This dataset contains audio files for Cumberland Plain Woodland SuperSite. was established in 2012 in a protected remnant of Shale Gravel Transition Forest, located on the Hawkesbury Campus of the University of Western Sydney in New South Wales. The vegetation at the site is dominated by Eucalyptus moluccana and E. fibrosa, which have hosted a population of mistletoe (Amyema miquelii); a subcanopy of Melaleuca decora is visible in some gaps. The ecosystem is subject to pressure from altered fire regimes, urban development, conversion to agriculture and extreme climate events. However, the forest patch at the site is in excellent condition with the exception of edge effects. For additional site information, see Cumberland Plain Woodland SuperSite
In 2019 four acoustic recorders were set up to collect audio data continuously as part of the Australian Acoustic Observatory (A2O) project. Two recorders were placed in relatively wet habitats and two in relatively dry habitats.
Credit
We at TERN acknowledge the Traditional Owners and Custodians throughout Australia, New Zealand and all nations. We honour their profound connections to land, water, biodiversity and culture and pay our respects to their Elders past, present and emerging.
The Cumberland Plain SuperSite is managed by the Hawkesbury Institute for the Environment, Western Sydney University.
Australian Acoustic Observatory: A Network to Monitor Biodiversity Project Team, with funding from the Australian Government through the Australian Research Council (LE170100033) (2018). Brisbane, QLD: QUT [www.acousticobservatory.org]
Purpose
Long-term acoustic recordings are collected to characterise the acoustic sources in the ecosystem. Recordings can be used to estimate biodiversity, monitor temporal changes in the soundscape, compare the acoustic characteristics of different locations, and assess the effect of particular events such as bushfires and floods.
Lineage
Four acoustic sensors are set up to collect audio data continuosly as part of the A2O project. Sensors are Frontier Labs Solar BAR. Each sensor has a Primo EM172 microphone with an 80Â dB signal-to-noise ratio, 14Â dBA self-noise, -28Â dB sensitivity, and a flat response (+2Â dB between 80Â Hz and 20Â kHz). Sensors have a gain of 50Â dB. They are mounted on 1.8Â m star pickets and powered by solar panels. Data are recorded continuously. Recordings are made as single channel, two-hour long flac files. They have a sampling rate of 22,050Â Hz and a depth of 16Â bits.
The four sensors are deployed in pairs. Each pair contains a wet and a dry sensor. Wet sensors are located within 50 m from the edge of a body of water. Dry sensors are located between 500 m and 5 km from their corresponding wet sensors. Wet–wet and dry–dry sensor points are at a distance between 500 m and 5 km.
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