Australian Government Department of Environment and Bureau of Meterology
Abstract
Speleothem growth relies on the supply of water which percolates from the surface,
through the unsaturated zone and discharges into cavernous voids. The flow path of
water feeding individual speleothems varies considerably depending on the karst
architecture e.g. micro-fractures, solution pipes, structural voids in the karst, storage
reservoirs, etc., all of which may alter the composition of drip waters over the flow
route. By monitoring drip waters, we can determine: 1) unsaturated zone flow
regimes; 2) connectivity between the surface and cave discharge zone; and 3)
thresholds for groundwater recharge. This information can be used to identify suitable
speleothems in caves for reconstruction of past climatic and hydrologic variability, at
least over the last few thousand years of similar mean climate state.
High-frequency, spatially-dense monitoring was conducted in Harrie Wood Cave,
Yarrangobilly, Snowy Mountains over a 15 month period to characterise the flow
regimes at 14 sites along a depth profile within the cave. Sites were monitored using
acoustic drip loggers (stalagmates®). Discharge rates and response to significant
rainfall events were highly variable between sites. A moderate relationship was found
between decreasing discharge rates and increasing depth (r2 = 0.40). We suggest
unsaturated zone storage and mixing, unrelated to depth, also have a significant
impact on flow regimes. Using a statistical approach, five different drip types, which
often had no spatial commonality, were identified. This information was used to
inform the choice of speleothems for paleo-climate reconstruction, using stalagmites
with differing hydrological regimes feeding growth, of which the preliminary data
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will be presented here. The study highlights the need to understand unsaturated zone
hydrology at the individual drip discharge level, prior to any speleothem study for
paleo-climate, to truly appreciate the drip water signal it is recording. Copyright (C) The Authors