in the northern part of the section, where it is covered by modern aeolian dunes up to 20 m high.
Lønstrup Klint Formation
The lower part of the Lønstrup Klint Formation is mud-
rich. It is exposed in the northern part of the section, where it was thrust above the hanging-wall flat from the décollement surface 25-28 m below sea level. The upper part of the formation is dominated by 0.5-1.5 m thick sand beds interlayered with thin beds of hor- izontally laminated mud, which typically has been mobilised to form hydrodynamic breccias. In the south- ern part of the section, the beds are strongly affected by ball-and-pillow deformation (Fig. 63).
Rubjerg Knude Formation
The Rubjerg Knude Formation comprises two units:
(1) a lower 3 m thick sand unit only exposed along the prominent normal fault in the central part of the Martørv Bakker Section, and (2) a c. 15 m thick diamic- tite interpreted as a glaciolacustrine mud with rede- posited clasts. The first unit was deposited on the L/R-unconformity, and comprises light yellowish me- dium-grained sand (Fig. 26). The diamictite unit rests partly on the lower sand unit, and partly on the L/R- unconformity at the top of the Lønstrup Klint For ma- tion. The diamictite is dark grey, and comprises weakly laminated mud interbedded with structureless, irre- gularly distributed matrix-supported beds containing
Fig. 65. A schematic diagram explaining the development of the hydrodynamic brecciation displayed in Fig. 63. The formation of the
structure was the result of three phases of defor mation. In the first phase, a succession of sandy turbidites interbedded with mud ( 1 )
was affected by loading to form the ball-and-pillow structures (
2
). In the second phase, the ball-and-pillow structures were dis-
placed by thrust faulting ( 3 ). During the third phase, the mobilised mud intruded up thorough the thrust-fault surface ( 4 ), demon-
strating the syntectonic development of the hydrodynamic brecciation.
82
unsorted clasts in a matrix of sandy mud (Fig. 26). In
the lower most 2 m of the diamictite succession, the matrix-supported clasts were probably derived by re- deposition of coarse-grained material eroded from the L/R-unconformity to the north. About 3 m up in the succession, a c. 1 m thick bed occurs with clay clasts 10 cm in size deposited in a weakly clay-laminated and sand-streaked silty mud. This bed is overlain by three 1.5-3 m thick units of isoclinally slump-folded, thin-bedded, fine-grained sand encased in dark struc- tureless mud (Fig. 26). These units are interpreted as slump-folded sheets derived from the Lønstrup Klint Formation (Fig. 64). The middle and upper slump-units
are separated by a
c.
5 m thick interval dominated by
sandy mud with scattered clasts and a few thin sand beds. The uppermost sand bed was not affected by slumping and shows lar ge-scale trough cross-bedding.
The lower part of the diamictite succession is strong-
ly disturbed by hydrodynamic brecciation with meso-
scopic-scale diapirs rising from the top of the Løn- strup Klint Formation and penetrating upwards into the diamict sediments. This indicates that the diamic- tites were part of the main sedimentation affected by glaciotectonic disturbances.
Structures
In the Martørv Bakker Section, three types of structural
elements were studied: (1) imbricate duplexes domi-
nating the southern part of the section, (2) the normal
fault in the central part of the section, and 3) hydro- dynamic brecciation contemporaneous with, or super- imposed on, ball-and-pillow structures (Figs 63, 65).
Imbricate duplexes
The imbricate duplexes in the souther n part of the
section constitute rhomb-shaped segments 10 to 25 m in
size bounded by low-angle thrust faults. Minor im-
bricates may occur along the thrust faults, but the thrust
faults are mainly narrow fracture surfaces without signi- ficant brecciation.
A mini-scale example of duplex formation is shown
in Fig. 66. Although the structure is related to intrafor-
mational deformation of the beds, it illustrates instruc- tively the formation of hanging-wall ramp propaga- tion of a stacked footwall ramp. Thus the footwall ramp
is formed by the trailing edges of two duplex seg-
ments that were displaced one over the other to form
a single planar ramp for the propagation of the upper
thrust sheet. Flame-like upright minor anticlines are interpreted as compressed hanging-wall anticlines
formed during the sequential propagation of the vari-
ous ramps. On top of the upper footwall hinge, a radial
flame structure probably indicates the site of incipient
diapirism (Fig. 66). The formation of foreland-dipping thrust structures above the tip of a lower duplex seg- ment is also apparent.
Normal fault
The normal fault in the central part of the section is
an uneven fault plane striking E-W with a dip of about 45° to the south. Displacement along the fault plane is about 25 m, and a set of minor normal listric faults displace the top of the hanging-wall block (Fig. 62). The footwall block comprises the Lønstrup Klint For- mation, which decreases in thickness southwards and forms an irregularly folded drag along the fault plane. At the top of the hanging-wall block, the diamict sed- iments described above are discordantly superposed on the light-coloured sand at the base of the Rubjerg Knude Formation.
Hydrodynamic brecciation
Ball-and-pillow structures occur in the sand-rich parts
of the Lønstrup Klint Formation, where hydrodynam- ic mud mobilisation created chaotic breccias (Fig. 63). The initial size of the sand ball-and-pillow structures is related to the primary thickness of the beds, but subsequent to the sedimentary load deformation they were distorted and deformed during thrust-fault related mud remobilisation. In Fig. 63, the distorted ball-and- pillow structures can be seen to be displaced by minor
thrust faults, and these thrust faults were intruded by
mobilised mud. The sequential development of this hydrodynamic brecciation is illustrated in Fig. 65, where three phases of deformation are recognised, although these probably developed progressively during thrust-fault displacement and related loading of superposed thrust sheets.
Interpretation of structural development
The thickness of MB01 implies that the décollement
surface in the southern part of the section is situated
83
at the 20 m level. The thickness of MB03 is 30 m,
implying that the décollement level stepped down 10 m somewhere in the central part of the section. A lower footwall ramp and a corresponding hanging- wall ramp must therefore be included in the balanced cross-section. The L/R-unconformity reference surface on top of the MB02 thrust sheet was about 20 m above present sea level prior to the normal fault displace- ment, which indicates that a duplex 20 m in thickness is situated below the trailing end of MB02. The lower footwall ramp responsible for the fault-propagation folding of the antiformal stack in the northern part of
the section, estimated from the bend of the trailing
ends of MB02 and MB03, must be situated below MB02. The structural model therefore suggests that a subsurface duplex was formed by segments of the MB02 thrust sheet situated between the 20 and 30 m levels (MB02u1-MB02u3). The footwall ramp thus constitutes two 10 m thick duplex segments stacked on top of each other.
Consequently, a hanging-wall anticline with a fore-
land-dipping limb formed above the hanging-wall
ramp of MB02 and was translated along a footwall flat. The model further suggests that the hanging-wall
Fig. 66. A model of duplex formation is here illustrated by a mini-scale structure related to intraformational deformation of beds in
the Lønstrup Klint Formation, central part of Martørv Bakker Section. The duplex comprises two segments, which were derived from
the bed underlying the lower footwall flat (lower FWF). The footwall ramp for the segments is situated to the left outside the frame
of the figure. The lower segment is a relatively short one, which was thrust over by the upper segment during the push from the
ramping of the upper thrust sheet. During propagation up the footwall ramp, the trailing edges of the two segments were displaced
to form one planar ramp for the upper thrust sheet, which was further translated over the duplex to a foreland-dipping bend created
above the tip of the lower duplex segment. The flame-like upright anticlines are interpreted as compressed hanging-wall anticlines
formed during the sequential propagation of the various ramps. Note the radial flame structures at the upper footwall hinge
indicating incipient diapirism. The small normal faults to the left of the trowel (15 cm in size) are thought to reflect similar foreland-
dipping features in the subsurface.
FWH
, footwall hinge;
FWR
, footwall ramp;
uFWF
, upper footwall flat;
HWF
, hanging-wall flat;
R
,
ramp. Photograph: June 1993.
84
structure is a composite feature partly constructed by
the hanging-wall anticline related to the tip of the MB02u3 segment folded over the footwall ramp of MB02u2, and partly by the hanging-wall anticline re- lated to the translation of the main hanging-wall ramp of MB02 along the 10 m level. The foreland-dipping limb of this structure corresponds well with a 45° south-dipping normal fault with a vertical displace- ment of about 20 m.
It is therefore concluded that the northern slope of
the diamict sedimentary basin was formed by the nor-
mal fault reflecting the foreland-dipping limb of a hanging-wall anticline. The souther n more gently dip- ping slope of the basin was formed by the bend of MB02 due to its propagation up along the footwall ramp and flat of MB01. This footwall thrust fault is a composite imbricate duplex, which hampers the ex- act distinction of ramp-flat relationships. The slump- folded units in the basin are interpreted as the result of gravity slides derived from the crest of the hang-
ing-wall anticline or the tip of the MB04 thrust sheet
propagating from the north. The sediments filling the basin represent redeposited material derived from the thrust-fault elevated part of the Lønstrup Klint Forma- tion, the coarse-grained clastics on the L/R-unconform- ity, and the lowermost part of the Rubjerg Knude For- mation. The basin is interpreted as a piggyback basin with syntectonic deposition during the translation of the MB02 thrust sheet.
Kramrende Section
From the south, the first significant macroscopic-scale
diapir occurs in the Kramrende Section (the Kram- rende diapir). Although mobilisation features also occur in sections farther to the south, this diapir is regarded as the most distal in the glaciotectonic thrust- fault complex. The thickness of the thrust sheet host- ing the Kramrende diapir suggests it is related to the
Fig. 67. The northern part of the KR01 thrust sheet where the lithostratigraphic reference section of the Lønstrup Klint Formation
(Fig. 21) is situated. The thrust sheet is fault-bend-folded up along an initially low-angle (
c.
8°) footwall ramp, which was subse-
quently folded into the present more steeply dipping orientation. Note the reverse faults interpreted as small back-thrust faults.
Photograph: June 1993.
85
deep level of thrust-fault rooting, which is about 30 m
below the L/R-unconformity. The thrust sheet to the south of the Kramrende diapir and two thrust sheets to the north are included in the section because they are all affected by the structures related to the diapir. The frontal edge of the Kramrende Section is formed by the footwall ramp beneath the first thrust sheet (KR01, see Plates 1, 2). This thrust fault is identical with the trailing-edge footwall ramp of the Martørv Bakker Section, which is responsible for the marked monoclinal fault-bend folding of the KR01 thrust sheet (Fig. 67). The steps to the beach are situated in the gully between the KR01 thrust sheet and the Kram- rende diapir. The steps lead up to the summerhouse
area at Oddervej, and are referred to as the Kram-
rende steps or the Oddervej Trappe.
Tectonic architecture
The Kramrende Section consists of four thrust sheets
(KR01-KR04; Plates 1, 2). The frontal thrust sheet (KR01)
is ramped over the MB04 footwall ramp in the Mar-
tørv Bakker trailing thrust sheet. At the north end of KR01, the L/R-unconformity is situated about c. 10 m a.s.l., which indicates that the KR01 hanging-wall ramp propagated along an inter mediate footwall flat (FWF). The upper ramping along the MB04 footwall ramp is
Fig. 68. Ball-and-pillow structure
developed in the sandy turbidite bed
between 4 and 5 m in Fig. 21. The
structure is interpreted as a load
structure formed immediately after
sedimentation. Additional load struc-
tures can be seen at the base of the
sand bed, where flame structures related
to the underlying clayey bed intrude the
base of the sand bed. Above the ball-
and-pillow structure, pinch and swell
structures within the sand bed are also
interpreted as gravity load structures.
Photograph: June 1993.
Fig. 69. In the upper part of the KR04
thrust sheet in the Kramrende Section,
the Rubjerg Knude Formation forms a
piggyback basin, which is overthrust by
the BR01 thrust sheet in the souther n
part of the Brede Rende Section. The
thrust fault displayed in the photograph
is a hanging-wall flat for the thrust sheet
BR01 ( BR01HWF ) and footwall ramp of
thrust sheet KR04 (
KR04FWR
). A minor
satellite thrust fault was formed below
the main thrust at a late stage of fault
propagation after the sand of the
Rubjerg Knude Formation had been
somewhat compacted. Photograph: June
1984.
86
responsible for the fault-bend-fold appearance of the
KR01 thrust sheet. Above the frontal part of the MB04 footwall ramp and flat, the KR01 thrust sheet is folded into a flat-topped anticline. In the involute part of this anticline, a splint or horse is present (the KR01 splint). This is a small thrust-sheet wedge torn off during thrust propagation, which created peculiar anticlinal features in the structural profile.
The KR02 thrust sheet takes the form of a major dia-
pir. Initially the diapir was a thrust sheet that was dis-
placed up along the KR01 footwall ramp and above the back of the KR01 thrust sheet. The KR03 and KR04 thrust sheets situated on the back of KR02 are charac- terised by marked dif ferences in the thickness of the Rubjerg Knude Formation. In the KR03 thrust sheet, the thickness is only about 8 m, whereas in KR04 the
thickness of the Rubjerg Knude Formation is up to 20
m. This indicates that the KR04 thrust sheet was thrust over the upper footwall flat of KR03 at an earlier stage compared to a probably longer time of deposition in the piggyback basin of KR04. The c. 20° northerly dip-
ping inclination of the KR03 footwall flat and related
parallel structures is due to the bend caused by the propagation of KR02 along the footwall ramp. The main décollement level below the Kramrende Section is situated at the 30 m level.
Sedimentary units
The description of the sedimentary units in the Kram-
rende Section is mainly based on sedimentological
Fig. 70. The KR01 footwall syncline
developed below the KR01 footwall
ramp ( KR01FWR ), which is overlain by
the KR02 hanging-wall flat (
KR02HWF
).
Note how the mobilised mud migrated
from the steeply dipping limb of the
footwall syncline up into the Kramrende
diapir, intrusively penetrating the thrust
fault. Photograph: June 1995.
Fig. 71. Mobilised mud from the lower
part of the Lønstrup Klint Formation in
the KR02 thrust sheet intruded the
turbidite sand beds in the upper part of
the formation. Photograph: June 1995.
87
logging of the Lønstrup Klint Formation in the KR01
thrust sheet (Fig. 21). The detailed section of the Ru- bjerg Knude Formation at the top of this log is uncer- tain due to poor exposure and dif ficulty of access. The Rubjerg Knude Formation exhibits variations in thickness throughout the Kramrende Section, and the description herein is based on scattered observations. A c. 1 m thick homogeneous, structureless sandy till caps the Kramrende Section. No preferred clast fabric has been recognised in the till, and its stratigraphic position is uncertain, although the occurrence of rare rhomb porphyry erratics may indicate an affinity with the Norwegian Ice (Kattegat Till Formation).
Lønstrup Klint Formation
In the Kramrende Section, the lower part of the Løn-
strup Klint Formation mainly occurs in the Kramrende diapir, within the KR02-03 thrust sheets. Remobilisa- tion of the mud has obliterated primary sedimentary structures, and the diapirism also affected the thrust sheet KR03, so that only primary bedding is recognis- able in the uppermost part of the formation. The pri- mary sedimentary structures of the upper part of the Lønstrup Klint Formation are reasonably preserved in the KR01 thrust sheet (Fig. 20), although the sediments here, dominantly constituting sandy turbidite beds (10- 50 cm thick), are strongly affected by hydrodynamic brecciation creating ball-and-pillow structures (Fig. 68).
The top of the Lønstrup Klint Formation in the Kram-
rende Section is truncated by the L/R-unconformity,
which displays an erosional relief of 1-2 m.
Rubjerg Knude Formation
The Rubjerg Knude Formation varies in thickness from
only 6-8 m at the top of the KR03 thrust sheet to about 20 m in the upper part of the KR04 thrust sheet (it is absent in KR02). The main part of the formation comprises thick-bedded, large-scale cross-bedded, medium-grained light yellow-grey sand. Some beds are rich in heavy mineral sand, which occurs in paral- lel-laminated strata. In the KR04 thrust sheet, the heavy mineral beds are present about 6 m above the L/R- unconformity and again about15 m above the base. These beds have a characteristic content of small (0.1- 1 cm), grey clayey mud-clasts, which are interpreted to reflect erosion of muddy thrust sheet units in the vicinity of the depocentre.
Pedersen (1987) described deposits, referred here
to the Rubjerg Knude Formation, that accumulated
syntectonically in footwall growth synclines. The de- posits were characterised as 'banana' shaped basins, and a similar type of sedimentary/structural featur e occurs in the KR04 thrust sheet (Fig. 69). The Rubjerg Knude Formation at the top of the Kramrende Section can be regarded as a piggyback basin and the foot- wall syncline as a growth-fault syncline. At the top of the piggyback basin, large-scale trough cross-bedded sand is truncated by small satellite thrust faults (simi- lar to that shown in Fig. 69), which are truncated by superposed c. 1 m thick trough cross-bedded sand beds.
Three succeeding developments of this inter ference
between thrusting and deposition reflect the syntec- tonic depositional dynamics of the piggyback basin.
Structures
Structures of significance in the Kramrende Section
are described under the following headings: (1) thrust faults, and in particular associated footwall ramps and footwall synclines, (2) the Kramrende diapir, with the diapiric breccias and intrusive structures formed by mobilised mud, and (3) reverse faults, here interpre- ted as back-thrust faults.
Thrust faults
The KR01 thrust sheet is bounded by the hanging-
wall ramp and flat (KR01HWR and HWF) at the base, and the KR01 footwall ramp and flat at the top (KR01FWR and FWF). The wedge-shaped geometry of the KR01 tip implies that the KR01HWR had a low angle of inclination, dipping about 15°N. Towards the trailing end of the thrust sheet, the ramp passes into a hanging-wall flat which is parallel to bedding in the Lønstrup Klint Formation. This thrust fault now dips at 25°N, although it is a hanging-wall flat situated on a footwall flat. This is due to the fault-bend folding related to the thrusting in the trailing part of the Mar- tørv Bakker Section.
At its trailing end, the KR01 thrust sheet is folded
into a footwall syncline (Fig. 70). The bend of the
northern limb in the syncline lifted the L/R-uncon- formity up to a position nearly 5 m higher than in the horizontal involute part of the fold, and the bedding in the Lønstrup Klint Formation was tilted into a near- ly vertical position (Fig. 70).
88
The KR02 thrust sheet was thrust up along a
c.
25°
dipping footwall ramp (KR01FWR) onto the upper
footwall flat above the Rubjerg Knude Formation of the KR01 thrust sheet. The KR02 thrust fault is appar - ently a hanging-wall flat which indicates a rather long displacement for thrusting. The top sur face of KR02 is a footwall flat upon which the KR03 hanging-wall flat is situated, only bringing different stratigraphic levels of the Lønstrup Klint Formation into contact. The dip of the thrust fault is parallel to the dip of the KR02- KR01 thrust fault. The footwall flat of the KR03 thrust sheet is overlain by a c. 80 m long hanging-wall flat of KR04. The Lønstrup Klint Formation is only about 8- 10 m thick above the hanging-wall flat (KR04HWF), in-
dicating a fairly long inter mediate flat (at the 10 m
level below the reference surface). At the trailing end of KR04, the thickness increases indicating the pr es- ence of a hanging-wall ramp at the base of the thrust sheet, and a footwall syncline similar to that described in KR01 is present. In the upper part of the KR04 thrust sheet, the sediments deposited in the footwall growth syncline became overturned along the northern limb during translation of the hanging-wall ramp of BR01, as described above (Fig. 69).
Kramrende diapir
The Kramrende diapir constitutes the main part of
KR02. The diapirism also affected the trailing end of KR01 (Fig. 70) as well as some parts of KR03. As shown in Fig. 71, mud of the lower part of the Lønstrup Klint Formation in KR02 became mobilised and intruded the overlying turbidite sand beds and also penetrated upwards into the overlying KR03 thrust sheet. Figure 70 illustrates a thrust fault penetrated by intrusive mud at the footwall ramp of KR01. Here, the mobilised mud from the steeply inclined northern limb of the foot- wall syncline intruded into the mud-breccia along and above the hanging-wall flat of KR02. A large part of the boundary between KR02 and KR03 was deformed in a similar way and the primary layering destroyed.
Reverse faults
In the Kramrende Section, significant steeply dipping
reverse faults occur in the northern part of KR01 (Fig. 67), and in the middle part of the KR03 thrust sheet. The displacement is only about 30-50 cm on the steep south dipping faults in KR01; the spacing between the faults varies from 3-9 m, and often the faults can be traced down into the tectonic breccia above the
Fig. 72. Reverse fault-splay fan developed on the back of
KR03
and also displacing the overlying
KR04
thrust sheet. The structure
is interpreted as a back-thrust fault-splay formed during the KR03 propagation over the upper footwall ramp situated on the back of
KR02. Photograph: July 1994; figure at fault-splay centre for scale.
89
hanging-wall flat. In the KR03 thrust sheet, the reverse
faults form a fault splay fan with individual faults dip-
ping moderately to steeply to the south (Fig. 72); dis- placement varies from about 20 cm up to about 3 m.
The reverse faults appear to have formed during
thrust-sheet propagation over a ramp hinge and are
interpreted as back thrusts. A bend over a shallow dipping ramp will only result in minor displacement on steeply dipping back thrusts, whereas bending over steeply dipping ramps creates low-angle back thrusts with potentially greater displacements.
Interpretation of structural development
The balanced cross-section indicates that the KR01
thrust sheet was about 350 m long, of which a major part of the front tip has been eroded away. The amount of displacement is deduced from a series of balanced approximations to be 160 m (see Plate 2). The foot- wall ramp of KR01 is interpreted to root in the 30 m
décollement level, which indicates that the lower hang-
ing-wall ramp of KR01 was displaced onto the inter- mediate footwall flat above the trailing segment of MB04. Thus the lift and steep tilt of the northern limb in the KR01 footwall syncline is interpreted to have formed during the displacement of the lower hang- ing-wall ramp (KR01HWR) along the trailing-end foot- wall flat of MB04 (MB04FWF).
The tip of the KR02 thrust sheet has been eroded
away. To avoid exaggeration, the thrust fault is inter-
preted to have continued only about 15 m up in the air further to the south, which implies that displace- ment of KR02 was in the order of 50 m. The main part of the KR02 thrust sheet present in the cross-section is above the hanging-wall flat brought up from the 30 m décollement level. It is evident that the mobilised mud was derived from this low level and that it was activated in diapirism during the thrust-sheet propa- gation over the footwall ramps (KR01FWR) and its hinge bend.
It is difficult to estimate the displacement for the
Fig. 73. The Brede Rende diapir in the frontal part of the Brede Rende Section. The frontal part of the
BR02
thrust sheet was thrust
up on its hanging-wall ramp (
BR02HWR
) along the footwall ramp, which turned into the
KR04
footwall flat (
KR04FWF
). At an
early stage of thrusting, probably while the hanging-wall ramp passed by a lower footwall hinge, diapirism developed. The mobil-
ised mud also intruded the L/R-unconformity and formed mushroom-shaped diapirs in the Rubjerg Knude Formation. Photograph:
June 1984. |