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  <front>
    <journal-meta><journal-id journal-id-type="publisher">HESS</journal-id><journal-title-group>
    <journal-title>Hydrology and Earth System Sciences</journal-title>
    <abbrev-journal-title abbrev-type="publisher">HESS</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Hydrol. Earth Syst. Sci.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1607-7938</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/hess-22-977-2018</article-id><title-group><article-title>Hydrological characterization of cave drip waters in a porous limestone: Golgotha Cave, Western Australia</article-title><alt-title>Hydrological characterization of cave drip waters in a porous limestone</alt-title>
      </title-group><?xmltex \runningtitle{Hydrological characterization of cave drip waters in a porous limestone}?><?xmltex \runningauthor{K.~Mahmud et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Mahmud</surname><given-names>Kashif</given-names></name>
          <email>k.mahmud@westernsydney.edu.au</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Mariethoz</surname><given-names>Gregoire</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Baker</surname><given-names>Andy</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1552-6166</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Treble</surname><given-names>Pauline C.</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Hawkesbury Institute for the Environment, Western Sydney University, Locked Bag 1797, Penrith, NSW, Australia</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Institute of Earth Surface Dynamics, University of Lausanne, Lausanne, Switzerland</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Connected Waters Initiative Research Centre, UNSW Australia, Sydney, NSW, Australia</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Australian Nuclear Science and Technology Organisation, Lucas Heights, NSW, Australia</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Kashif Mahmud (k.mahmud@westernsydney.edu.au)</corresp></author-notes><pub-date><day>6</day><month>February</month><year>2018</year></pub-date>
      
      <volume>22</volume>
      <issue>2</issue>
      <fpage>977</fpage><lpage>988</lpage>
      <history>
        <date date-type="received"><day>6</day><month>March</month><year>2017</year></date>
           <date date-type="rev-request"><day>6</day><month>June</month><year>2017</year></date>
           <date date-type="rev-recd"><day>19</day><month>December</month><year>2017</year></date>
           <date date-type="accepted"><day>28</day><month>December</month><year>2017</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2018 Kashif Mahmud et al.</copyright-statement>
        <copyright-year>2018</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://hess.copernicus.org/articles/22/977/2018/hess-22-977-2018.html">This article is available from https://hess.copernicus.org/articles/22/977/2018/hess-22-977-2018.html</self-uri><self-uri xlink:href="https://hess.copernicus.org/articles/22/977/2018/hess-22-977-2018.pdf">The full text article is available as a PDF file from https://hess.copernicus.org/articles/22/977/2018/hess-22-977-2018.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e128">Cave drip water response to surface meteorological conditions is
complex due to the heterogeneity of water movement in the karst unsaturated
zone. Previous studies have focused on the monitoring of fractured rock
limestones that have little or no primary porosity. In this study, we aim to
further understand infiltration water hydrology in the Tamala Limestone of
SW Australia, which is Quaternary aeolianite with primary porosity. We build on
our previous studies of the Golgotha Cave system and utilize the existing
spatial survey of 29 automated cave drip loggers and a lidar-based flow
classification scheme, conducted in the two main chambers of this cave. We
find that a daily sampling frequency at our cave site optimizes the capture
of drip variability with the least possible sampling artifacts. With the optimum
sampling frequency, most of the drip sites show persistent autocorrelation
for at least a month, typically much longer, indicating ample storage of
water feeding all stalactites investigated. Drip discharge histograms are
highly variable, showing sometimes multimodal distributions. Histogram
skewness is shown to relate to the wetter-than-average 2013 hydrological year
and modality is affected by seasonality. The hydrological classification
scheme with respect to mean discharge and the flow variation can distinguish
between groundwater flow types in limestones with primary porosity, and the
technique could be used to characterize different karst flow paths when
high-frequency automated drip logger data are available. We observe little
difference in the coefficient of variation (COV) between flow classification
types, probably reflecting the ample storage due to the dominance of primary
porosity at this cave site. Moreover, we do not find any relationship between
drip variability and discharge within similar flow type. Finally, a
combination of multidimensional scaling (MDS) and clustering by <inline-formula><mml:math id="M1" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> means is
used to classify similar drip types based on time series analysis. This
clustering reveals four unique drip regimes which agree with previous flow
type classification for this site. It highlights a spatial homogeneity in
drip types in one cave chamber, and spatial heterogeneity in the other, which
is in agreement with our understanding of cave chamber morphology and lithology.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e147">Karst features in limestone are typically developed from the solutional
dissolution of fractures and bedding planes in carbonate rocks (Arbel et
al., 2010; Kurtzman et al., 2009). Worldwide, karst regions represent
significant geographical areas with potentially high rates of infiltration
through fractured and karstified carbonate rocks. The most usual recharge
method in karstic aquifers is the faster infiltration through the deep
karstic openings (Ford and Williams, 2007). Complex spatial spreading
of various karst features such as solutionally widened fractures, caves, and
conduits makes the monitoring and precise groundwater recharge modeling
very difficult (Lange et al., 2003; Arbel et al., 2010). The upper part
of karstified rock (the epikarst zone) has higher permeability than the
underlying vadose zone (Klimchouk, 2004). Therefore, infiltration into
the epikarst zone is faster compared to the drainage through it, and water
is kept stored in<?pagebreak page978?> this region. This stored water in the vadose zone seeps
slowly and finally emerges inside caves as infiltrating drip waters (Williams, 1983).</p>
      <p id="d1e150">Karstic features such as speleothems, commonly used to reconstruct
paleo-environmental records, are formed due to calcite deposition from cave
drip water. Therefore, the knowledge of drip water hydrology is critical to
study the paleoclimatic records (Baldini et al., 2006).
An early study using tipping bucket loggers formulated a relationship
between maximum discharge and coefficient of variation of discharge to
categorize cave discharges (Smart and Friederich, 1987), for a
fractured-rock limestone system with a vertical range of approximately 140 m
(GB Cave, Mendip Hills, UK). They found that the drips close to the surface
have extreme coefficients of variation, whereas the drips at depths have
fairly constant flow rates over time, with a significant possibility of
water storage in vadose zone fractures. Thus the stalagmite record resulting
from slower drips may be more closely related to the karst hydrology rather
than palaeoclimate (Baldini et al., 2006). This may
also be a consequence of the developed connection between the surface and
the cave. Quantitative analysis of such stalagmite drip data has, in the
past, used manual observations of cave drips (e.g., Baker et al., 1997).
However, the recent development of automatic cave drip loggers
(Collister and Mattey, 2008) has enabled generation of
high temporal resolution and continuous drip discharge time series
(e.g., Jex et al., 2012; Cuthbert et al., 2014; Markowska et al., 2015;
Mariethoz et al., 2012), providing new opportunities for quantitative
hydrological analysis.</p>
      <p id="d1e153">Here we present monitoring data from Golgotha Cave located in SW Western
Australia that has been extensively monitored since 2005, with the aim of
better understanding karst drip water hydrogeology and the relationship
between drip hydrology and surface climate. We build on the work of
Mahmud et al. (2016), which presented the largest spatial
and temporal survey of automated cave drip monitoring with matrix (primary)
porosity published to date. This previous study consisted of data from two
large chambers within this cave, measured in the period from August 2012 to
March 2015, using a highly spatially (29 sites in two separate chambers) and
temporally (0.001 Hz, 15 min intervals) resolved data set. In a separate
study, Mahmud et al. (2015) performed morphological analysis of
karstic features, based on ground-based lidar data, to identify different
flow processes in karstified limestone. Based on the findings of these two
studies, here we investigate the relationship between drip water hydrology
and cave depth, spatial location, and stalactite type, and develop a
hydrological classification scheme that is appropriate to high-frequency
drip logger data and limestones with a primary porosity. This classification
scheme is also compared with previous studies (Smart and Friederich,
1987; Baker et al., 1997) to examine the limitations of these previous
schemes. These findings will also help better characterize and understand
water movement in highly porous karst formations.</p>
      <p id="d1e156"><?xmltex \hack{\newpage}?>Finally, we use a combination of multidimensional scaling (MDS) and the
popular <inline-formula><mml:math id="M2" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> means algorithm for clustering similar drip characteristics. Time
series clustering has been shown to be effective in providing useful
information in various domains (Liao, 2005) and is implemented
here to determine the degree of similarity between two drip time series.
There seems to be an increased interest in time series clustering as part of
the research effort in temporal data mining. The method we use here is
suitable for large data sets, has been studied extensively in the past and
achieves good results with minimum computational cost (Jex et al., 2012;
Scheidt and Caers, 2009; Borg and Groenen, 1997).</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Site description</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Studied cave</title>
      <p id="d1e182">The cave site has been explained in detail by Treble et al. (2013). Briefly,
the field site Golgotha Cave is 200 m in length and up to
25 m in width (Fig. 1), and developed in
Quaternary aeolianite, which consists of wind-blown calcareous sands that
were deposited along the southwest coast of Australia (Brooke et al., 2014).
Vadose zone water flow, and subsequent widening by ceiling collapse, formed
the cave chambers. Treble et al. (2013) described the cave
site as being developed in the Spearwood system of the Tamala Limestone and
is mantled by a variable thick layer of sand formation having depths of
between 0.3 and 3 m. Diffuse (or matrix) flow is likely to be dominant in
the Tamala Limestone formation due to its high matrix porosity as 0.3–0.5
(Smith et al., 2012). Karst in this region is also called
“syngenetic” (Treble et al., 2013), implying processes
like preferential vertical dissolution and varying morphology of the
subsurface caprock. These processes may establish vadose zone preferential
flow extending to the cave ceiling, with occasional rapid delivery of
percolating waters deep into the calcarenite which end up seeping through to
the cave ceiling. Therefore, this young limestone formation offers various
opportunities for preferential flow into the host rock and storage within it
(Brooke et al., 2014). Golgotha Cave was chosen
because (a) it is located in an intensively studied karst area (Treble et al.,
2013, 2015, 2016), which has over 10 years of manual and 3 years of automated drip water monitoring, (b) it
contains actively growing speleothems, and (c) it is accessible year-round.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e187"><bold>(a)</bold> Coastal belt of SWWA (southwest Western Australia).
<bold>(b)</bold> Golgotha Cave plan view displaying both Chamber 1 (green marked
area), which comprises Site 1, and Chamber 2 (blue marked area) containing Site 2.
Average limestone thickness from cave ceiling to ground surface over Site 1
and 2 is 32.33 and 40.24 m, respectively. Lidar scans of drip sites on
<bold>(c)</bold> Chamber 1 north floor, <bold>(d)</bold> Chamber 1 south floor, and
<bold>(e)</bold> Chamber 2 floor. The red arrows show the geographic orientation <bold>(c, d, e)</bold>.
<inline-formula><mml:math id="M3" display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula> indicates the sites where the stalagmite loggers are not clearly visible
in the lidar floor images as they are obscured by formations in front of them,
however the approximate locations are marked with yellow circles. Additional scans
of cave ceiling and photographs of underlying stalagmites are shown in Fig. 3 of
Mahmud et al. (2016).</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://hess.copernicus.org/articles/22/977/2018/hess-22-977-2018-f01.png"/>

        </fig>

      <p id="d1e223">Based on previous studies at this site, we determined previously that
Chamber 1 (Fig. 1b–d) is mostly dominated
by matrix flow representing water flowing down and seeping through the rock
matrix, characterized by both icicle-shaped and soda-straw stalactites with
slow drip rates of low variability. In contrast, Chamber 2
(Fig. 1b and e) is typically controlled by
fracture and combined flow, with high drip rates that are shown to vary over
time depending upon the mode of water delivery to the preferential flow
system.<?pagebreak page979?> In fracture flow, water moves along the fracture orientation,
forming curtain-shape stalactites in the direction of highest fracturing.
Finally, combined flow is defined as the combination of conduit, matrix, and
fracture flow, resulting in a circular pattern of stalactite formation.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Climate and meteorology</title>
      <p id="d1e234">A comprehensive description of the climate at our study site has been
presented in Treble et al. (2013). To summarize, the site
is a Mediterranean climate, associated with wet winters and dry summers.
Annual rainfall recorded at Forest Grove weather station
(Fig. 1a, 5 km away from the study site) is
1136.8 <inline-formula><mml:math id="M4" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 184 mm, among which <inline-formula><mml:math id="M5" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 75 % occurs between May
and September, with an average daily maximum temperature variation from
16 <inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C (in July) to 27 <inline-formula><mml:math id="M7" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C (in February; BoM,
2017). Typically, the peak rainfall begins in late autumn (May) and the wet
season continues until end of September with a median monthly rainfall of
<inline-formula><mml:math id="M8" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 100 mm. Each hydrological year is defined as April to March,
as April has the lowest water budget (precipitation less evapotranspiration).</p>
      <p id="d1e276"><?xmltex \hack{\newpage}?>As reported in previous studies, all hydrological years have water deficit
during the dry season (October to April) and significant infiltration during
the wet period. Low evaporative conditions during winter should permit
increased infiltration to the caves, enhancing the drip discharge response
to winter rainfall. The hydrological year 2012 had roughly similar annual
rainfall of 1008.6 mm to the long-term annual mean, whereas 2013 was rather
wet (total rainfall of 1239.8 mm) and 2014 was a relatively dry year with a
total rainfall of 943.8 mm. Recorded rainfall was significantly above
average in the 2013 hydrological year for various weather stations in
Western Australia (BoM, 2017). Therefore, our site had a wetter
winter in 2013 with an estimated annual recharge of 858.67 mm which is very
much above average (10-year mean annual recharge is 564 mm).</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Drip data acquisition and characteristics</title>
      <p id="d1e288">Data acquisition and pre-processing has been previously described in
Mahmud et al. (2016) and is concisely summarized here.
Stalagmite drip loggers (<uri>http://www.driptych.com</uri>) were set up in approximate
transects throughout the<?pagebreak page980?> two large chambers from higher to lower ceiling
elevations in 34 locations and have been monitored since August 2012.
Both chambers of Golgotha Cave have contrasting discharge, dune facies, and karst features (Fig. 1). Data loggers were set
to record continuously at 15 min intervals. The notation used for site
identification follows the same style as described in previous studies,
consisting of a numerical number (representing the chamber) and a
letter/roman number (representing a drip site within the given chamber, with
a letter indicating the sites having both manual and automatic drip counts
and a roman number specifying the sites only having drip logger data). Based
on previous studies of the site, 29 sites are considered in the time series
analysis although short periods of poor quality data were omitted if they
were associated with changes in the mean and variability at the time of
fieldwork. This impacted sites 1A, 1B, 2A, 2B, 2E as the logger was
temporarily placed aside every 6 weeks in order to sample water from a
collection bottle underneath the logger. Time series gaps are filled with
synthetic data based on the drip statistics and correlation between drip rates.</p>
      <p id="d1e294">As previously reported, drip rates in Chamber 1 are generally very low (the
fastest drip rate was 25 drips per 15 min) consistent with the predominance
of matrix flow in this chamber. However, it is obvious that most drip
loggers exhibit a clear response to the 2013 wet winter and also indicate
the substantial interannual variation in discharge between three
hydrological years. All Chamber 1 drip sites (except Site 1x) show a gradual
drip rate decrease during summer 2012 to winter 2013 due to below average
rainfall in 2012. Then after displaying the sudden increase in all drip
discharges that express the 2013 wet winter, the drip rates further reduce
due to the dry 2014 hydrological year. This intra-annual variation is
identified to be much greater than the interannual discharge variation of the
drip sites, as previously observed in Baker et al. (1997). This suggests
that high-resolution intra-annual drip rate data is
helpful to obtain a complete picture of changing flow variability with
recharge. The high resolution of the data sets includes precise
characterization of the temporal behavior of an individual drip,
illustrating the differences inherent to the drip sites.</p>
      <p id="d1e297">In contrast, Chamber 2 drip rates present more variability between sites
both in intra- and interannual discharges, except few very slow
dripping sites. Of the Chamber 2 drips, the slow drip sites have the lowest
coefficients of variation (COVs) and lowest discharges, indicative of matrix
flow types. The timing of maximum drip rates is generally delayed in Chamber 2
versus Chamber 1: Chamber 1 drip rates typically peak in late spring/early
summer (October–December) while Chamber 2 drips tend to peak a few months later
(December–May), reflecting a longer water residence time. This may be a function
of the thicker ceiling above Chamber 2 (40.24 versus 32.33 m) but also
heterogeneity in flow paths to each chamber. Overall the drip response to
the 2013 wet winter is amplified in Chamber 2 versus Chamber 1, consistent
with the presence of greater fracture flow in Chamber 2.</p>
      <p id="d1e300">By applying morphological analysis of ceiling features acquired by lidar
data, Mahmud et al. (2015) distinguished three flow patterns
(i.e., matrix flow, fracture flow, and a combination of conduit, fracture,
and matrix flow) for the observed ceiling morphological features. All the
drip sites were then characterized according to this flow classification in
Mahmud et al. (2016), which is used here as a reference for clustering similar drip time series.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Methods</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Hydrological classification of cave drips</title>
      <p id="d1e319">Research involving automated drip monitoring systems is increasing, for
example at Cathedral Cave in Wellington (Cuthbert et
al., 2014) and Harrie Wood Cave in the Snowy Mountains, Yarrangobilly
(Markowska et al., 2015). The variability of the drip
discharge might not only be a function of discharge itself; it could also
depend on the sampling frequency. We investigate this possibility by
plotting the COV versus sampling interval (the original 15 min and
calculated by resampling the data at 1 h, 1 day, 1 week, and 1 month). COV
is supposed to be artificially high at the high frequency of 15 min because
of sampling bias that artificially increases the noise. The resampling at
low frequencies is simply a way of smoothing out this noise. Using the optimum
sampling frequency to minimize its effect on drip variability, we plot drip
rate histograms to identify the response of drips between the flow
classifications and the response to intra- and interannual variability in
infiltration. We also plot the autocorrelation functions (ACFs) to
investigate the relationship between the strength of correlation and the
lidar-based flow type. Finally, we summarize the mean discharge of drip
sites in relation to the variability in discharge using the optimum sampling
frequency. These are the same drip discharge parameters as used in the
classification method proposed by Friederich and Smart (1982),
Fairchild et al. (2006), and Baker et al. (1997) that were based on manual
drip collection at low frequency.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Clustering of similar drip time series</title>
      <p id="d1e330">We employed multidimensional scaling (MDS), which allows data
dimensionality reduction, i.e., mapping complex multidimensional data on a
low-dimensional manifold. MDS is a technique that embeds a set of points in
a low-dimensional space, so that the distances between the points resemble
as closely as possible a given set of dissimilarities between the objects
they represent (Birchfield and Subramanya, 2005). MDS requires a
distance matrix to be computed in which a single scalar number
characterizes the similarity between any two time series. In our case, each
drip logger is an object and a specific distance between drip loggers is
considered to characterize the similarity between any two loggers. It takes
an input matrix giving dissimilarities between pairs of items and outputs a
coordinate matrix whose configuration minimizes a loss function. MDS is also
known as principal coordinates analysis (PCoA). MDS operates on a distance
or dissimilarity matrix (Pisani et al., 2016), which is different than
principal component analysis (PCA) that is based on a covariance matrix.
Even if PCA and MDS methods can return the same results in specific
contexts, MDS can be considered more general because it remains valid for
non-Euclidean distances, such as the distance matrix (<inline-formula><mml:math id="M9" display="inline"><mml:mi mathvariant="bold">D</mml:mi></mml:math></inline-formula>) chosen in this
study. MDS is used to translate these distances into a configuration of
points defined in an <inline-formula><mml:math id="M10" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>-dimensional Euclidean space (Cox and Cox, 1994).
MDS results in a set of points arranged so that their corresponding
Euclidean distances indicate the dissimilarities of the time series.
According to Birchfield and Subramanya (2005) the basic steps of
performing the MDS algorithm are as follows:
<list list-type="custom"><list-item><label>i.</label>
      <p id="d1e349">Construct the distance matrix <inline-formula><mml:math id="M11" display="inline"><mml:mi mathvariant="bold">D</mml:mi></mml:math></inline-formula>: one key component in clustering is the
function used to measure the temporal similarity (or distance) between any
two time series being compared. To define an appropriate measure of
similarity between time series, we determine two factors: firstly, the
offset (<inline-formula><mml:math id="M12" display="inline"><mml:mi>O</mml:mi></mml:math></inline-formula>) to match two time series based on their maximum correlation, and
secondly the complement of the correlation coefficient (1 <inline-formula><mml:math id="M13" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M14" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>) between the time
series (Jex et al., 2012). Initially, we compute the cross-correlation
function, a measure of similarity of two time series as a function of the
displacement of one relative to the other. The cross-correlation function is
an estimate of the covariance between two time series, <inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mi>t</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi>t</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, at lags <inline-formula><mml:math id="M17" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M18" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0, <inline-formula><mml:math id="M19" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1, <inline-formula><mml:math id="M20" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>2, …. The offset (<inline-formula><mml:math id="M21" display="inline"><mml:mi>O</mml:mi></mml:math></inline-formula>) is
defined as the lag time based on the maximum correlation between two
time series. Next, we define R as the correlation coefficient with the time
series being moved by the offset amount <inline-formula><mml:math id="M22" display="inline"><mml:mi>O</mml:mi></mml:math></inline-formula> to have maximum correlation
coefficient. Both <inline-formula><mml:math id="M23" display="inline"><mml:mi>O</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M24" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> are calculated to all <inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>n</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M26" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> 1)/2 pairs of drip data, where <inline-formula><mml:math id="M27" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> is
the number of drip data. Here, we use the original recorded drip counts in
15 min interval. The sampling bias discussed in Sect. 3.1 only affects the drip variability, not the
cluster analysis. Moreover, high-resolution (15 min interval) data are more
suited for the cluster analysis because it allows better defining the
cross-correlation between drips, as sometimes the offset of maximum
correlation <inline-formula><mml:math id="M28" display="inline"><mml:mi>O</mml:mi></mml:math></inline-formula> might be less than a day. Finally, the distance matrix <inline-formula><mml:math id="M29" display="inline"><mml:mi mathvariant="bold">D</mml:mi></mml:math></inline-formula> is
computed for each pair of loggers using the following equation (Jex et al., 2012):<disp-formula id="Ch1.Ex1"><mml:math id="M30" display="block"><mml:mstyle class="stylechange" displaystyle="true"/><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="bold">D</mml:mi><mml:mo>=</mml:mo><mml:mi>O</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>The distance matrix (<inline-formula><mml:math id="M31" display="inline"><mml:mi mathvariant="bold">D</mml:mi></mml:math></inline-formula>) is square, symmetric, and has dimension equal to the
number of drip loggers.</p></list-item><list-item><label>ii.</label>
      <p id="d1e541">Compute the inner product matrix <inline-formula><mml:math id="M32" display="inline"><mml:mi mathvariant="bold">B</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M33" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:mi>J</mml:mi><mml:mi mathvariant="bold">D</mml:mi><mml:mi>J</mml:mi></mml:mrow></mml:math></inline-formula>, where
<inline-formula><mml:math id="M35" display="inline"><mml:mi mathvariant="bold">J</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M36" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M37" display="inline"><mml:mi>I</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M38" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mn mathvariant="normal">1</mml:mn><mml:mi>n</mml:mi></mml:mfrac></mml:mstyle><mml:msup><mml:mn mathvariant="bold">11</mml:mn><mml:mi>T</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> is the double-centering matrix and <inline-formula><mml:math id="M40" display="inline"><mml:mn mathvariant="bold">1</mml:mn></mml:math></inline-formula> is a
vector of ones.</p></list-item><list-item><label>iii.</label>
      <p id="d1e632">Decompose <inline-formula><mml:math id="M41" display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula> as <inline-formula><mml:math id="M42" display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M43" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:mi>V</mml:mi><mml:mi mathvariant="normal">Λ</mml:mi><mml:msup><mml:mi>V</mml:mi><mml:mi>T</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M45" display="inline"><mml:mi mathvariant="bold">Λ</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M46" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> diag(<inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, …, <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi>n</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>,
the diagonal matrix of eigenvalues of <inline-formula><mml:math id="M49" display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M50" display="inline"><mml:mi mathvariant="bold">V</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M51" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> [<inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, …,
<inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>], the matrix of corresponding unit eigenvectors.
Sort the eigenvalues in non-increasing order: <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M55" display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> … <inline-formula><mml:math id="M56" display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M58" display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 0.</p></list-item><list-item><label>iv.</label>
      <p id="d1e799">Extract the first <inline-formula><mml:math id="M59" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> eigenvalues <inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Λ</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M61" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> diag(<inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, …, <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and corresponding eigenvectors
<inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M65" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> [<inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, …, <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>].</p></list-item><list-item><label>v.</label>
      <p id="d1e891">The corresponding Euclidean distances of the set of points, indicating
the dissimilarities of the time series, are now located in the <inline-formula><mml:math id="M68" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M69" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M70" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula>
matrix <inline-formula><mml:math id="M71" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M72" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> [<inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, …, <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:msup><mml:mo>]</mml:mo><mml:mi>T</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M75" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:msubsup><mml:mi mathvariant="normal">Λ</mml:mi><mml:mi>p</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>.</p></list-item></list>
The <inline-formula><mml:math id="M77" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> means clustering algorithm is then used to divide these points into
<inline-formula><mml:math id="M78" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> clusters, which corresponds to a categorization of the drip data time
series. <inline-formula><mml:math id="M79" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> means clustering, or Lloyd's algorithm (Lloyd, 1982), is a
method of vector quantization that is popular for cluster analysis in data
mining. <inline-formula><mml:math id="M80" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> means clustering aims to partition <inline-formula><mml:math id="M81" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> observations into <inline-formula><mml:math id="M82" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> clusters
in which each observation belongs to the cluster with the nearest mean,
serving as a prototype of the cluster. The algorithm proceeds as follows:
<list list-type="custom"><list-item><label>i.</label>
      <p id="d1e1033">Choose <inline-formula><mml:math id="M83" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> initial cluster centers (centroid): here, we use <inline-formula><mml:math id="M84" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M85" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 4 clusters as this was
the number of flow categories identified in previous work at this site.</p></list-item><list-item><label>ii.</label>
      <p id="d1e1058">Compute point-to-cluster-centroid distances of all observations to each
centroid. There are two steps to follow: first assign each observation to
the cluster with the closest centroid. Then individually assign observations
to a different centroid if the reassignment decreases the sum of the
within-cluster, sum-of-squares point-to-cluster-centroid distances.</p></list-item><list-item><label>iii.</label>
      <p id="d1e1062">Compute the average of the observations in each cluster to
obtain <inline-formula><mml:math id="M86" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> new centroid locations.</p></list-item><list-item><label>iv.</label>
      <p id="d1e1073">Repeat steps 2 and 3 until cluster assignments do not change, or the
maximum number of iterations is reached.</p></list-item></list></p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e1078">Optimum sampling frequency that minimizes sampling artifacts while
maximizing the capture of natural variability.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://hess.copernicus.org/articles/22/977/2018/hess-22-977-2018-f02.png"/>

        </fig>

</sec>
</sec>
<?pagebreak page981?><sec id="Ch1.S4">
  <label>4</label><title>Results and discussion</title>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Determining the relationship between sampling frequency and drip discharge COV</title>
      <p id="d1e1103">We test the variability of drip discharge COV with the sampling frequency in
Fig. 2, to find the optimum sampling frequency that minimizes sampling
artifacts while maximizing the capture of natural variability. For high
discharge, COV increases with sampling frequency, which we explain by the
smaller sampling interval better capturing the actual drip variability. For
low discharges, COV also increases with<?pagebreak page982?> sampling frequency, which we explain
by the variability introduced due to drip rates being less than the sampling
frequency. From the data presented in Fig. 2, we can conclude that for
both chambers and to compare all different types of flow, a sampling
frequency of 1 day gives the minimum COV, which does not change
significantly with a finer sampling frequency. Therefore, we use a sampling
frequency of 1 day that minimizes sampling artifacts while maximizing the
capture of natural variability. For Golgotha Cave, this would be to sum the
15 min drip rates over a 1-day period. This optimized sampling frequency
is used to plot the histograms (Sect. 4.2) and ACFs
(Sect. S1 in the Supplement), and to examine the drip discharge behavior with drip
variability for various flow types (Sect. 4.3).</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Drip rate frequency distributions</title>
      <p id="d1e1114">Figure 3 shows the drip rate histograms for representative drip sites and
different flow categories with optimum sampling frequency of 1 day. Drip
sites are organized from lowest to highest discharge in each flow
classification. Slow dripping soda-straw flows (e.g., sites 2xi, 2iii, and 1v)
show variation of drips with seasonality and the response to wetter recharge
period with an approximate 6-month lag, which suggests the drip water is
supplied from storage in the limestone formation. Among these, Site 1v
displays the response to recharge in much shorter duration, the 6 months
following 2013 recharge and then a shift to lower flow rates which may
represent flow poaching. The histograms for icicle and combined flow systems
represent unimodal skewed to bimodal distributions, indicating the shift to
higher drip rates in response to the wetter 2013 hydrological year (except
Site 2xiii, which shows a shift to lower drip rates). The rest of the
fracture sites show bimodal or multimodal distributions. With the limited
temporal scale of the analysis, it seems that the histograms with skewed
distributions represent the consequences of wetter 2013 hydrological year.
These skewed distributions seem to have higher drip rate response to the
drier 2014–2015 period rather than the earlier normal/wetter years. This
clearly denotes potential refilling of storage within the system during the
2013 wet winter, and later supplying drip water in 2014–2015 seasons. In
contrast, the bimodal distribution of Site 2viii indicates the drip response
to the annual cycle of wet and dry seasons of each hydrological year with an
approximate 6-month lag. Several bimodal (e.g., Site 1x) and multimodal
(e.g., sites 2xvi, 2vi) distributions, characterized as fracture flow, also
distinguishes the dry period of 2012–2013 (having low drip rates) from the
later period of 2013 wet winter (with high drip rates).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e1119">Histogram plots of both chambers' drip data according to four flow types
identified in Mahmud et al. (2016). Each histogram represents the frequencies
of the drip counts per day (the axes labels are shown in the first histogram).
Bin size is uniform for all plots and the external tick marks in <inline-formula><mml:math id="M87" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> axes
delineate the bin intervals. The legend shows all the seasons over the
monitoring period (blue to cyan for wet seasons: April to September; red to
yellow for dry seasons: October to March, with the color gradually shifting for
different years). The 2012 wet season experienced similar rainfall to the
long-term annual mean, whereas 2013 was rather wet and 2014 was a relatively
dry year. Histogram data for all sites appear in Fig. S1 in the Supplement.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://hess.copernicus.org/articles/22/977/2018/hess-22-977-2018-f03.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Autocorrelation functions (ACFs)</title>
      <p id="d1e1143">We investigate the use of ACFs to analyze drip behavior using the optimum
sampling frequency of 1 day and until lags of 365 days. We do not find
significant yearly autocorrelation with this limited 3 years of data. In
some drips, a negative correlation occurred, but it is very insignificant
and no physical process can explain a negative yearly correlation.
Therefore, we plot ACFs in Fig. 4 for different flow categories with the
optimum sampling frequency of 1 day and lag time of 200 days. All sites have
an autocorrelation that persists for at least a month, and often much
longer. However, there is no relationship between the strength or the
temporal decay of the correlation and the lidar-based flow classification.
This indicates the presence of ample storage in the system, supplying all stalactite types.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e1148">Autocorrelation functions of both chambers' drip data according to flow
classification of Mahmud et al. (2016). <inline-formula><mml:math id="M88" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M89" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axes of individual plots
represent the lag (in days) and ACF, respectively (the axes labels are shown in
the first ACF plot). ACFs for all sites appear in Fig. S2.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://hess.copernicus.org/articles/22/977/2018/hess-22-977-2018-f04.png"/>

        </fig>

<?xmltex \hack{\newpage}?>
</sec>
<?pagebreak page983?><sec id="Ch1.S4.SS4">
  <label>4.4</label><title>Hydrological classification of cave drips</title>
      <p id="d1e1181">We examine the hydrological behavior of the drips at daily resolution with
respect to mean discharge and flow variation in Fig. 5. It is clear from
Fig. 5 that there is no relationship between COV and flow type. One
soda-straw discharge (Site 2xi) has seasonal dryness, a very low
discharge, and a very high coefficient of variation due to its irregular
dripping. Otherwise, nearly all soda-straw flow, icicle flow, combined flow
and fracture flow drips have COV <inline-formula><mml:math id="M90" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 60 %, with the exception of one
fracture flow site showing the highest COV (Fig. 5). But in general, there
is little difference in the COV between classification types, probably
reflecting the ample storage (Sect. S1) due to the dominance
of primary porosity at this cave. We do not clearly observe increasing
variability with decreasing discharge within similar flow type, in contrast
to other studies from older, fractured rock limestones (Smart and
Friederich, 1987; Baldini et al., 2006; Baker et al., 1997). This shows that
Golgotha Cave drip sites do not fit within the drip classification method
proposed by Smart and Friederich (1987) and
Baker et al. (1997), which were based on manual drip
counts with limited number of intermittent drip sites. Moreover, we utilize
drip data from a cave with primary porosity, capturing the full range of
flow types from matrix through to fracture, whereas the previous
classifications only captured slow vs. fast drips that were likely dominated
by fracture flow paths given the host rock setting.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e1193">Hydrological behavior of drip sites expressed in terms of daily mean
discharge versus daily discharge variability calculated from the automatic drip
rate data for three hydrological years. Measured drip rates are converted to
volume units assuming a drip volume of 0.1433 mL (Genty and Deflandre, 1998).
Blue lines and symbols reflect flow classification given in Mahmud et al. (2015).</p></caption>
          <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://hess.copernicus.org/articles/22/977/2018/hess-22-977-2018-f05.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS5">
  <label>4.5</label><title>Clustering of similar drip time series</title>
      <p id="d1e1211">The clustering results are overlaid upon the chamber ceiling images in
Fig. 6 and also summarized in Tables 1 and 2 with the average drip
discharges and flow type classification<?pagebreak page984?> based on lidar. Average drip
discharges are calculated from the 15 min drip rates. As mentioned above,
drip logger time series are deemed similar if they are well correlated and
only have a small offset with each other, and so these time series should
cluster together. Most of the drip sites that are identified as matrix flow
(soda-straw and icicle flow) cluster together in C1. However, three of the
icicle flow sites with drip rates greater than 4 per 15 min fall in C2.
The combined flow category and the fracture type usually cluster in C3
and C4,
respectively. Therefore we observe that our clustering generally agrees
with the morphology-based flow classification of Mahmud et
al. (2016). Few of the flow classes show exceptions, for example Site 2vi is
a fracture type flow and cluster in C1. This site has really high discharge
with high variability, showing irregular drip rate.</p>
      <p id="d1e1214">One consistent feature that appears from the cluster analysis of Fig. 6 is
the spatial homogeneity of the clusters in Chamber 1, suggesting that they
are spatially connected, or that their flow paths are connected to the same
hydrological domain (the karst matrix), and supporting the overall dominant
matrix flow patterns (both soda-straw and icicle). Chamber 2 presents a
completely different situation, where it is obvious that drip sites can have
similar behavior (well correlated with a small lag), and be
spatially distinct features, separated by spans of approximately 6 m
(Fig. 6). In particular, clusters 3 and 4 are spatially scattered,
representing the presence of fractures and combined flow systems throughout
the chamber ceiling. This indicates an overall strong heterogeneity of the
flow paths between the surface and the cave for Chamber 2. Hence, in Chamber 2
we expect flow paths to be more complex with routing between multiple
stores and interconnected fracture networks potentially resulting in
non-linear response to infiltration. This is supported by drip water <inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O
data for this chamber (Treble et al., 2013).</p>
</sec>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Implications of the findings and future research</title>
      <p id="d1e1238">Starting with the time series analysis, this research presents a methodology
that can be applied globally for drip logger data. The results show that
some data integration is necessary to avoid artifacts from slow drip sites.
For sites where there is significant matrix flow, our study has demonstrated
that the Smart and Friederich classification is not appropriate. Therefore,
this study has presented alternative hydrological classification schemes
that are suitable for cave sites that include matrix flow. The times series
approach adopted in<?pagebreak page985?> this study also opens the way for improved analysis and
classification of hydrology time series in general, i.e., tests for histogram,
autocorrelation, cluster analysis, and all of these will certainly benefit
our understanding of the hydrology of karst systems.</p>
      <p id="d1e1241">In this study, we also extend the analysis of drip time series to multiple
sites, whereby we take advantage of the ensemble of loggers to extract
common properties by clustering, which would not be possible with single
site analysis. The results show that by considering multiple simultaneous
time series, one can make better inferences about water flow and unsaturated
zone properties. The main impact is to recommend the use of spatial networks
of loggers over individual loggers. It should be noted that currently, most
researchers deploy only a few loggers to understand the flow to individual
sites. This study also proposes a possible methodology for the analysis of
such data sets.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e1247">MDS cluster groups with statistical properties of Chamber 1 drip data.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="center"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Site/</oasis:entry>
         <oasis:entry colname="col2">MDS</oasis:entry>
         <oasis:entry colname="col3">Average</oasis:entry>
         <oasis:entry colname="col4">Flow</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">stalagmite</oasis:entry>
         <oasis:entry colname="col2">cluster</oasis:entry>
         <oasis:entry colname="col3">drip</oasis:entry>
         <oasis:entry colname="col4">type</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">group</oasis:entry>
         <oasis:entry colname="col3">discharge</oasis:entry>
         <oasis:entry colname="col4">(lidar-</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">(L yr<inline-formula><mml:math id="M92" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col4">based)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">1A</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">19.8</oasis:entry>
         <oasis:entry colname="col4">Icicle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1B</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">12.6</oasis:entry>
         <oasis:entry colname="col4">Icicle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1i</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">6.6</oasis:entry>
         <oasis:entry colname="col4">Icicle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1ii</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">11.2</oasis:entry>
         <oasis:entry colname="col4">Icicle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1iii</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">8.1</oasis:entry>
         <oasis:entry colname="col4">Icicle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1v</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">6.7</oasis:entry>
         <oasis:entry colname="col4">Soda-straw</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1vi</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">7.4</oasis:entry>
         <oasis:entry colname="col4">Icicle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1viii</oasis:entry>
         <oasis:entry colname="col2">2</oasis:entry>
         <oasis:entry colname="col3">60.9</oasis:entry>
         <oasis:entry colname="col4">Combined</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1ix</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">14.8</oasis:entry>
         <oasis:entry colname="col4">Icicle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1x</oasis:entry>
         <oasis:entry colname="col2">3</oasis:entry>
         <oasis:entry colname="col3">86.2</oasis:entry>
         <oasis:entry colname="col4">Fracture</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1xi</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">12.7</oasis:entry>
         <oasis:entry colname="col4">Icicle</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e1509">MDS cluster groups with statistical properties of Chamber 2 drip data.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="center"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Site/</oasis:entry>
         <oasis:entry colname="col2">MDS</oasis:entry>
         <oasis:entry colname="col3">Average</oasis:entry>
         <oasis:entry colname="col4">Flow</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">stalagmite</oasis:entry>
         <oasis:entry colname="col2">cluster</oasis:entry>
         <oasis:entry colname="col3">drip</oasis:entry>
         <oasis:entry colname="col4">type</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">group</oasis:entry>
         <oasis:entry colname="col3">discharge</oasis:entry>
         <oasis:entry colname="col4">(lidar-</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">(L yr<inline-formula><mml:math id="M93" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col4">based)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">2A</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">9.4</oasis:entry>
         <oasis:entry colname="col4">Icicle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2B</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">17.1</oasis:entry>
         <oasis:entry colname="col4">Icicle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2E</oasis:entry>
         <oasis:entry colname="col2">3</oasis:entry>
         <oasis:entry colname="col3">140.3</oasis:entry>
         <oasis:entry colname="col4">Combined</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2i</oasis:entry>
         <oasis:entry colname="col2">4</oasis:entry>
         <oasis:entry colname="col3">243.0</oasis:entry>
         <oasis:entry colname="col4">Fracture</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2iii</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">4.2</oasis:entry>
         <oasis:entry colname="col4">Soda-straw</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2iv</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">14.6</oasis:entry>
         <oasis:entry colname="col4">Icicle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2v</oasis:entry>
         <oasis:entry colname="col2">3</oasis:entry>
         <oasis:entry colname="col3">67.8</oasis:entry>
         <oasis:entry colname="col4">Combined</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2vi</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">985.0</oasis:entry>
         <oasis:entry colname="col4">Fracture</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2vii</oasis:entry>
         <oasis:entry colname="col2">2</oasis:entry>
         <oasis:entry colname="col3">25.0</oasis:entry>
         <oasis:entry colname="col4">Icicle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2viii</oasis:entry>
         <oasis:entry colname="col2">3</oasis:entry>
         <oasis:entry colname="col3">113.8</oasis:entry>
         <oasis:entry colname="col4">Combined</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2ix</oasis:entry>
         <oasis:entry colname="col2">4</oasis:entry>
         <oasis:entry colname="col3">360.2</oasis:entry>
         <oasis:entry colname="col4">Fracture</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2x</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">7.0</oasis:entry>
         <oasis:entry colname="col4">Icicle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2xi</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">0.6</oasis:entry>
         <oasis:entry colname="col4">Soda-straw</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2xiii</oasis:entry>
         <oasis:entry colname="col2">2</oasis:entry>
         <oasis:entry colname="col3">26.2</oasis:entry>
         <oasis:entry colname="col4">Icicle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2xiv</oasis:entry>
         <oasis:entry colname="col2">2</oasis:entry>
         <oasis:entry colname="col3">42.8</oasis:entry>
         <oasis:entry colname="col4">Icicle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2xv</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">11.6</oasis:entry>
         <oasis:entry colname="col4">Icicle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2xvi</oasis:entry>
         <oasis:entry colname="col2">3</oasis:entry>
         <oasis:entry colname="col3">266.9</oasis:entry>
         <oasis:entry colname="col4">Fracture</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2xvii</oasis:entry>
         <oasis:entry colname="col2">1</oasis:entry>
         <oasis:entry colname="col3">7.0</oasis:entry>
         <oasis:entry colname="col4">Icicle</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e1876">Cluster group plot overlaid upon the cave ceiling for both chambers.
The ceiling images are captured by lidar and the circles represent the ceiling
locations of stalactites dripping on various stalagmites in both chambers
(shown in Fig. 1). The color of the circles indicates individual MDS cluster
group. The blue arrows in both figures show the geographic orientation and the
green arrows represent the approximate transects throughout the chambers from
higher to lower ceiling elevations.</p></caption>
        <?xmltex \igopts{width=256.074803pt}?><graphic xlink:href="https://hess.copernicus.org/articles/22/977/2018/hess-22-977-2018-f06.png"/>

      </fig>

      <p id="d1e1885">Regarding the application of our findings, we believe that our methodology based
on drip logger data sets can provide direct evidence of deep drainage, and
therefore the timing of diffuse recharge, which could be used for basic
model calibration. Spatial drip data (possibly combined with lidar) is
beneficial to infer flow types (e.g., the proportion of fracture versus matrix) which could be used for model configuration to produce realistic karst
recharge (Hartmann et al., 2012), and hence large-scale
groundwater estimation (Hartmann et al., 2015). Another
potential application is the integration of flow types in groundwater models
through inverse modeling. Such data could also be used to constrain water
isotope model configurations used for forward modeling speleothem
<inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O (Bradley et al., 2010; Treble et al., 2013). Overall, the
findings of this work will definitely provide a better understanding of
processes that control vadose zone flow and transport processes, which would
ultimately help develop approaches to incorporate these processes into
simulation models (Hartmann and Baker, 2017).</p>
      <p id="d1e1899">The analysis, presented here and combined with the findings of previous work
at this site, provides valuable information for paleoclimatologists and
geochemists wishing to sample stalagmites. While these studies have
characterized<?pagebreak page986?> Golgotha Cave, they could be applied to any other cave system.
In our previous work we (1) devised a classification for flow type
based on stalactite morphology; (2) quantified the recharge response of each
flow type to infiltration; (3) combined the findings of points 1–2 to
estimate the total volume of cave discharge; and (4) compared cave discharge with
infiltration to estimate the total recharge volume and identify highly
focused areas of recharge. The current study has further developed the
spatial and temporal statistical relationships between the flow sites,
allowing both quantification and visualization of the hydrology between the
ground surface and the cave ceiling. More generally, these studies
illustrate the heterogeneity between flow sites and demonstrate methods that
can be applied to any cave system for studying diffuse recharge and
paleoclimate records from speleothems.</p>
      <p id="d1e1902">We further propose some ideas for future research that have evolved from
this study:
<list list-type="custom"><list-item><label>a.</label>
      <p id="d1e1907">Combining a drip logger network with a surface weather station and soil
moisture network to constrain the water balance in hydrological models.
Additionally, employing sap flow meters could allow constraining tree water use.
<?xmltex \hack{\newpage}?></p></list-item><list-item><label>b.</label>
      <p id="d1e1912">Combining the logger network, which constrains diffuse recharge, to
boreholes measuring groundwater level to understand the relative importance
of diffuse and river recharge.</p></list-item><list-item><label>c.</label>
      <p id="d1e1916">Combining cave drip logger data with surface geophysics data to track water movement.</p></list-item></list></p>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Conclusion</title>
      <p id="d1e1927">Cave drip water response to surface climatic conditions is often complex due
to numerous interacting drip routes with varying response times
(Baldini et al., 2006). This study explores the
relationship between drip water and rainfall in a SW Australian karst, where
both intra- and interannual hydrological variations are strongly controlled
by seasonal variations in recharge. The multi-year drip response data
capture the interannual drip water variability that are likely to be
greater than intra-annual variability as suggested by
Baker et al. (1997). Building on previous work, we
further analyze a set of statistical properties of three hydrological years
of drip data under varying precipitation rates. We test the relationship
between drip discharge variability and drip data<?pagebreak page987?> sampling frequency to
determine the optimum sampling frequency that maximizes the capture of
natural variability with minimum sampling artifacts. Using the daily optimum
sampling frequency, the histogram distributions of various drip data time
series illustrate the differences between the flow classifications. Most of
the drip sites show persistent autocorrelation for at least a month. The
hydrological behavior of the drips is examined with respect to mean
discharge and the flow types similar to the classification method proposed
by previous researchers (Smart and Friederich, 1987; Baldini et al.,
2006; Baker et al., 1997). The drip sites at Golgotha Cave described in this
study do not fit within the drip classification method proposed by
Smart and Friederich (1987) and Baker et al. (1997). These previous studies were based on manual drip counts with limited
number of intermittent drip sites. Here we overcome these limitations with
automated drip monitoring system.</p>
      <p id="d1e1930">Finally, we apply a well-developed clustering method to determine the degree
of similarity between drip time series. The clustering indicates one
dominating group, C1 (characterized by matrix flow type), with very slow
continuous drip discharge indicating matrix porosity in the thick limestone
formation. This finding concurs with the observed cave chamber morphology
and lithology. Moreover, the cluster analysis agrees with the flow
classification of Mahmud et al. (2016) by grouping similar
flow type in one single cluster. Overall this study establishes a novel way
to characterize cave hydrology, which can be obtained by applying the methodologies of Mahmud et al. (2015) and Jex
et al. (2012) together. It relies on a metric that defines drip logger time series as
similar if they are well correlated and only have a small offset with one
another, and therefore these time series should cluster together. The MDS
analysis supports this hypothesis and moreover displays the spatial
patterns of the flow paths between the surface and the cave chambers. This
technique shows potential for classifying, quantifying, and visualizing the observed
relationships between infiltration through the fractured limestone rocks and
surface climate inputs.</p>
      <p id="d1e1933">Over the last decade, the automation of cave drip water hydrology
measurements has permitted the routine generation of continuous hydrological
time series for the first time. This study demonstrates a complete
methodology for such data sets, which will help better characterize karst
drip water hydrogeology and understand the relationship between drip
hydrology and surface climate at any cave site where such measurements are
made. We demonstrate that the analysis of the time series produced by cave
drip loggers generates useful hydrogeological information that can be
applied generally, beyond the example presented here. The time series
behavior integrates a variety of characteristics that combine the
properties of epikarst (storage), fracture configuration, and recharge.
The clustering approach can identify which drip behaviors are related to
these cave characteristics, and their spatial relationship. Most
importantly, information on cave characteristics can now be gathered at a
very low cost in terms of measurement and time.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e1940">The raw data and the Matlab code to perform the data processing
and analysis are freely available in a Git repository (<uri>https://github.com/kashifmahmud/Golgotha-cave-drip-analysis</uri>).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e1946">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/hess-22-977-2018-supplement" xlink:title="pdf">https://doi.org/10.5194/hess-22-977-2018-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e1955">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e1961">This paper is based on work supported by UNSW Australia, UNSW Connected
Waters Initiative Research Centre, and the National Centre for Groundwater
Research and Training. The authors wish to thank the individuals (Andy Spate,
Alan Griffiths, Liz McGuire, Carolina Paice, Anne Wood, Monika Markowska, and
others) who assisted in data acquisition at the Golgotha Cave site. <?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: Alberto Guadagnini <?xmltex \hack{\newline}?>
Reviewed by: two anonymous referees</p></ack><ref-list>
    <title>References</title>

      <ref id="bib1.bib1"><label>1</label><mixed-citation>Arbel, Y., Greenbaum, N., Lange, J., and Inbar, M.: Infiltration processes and
flow rates in developed karst vadose zone using tracers in cave drips, Earth
Surf. Proc. Land., 35, 1682–1693, <ext-link xlink:href="https://doi.org/10.1002/esp.2010" ext-link-type="DOI">10.1002/esp.2010</ext-link>, 2010.</mixed-citation></ref>
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    <!--<article-title-html>Hydrological characterization of cave drip waters in a porous limestone: Golgotha Cave, Western Australia</article-title-html>
<abstract-html><p>Cave drip water response to surface meteorological conditions is
complex due to the heterogeneity of water movement in the karst unsaturated
zone. Previous studies have focused on the monitoring of fractured rock
limestones that have little or no primary porosity. In this study, we aim to
further understand infiltration water hydrology in the Tamala Limestone of
SW Australia, which is Quaternary aeolianite with primary porosity. We build on
our previous studies of the Golgotha Cave system and utilize the existing
spatial survey of 29 automated cave drip loggers and a lidar-based flow
classification scheme, conducted in the two main chambers of this cave. We
find that a daily sampling frequency at our cave site optimizes the capture
of drip variability with the least possible sampling artifacts. With the optimum
sampling frequency, most of the drip sites show persistent autocorrelation
for at least a month, typically much longer, indicating ample storage of
water feeding all stalactites investigated. Drip discharge histograms are
highly variable, showing sometimes multimodal distributions. Histogram
skewness is shown to relate to the wetter-than-average 2013 hydrological year
and modality is affected by seasonality. The hydrological classification
scheme with respect to mean discharge and the flow variation can distinguish
between groundwater flow types in limestones with primary porosity, and the
technique could be used to characterize different karst flow paths when
high-frequency automated drip logger data are available. We observe little
difference in the coefficient of variation (COV) between flow classification
types, probably reflecting the ample storage due to the dominance of primary
porosity at this cave site. Moreover, we do not find any relationship between
drip variability and discharge within similar flow type. Finally, a
combination of multidimensional scaling (MDS) and clustering by <i>k</i> means is
used to classify similar drip types based on time series analysis. This
clustering reveals four unique drip regimes which agree with previous flow
type classification for this site. It highlights a spatial homogeneity in
drip types in one cave chamber, and spatial heterogeneity in the other, which
is in agreement with our understanding of cave chamber morphology and lithology.</p></abstract-html>
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