The starting question for any magnetic survey technology evaluation is whether the sensor noise floor is below the anomaly amplitude you expect to detect at the depth and contrast of your target. For hard-rock mineral exploration in Archaean terrains, the answer to this question depends on the target type (sulphide, magnetite, iron formation), the depth, and the lateral dimension of the target. Before evaluating whether quantum sensing is relevant to a specific survey program, it is worth building out what the expected anomaly amplitudes actually are. This is often skipped in technology discussions that focus on sensor specifications without grounding them in the geophysical forward problem.
Magnetic susceptibility and the source of gradient anomalies
Most hard-rock magnetic survey targets gain contrast from elevated magnetic susceptibility relative to the host rock. Magnetite-bearing iron formation, BIF-hosted gold deposits, sulphide-associated alteration assemblages with magnetite, and komatiite-hosted nickel sulphides all produce susceptibility contrasts that generate measurable magnetic anomalies. The magnitude of the surface anomaly for a given target depends on three parameters: the susceptibility contrast, the depth from surface to the top of the target, and the lateral and vertical dimensions of the target body.
For a sphere approximation, the peak magnetic field anomaly scales with susceptibility contrast times volume divided by distance cubed. The field gradient scales with the same numerator divided by distance to the fourth power. As depth increases, gradient anomalies attenuate faster than total field anomalies, which makes gradient measurements less useful for very deep targets but more diagnostic (sharper lateral definition) for shallow targets.
Representative susceptibility contrasts for economic target types in Archaean hard rock: sulphide-altered BIF gold deposits typically have susceptibility contrasts of 0.05 to 0.5 SI relative to barren greenstone; massive sulphide bodies may be paramagnetic (low contrast) or may contain magnetite alteration halos with contrast of 0.01 to 0.1 SI; komatiite-hosted nickel sulphides often occur in low-susceptibility ultramafic hosts and may rely on pyrrhotite remanence rather than susceptibility contrast.
Gradient anomaly amplitudes at exploration depths
Using published forward models for tabular bodies (appropriate for steeply dipping mineralised shear zones), the expected peak gradient anomaly at surface for representative target geometries:
A BIF gold target with susceptibility contrast 0.1 SI, 5-metre-thick tabular geometry at 100 metres depth, dipping steeply: peak gradient anomaly approximately 2 to 5 nT/m at 10-metre line spacing. This is well above the noise floor of fluxgate gradiometers (typically 1 to 2 nT/m baseline noise in field conditions) and comfortably above NV-center gradiometer noise (0.3 to 0.5 nT/m in field conditions).
The same target geometry at 200 metres depth: peak gradient anomaly approximately 0.3 to 0.8 nT/m. This falls below the fluxgate noise floor but remains above NV-center field sensitivity. The improvement in detection capability is real for this target class at these depths.
A low-contrast massive sulphide body with susceptibility contrast 0.01 SI, 20-metre extent at 150 metres depth: peak gradient anomaly approximately 0.05 to 0.15 nT/m. This is below the noise floor of current NV-center sensors in field conditions and would require either a stronger contrast unit, a shallower target, or substantially improved sensor sensitivity to detect.
What the gradient versus total-field choice means
Magnetic gradiometry (measuring the spatial gradient of the field using two sensors separated by a fixed baseline) is preferred over single-sensor total-field measurement for detailed close-range surveys because it suppresses slowly varying regional and diurnal field variations, reducing the amplitude of long-wavelength noise that would otherwise mask small anomalies. For an NV-center instrument operating with a 0.5-metre sensor baseline, the gradiometric configuration effectively removes most ambient field drift and regional field variation, leaving the geological gradient as the dominant signal.
The trade-off is that gradient anomalies have smaller amplitude and sharper lateral extent than total-field anomalies, which means they require higher sensitivity to detect at a given target depth but provide better horizontal resolution. For the follow-up detailed survey application where we operate, this trade-off favours gradiometry: the exploration team has already identified a target from total-field data and wants to resolve the geometry at the drill-target scale.
Translating sensitivity to drilling decision quality
The practical value of improved gradient sensitivity is not simply detecting more anomalies. It is resolving the lateral extent and strike direction of known anomalies with enough accuracy to reduce the number of infill drill holes needed to confirm the target geometry before committing to an expensive hole. An anomaly resolved to 5-metre lateral accuracy at the surface allows drill hole collars to be sited within the projected target footprint with higher confidence than one resolved to 20-metre accuracy from lower-sensitivity data.
For a 200-metre depth target where one deep hole costs roughly 100,000 to 200,000 Australian dollars in the terrains we survey, reducing the uncertainty in collar siting by one hole is a concrete economic outcome. We are not claiming the sensor directly changes the geological probability of mineralisation, but it changes the probability that a given drill hole intersects the mapped target.
We should be direct about what this framework does not cover: remanent magnetism, self-demagnetisation in high-susceptibility bodies, structural complications in steeply plunging mineralisation, and the spatial aliasing from 10-metre survey grids all add uncertainty that instrument sensitivity alone cannot resolve. The measurement improvement has real value within its scope but does not replace geological interpretation.
The DeteQt team can model expected anomaly amplitudes for your specific target geology and depth to help assess whether the current sensor specification changes your detection envelope.
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