barred beaches - universiteit twente · 2020. 4. 6. · barred beaches kathelijne m. wijnberg*,...
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Barred beaches
Kathelijne M. Wijnberg*, Aart Kroon
Department of Physical Geography, Institute for Marine and Atmospheric Research, Utrecht University, P.O. Box 80115,
3508 TC Utrecht, The Netherlands
Received 23 November 1999; received in revised form 23 June 2000; accepted 24 January 2002
Abstract
Seven different bar types are distinguished to provide a framework for comparing morphodynamic studies conducted in
different areas. Five types occur in semiprotected or open coast settings, of which two are intertidal and three are subtidal. Two
types occur in highly protected settings. The occurrence of a certain bar type is generally determined by the wave energy and tidal
range, although the nearshore slope may also be a differentiating boundary condition. The theory behind the generation, evolution
and decay of bars has evolved most for the subtidal bars in the semiprotected and open coast settings, for which three types of
competing mechanisms have been formulated (breakpoint, infragravity waves, self-organisational). Most research has focused on
these processes on the time scale of storm events and post-storm recovery. However, to understand the longer-term behavior of bar
systems, knowledge of the role of relaxation time andmorphologic feedback is needed as well. At present, such knowledge is very
limited. We think it can best be obtained from the analysis of long time series of morphology and forcing conditions, rather than
from intensive field experiments. In case of a feedback-dominated response (self-organisational), we expect to find no correlation
between the time series of external forcing and the morphologic response. In case of a relaxation time-dominated response, we do
expect to find such a correlation, albeit filtered. This discussion is illustrated by a case study of the Dutch coast.
D 2002 Elsevier Science B.V. All rights reserved.
Keywords: Coastal morphology; Nearshore bar; Feedback; Relaxation time
1. Introduction
Sandy beaches are among the most widely studied
types of shore in process-oriented coastal geomorpho-
logic research. Nearshore bars in both the intertidal
and subtidal domains are common features on these
types of coast (Table 1). Nearshore bars exist under a
wide range of hydrodynamic regimes, ranging from
microtidal to macrotidal and from swell-dominated to
storm-dominated wave environments. All nearshore
bars are affected by the flow field induced by the
incident waves. Because of their close relationship
with wave-induced flow fields, nearshore bars are also
referred to as wave-formed bars (Greenwood and
Davidson-Arnott, 1979). The incident waves shoal,
break, reflect, and refract on the nearshore topogra-
phy, generating complex flow fields, including asym-
metric oscillatory flow, undertow, horizontal cell
circulation, edge waves, and swash–backwash mo-
tion. The local tidal range and the wave climate de-
termine the frequency and intensity with which
nearshore bars along individual beaches are affected
by the various types of flow field.
0169-555X/02/$ - see front matter D 2002 Elsevier Science B.V. All rights reserved.
PII: S0169 -555X(02 )00177 -0
* Corresponding author. Fax: +31-30-2540604.
E-mail addresses: [email protected] (K.M. Wijnberg),
[email protected] (A. Kroon).
www.elsevier.com/locate/geomorph
Geomorphology 48 (2002) 103–120
Notwithstanding their common occurrence and the
considerable existing research on these features, near-
shore bars are still poorly understood. The prime
concern of this paper is to review the present knowl-
edge of wave-formed bars using the framework of the
morphodynamic system approach. This approach
helps to highlight an area of research that is poten-
tially fruitful for deepening our understanding of
nearshore bars and their behavior.
A nearshore morphodynamic system consists of
three components: the water motion component, the
sediment transport component, and the morphology
component (Fig. 1). Energy input into the nearshore
morphodynamic system, through waves, winds, and
tides, induces a flow field in the nearshore zone that is
modulated by the nearshore morphology. This flow
field induces sediment transport, which will result in
bathymetric change if transport gradients exist. This
modification of the morphology will change the
modulation of the incoming energy, and consequently,
the nearshore flow field. The boundary conditions for
the nearshore morphodynamic system are imposed by
the long-term evolution of the coast on the one hand,
through the composition of the substrate and the
geometric setting (offshore and nearshore slope,
shoreline orientation), and, on the other hand, by the
geographic location and geometry of the sea or ocean
basin (prevailing weather systems, fetch, tidal wave
characteristics).
From the above perspective, it is apparent that the
nearshore system can be studied on two levels. On
the most aggregated level, the focus is on the general
expression of the morphodynamic system as a func-
tion of a set of boundary conditions, i.e., the aim is
to identify different bar types with different behavior
in relation to environmental parameters (cf. bar type
X with dynamics Y only occurs on coasts with tidal
range A and nearshore slope B). On the more detailed
level, the morphodynamic relationships in the system
itself are studied for each specific bar type. Of
course, the physics of water motion and sediment
transport is the same in every nearshore zone, but
Table 1
Examples of locations of nearshore bar observation
Geographic location References
Atlantic Ocean
(USA, Europe)
Strahler, 1966; Sonu and van Beek, 1971; Sonu, 1973; Nordstrom, 1980;
Sallenger et al., 1985; Froidefond et al., 1990; Larson and Kraus, 1992; Liu and Zarillo, 1993
Baltic Sea Pruszak et al., 1997
Beaufort Sea Short, 1975
Black Sea Zenkovich, 1967
Chukchi Sea Short, 1975
Gulf of St. Lawrence Owens and Frobel, 1977; Greenwood and Mittler, 1984
Gulf of Mexico Davis and Fox, 1975
Indian Ocean (Australia) Wright and Short, 1984
Lake Michigan Davis et al., 1972; Weishar and Wood, 1983
Mediterranean King and Williams, 1949; Bowman and Goldsmith, 1983; Guillen en Palanques, 1993;
Barusseau et al., 1994; Aminti et al., 1996
North Sea King and Barnes, 1964; Aagaard, 1990; Ruessink and Kroon, 1994; Wijnberg and Terwindt, 1995;
Dette et al., 1996; Simmonds et al., 1997
Pacific Ocean (USA, Japan) Shepard, 1950; Hunter et al., 1979; Sunamura, 1988
Sea of Japan Sunamura, 1988
Tasman Sea Chapell and Eliot, 1979; Wright and Short, 1984
Fig. 1. Conceptual diagram of nearshore morphodynamic system of
a sandy coastal system. WM=water motion, ST= sediment trans-
port, M=morphology.
K.M. Wijnberg, A. Kroon / Geomorphology 48 (2002) 103–120104
apparently different terms in the nonlinear equations
describing flow–topography interaction and sediment
transport are dominant for different sets of boundary
conditions.
In this paper, barred beaches are first addressed on
the most aggregated level. An overview is presented
of the full range of nearshore bar types reported in the
literature. Morphologic characteristics and environ-
mental setting of the various bar types are summar-
ised. Next, nearshore bars are addressed on the more
detailed level of the morphodynamic relationships,
focusing on the most widely studied types of near-
shore bar, namely, the bars on semiprotected to fully
open coasts. These relationships relate to time scales
on which bars have been observed to respond, that is,
the time scale of a storm event and the post-storm
recovery phase. This is followed by a discussion of
the dynamics of nearshore bars on longer time scales,
which result from the integrated effect of many storm-
recovery sequences. Issues discussed are the effects of
relaxation time and morphologic feedback. This dis-
cussion will be illustrated by a case study of the Dutch
coast.
2. Types of wave-formed nearshore bars
Nearshore bars are dynamic features which may
change their plan view shape, amplitude or cross-
shore position in response to changing wave condi-
tions. This results in what is apparently a continuum
of bar morphologies. For example, the plan view
shape of bars may be linear, crescentic, or undulating
in a more irregular manner (Figs. 2, 3, and 4). The
orientation of nearshore bars varies from shore-paral-
lel to shore-perpendicular. In addition, nearshore bars
can occur in a cross-shore ordered series of essentially
shore-parallel bars, in which case the set of bars is
referred to as a multiple or multi-bar system.
It is not a trivial task to set up a classification
scheme to cover the wide variety of nearshore bar
shapes. A classification of nearshore bars in terms of
distinctive bar types should provide a framework for
making sensible comparisons between morphody-
namic studies conducted in different areas. Generally,
criteria used to classify nearshore bars are based on
morphological and locational characteristics, such as
plan view shape and cross-shore position in the
nearshore zone (e.g., Greenwood and Davidson-
Arnott, 1979; Chapell and Eliot, 1979; Wright and
Short, 1984; Lippmann and Holman, 1990). These
criteria are implicitly or explicitly assumed to reflect
the processes that control the bar behavior. At present,
no worldwide applicable, universal classification of
wave-formed nearshore bars is available because there
is still an ongoing debate on the mechanisms that
govern nearshore bar formation and development.
The vast majority of studies on nearshore bars deal
with bars on semiprotected and open coast beaches,
i.e., beaches facing oceans, seas, or vast inland lakes
like the Great Lakes in North America. Some of these
beaches may be sheltered from large waves from
certain directions, but all are exposed to moderate to
high wave conditions from at least one directional
sector. A limited number of studies report on wave-
formed nearshore sand bars in highly protected set-
tings such as back-barrier lagoons, estuaries, and
sheltered embayments like Cape Cod Bay (Nilsson,
1972). These differences in environmental setting
seem to warrant a distinction between bars formed
on semiprotected and open coast beaches and bars
formed in highly protected settings.
Because of the bias in the literature, this paper will
pay attention mainly to bars on semiprotected and
open coast beaches. A classification of bars in this
type of setting is presented in the next section. Based
on only scarce literature, two types of bars are
described for the highly protected setting.
2.1. Bars on semiprotected and open coasts
We use locational characteristics as the main attrib-
ute for describing bar types in the semiprotected and
open coast setting, and morphology as the subordinate
attribute (Table 2). The positioning of a bar in the
nearshore strongly reflects water depth characteristics,
which in turn reflects a typical flow field regime for
that location. On the highest level, intertidal bars are
distinguished from subtidal bars. Bars in the intertidal
zone are affected by swash processes and currents
induced by the filling and emptying of trough features
as the tide rises and falls. These processes are absent
in the subtidal zone. In the subtidal zone, the flow
field induced by the shoaling and breaking of waves is
assumed to be dominant. Tides and winds are
assumed to act only as modifiers of this flow field,
K.M. Wijnberg, A. Kroon / Geomorphology 48 (2002) 103–120 105
e.g., through changes in the water level (tidal cycle,
wind set-up/set-down), through adding additional
longshore current vectors, or through the effect of
winds on wave breaking. On a more refined level,
bars will experience a range of hydrodynamic pro-
cesses that depend on tidal range and wave climate.
For instance, a bar located in the lower intertidal zone
of a macrotidal beach will experience both intertidal
and subtidal processes. Bar morphology may then
express the flow field mode that dominates in a given
situation.
2.1.1. Morphologic characteristics and environmental
setting of intertidal bars
Two morphological subtypes of intertidal near-
shore bars can be distinguished: ‘‘slip-face ridges’’
and ‘‘low-amplitude ridges.’’ We abandoned more
commonly used terminology, such as ‘‘swash bar’’
or ‘‘ridge-and-runnel topography,’’ because various
authors applied that terminology with different inter-
pretations (see Orford and Wright, 1978).
Slip-face ridges are intertidal bars with a well-
defined, landward-facing slip-face. They include the
Fig. 2. Time exposures pictures of the surf zone near Noordwijk, The Netherlands (September 9, 1995); the white bands are preferred locations
of wave breaking and as such reflect the plan shape pattern of the underlying bar topography: (a) oblique image, (b) rectified image; tickmark
spacing is 250 m.
K.M. Wijnberg, A. Kroon / Geomorphology 48 (2002) 103–120106
Group II bars defined by Greenwood and Davidson-
Arnott (1979), which were named ‘‘swash bars’’ by
Carter (1988). In addition, they include the bar type
occurring in the ‘‘Ridge-and-Runnel/Low-Tide-Ter-
race’’ beach state defined by Wright and Short
(1984). The typical cross-shore scale of slip-face
ridges is of order 101 m. The bar height, defined as
the elevation difference between the crest of the ridge
and the trough area landward of it (also called runnel),
is of the order of tens of centimeters to well over a
meter. Slip-face ridges are elongated features that tend
to line up with the general shoreline configuration.
However, these intertidal ridges may also be shore-
oblique, spit-shaped features (Fig. 5). Slip-face ridges
are often cut by small rip channels, which drain the
shallow trough landward of it. The spacing of these
drainage rips may vary from several tens of meters to
a couple of hundred meters (Short, 1985). Slip-face
ridges may migrate onshore at rates of order 100 m
day � 1 (Owens and Frobel, 1977; Kroon, 1994).
During appropriate conditions, the ridge will become
stranded at the high tide mark where they form a
‘berm’. Slip-face ridges occur on mild slopes of order
0.01–0.03 generally under microtidal to mesotidal
regimes (King and Williams, 1949; Davis et al.,
1972).
Fig. 3. Time exposures pictures of the surf zone of Palm Beach (NSW), Australia (March 17, 1996); the white bands are preferred locations of
wave breaking and as such reflect the plan shape pattern of the underlying bar topography: (a) oblique image, (b) rectified image; tickmark
spacing is 80 m.
K.M. Wijnberg, A. Kroon / Geomorphology 48 (2002) 103–120 107
Low-amplitude ridges are intertidal bar features
without a slip-face. They generally occur in a cross-
shore sequence of shore-parallel ridges that align with
the general shoreline planform. Many ridges remain
apparently static and only respond to movements of
the still water level as they migrate with spring–neap
tidal movement (Orford and Wright, 1978). This type
of intertidal bar morphology is the same as the ridge-
and-runnel topography described by King and Wil-
liams (1949). It also includes the ‘‘Group II’’ bars
defined by Short (1991) for intermediate wave energy,
meso- and macrotidal beaches, as well as the Group I
bars defined by Greenwood and Davidson-Arnott
(1979). In cross-section, the ridges may be asymmet-
ric in landward direction (Greenwood and Davidson-
Arnott, 1979; Short, 1991). Their height is at most a
few tens of centimeters (Short, 1991) and their cross-
shore width is at most a few tens of meters. They
occur on lower angle slopes than those associated
with slip-face ridges, with beach gradients of about
0.005–0.01. Generally, the smaller beach slopes are
related to a larger tidal range, such that low-amplitude
Fig. 4. Time exposures pictures of the surf zone of Agate Beach (Oregon), USA (April 24, 1994); the white bands are preferred locations of
wave breaking and as such reflect the plan shape pattern of the underlying bar topography: (a) oblique image, (b) rectified image; tickmark
spacing is 250 m.
K.M. Wijnberg, A. Kroon / Geomorphology 48 (2002) 103–120108
ridges may be expected under meso- to macrotidal
conditions. In addition, the formation of these ridges
tends to be restricted to sea environments, as opposed
to swell (Short, 1991). Note that low angle slopes may
also occur under microtidal conditions in low wave
energy environments (see Section 2.2).
2.1.2. Morphologic characteristics and environmental
setting of subtidal bars
Subtidal nearshore bars are found both in single-
and multi-bar settings, the latter typically consisting of
two to four bars (Greenwood and Davidson-Arnott,
1979). Subtidal bars are found on nearshore slopes
with gradients of order 0.005–0.03 (Short and
Aagaard, 1993; Ruessink and Kroon, 1994). The
gentler nearshore slopes seem to favor a larger num-
ber of bars, although there is no unique relation
between these two factors (Davidson-Arnott, 1987;
Short and Aagaard, 1993; Wijnberg, 1995). The cross-
shore spacing between bars in multi-bar systems is of
order 101–102 m and increases in the offshore direc-
tion. The height of this bar type is of order 10� 1–100
m. For example, bar heights of up to 3 m have been
reported for the Terschelling coast, The Netherlands
(Ruessink and Kroon, 1994). Bar height tends to
increase with distance offshore (Komar, 1998). How-
ever, in multi-bar systems, this trend often reverses at
some distance offshore (Lippmann et al., 1993; Rues-
sink and Kroon, 1994; Wijnberg and Terwindt, 1995;
Pruszak et al., 1997).
Subtidal nearshore bars may migrate both onshore
and offshore. Near Duck, NC (USA), offshore migra-
tion rates of up to 2.2 m h� 1 were observed (Sal-
lenger et al., 1985). Onshore migration rates are
generally slower, namely, of order 10 � 1 m h � 1
(Sunamura and Takeda, 1984). However, onshore
migration rates may locally be as large as 1 m h� 1
when related to the development of crescentic top-
ography (Sallenger et al., 1985).
Subtidal nearshore bars are most commonly
studied in nontidal to microtidal environments, but
Table 2
Classification of nearshore bars on sandy coasts with indication of environmental setting
Fig. 5. Intertidal slip-face ridges near Noordwijk, The Netherlands:
(a) shore-oblique orientation (May 26, 1995), (b) shore-parallel
orientation (December 28, 1997).
K.M. Wijnberg, A. Kroon / Geomorphology 48 (2002) 103–120 109
their occurrence is not limited to these settings (e.g.,
Davidson et al., 1997). The influence of tidal range on
subtidal bars is not clear. Wright et al. (1987) suggest
that a larger tidal range may be associated with more
subdued bar–trough topography. However, their con-
clusion is based on variation of bar topography over
spring–neap cycles on a microtidal coast.
The morphological appearance of a subtidal near-
shore bar is highly variable. Based on plan view
characteristics, we distinguish three families of bar
morphology: two-dimensional longshore bars, three-
dimensional longshore bars, and shore-attached bars.
A two-dimensional longshore bar is a uniform,
straight bar oriented parallel to the shoreline. It
resembles the bar morphology in the so-called Long-
shore-Bar-and-Trough state defined by Wright and
Short (1984).
A three-dimensional longshore bar is any non-
straight bar where the onshore protruding parts do
not attach to the shore; that is, these parts are
separated from the beach by a distinct trough feature.
Longshore variability may range from regular cres-
centic patterns, which may be skewed (cf. Rhythmic-
Bar-and-Beach state defined by Wright and Short,
1984), to highly irregular and complex patterns (cf.
‘‘non-rhythmic 3D bar’’ state defined by Lippmann
and Holman, 1990). Length scales of longshore var-
iability are of order 102–103 m, where larger scales
tend to be related to bars located farther offshore (e.g.,
Sonu, 1973; Bowman and Goldsmith, 1983). Due to
the limited understanding of the mechanisms control-
ling the wide variety of three-dimensional patterns, we
could not justify a distinction between different types
of three-dimensionality.
The shore-attached bars are, as expressed by their
name, bar features that are attached to the shore.
Generally, they are located just below the low-tide
water level. Their morphology is to a large extent
defined by well-developed rip and feeder channels
(see Fig. 3b, a shore-attached bar is present in the
forefront of the oblique image and on the left side in
the rectified image). The rip channels are oriented
perpendicularly or obliquely to the shore (cf. ‘‘Trans-
verse-Bar-and-Rip’’ state defined by Wright and
Short, 1984; and the bar–rip systems described by
Hunter et al., 1979). In these systems, bars are almost
parallel to the shore, but they attach to the shore at one
end and terminate by a rip channel at the other end. A
measure for the longshore length scales of the shore-
attached bars is rip spacing, which is generally of
order 101–102 m (e.g. Hunter et al., 1979; Wright and
Short, 1984). It should be noted that the place where
the bar attaches to the shore may partially emerge at
low tide, inducing a low-tide shoreline with a some-
what cuspate appearance (Hunter et al., 1979).
The three bar types described above largely resem-
ble three of the states of the Wright and Short (1984)
bar-beach state model. Wright and Short found a
correlation between the occurrence of these states
and the value of the Dean parameter X (X =Hb/xsT,
with Hb = breaker height [m], xs = sediment fall veloc-
ity [m s � 1], T =wave period [s]). Therefore, the
occurrence of our three types of plan shape morphol-
ogy should probably correlate with X, too. If so, two-
dimensional longshore bars would tend to be related
to higher values of X than three-dimensional long-
shore bars, which should be related to higher X values
than shore-attached bars. Since the value of X is most
sensitive to breaker height (Short and Aagaard, 1993),
the above sequence can also be interpreted in terms of
decreasing levels of wave energy (Table 2). For
Australian single-bar beaches, distinct X-threshold
values were determined, but the universal validity of
these threshold values is still in question (Short and
Aagaard, 1993).
2.2. Bars on highly protected coasts
The nearshore bars observed in back-barrier
lagoons, estuaries, and sheltered embayments (low
wave energy environments) only occur on gentle
nearshore slopes (Table 2). Two types of bars may
occur: ‘multiple parallel bars’ and ‘transverse bars’
(Greenwood and Davidson-Arnott, 1979). To prevent
confusion with terminology often applied in open
coast bar classification, we refer to the latter bar type
as ‘transverse finger bars’ (after Niederoda and Tan-
ner, 1970).
In plan view, multiple parallel bars are straight to
undulating features that are often oriented parallel to
the shoreline, although they also may occur at an
angle with the shoreline (Nilsson, 1972). The multiple
parallel bars are spaced more or less equidistantly,
with a spacing in the order of 101 m and a longshore
length scale of 100 m (Zenkovitch, 1967; Nilsson,
1972; Greenwood and Davidson-Arnott, 1979). The
K.M. Wijnberg, A. Kroon / Geomorphology 48 (2002) 103–120110
number of bars is on the order of 4–10 (Greenwood
and Davidson-Arnott, 1979), but it may be as large as
30 (Nilsson, 1972). In cross-section, this bar type is
generally symmetric, and the height of the ridges, on
the order of 10 � 1 m, is nearly uniform offshore
(Greenwood and Davidson-Arnott, 1979). Some
uncertainty exists about the characteristic tidal range
for this bar type. Greenwood and Davidson-Arnott
(1979) mention a small tidal range as the characteristic
environmental setting, whereas Nilsson (1972) states
that a large tidal range is required. More recently,
Short (1991) observed that multiple low-amplitude
bars that occur on wide, flat intertidal slopes of
macrotidal, low wave energy beaches (‘Group III’
bars) are morphologically similar to the multiple
parallel bars that occur subtidally on low-energy
microtidal beaches. No indication is given whether
these bars are also genetically similar.
The transverse finger bars are linear features
oriented perpendicular to or at a high angle to the
shoreline. They have a typical length scale of 102 m,
where very long bars tend to have forked ends at the
seaward side (Niederoda and Tanner, 1970). The
longshore spacing of these transverse bars ranges
from 101 to 102 m, with bar heights on the order of
10� 1 m (Greenwood and Davidson-Arnott, 1979).
Prerequisites for the occurrence of transverse finger
bars are a small tidal range, small nearshore slopes,
and the low wave energy (Niederoda, 1972; Green-
wood and Davidson-Arnott, 1979).
3. Morphodynamics of intertidal ridges
3.1. Generation of intertidal ridges
The formation of intertidal slip-face ridges is
associated with storm activity (e.g., Davis et al.,
1972). During the storm, the beach erodes, becomes
planar or concave, and the sediment is deposited in the
low-tide area. In the days following a storm, an initial
ridge feature is formed. The exact mechanism for the
initial ridge formation is not known, but swash and
backwash processes seem to play an important role in
combination with the temporary still stand of the
water level around low tide (Kroon, 1994). The land-
ward-directed swash velocity near the bed exceeds the
seaward-directed backwash velocity due to the wave
asymmetry effect. Part of the volume of the swash
may infiltrate into the beach and thus does not flow
seawards as backwash. On beaches with a gentle to
moderate slope, these differences between swash and
backwash transport capacities may result in initial
ridge formation near the water level. On steeper
beaches, this process leads to the direct development
of a berm (e.g., Sonu and van Beek, 1971). Other
studies suggest that these ridges are formed as bars in
the subtidal zone and migrate onshore into the inter-
tidal zone (e.g., Davis et al., 1972; Aagaard et al.,
1998).
The development of an initial ridge feature occurs
over several tidal cycles. At first, the dominant pro-
cesses are still swash and backwash over the crest. At
some point, the height of the ridge is such that the
swash water that overtops the crest is trapped in the
depression landward of the ridge and no longer flows
back to sea as backwash. The water in the depressed
area eventually flows back to sea through small rip
channels. At this stage, the ridge develops a landward-
facing slip-face. An incompletely eroded ridge feature
on the middle or upper intertidal beach (see Section
3.2) may serve as an ‘initial ridge feature’ away from
the low-tide area (Kroon, 1994). Therefore, the build
up of a slip-face ridge may also be observed away
from the low-tide area.
The generation of the multiple low-amplitude
ridges has not been satisfactorily explained. King
and Williams (1949) suggested that the formation of
these bars could be related to the local process of
beach gradient adjustment at temporary still stands of
the water level such as those that occur during low
and high, spring or neap tides. Simmonds et al. (1997)
argue that this is an unlikely mechanism because of
the large variation in the number of ridges observed
on natural beaches. They suggest that the multiple bar
formation could be enforced by cross-shore standing
long waves.
3.2. Evolution of intertidal ridges
Once an initial intertidal slip-face ridge is present,
and provided the wave-energy level remains low to
moderate, the slip-face ridge will migrate onshore or
stabilise (e.g., Davis et al., 1972; Mulrennan, 1992;
Kroon, 1994). Migration of the ridge in the landward
direction occurs as long as the swash can overtop the
K.M. Wijnberg, A. Kroon / Geomorphology 48 (2002) 103–120 111
ridge crest. Sedimentary structures show that this
onshore migration is a coherent progradation of the
complete slip-face (Dabrio and Polo, 1981). Stabilisa-
tion of the ridge feature may occur when the elevation
of successive maximum high water levels decreases,
which happens when moving from spring tide to neap
tide conditions (Kroon, 1994). This implies that over-
topping of the bar crest by the swash ceases, but
swash and backwash processes are still active on the
seaward slope of the bar. This may result in an overall
increase in elevation of the feature due to accretion on
the seaward side of the ridge and to steepening of the
foreshore. This resembles the beach face development
during accretionary conditions (e.g., Sonu, 1973).
Little is known about the evolution of low-ampli-
tude ridges, other than that they seem to migrate with
spring–neap tidal movement (Orford and Wright,
1978).
3.3. Decay of intertidal ridges
The decay of an intertidal slip-face ridge is related
to high-energy wave conditions (Davis et al., 1972;
Owens and Frobel, 1977; Kroon, 1994). With an
increase in wave energy, the wave set-up becomes
larger and the higher energy conditions are often
accompanied by an additional wind set up. This
implies that processes like undertow may temporarily
become dominant over the intertidal beach, especially
during high tide, which apparently results in a flat-
tening of the beach (Kroon, 1994). However, no exact
mechanism is given that explains the divergence of
transport over the ridge crests.
The decay of low-amplitude ridges is also related
to high-energy wave conditions (e.g., King and Wil-
liams, 1949), but knowledge of the exact mechanism
is lacking.
4. Morphodynamics of subtidal bars
4.1. Generation of subtidal nearshore bars
Over the past decades, a variety of mechanisms
have been proposed to explain the generation of
subtidal nearshore bars. These mechanisms can be
placed into three general groups: breakpoint-related
mechanisms, infragravity wave-related mechanisms,
and self-organisational mechanisms. The first two
types of mechanisms have been most widely explored.
Although fundamental differences exist between these
two mechanisms, both start off from the same concept
that bars form because a template in the flow field is
imprinted on the seabed. The self-organisational
mechanisms, on the contrary, are based on the concept
that the formation of bars occurs completely due to
interaction between nonlinear flow and topography,
without any predefined template in the flow field. So,
starting from a barless and completely smooth profile,
self-organisational mechanisms cannot form bars
while the other mechanisms can. Note that in reality
there will never be a lack of perturbations on a
nearshore profile.
Breakpoint-related mechanisms predict longshore
bar formation (two-dimensional) where short period
incident waves (sea and swell) initially break, that is,
at the breakpoint. All proposed concepts suggest that
bar formation depends in some way on gradients of
processes occurring in the vicinity of the breakpoint
(e.g., King and Williams, 1949; Dyhr-Nielsen and
Sørensen, 1970; Dally and Dean, 1984; Stive, 1986;
Sallenger and Howd, 1989). These gradients may
relate to a single process (e.g., scouring by the action
of plunging breakers) as well as to the transport
processes induced by a composite flow field (e.g.,
cross-shore gradients induced by the combined effect
of undertow and wave asymmetry). The latter
approach has even been extended to include the effect
of long period waves on the nearshore flow field
(Roelvink and Stive, 1989). That study suggested that
two-dimensional bar formation could be related to the
transition of horizontally asymmetric, groupy, non-
breaking waves to vertically asymmetric, surf-beat
modulated breaking waves. Therefore, this hybrid
model is still considered an exponent of bar formation
near the breakpoint. According to the breakpoint
concept, multiple subtidal nearshore bars should form
due to multiple breakpoints related to the reformation
of broken waves. Flume tests showed evidence for
breakpoint mechanisms (Dally, 1987). In the past,
field observations have generally not been conclusive
(Sallenger and Howd, 1989), but more recent obser-
vations are suggestive of bar formation by the break-
point mechanism (Aagaard et al., 1998).
Infragravity wave-related mechanisms have the
potential to produce any of the three types of subtidal
K.M. Wijnberg, A. Kroon / Geomorphology 48 (2002) 103–120112
bar. Infragravity waves are long period waves (20–
300 s) and their existence is usually attributed to the
natural occurring groupiness of the incident, short
period waves (e.g., List, 1991; Roelvink, 1993; Rues-
sink, 1998). The long wave mechanism that has been
explored most widely, because it was suggested first,
is bar formation due to a second-order drift velocity
associated with standing long waves (Carter et al.,
1973). This mechanism predicts that two-dimensional
bars form under the nodal or antinodal location of
cross-shore standing infragravity waves (leaky waves)
(e.g., Short, 1975) or longshore progressive edge
waves (Bowen, 1980). Three-dimensional patterns
and shore-attached bars may form due the longshore
standing edge wave structures (Bowen and Inman,
1971; Holman and Bowen, 1982). The formation of
multiple subtidal nearshore bars is attributed to the
presence of multiple nodes or antinodes in the cross-
shore direction, related to the presence of leaky waves
or higher mode edge waves. The existence of low-
frequency water motions in the surf zone has been
confirmed on many occasions. However, although
some studies are suggestive of the correctness of the
edge wave mechanism (Bauer and Greenwood, 1990),
no firm evidence has been found for the actual forcing
of subtidal nearshore bars by this mechanism (Holman
and Sallenger, 1993).
A weak point of the second-order drift velocity
concept is the requirement of a single dominant
frequency, which is usually lacking in barred surf
zones. This problem does not exist for a more recently
proposed long wave mechanism, which relates two-
dimensional bar formation to the phase coupling
between the primary orbital motion of partially stand-
ing long waves and groupy short waves (O’Hare and
Huntley, 1994). Theoretically, the mechanism gener-
ates bars for a broad-band spectrum of long waves (as
usually observed in nature), especially when break-
point-forced long waves dominate over bound long
waves (O’Hare and Huntley, 1994). The present
literature, however, does not indicate this to be a
likely condition (Ruessink, 1998).
The conclusion of a lack of a single dominant
frequency in natural surf zones is often derived from
wave run-up spectra measured at the shoreline
(Bowen, 1997). However, theory shows that edge
waves may also be trapped and amplified on long-
shore currents (such that wave energy spectra offshore
will differ from those measured at the shoreline) and
form bars (Howd et al., 1992). Once formed, bars may
trap edge waves themselves (Bryan and Bowen,
1998). However, under realistic conditions concerning
the shape of the longshore current profile and the
presence of tidal modulations of the sea level, this
mechanism is unlikely to produce significant morpho-
logical change unless the current is very strong (Bryan
and Bowen, 1998).
Self-organisational mechanisms encompass a
range of mechanisms that are intended to be capable
of producing all three types of observed nearshore bar
patterns. Mechanisms proposed include nonlinear
interaction between the wave-driven longshore current
and the bed (Hino, 1974; Damgaard Christensen et al.,
1994; Falques et al., 1996) and the nonlinear inter-
action between shoaling, incident waves and the bed
(Boczar-Karakiewicz and Davidson-Arnott, 1987).
The self-organisational mechanisms are attractive
because they exploit the fact that the ubiquitous non-
linearities in sediment transport processes and surf
zone hydrodynamics have a large potential to induce
self-organised behavior. This approach implies that
the influence of the morphology on the local flow
field overwhelms the effect of preexisting structures in
the external hydrodynamic input (Fig. 1). This con-
cept may explain how different bar morphologies can
develop along a given coastline with virtually the
same overall characteristics concerning sediment,
nearshore slope, and wave conditions (e.g., Bowman
and Goldsmith, 1983; Wijnberg, 1995). However, part
of the bar characteristics predicted by the currently
existing nonlinear feedback models are not in line
with observations, such as the orientation of bars
relative to the longshore current (Damgaard Christen-
sen et al., 1994), or the scale of cross-shore spacing of
bars (Hulscher, 1996).
To conclude, no firm field evidence has been found
that justifies the selection of any of the individual
mechanisms as the nearshore bar-generating mecha-
nism. This may indicate that possibly all elements of
the flow field act in concert to form bars, rather than
having one dominant process. For instance, an ele-
ment of the nearshore flow field not mentioned so far
is the oscillatory motion in the far infragravity range,
having its origin, for example, in shear instabilities in
the longshore current (e.g., Bowen and Holman, 1989;
Dodd et al., 1992). These far infragravity motions can
K.M. Wijnberg, A. Kroon / Geomorphology 48 (2002) 103–120 113
contribute significantly to sediment transport in the
cross-shore direction and thus to the evolution of the
nearshore profile (Aagaard and Greenwood, 1995). It
is also possible that different mechanisms predomi-
nate in different settings (Aagaard et al., 1998). If so,
insight into such setting-dependent forcing mecha-
nisms could provide a useful basis for setting up an
improved bar classification.
4.2. Evolution of subtidal nearshore bars
The majority of proposed bar-generation mecha-
nisms form bars in the surf zone or at the outer limit of
the surf zone, often during fairly energetic conditions
(associated with the ‘dissipative assemblage’ of
Wright and Short, 1984). In nature, these energetic
conditions are generally of limited duration. When
wave energy level drops, bars may migrate onshore
and merge with the beach if wave energy drops
sufficiently (e.g., Wright and Short, 1984), they may
decay in situ (Larson and Kraus, 1992), or they may
get arrested when wave energy drops dramatically
(Short and Aagaard, 1993). Except for the latter case,
the final stage is an unbarred berm profile (associated
with the ‘reflective assemblage’ of Wright and Short,
1984).
In the case of onshore migration under falling wave
energy levels, bars tend to change in type, from the
two-dimensional longshore bar type to the three-
dimensional longshore bar type, to the shore-attached
bar type (e.g., Wright and Short, 1984; Lippmann and
Holman, 1990). Often, wave energy levels do not
drop low enough, or for long enough, to complete this
full sequence. As a consequence, subtidal bars
become permanent features that tend to shift between
two or all three morphologic subtypes.
The debate on the mechanisms that cause the
transitions between morphologic subtypes is as unde-
cided as that on generation mechanisms, as they tend
to be taken as equivalent. The flow template mecha-
nisms presume a dominant influence of the hydro-
dynamic input on the local flow field. This implies
that the variation in the external input will dominate
the influence of the morphology on the local flow
field, and hence, on the transport gradients (Fig. 1).
Therefore, according to the template mechanisms, a
change in bar type should be explicitly related to a
particular type of hydrodynamic input. For example,
Bauer and Greenwood (1990) related the development
from a two-dimensional bar to a three-dimensional bar
to forcing by an observed standing edge wave.
For self-organisational mechanisms, the dominance
of flow–topography feedback is self-evident because
it is the underlying concept for this mechanism. This
concept implies that the morphologic feedback effect
overwhelms the effect of the variation in the energy
input (Fig. 1). That is, energy input into the nearshore
system is needed to move the sediment, but the pattern
of transport gradients is determined by the preexisting
morphology. For example, longshore currents along a
two-dimensional bar may preferentially amplify irreg-
ularities in the crestline with specific wave lengths
(Deigaard et al., 1999).
It should be noted that the nearshore morphology
may change considerably without changing bar type.
For example, the spatial scale of longshore variability
of three-dimensional bars may evolve over time, and
bars may migrate in the longshore direction. The types
of processes that will govern these changes will differ
for each morphologic subtype, because each subtype
has its own process signature (Wright and Short,
1984). The flow field over two-dimensional longshore
bars will be rather uniform alongshore, and, under
dissipative conditions, vertical circulation will domi-
nate the flow field (Wright and Short, 1984). When
bars become more three-dimensional in shape, weak
to moderate rip circulation will prevail and rips will be
persistent in location (Wright and Short, 1984). The
dominant flow field over shore-attached bars will be a
strong rip circulation, such that horizontal circulation
will dominate the flow field (Hunter et al., 1979;
Wright and Short, 1984).
4.3. Decay of subtidal nearshore bars
Few studies address the decay of bar features.
Decay is not to be confused with the disappearance
of a bar feature due to the welding of the bar to the
beach. Some studies indicate that bar features may
decay under the action of highly asymmetric, non-
breaking waves (Larson and Kraus, 1992; Wijnberg,
1995, 1997; Ruessink, 1998). This seems in line with
the observation that the type of plan shape morphol-
ogy of subtidal nearshore bars is mainly a function of
breaker height (Short and Aagaard, 1993). This
implicitly suggests that bars do not decay in the
K.M. Wijnberg, A. Kroon / Geomorphology 48 (2002) 103–120114
breaking wave regime. However, the precise mecha-
nism of in situ bar decay is not yet clear.
5. Integrated, long-term nearshore bar dynamics:
a discussion
As reflected in the previous sections on the mor-
phodynamics of nearshore bars, most studies focus on
short-term morphodynamics which involve the
response of the nearshore morphology to individual
storm events and subsequent post-storm recovery.
Long-term bar system behavior is the result of many
storm-recovery sequences. Therefore, to arrive at
these large scales, the integrated effect of short-term
storm-recovery sequences needs to be understood.
In the simplest case, the response of the nearshore
morphodynamic system is dominated by variation in
the forcing of the system (Fig. 1), and the response is
more or less instantaneous. The relaxation time of the
system is small compared to the duration of the
forcing events. In this case, each forcing sequence is
uniquely related to a particular morphologic response
sequence; i.e., independent from the initial morpho-
logical condition, a given forcing sequence will pro-
duce one and the same morphological sequence.
In reality, the duration of events is often not long
enough to let the bar system reach an equilibrium with
the conditions (e.g., Bauer and Greenwood, 1990;
Holman and Sallenger, 1993). When the relaxation
time is large compared to the duration of the event, the
chronology in the forcing events becomes important
for understanding the evolution of the bar system. In
this case, the initial morphology is relevant for the
morphologic response sequence induced by a given
forcing sequence.
Interestingly, if a nearshore bar system is a feed-
back-dominated system, the initial morphological
condition is important, too, but the chronology of
wave events will only be of minor importance. The
evolution of such a system is largely dependent on the
preexisting morphology instead of on the details of
the forcing sequence. In this case, different forcing
sequences (but statistically similar) starting out on the
same initial morphology can produce similar sequen-
ces of morphologic response.
It is of crucial importance for predictive purposes
to know the extent to which the nearshore system is
dominated by morphologic feedback or by relaxation
time effects. In general, it is difficult to discriminate
between self-organised responses and relaxation time
effects from morphological observations during field
experiments because of their limited duration. A
possible approach to distinguish between relaxation
time effects and self-organised response in bar sys-
tem change is to analyse long time series of mor-
phologic evolution and forcing conditions. In case of
feedback-dominated, self-organised response, we
expect to find no correlation between the forcing
signal and the morphologic response. In the case of
relaxation time affected responses, however, we
expect to find a correlation with the forcing signal,
albeit filtered. The usefulness of this approach can be
illustrated by a case study of the decadal behavior of
multi-bar systems along the Holland coast (The
Netherlands).
Analysis of 28 years of annual bathymetric data
along the Holland coast (JARKUS data set) indicates
that the long-term behavior of multi-bar systems along
this coast exhibits characteristics of feedback-domi-
nated behavior (Wijnberg, 1995). Along the Holland
coast, two multi-bar systems (two to four bars) are
present, which are separated by a set of jetties that
extend about 2 km offshore. Both bar systems exhibit
systematic, cyclic behavior. All bars migrate in a net
offshore direction, with the outer bar decaying off-
shore and a new bar being generated near the shore-
line; this new bar also migrates net offshore, and so on
(e.g., De Vroeg, 1987; Kroon, 1994). This implies that
a given bar system configuration reappears on a
periodic basis. It should be noted that the observed
offshore migration is not an apparent migration due to
longshore migration of obliquely oriented bars. In one
bar system, this time period is about 4 years, whereas
in the other bar system, it takes about 15–18 years to
complete one cycle. This change in cycle period
occurs abruptly across the jetties (Wijnberg and Ter-
windt, 1995). Because both bar systems are forced by
the same sequence of wave conditions, the cyclicity in
the morphologic behavior cannot simply be explained
by a matching cyclicity in the forcing sequence.
Therefore, it seems inevitable to conclude that, in this
case, morphologic feedback plays a dominant role in
the response of the nearshore bar system.
A useful approach for further analysis of a feed-
back-dominated system is to identify the essential
K.M. Wijnberg, A. Kroon / Geomorphology 48 (2002) 103–120 115
feedback mechanisms. A simple model including
these mechanisms can then be used to explore the
stability of multi-bar system behavior. The feedback
in a multi-bar system consists of local flow–topog-
raphy interaction over individual bars but also
includes interaction between bars. Bars interact by
affecting the nearshore flow field in a global sense
(e.g., wave breaking over a bar reduces the wave
height experienced by a more landward located bar)
and by sediment exchange.
The above types of feedback can be illustrated by
the Holland coast case study. The cyclic behavior of
the Holland coast bar systems is essentially a cross-
shore redistribution of sediment (Wijnberg, 1995).
Fig. 6. Nearshore bathymetry along the North-Holland coast, The Netherlands (JARKUS database) in 1967 and 1973.
K.M. Wijnberg, A. Kroon / Geomorphology 48 (2002) 103–120116
Therefore, the sediment of the decaying outer bar is
apparently transported onshore and this sediment
somehow needs to be accommodated in the inner
nearshore zone, inducing morphologic change. The
sediment exchange interaction may also be of rele-
vance in the formation of the new bar near the shore-
line. Possibly, the inner bar does not form until
sufficient sediment can be eroded from the beach. If
so, we might expect to find a relation between inner
bar generation and long-term beach accretion, which
along the Holland coast tends to occur by intertidal
slip-face ridge stranding (Kroon, 1994). In that case, a
matching long-term cycle in intertidal slip-face ridge
behavior should be present. For example, in certain
stages of the long-term, subtidal bar cycle, intertidal
ridges might be less prone to erosion by storm events
(global flow–topography feedback). Another concept
for the formation of the new inner bar is that a slip-
face ridge near the low-tide level transforms into a
subtidal bar (local flow– topography feedback).
Because of its location near low-tide level, the slip-
face ridge will experience subtidal processes for a
large amount of the time. If this is true, this implies
that a continuum exists between the subtidal and
intertidal bar forms, because not only may bars
migrate from the intertidal into the subtidal zone, as
suggested by some authors (Section 3.1), but also the
other way around.
The Holland coast case study also illustrates the
necessity of considering large stretches of coast for
longer-term coastal behavior. For example, the abrupt-
ness of the change in bar cycle period across the
jetties, which is an essential indicator of the dominant
role of feedback, would have been missed if only a
single kilometer of coast had been considered. In
addition, the longshore coherence and regularity in
the cyclic behavior becomes especially apparent when
considering large stretches of coast. For example, the
net offshore progression of nearshore bars occasion-
ally gets out of phase in the longshore direction (i.e.,
some parts of the bar system temporarily move faster
than others), resulting in ‘outer bar’– ‘inner bar’
attachments (Fig. 6). As a result, the bar behavior
observed in two neighbouring stretches of coast can
locally deviate considerably over a period of many
years (Wijnberg and Wolf, 1994). On the large scale
and long term, however, the bar system behavior
appears to be very systematic and coherent and the
bar attachment events are only details of the full bar
system dynamics (see Wijnberg and Terwindt, 1995).
On the basis of the analysis of long-term morpho-
logic data, combined with small-scale process knowl-
edge, conceptual bar behavior models can be
formulated. To further explore the realm of long-term
bar dynamics, such models should be translated into
simple simulation models (e.g., Plant et al., 1999).
These models may build on first principle physics (cf.
Hulscher et al., 1993), or use paramaterised sediment
transport relationships that are derived from field
experiments (e.g., Ruessink, 1998).
6. Conclusions
The sandy coast morphodynamic system is able to
express itself with a variety of nearshore bar types.
Based on the literature, seven types of bars are
distinguished (Table 2). These different expressions
of the nearshore morphodynamic system are associ-
ated with differences in boundary conditions concern-
ing wave energy, nearshore slope, and tidal range.
The specific morphodynamic relationships that
govern the formation and evolution of the different
bar types have been the subject of considerable
research to date. Most research has focused on under-
standing the processes and morphologic response on
the time scale of storm events and post-storm recov-
ery. Understanding the long-term behavior of bar
systems, however, also requires knowledge of more
generic properties of the nearshore morphodynamic
system such as the extent to which relaxation time
and morphologic feedback affect the bar behavior.
Such knowledge is probably best obtained from the
analysis of long time series of morphology and
forcing conditions, rather than from intensive field
experiments.
Fortunately, some monitoring programs for mor-
phologic and hydrodynamic data already exist and
have created valuable long-term data sets, such as the
JARKUS data set (The Netherlands), the Duck data set
(NC, USA), the Lubiatowo data set (Poland), or the
ARGUS video data set (USA, UK, The Netherlands,
Australia) (Hamm, 1997). These and hopefully addi-
tional, new monitoring programs will help increase
our understanding of the intriguing phenomenon of
nearshore bars along sandy shorelines.
K.M. Wijnberg, A. Kroon / Geomorphology 48 (2002) 103–120 117
Acknowledgements
K.M.W.’s work on this paper was funded by the
EU-sponsored Marine Science and Technology Pro-
gramme (MAST-III), as part of the PACE-project
under contract number MAS3-CT95-0002. The work
was co-sponsored by the Andrew Mellon Foundation.
A.K.’s work on this paper was partly funded by the
EU-sponsored Marine Science and Technology Pro-
gramme (MAST-III), as part of the SAFE-project
under contract number MAS3-CT95-0004. Gerben
Ruessink (Utrecht University) is thanked for his useful
comments on the manuscript. Further, all images of
barred beaches in this paper originate from the ARGUS
video image database of Rob Holman (Oregon State
University). We are grateful for access to this great
database of nearshore bars. Finally, we thank the
reviewers, Brian Greenwood and Robin Davidson-
Arnott, for their useful suggestions to improve the
manuscript.
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