the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Improving understanding of groundwater flow in an alpine karst system by reconstructing its geologic history using conduit network model ensembles
Chloé Fandel
Ty Ferré
François Miville
Philippe Renard
Nico Goldscheider
Reconstructing the geologic history of a karst area can advance understanding of the system's present-day hydrogeologic functioning and help predict the location of unexplored conduits. This study tests competing hypotheses describing past conditions controlling cave formation in an alpine karst catchment, by comparing an ensemble of modeled networks to the observed network map. The catchment, the Gottesacker karst system (Germany and Austria), is drained by three major springs and a paleo-spring and includes the partially explored Hölloch cave, which consists of an active section whose formation is well-understood and an inactive section whose formation is the subject of debate. Two hypotheses for the formation of the inactive section are the following: (1) glaciation obscured the three present-day springs, leaving only the paleo-spring, or (2) the lowest of the three major springs (Sägebach) is comparatively young, so its subcatchment previously drained to the paleo-spring. These hypotheses were tested using the pyKasso Python library (built on anisotropic fast-marching methods) to generate two ensembles of networks, one representing each scenario. Each ensemble was then compared to the known cave map. The simulated networks generated under hypothesis 2 match the observed cave map more closely than those generated under hypothesis 1. This supports the conclusion that the Sägebach spring is young, and it suggests that the cave likely continues southwards. Finally, this study extends the applicability of model ensemble methods from situations where the geologic setting is known but the network is unknown to situations where the network is known but the geologic evolution is not.
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Mapping subsurface cave and conduit networks in karst systems provides crucial information for water resource management, hazard prevention, archeological research, and the protection of important ecological and cultural sites. Even small-diameter conduits play an important role in groundwater flow. However, mapping conduit networks is a challenging task (Trimmis, 2018; Sellers and Chamberlain, 1998). Conduits can extend far below the surface, and speleologists attempting to explore them may experience dangers such as flash floods, falling rocks, hypothermia, and disorientation. Even in well-explored systems, the full network is impossible to map, because small-diameter conduits (< 0.5 m) are inaccessible to humans and difficult to detect by geophysical methods (Jaquet and Jeannin, 1994).
Understanding the speleogenetic processes driving cave formation and the geologic history of an area can help guide cave exploration, data collection, and groundwater resource management. Karst systems commonly evolve over time in several phases, during which different climate and geologic conditions control which parts of the system (e.g., diffuse recharge zones, focused inlets, outlets, conduits) are actively transmitting flow. Conduits or springs that see active flow during one phase of karstification may go dry when conditions change. Although these older parts of the system may become inactive, they are still open and can be reactivated during extreme flow events or when climate conditions shift again (Audra and Palmer, 2011). An experienced geologist may be able to reconstruct how the karst system functioned in the past and therefore predict the likely locations of presently inactive conduits. These predictions can sometimes be tested through targeted exploration of the locations where caves are suspected to exist. Some hypothesized conduits, however, may be inaccessible, making it impossible to confirm or refute their existence through exploration. In other cases, several different historical scenarios may appear equally plausible, making it difficult to determine how the system evolved. As a result, geologic intuition alone may not be sufficient to fully understand a karst area. This can lead to knowledge gaps or misconceptions that limit the reliability of future simulations of the system's behavior under projected climate or land use scenarios that differ from present-day conditions.
This study uses a model-based approach to identifying the geologic processes which could explain the formation of a particular cave in the Gottesacker karst system. In this system, detailed cave maps are available in parts of the conduit network.
While some portions of the explored cave system are very active, containing an accessible cave stream with open-channel flow that connects to a major karst spring, other portions of the explored system are now inactive and are thought to have formed when past conditions were different from the present configuration of the system. However, two different explanations are possible: (1) glaciation obscured all of the present-day springs, leaving only the paleo-spring as the primary drainage point for the entire karst system, or (2) the lowest of the major present-day springs is significantly younger than the others, so the paleo-spring and the two uppermost springs jointly drained the aquifer system.
These competing hypotheses were tested using a computationally efficient karst network model to generate probability maps of possible conduit locations under each of the proposed past scenarios. The simulated conduit networks under each scenario were then compared with the mapped portion of the inactive cave system to determine which scenario best matched the observed network. Finally, the analysis was extended to propose possible locations of the unmapped parts of the system.
The modeling approach demonstrated in this study was tested on the complex, extensively studied Gottesacker karst system in the German and Austrian Alps, described in Goldscheider (2005). This 35 km2 catchment consists of a series of plunging synclines and anticlines draining to the Schwarzwasser valley, which cuts roughly perpendicularly across the fold axes (Fig. 1). The karst aquifer lies north and northwest of the valley in a limestone unit widely exposed at the surface. It is locally overlain by sandstone and younger units and underlain by non-karstifiable marl and older units.
This karst system is also the site of one of the longest caves in Germany, the 12 km Hölloch cave in the Mahdtal valley, which has been the subject of avid exploration and of several books and documentary films since the early 1900s (Höhlenverein Sonthofen, 2006). The local caving club has created and shared a detailed map of the explored portion of the cave. The northern part of the cave (trending SE) is active and contains a cave stream, while the southern part (trending NNW) is inactive and does not have any continuous underground drainage or cave streams.
Three major springs drain the system: an estavelle (QE, elevation 1120 m a.s.l.), the Aubach spring (QA, elevation 1080 m a.s.l.), and the Sägebach spring (QS, elevation 1035 m a.s.l.). The estavelle acts as swallow hole during low-flow conditions but acts as a spring during high-flow conditions. A paleo-spring (QO, elevation 1190 m a.s.l.) partway up the Mahdtal valley, near Höflealpe, remains dry for time spans of years to decades. In 2005, QO temporarily re-activated, during extreme high-flow conditions (Fig. 2). This is the only recorded flow event ever observed at this spring.
QO is located at a geological contact between the karstified limestone aquifer and overlying low-permeability formations (sandstone and marl). Upstream from QO, the karstified limestone is exposed at the land surface, so precipitation infiltrates rapidly and does not generate any significant surface flow. However, since QO is located directly above and is connected to the cave stream in the conduit system beneath it, any surface water that does exceed the infiltration capacity of the karst or is injected at QO would reach the cave stream and flow to Sägebach spring (QS). Downstream of QO, the overlying sandstone and marl in the core of the syncline confine the karst aquifer, which drains to the Sägebach spring (QS). QO can therefore act as an overflow when the discharge capacity of QS is exceeded, and large-scale backflooding occurs, as observed in 2005. In this lower part of the area, extending into the Schwarzwasser valley, the karst aquifer was (and partly still is) confined by overlying low-permeability sandstone and marl and by widespread moraine deposits.
South of the main Schwarzwasser valley, non-karstifiable flysch and marl lithology prevents conduit development, and drainage occurs instead through a network or surface streams. Several other geologic units and small springs are present, but for the purposes of conduit modeling, the geology was represented using a simplified model focused on delineating the boundaries of the karstifiable limestone unit.
The general configuration of the conduit network (referred to in the rest of this paper as the expected network) was originally defined by Chen and Goldscheider (2014), and it was refined by Chen et al. (2018), based on geologic mapping by Wagner (1950); predominant fracture orientations documented by Cramer (1959); several decades of speleological investigations by the regional caving club (Höhlenverein Sonthofen); 18 quantitative multi-tracer tests by Goldscheider (2005), Göppert and Goldscheider (2008), Goeppert et al. (2020) and Sinreich et al. (2002); and hydrogeological field observations by Goldscheider (2005). Anticlinal axes act as groundwater divides, sectioning the region into sub-basins, each drained by a major conduit following synclinal axes. These conduits merge into a primary conduit that parallels the surface stream in the Schwarzwasser valley. The expected network map does not represent exact conduit locations but rather the general configuration and approximate location of the conduits. This network map has been used successfully for several previous groundwater flow modeling efforts (Chen and Goldscheider, 2014; Chen et al., 2017; Chen et al., 2018; Fandel et al., 2021).
Two different hypotheses are currently under consideration to explain the formation of the inactive part of the Hölloch cave system:
Hypothesis 1. The Schwarzwasser valley was covered by a glacier, overlying the karstifiable units up to the elevation of the paleo-spring (QO), which was the primary spring draining the entire system.
Geologic evidence. Widespread moraines and other geomorphologic evidence indicate the presence and extent of the main glacier in the Schwarzwasser valley, which covered all of the locations of present-day valley springs (QE, QA, QS) and filled the valley up to an elevation just below the paleo-spring (QO), located approximately 200 m above the valley floor. The glacier appears to have filled the rest of the valley with roughly the same thickness of ice, creating a boundary just below and parallel to the inactive portion of the mapped conduits. There is clear geomorphologic evidence that the entrance shaft of the Hölloch cave was formed by sinking glacial meltwater and that it was an active inlet during and after glaciation. The streambed created by meltwater flowing down the valley is still visible and still channels temporary surface flows during snowmelt or intense rainfall. End moraines further up the Mahdtal valley indicate the presence of a local glacier in the upper part of this valley, as well as in the upper part of the valley located in the breached syncline northeast of Hoher Ifen.
Hypothesis 2. Low-permeability sedimentary formations covered the Sägebach spring (QS), so the paleo-spring (QO) drained the Mahdtal valley and connected to the Aubach spring (QA), which was at the time the lowest spring in the system.
Geologic evidence. Field evidence indicates that the Sägebach spring (QS) is much younger than the Aubach spring (QA), but it is difficult to estimate the exact age difference. QA is located in a large gorge (hundreds of meters long and tens of meters deep), with many open fractures and cavities and a cave entrance. It is in the middle of a zone of exposed and highly karstified limestone. It does not appear to have an upper limit of discharge, and it looks like a very well-developed, older outlet for the karst aquifer system. QS, on the other hand, is located along a fault in a short, narrow, and shallow gorge. The karstified limestone is only very locally exposed and is surrounded and overlain by younger, less-permeable units (sandstone, marl, and glacial moraine deposits). QS has limited discharge, causing backflooding when the discharge capacity of the spring is exceeded. This geologic setting suggests very young (probably postglacial) exposure by erosion of the confining layers along the fault.
Both of these scenarios are supported by field observations, so the question is not whether they occurred but whether they were determinant for the formation of the now-inactive portion of the cave network. This depends both on the temporal order and on the duration of the different processes at work. One of the reasons for this question is that we do not have enough clear field evidence to determine whether the glaciation preceded or followed the uncovering of QS.
To test these hypotheses, many possible network configurations were modeled using a stochastic simulation method implemented in the Python karst modeling package pyKasso (Fandel et al., 2022). This package implements the SKS approach originally proposed by Borghi et al. (2012) but uses an anisotropic fast-marching algorithm (Sethian, 1999; Mirebeau, 2014). Anisotropic fast-marching algorithms calculate the optimal path from one point to another through a medium, in which the ease of travel varies both spatially and directionally. Karst conduits can be simulated using this type of algorithm based on the assumption that a conduit represents the fastest path from an inlet (such as a doline or swallow hole) to an outlet (a spring) (Borghi et al., 2012). Luo et al. (2021) also implemented the use of an anisotropic fast-marching algorithm to simulate karst systems, with a focus on representing the anisotropy resulting from a fracture network by using 3D fields of equivalent permeability tensors. The SKS approach presented by Borghi et al. (2012) is three-dimensional but isotropic. The approach presented by Luo et al. (2021) is 3D and anisotropic. As in SKS and in pyKasso, this last approach requires generating a discrete fracture network model, but then it estimates by iterative calculations the size of the representative elementary volume and computes the equivalent permeability tensors for all the cells of the model by solving multiple local flow problems in different directions. The anisotropic fast-marching algorithm is then carried out using the upscaled field of spatially varying equivalent permeability tensors. The advantage of this approach is that it permits the representation of fractures at a subgrid scale. The preprocessing calculations are, however, rather computationally intensive. The pyKasso package presented in Fandel et al. (2022) is 2D (with a more recent 3D version now functioning), and it uses an anisotropic fast-marching algorithm in a slightly different framework. It focuses on enabling rapid generation of numerous possible conduit networks influenced by multiple factors, such as the topography of the geologic surface on which karst conduits develop. To test the hypotheses presented in this paper, the 2D anisotropic version of pyKasso was chosen, because of its computational efficiency in generating numerous possible conduits and its ability to consider the effects of bedding plane topography, spatial variations in travel cost, and inlet/outlet pairings, in addition to fracture networks. For karst systems in which the conduits are more strongly influenced by the fracture network than by the structure of the contacts between geologic units and in which conduits develop equally extensively in all three dimensions, rather than mostly in the x and y directions, the implementation by Luo et al. (2021) may be a better choice.
In pyKasso, the travel medium represents the geologic setting, in which some rock units are more soluble than others (i.e., easier for conduits to travel through). Conduits are also assumed to form preferentially in certain orientations: in the direction of the maximum downwards hydraulic gradient and/or along the dip direction of bedding planes (Audra and Palmer, 2011; Dreybrodt et al., 2005). The user can specify which plane should influence conduit orientation. For shallow, unsaturated karst systems with an impermeable basal unit such as the example presented here, the gradient of the lower contact between the karstifiable unit and the underlying non-karstifiable unit is the dominant influence, because water recharging downwards from the land surface encounters a low-permeability barrier and subsequently flows laterally along this low-permeability surface (Filipponi, 2009).
Stochasticity can be introduced to the simulations through the generation of a unique fracture network for each model realization, based on the statistical distribution of fracture families observed in the field. The statistical metrics describing the fracture network are the density, the minimum and maximum strike, and the minimum and maximum length. For a table of fracture statistics, see Fandel et al. (2022). Fractures are assumed to be easier for conduits to travel through than the surrounding rock.
Additional controls on the configuration of the simulated network are possible by iterating over multiple phases of karst development and over multiple outlets. The inlets to the system can also be divided into groups and assigned to separate outlets, representing different subcatchments within the larger system. These aspects tend to contribute more variability to the resulting networks than stochasticity arising from fractures only. All these aspects can be controlled in a deterministic or stochastic manner depending on the available information for a given site (see Fandel et al., 2022, for a full explanation of possible variations).
The primary advantages of fast-marching methods are their low data requirements and their computational efficiency compared to other conduit network models. These characteristics allow for the rapid simulation of hundreds of network realizations for a single site (for this study, 100 simulations ran in under 2 minutes on a laptop with a 2.7 GHz dual-core i7 processor and 16 GB of RAM). However, this approach does not represent the actual physical and chemical processes driving speleogenesis. Unlike more complex speleogenetic models, each individual pyKasso model realization, as it is based on very little information, is unlikely to capture the true network configuration. Instead, this method is more appropriate for rapidly exploring various scenarios and generating probability maps: visual representations of a model ensemble indicating the likelihood of a simulated conduit being present at any given location.
5.1 Quality check: accuracy of network simulations
To represent the Gottesacker karst system with pyKasso, the medium through which conduits form was bounded using a three-dimensional geologic model, created using the Python package GemPy (de la Varga et al., 2019). For a detailed description of the geologic model, see Fandel et al. (2021). For use with pyKasso (only available in 2D at the time of this work), the 3D extent of the karstifiable limestone unit was projected onto a 2D plane and used as the initial cost map (see Table 1 for travel cost values). The resulting 2D geologic map has a resolution of 181 × 141 cells, with 50 m × 50 m pixels (Fig. 3b and c). This resolution was chosen because it is detailed enough to represent the criteria used to test the hypotheses under consideration in this study (the general location and orientation of conduits) but coarse enough to maintain the fast computation times needed to run hundreds of simulations. A model with 5 m × 5 m pixels was originally tested but was discarded because it significantly increased the computation time (nearly 50 min compared to less than 2 min to run 100 simulations) without significantly increasing the degree of confidence with which the study questions could be answered. The gradient driving the preferred orientation of conduit formation was calculated from the surface of the contact between the base of the karstifiable limestone and the less-permeable underlying marl. Previous work by Filipponi (2009) demonstrated that in the stratigraphic sequence present at this study site, where the Schrattenkalk limestone is the primary karstifiable unit, conduits form preferentially along the lower contact between the Schrattenkalk and the underlying Drusberg marl, parallel to bedding planes.
Outlet coordinates were assigned based on mapped spring locations (Goldscheider, 2005). Inlet coordinates and inlet/outlet pairings were assigned based on locations and springshed boundaries inferred from tracer test evidence and geologic structure in previous flow modeling efforts (Chen and Goldscheider, 2014). For a full description of the original conduit model parameters, results, and limitations, see Fandel et al. (2022). The conduit model presented in this paper is modified from that in Fandel et al. (2022) in that it uses as input the 2D actual areal extent of the karstifiable unit (rather than a map of where the limestone crops out at the land surface) for the cost maps and the altitude map of the contact surface between limestone and marl (rather than the land surface) for the gradient calculations. The inlet/outlet pairings were also fixed in this paper, whereas in Fandel et al. (2022) results with both fixed and random inlet/outlet pairings were compared. As described in Fandel et al. (2022), holding the inlet/outlet pairings fixed reduces the variability in the resulting conduit networks. The results presented in this paper are therefore most likely less variable but more realistic representations of the system than the results presented in Fandel et al. (2022). The pyKasso-generated probability map of conduit locations in both cases closely matched the branching pattern of the expected network (Fig. 3a), despite the limitations of using a low-resolution, simplified, 2D geologic model as the travel medium and a proxy for the hydraulic gradient. These results support placing confidence in the ability of pyKasso-generated ensembles to provide information about the approximate configuration of karst conduit networks in this system. Displaying the ensemble of simulations on the same map also provides information about the probability of conduit occurrence in different zones of the study area: zones where most of the simulations generate conduits in the same general location and orientation suggest that the probability of a real conduit existing in that location and orientation is higher (e.g., conduits departing from inlet N16 in Fig. 3a), while zones where there is a wide spread of simulated conduit locations and orientations indicate that lower confidence should be placed in model predictions for that part of the study area (e.g., conduits departing from inlet N6 in Fig. 3a).
5.2 Hypothesis testing
To test the two hypotheses for the past geologic conditions controlling conduit formation, 100 network realizations were run for each scenario using pyKasso, at the same model resolution previously used to simulate present-day conditions (50 m × 50 m cells).
To simulate hypothesis 1 (glaciation closing all springs except QO), the model cells covered by the glacier were assigned a very high travel cost, discouraging conduits from crossing the glaciated area (Table 1). The inlets and outlets covered by the main glacier and the two smaller valley glaciers (inlets N21 and N16 and outlets QE, QA, and QS) were removed from the model, and inlet N16 was replaced with an inlet at the entrance to the Hölloch cave. Under this scenario, inlet N1 was separated from the rest of the karst system by the glacier and was assumed to have drained to a local spring with unknown exact location that is no longer active today (QI). However, the extent of the glacier in this subcatchment is uncertain, so the focus of this simulation remains on the eastern portion of the karst network connected to the paleo-spring (QO), which drained all remaining inlets not covered by the glacier (Fig. 4a).
To simulate hypothesis 2 (QS is much younger than the other springs), the Sägebach spring was removed from the list of system outlets and replaced with the paleo-spring (Fig. 4b). The existing inlets remained the same as the present-day configuration. Under this scenario, the Aubach spring (QA), which is lower in elevation than the paleo-spring, was assumed to have served as an “attractor” receiving flow from the entire system, including the Mahdtal valley. An additional inlet was therefore co-located with the paleo-spring and assigned to the Aubach spring.
For both scenarios, the inlet/outlet pairings and iteration order were kept constant. A new fracture network was stochastically generated for each realization, using the same input statistics as the simulations of the present-day network. All other parameters were held constant.
The modeled probability maps support hypothesis 2 (a comparatively young QS) more than hypothesis 1 (glaciation) (Fig. 4). The simulated networks under hypothesis 1 (glaciation) only matched the location and orientation of the mapped conduits in the active upper portion of the cave system, not in the inactive lower portion which is the focus of inquiry (Fig. 4a). Of note is that the spread of predicted conduit locations in this area includes a wide range of possible conduit locations northwest of the mapped cave system. But out of the 100 simulations, not a single one predicted conduits located along the axis of the actual cave system. These results support the conclusion that hypothesis 1 has a low probability of explaining the formation of the inactive conduits.
The simulated networks matched the location and orientation of the mapped cave system better under hypothesis 2, when the Sägebach spring was removed from the list of outlets and replaced with the paleo-spring. The orientation of the simulated conduits is tightly clustered and matches well, while the location of the simulated conduits is slightly to the east of the mapped conduits with more overlap in the southern portion (Fig. 4b).
Under this scenario, in the present day, the partially mapped inactive conduits should extend to make a connection from QO to QA. Because QO is at a higher elevation than QA, the general flow direction when these conduits were active would have been from QO towards QA, even if the inclination of some individual conduits is inverse. Although these conduits now are generally dry, it is possible that under extreme high-flow conditions groundwater in the Mahdtal syncline overflows the southwards-bordering anticline and flows towards the Aubach spring (QA).
While these results indicate that hypothesis 2 is a more likely representation of the past geologic conditions that led to the formation of the inactive portion of the Hölloch cave system than hypothesis 1, other explanations cannot be ruled out. The primary contribution of the model results is that hypothesis 1 can be ruled out as significantly less probable than originally expected based solely on tracer tests and hydrogeological intuition.
The model ensembles in this study clearly support one hypothesis over the other: the probability map for hypothesis 1 shows a range of possibilities but no conduits along the mapped portion of the inactive cave system, while the map for hypothesis 2 shows a cluster of conduits, suggesting that the inactive portion of the Hölloch cave continues southeast for several hundred meters before turning first southwest then due south to connect to the Aubach spring (Fig. 4b). This configuration is illustrated schematically in Fig. 5.
These results suggest two additional ways that these hypotheses could be further tested by fieldwork:
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The first is additional speleological explorations, focusing on the passages trending in the directions projected by the probability map. If the hypothesis is correct, these passages will continue rather than terminating in dead-ends. This information may be helpful in guiding future speleological exploration.
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The second is tracer injection under extreme high-flow conditions at the Hölloch cave entrance in the Mahdtal valley with sampling at the Sägebach spring (QS) and the Aubach spring (QA). When, under high-flow conditions, the water level in the cave system is greater than the elevation of the Aubach spring (QA), the paleo-spring (QO) becomes active. Previous tracer tests under normal flow conditions found a connection only to the Sägebach spring, but under extreme high-flow conditions, the normally inactive conduits projected to connect to the Aubach spring may reactivate. Unfortunately, the logistical challenges of waiting for such an extreme event to occur and then achieving a high-quality tracer test on short notice are significant.
A third hypothesis is also possible, a combination of the two scenarios explored in this study: that an initial phase of conduit formation occurred that was dominated by the influence of the glacier covering the valley, another phase occurred after the glacier had retreated but before the Sägebach spring was exposed, and the most recent phase developed with all three major springs (QE, QA, and QS) active. If this were to have occurred, two sets of inactive conduits should be present, corresponding to the two past phases of karstification. Currently, no conduits have been found along the paths expected if glaciation had influenced conduit formation. However, exploration of the Hölloch system is incomplete. If future exploration reveals new conduits along the paths simulated under the glaciation scenario, this hypothesis of multi-phase karstification could also be supported.
While the model results provide insight into this area's geologic past, some questions and limitations remain. In both scenarios, the underlying geologic model is a limitation. A 2D geologic map simplifies the complex three-dimensional reality. However, a preliminary test using a 3D development version of pyKasso, with the 3D geologic model as input, yielded conduit maps that did not appear significantly different from the 2D version used in this paper.
The simulations representing each scenario were generated based on the same set of model parameters (chosen based on their ability to reproduce the present-day network), with stochasticity arising from the fractures and hierarchical approach. This approach was chosen to minimize the number of variables under consideration. However, it may limit the range of network configurations generated. For example, with the chosen parameters, more direct connections between inlets and outlets are somewhat favored, whereas with different parameters paths following the anisotropy gradient or paths following fractures might have been more favored, even if they are longer. Different parameter choices could potentially have led to different results for the scenarios considered; for example, under hypothesis 1 (glaciation), parameters de-emphasizing the importance of choosing a more direct path could have led to conduits that descended the gradient more directly until they encountered the edge of the glacier and then turned northeast to develop along contours, more closely matching the mapped inactive conduits. This highlights the importance of designing modeling experiments carefully and of choosing a consistent parameterization strategy before actually running the simulations.
One limitation of this study is that the order of events and the rate of change in the landscape is not precisely known. Field observations suggest a late glacial to postglacial age of the Sägebach spring and a relatively rapid exposure. The lack of precise dating limits our understanding of the system as a whole. Another question arises from the observation that although the simulated conduits under hypothesis 2 (a young QS) are much more similar to the inactive portion of the Hölloch cave than under hypothesis 1 (glaciation), they do not exactly match the mapped cave system. The simulated conduits tend to lie slightly to the east of the mapped conduits, skirting the edge of the overlying sandstone unit. This is likely due to our simplification of the geology – in reality, the karstifiable limestone in this part of the system is covered by non-karstifiable sandstone, marl, and Quaternary sediments. These overlying units may have made it more difficult for conduits to develop beneath them, encouraging conduit development along their northwestern boundary. However, the mismatch may also indicate a conceptual gap in our understanding of the system.
A few examples of factors not considered in this study that could affect conduit formation include the following:
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The first is the presence of an unmapped tectonic feature with higher or lower conduit-forming propensity than the surrounding rock. This would attract or repel conduits in the model.
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An eastwards (downgradient) shift in the location of the contact between the karstifiable limestone and the thin overlying sandstone unit may also play a role as the sandstone erodes over time. The modeled conduits in this specific location tend to follow the contact, so the real conduits being slightly westwards of the modeled conduits could be explained if the contact were previously also slightly westwards of its current location.
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More phases of karstification than hypothesized could have occurred, in various orders, resulting in a conduit network that is partially but not fully explained by the hypotheses presented here.
This study demonstrates the application of anisotropic fast-marching methods for rapid model ensemble generation to test competing hypotheses describing the past geologic conditions that controlled karst conduit evolution in a real catchment. It extends the applicability of these methods from situations where the goal is to generate a map of an unknown conduit network to situations where the goal is to understand how an already-mapped conduit network was formed.
For the field site investigated in this study, the Gottesacker karst system, comparing the conduit network under different past scenarios (based on model-generated probability maps of conduit locations) to the actual conduit network (based on maps of the explored present-day cave system) allowed for the identification of the past conditions with the greatest influence on cave development. The model results indicate that the most probable scenario is that the conduits of interest formed before the lowermost spring in the catchment came into existence, and they drained to the other two major springs in the system (as opposed to conduit formation being dominantly influenced by glaciation occluding all three major present-day springs). The modeling results also enabled us to make recommendations to guide cave exploration efforts and future data collection that could further test the conduit formation hypotheses.
The strength of the anisotropic fast-marching method is its comparatively low cost in terms of computational resources and quantity of initial input data required. This allows for rapid iteration and exploration of many different scenarios, which makes it especially well-suited for ensemble modeling. The model ensemble approach demonstrated in this study could be applied to other karst systems with mapped conduit networks, both to better understand the past geologic conditions that influenced the conduit network development and to better target future mapping and data collection efforts to answer outstanding questions about the system. It also holds potential for exploring competing conceptual understandings of a karst system, and identifying possible conceptual gaps, both of which are significant sources of uncertainty in predicting karst systems' responses to anthropogenic stresses.
The Python code presented in this study was developed by the authors, using publicly available Python libraries, which are listed in the Dependencies section of the code documentation. The code is available in a GitHub repository, which has also been archived at the Zenodo DOI https://doi.org/10.5281/zenodo.10182888 (Fandel et al., 2020). For ease of interpretation and use, a Jupyter Notebook stepping through all of the analyses and figures presented in this paper is included in the repository and can be found at the following permalink: https://github.com/randlab/pyKasso/blob/c295727053c51d9f4ba735a171a5e94df4e1f48a/notebooks/Fandel_et_al_2023_HESS.ipynb (Fandel, 2023a). Following this study, an updated version of pyKasso has been released, and is available in the following GitHub repository https://github.com/randlab/pyKasso (Fandel, 2023b). This code is still under development.
The raw datasets used in this study are available in the same GitHub repository as the code. Both the code and datasets have been more permanently archived using Zenodo, with the https://doi.org/10.5281/zenodo.10182888 (Fandel et al., 2020). Explanations and visualizations of the data are presented in a Jupyter Notebook within this repository for ease of use. The Jupyter Notebook is titled Fandel_et_al_2023_HESS.ipynb and can be found at the following permalink: https://github.com/randlab/pyKasso/blob/c295727053c51d9f4ba735a171a5e94df4e1f48a/notebooks/Fandel_et_al_2023_HESS.ipynb (Fandel, 2023a). The datasets consist of rasters representing geologic and topographic maps, as well as points representing inlets and outlets. These datasets were generated by the authors from a combination of digitizing existing geologic maps (all of which are individually cited in the references section) and field mapping done by the authors themselves.
NG developed the concept for the paper and the hypotheses and provided data on the study site. FM, CF, and PR developed and debugged the pyKasso modeling package. CF implemented the model and performed the simulations. TF provided research supervision and guidance for the use of model ensemble approaches. CF created the figures and wrote the manuscript draft, and NG and PR reviewed and edited the manuscript.
The contact author has declared that none of the authors has any competing interests.
Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors.
The authors wish to thank the many speleologists of the Höhlenverein Sonthofen who contributed to mapping and digitizing the Hölloch cave system, particularly Andreas Wolf from the German Institute for Karst and Cave Science. This research would not have been possible without their exploration efforts and generosity in sharing data.
The article processing charges for this open-access publication were covered by the Karlsruhe Institute of Technology (KIT).
This paper was edited by Alberto Guadagnini and reviewed by two anonymous referees.
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- Abstract
- Introduction
- Approach
- Field site: Gottesacker
- Hypotheses
- Method: anisotropic fast-marching algorithm to generate probability maps
- Findings
- Discussion
- Conclusion
- Code availability
- Data availability
- Author contributions
- Competing interests
- Disclaimer
- Acknowledgements
- Financial support
- Review statement
- References
- Abstract
- Introduction
- Approach
- Field site: Gottesacker
- Hypotheses
- Method: anisotropic fast-marching algorithm to generate probability maps
- Findings
- Discussion
- Conclusion
- Code availability
- Data availability
- Author contributions
- Competing interests
- Disclaimer
- Acknowledgements
- Financial support
- Review statement
- References