1. Introduction
Numerous studies of the effects of high-frequency relative sea-level changes in carbonates show that cycles are excellent indicators of sea-level fluctuations because their formation is highly dependent on many various parameters [1-7]. Thus, the cycle architecture depends on environmental factors that change periodically causing rapid facies changes trough time. These facies changes occur when a physical, chemical, and/or biological treshold is passed, and when the sediment acquires a new composition and texture [6]. The cyclic stacking pattern always reveals very similar characteristics.The general increase in grain size, decrease in mud content and sometimes even progresive change in style of sedimentary structures are commonly within single coarsening-upward cycle. Because of my frequent encounters with cyclic sedimentary signatures throughout the Karst Dinarides, especially within the Jurassic carbonate beds, one simple model for the entirely autoycyclic mechanism of coarsening-upward cycles origin can be proposed.
2. Samples and Methods
For the purpose of this paper one Lower Jurassic succession from Platak locality situated NE from town of Rijeka (Karst Dinarides - Croatia) (Figure 1) were taken into account. Oriented rock samples are collected in the field using a rock pick. A minimum of three rock samples is taken from each sample site. Samples are first analyzed in their natural state and then as the thin sections under the microscope. One thin section is produced when a thin sliver of rock is cut from the rock sample with a diamond saw and ground optically flat. It is then mounted on a glass slide and then ground smooth using progressively finer abrasive grit until the sample is only 30 μm thick. Then the sample, now as a thin section, is ready for viewing and imaging under the microscope. Based on field and laboratory observation under the microscope, carbonate facies were identified within the successions and two types of coarsening-upward cycles have been recognized. These are cycles with the peloidal-bioclastic upper cycle members (1), and the cycles with the oolitic upper cycle members (2)(Figure-2).
3. Results - Petrography of Carbonate Facies
3.1 Cycles with peloidal-bioclastic upper cycle members
These coarsening-upward cycles contain mudstone or peloidalbioclastic wackestone as the lower cycle members. The thickness of the lower cycle members varies from 0.7-2 m, whereas the upper cycle members range from 0.1-0.6 m. Mudstones and peloidal-bioclastic wackestones are composed of micrite with variable amounts of peloids, molluscan and ostracode fragments and individual benthic foraminifera (Figure 3). Separate LLH stromatolitic laminae and laminoid fenestrae are sporadically present. Bioturbation occurs locally. Within these mud-rich limestone types, intercalations of horizontally laminated peloidal-bioclastic packstone-grainstone, 0.1- 0.3 m thick, can be occasionally found. Single horizontal 1-3 mm thick laminae are graded. These intercalations are always separated at their bottom by sharp, erosional surfaces. They have gradational upper boundaries into overlying mudstones or wackestones. Peloids, foraminifera, small echinoid and ostracode fragments embedded in micrite and/or drusy cement dominate. Elongated bioclasts are always oriented parallel to bedding. Coarse-grained particles are present within upper cycle members. These wackestone/packstones to grainstones are abundant in peloids, coarser molluscan and sporadic echinoderm bioclasts (Figure 4 and Figure 5). More rarely, they contain subrounded micritic intraclasts and concentric oncoids with bioclastic nuclei surrounded by few cryptocrystalline envelopes. Coarser-grained bioclasts are always more or less recrystallized and randomly oriented. Some beds contain rich foraminiferal debris. In places, horizontal lamination is present, when sharp and uneven erosional contacts with underlying unlaminated beds are visible.
By periodically changing conditions, from low-energy shallow subtidal to higher-energy subtidal above the fair-weather wave base, a series of coarsening-upward cycles have been produced. During low-energy shallow subtidal conditions with slow and constant rate of sediment accumulation a large amount of carbonate mud with rare bioclasts were deposited. A much more intensive production of various coarser-grained particles occurred during periodical subtidal shallowing above the fair-weather wave-base (see Discussion). Sporadic horizontal lamination observed within the packstone-grainstone intercalations and even wackestone/ packstone to grainstone beds was formed during periods of intensive unidirectional tidal and/or storm currents. These currents eroded the subtidal bottom, winnowed the muddy-peloidal-bioclastic material, removed the carbonate mud, oriented elongated bioclasts parallel to bedding, and formed the horizontal, graded laminae.
3.2 Cycles with oolitic upper cycle members
The same features as were described in the previous chapter characterize mudstones or peloidal-bioclastic wackestones as the lower members of these cycles. However, their thicknesses are generally smaller, amounting to 0.4-1.1 m. The upper cycle member is represented by ooid grainstones and/or ooid-bioclastic packstones to grainstones. Ooid grainstones consist of well-sorted ooids with peloidal or bioclastic nuclei, surrounded by an envelope of radial fibrous fabric (Figure 6). The ooids are white to cream in color, have a pearly luster, and usually range in size from 0.2 mm to 1.0 mm. They have frequently recrystallized envelopes and even nuclei. The diagenesis of these grainstones includes fibrous calcite on the surface of the ooids and drusy calcite spar in the intergranular pores. Sporadically, pore spaces are filled up by crystal silt. Among the ooids there are sporadic small molluscan fragments and foraminiferal tests. Distinct cross- and/or horizontal lamination can be sporadically observed. However, these structures are mostly hard to be recognized because of the well-sorted nature of the grainstones. The bases of oolitic members are commonly erosional surfaces. In drusy calcite spar or micritic matrix the ooid-bioclastic packstones to grainstones contain ooids and variety of poorly sorted, abraded and broken molluscan, echinoderm and hydrozoan fragments, as well as variously sized intraclasts (Figure 7). Elongated coarser-grained particles are mostly randomly oriented.
These cycles also represent a sedimentary response to cyclic environmental changes from low-energy shallow subtidal to higher-energy subtidal above the fair-weather wave base. However, environmental conditions during the formation of the oolitic upper cycle members were different when compared with conditions where peloidal-bioclastic upper cycle members were deposited in (see Discussion). At first glance it is recognized by the frequent erosional surfaces underlying the oolites and by absence of micrite and peloids. That implies shallower and higher energy subtidal conditions of oolitic shoals that were migrated laterally over the relatively deeper subtidal environments. Their migration by tidal and/or storm currents of different energy led to formation of sporadic cross- and/ or horizontal lamination. Rare findings of crystal silt in pore spaces of oolites indicate neighboring presence of the vadose zone from which. calcite crystals were washed and transported in suspension to the oolitic shoals.
4. Discussion
The high-frequency cycles described in this paper are usually referred to as parasequences [4]. They are often interpreted to be of allocyclic origin and to be caused by climatic fluctuations associated with Milankovitch cycles [8]. Milankovitch cycles are orbital cycles that modulate insolation and are commonly related to fluctuations of climate, whereby the waxing and waning of ice caps, especially during glaciations (such as nowadays), act as amplifier of the inherently weak insolation signal. Orbitally controlled waxing and waning of ice caps translate into high-frequency sea-level fluctuations that may lead to metre-scale shallowing- and coarsening upward cycles, [6,9,10]. However, it is difficult to correlate here studied cycles with Milankovitch cycles because during the Jurassic, ice in high latitudes probably was present but ice-volumes were not sufficient to induce important glacio-eustatic fluctuations [11-13], although volume changes of alpine glaciers could make a small contribution [13,14]. Additionally, the Early Jurassic is a time of climatic warming [15] because of rapid rise in CO2 levels caused by the outpouring of the Central Atlantic Magmatic Province as a result of the rifting of Pangea [16,17]. In such circumstances, there was probably no pronounced seasonality during Early Jurassic. However, it can be assumed that high-frequency sea-level fluctuations of allocyclic origin were present during Early Jurassic, but were small and thus hardly perceptible in the sedimentary record. Therefore, predominantly based on sedimentary mechanisms that are active in platform shallow-water environments, it can be interpreted that above described coarsening-upward cycles as being the result of autocyclic processes, but having in mind that some allocyclic signal was also present but for the time being hard to be recognized.
Large carbonate platforms, without prominent elevation differences, are characterized by small water depths (mainly less than 10 m), and the fair-weather wave-base is at less than 5 m [18]. Judging from this, one can presume that successive series of coarsening-upward cycles may be a record of changes in water depth through varying sediment accumulation, when sea-bottom seemingly oscillates around the fairweather wave-base (the fair-weather wave-base - FWWB amounts to half of the wavelength - WL/2). This assumption is based on two wellknown facts: (1) under optimum conditions carbonate sediments can accumulate rapidly, resulting in high and mostly constant carbonate production rate [19,20]; and (2) carbonate production in modern depositional environments, as a rule, exceeds an average amount of platform subsidence and moderate eustatic sea-level rise [18]. Typical sedimentation rate of modern carbonate deposits is 1 m per 1000 yr, typical subsidence rates of passive continental margins, where many ancient carbonate platforms developed, are 0.01-0.1 m per 1000 yr, and typical eustaic sea-level changes are 0.01 m per 1000 yr [18]. Rapid subsidence, generally fault-induced and major sea-level rises through glacial melting, is not included. From these, it can be presumed that facies differences, i.e. cycle architecture, are mainly the result of processes operating within thecarbonate platform realm. Among those processes, aggradation of subtidal carbonate deposits and progradation of small ooid shoals appear to be most important.
During periods when the water depth (i.e., accommodation space) (D) on many carbonate platform areas was greater than one-half of the wavelength (D>WL/2), there was no movement of sediment particles at the sea bottom (SB) (Figure 8a). Therefore, in quiet subtidal environments below the fair-weather wave-base, peloids and calcareous mud, as well as benthic forams occasionally associated with various bioclasts, were predominantly accumulated, producing muddy carbonate deposits (Figure 8b 8c, points 1-2 and 4-5 - tA) ("catch up" phase sensu [21]).
It is presumed that the carbonate production rate exceeded both the
rate of subsidence and the rate of eustatic sea-level rise (i.e. relative
sea-level rise). Such high carbonate accumulation rate caused gradual
reducing of accommodation space, i.e., decrease of water depth.
When the water depth became less than one-half of the wavelength
(D
In contrast to that, environmental conditions within sporadically
presented subtidal topographic highs were rather different (Figuress.
8d-f). In these places, the water depth was smaller and the wavelength
was consequently shortened, so the sea-bottom (SB) was positioned
closer to the fair-weather wave-base (FWWB) (Figure 8d). Thus,
when the water depth became less than one-half of the wavelength
(D
During periods without oolitic shoal progradations, only vertical aggradation of subtidal carbonate deposits occurred, producing successive series of coarsening-upward cycles with peloidal-bioclastic upper cycle members.
5. Conclusion
The examined coarsening-upward cycles were formed within the shallow-water realm of the carbonate platform area. They reveal coarsening-upward trend from the subtidal below the fair-weather wave-base to the subtidal above the fair-weather wave-base as the predominant response to the autocyclicity in the sedimentary environment. Gradual aggradation of the muddy carbonate material, deposited below the fair-weather wave-base reduced the accommodation space, causing the sea bottom to rise above the fairweather wave-base. Here, more grainy carbonates were deposited, creating one coarsening upward cycle with mudstones or peloidalbioclastic wackestones as the lower cycle member and peloidalbioclastic wackestone/packstones to grainstones as the upper cycle member. During the "lag phase", the sea bottom has sunk belowthe fair-weather wave-base, what enabled the formation of the next coarsening-upward cycle. The progradations of neighboring oolitic shoals periodically and randomly interrupted this process. Oolitic shoals that were sporadically formed on topographic highs within the subtidal area prograded over the surrounding environment below or above the fair-weather wave-base, producing sporadic coarseningupward cycles with ooid grainstones and/or ooid-bioclastic packstones to grainstones as the upper cycle member. Therefore, coarsening-upward architecture resulted from interplay of repeated sediment aggradations, interrupted by periodical and random oolitic shoals progradations.
Acknowledgments
We thank the editor and two anonymous reviewers for their constructive comments, which helped us to improve the manuscript.