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Airborne Gravity 2010 - Geoscience Australia

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<strong>Airborne</strong> <strong>Gravity</strong> <strong>2010</strong><br />

Figure 2. Different platforms successfully used for FTG data acquisition by Bell Geospace. (a)<br />

Marine acquisition aboard a ship, (b) Cessna Grand Caravan 208B, (c) Zeppelin NT Airship, and<br />

(d) Basler BT67.<br />

Bell Geospace now uses BT67 aircraft for airborne surveys (Figure 2). The BT67 is a reconditioned<br />

fixed wing DC-3 aircraft that employs turbo prop engines and a suite of modern avionics that make it<br />

ideally suited to airborne geophysical operations. An added benefit of having twin engines is that the<br />

instrument can remain permanently installed between jobs for easier worldwide mobilisation. The<br />

aircraft is larger than the Cessna Caravan and with its wider wingspan, is better suited for long<br />

duration survey work. Increased stability in the air reduces the impact of turbulence on resultant data<br />

and routinely yields final noise roof estimates of 5 to 6 Eo 2 km in final processed data, i.e., approaching<br />

that of airship quality. However, the BT67 flies at average speeds of 105 knots (55 m/s) and so, the<br />

final sampling rate, although better than that of the Cessna Caravan, is 55m. Nevertheless, the<br />

improved stability and lower noise over the Cessna Grand Caravan (Table 1) routinely yields a<br />

geological detectability of 2 to 3 Eo over 200 m wavelengths.<br />

Table 1 summarises the noise performance achieved over time with 3 airborne platforms used by Bell<br />

Geospace, demonstrating the continued improvement with FTG technology in terms of reducing noise<br />

and improving geological detectability on airborne surveys since 2004. The benefits of a low noise<br />

platform as exemplified by the airship and also with the BT67 aircraft are immense with increased<br />

sensitivity to sub-surface geology producing repeatable subtle signature patterns in the data. BT67<br />

fixed wing Air-FTG ® surveys permit geological features generating 2 to 3 Eo Tzz anomalies with<br />

wavelengths of 200 m to be detectable.<br />

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