Shotpoint: Seismic Source Stations, Vibroseis Versus Dynamite, and 3D Survey Geometry

A shotpoint is one of the surveyed surface locations at which a seismic energy source is activated during a reflection seismic survey. The name is a holdover from the era when the source was almost always a charge of dynamite lowered into a shallow drilled shot hole and detonated, but the term now covers any source station regardless of whether the energy comes from buried explosives, a vibroseis truck sweeping a controlled frequency band through a baseplate pressed to the ground, or an accelerated weight drop. Each shotpoint has a precise surveyed coordinate and elevation, a station number, and a planned source effort, and it is the spatial partner of the receiver station where geophones record the returning wavefield. When the source fires, elastic energy radiates downward, reflects off acoustic impedance contrasts at formation boundaries, and returns to the spread of receivers laid out along or around the line, so the shotpoint defines where energy entered the earth and the receiver stations define where it was measured. In a 2D program the shotpoints sit along a single line at a regular interval, often every second or third receiver station, giving a source spacing on the order of 55 to 165 m (180 to 540 ft), while in a modern 3D program the shotpoints populate a grid of source lines that cross the receiver lines, and the density of shotpoints per square kilometre directly controls the fold, the signal-to-noise ratio, and the imaging resolution of the final volume. In the Western Canadian Sedimentary Basin, shotpoint design is a major cost and permitting driver for exploration targeting the Montney, Duvernay, and deeper Devonian carbonates such as Leduc and Nisku, because dynamite shooting requires drilling thousands of shot holes 6 to 20 m (20 to 66 ft) deep, each needing surface access, landowner consent, and adherence to AER and provincial setback rules, whereas vibroseis avoids drilling but needs trafficable terrain and larger cut lines. The choice between explosive and vibroseis shotpoints is governed by terrain, environmental sensitivity, near-surface conditions, and the frequency content required to resolve thin reservoir intervals, and it feeds directly into survey economics, since a heli-portable dynamite program in muskeg or the foothills can cost several multiples of a vibroseis grid on open prairie. The surveyed shotpoint record, tied to receiver geometry, is what the processing centre uses to bin traces, compute fold, apply statics, and ultimately migrate reflections into a structurally correct subsurface image.

Key Takeaways

  • Surveyed source station: A shotpoint is a precisely located surface point, with coordinate, elevation, and station number, where the seismic source is fired. It pairs with receiver stations that hold the geophones, so the shotpoint marks where energy enters the earth and receivers mark where the reflected wavefield is recorded for imaging.
  • Dynamite or vibroseis: The classic source is dynamite in a 6 to 20 m (20 to 66 ft) shot hole, but most WCSB land programs now use vibroseis trucks sweeping a controlled frequency band, or weight drop. Vibroseis avoids thousands of drilled holes but needs trafficable ground; dynamite handles muskeg, foothills, and sensitive terrain that trucks cannot cross.
  • Geometry sets the fold: Shotpoint interval and grid density control subsurface fold and signal-to-noise. In 2D, sources sit every second or third station; in 3D, source lines cross receiver lines, and shotpoints per square kilometre govern the bin fold that determines whether thin Montney or Duvernay intervals are resolvable.
  • WCSB permitting cost: Dynamite shotpoints require shot-hole drilling, landowner consent, and AER-aligned setbacks from wellheads, pipelines, and dwellings. A foothills heli-portable dynamite grid can cost several times a prairie vibroseis survey, so shotpoint method is one of the largest single levers on total seismic program budget.
  • Processing anchor: Every recorded trace is tagged with its shotpoint and receiver coordinates. Processors use that geometry to bin traces into common midpoint gathers, compute refraction and elevation statics, and migrate reflections, so a survey error at the shotpoint propagates into mispositioned structure on the final seismic section.

Source Effort and Near-Surface Statics

Shotpoint design must account for the low-velocity weathered layer near surface, which delays and distorts arrivals and must be removed through statics. Dynamite shotpoints are drilled below the weathered zone where possible so energy couples into competent rock, improving high-frequency content needed to resolve a 15 to 30 m (49 to 98 ft) Montney bench. Vibroseis compensates with multiple sweeps stacked at each shotpoint and longer sweep lengths to build signal. On a Duvernay shale program near Fox Creek, a designer might specify 2 kg charges at 15 m depth on a 200 m source-line spacing, or four 12-second vibroseis sweeps per shotpoint, and the near-surface model derived from uphole surveys and first breaks sets the datum statics that align every shotpoint gather.

3D Bin Fold and Shotpoint Density

In 3D acquisition the number and spacing of shotpoints, combined with receiver-line spacing, determine the nominal fold in each subsurface bin, typically a 25 m by 25 m (82 ft by 82 ft) cell. Higher shotpoint density raises fold, suppresses random noise, and sharpens the image of faults and stratigraphic pinchouts, but it also multiplies shot-hole drilling or vibroseis pass count and therefore cost. A Montney operator near Dawson Creek might target 30 to 60 fold to resolve subtle channel geometry, balancing shotpoint density against a program budget that can run CAD 15,000 to 40,000 per square kilometre depending on source method, terrain, and access constraints across BC-ER and AER jurisdictional boundaries.

Fast Facts

Vibroseis was developed by Conoco in the 1950s specifically to replace dynamite, and its correlated sweep signal lets crews inject a long, low-energy vibration that is mathematically compressed into a sharp pulse during processing, delivering comparable resolution without a single drilled shot hole. On a large WCSB 3D survey the difference is stark: an explosive program may require tens of thousands of individually drilled and loaded shotpoints, while a vibroseis fleet can occupy and sweep the same source grid faster, cheaper, and with far smaller surface disturbance on accessible terrain.

A shotpoint only has meaning alongside the receivers and the processing chain it feeds. The geophone is the surface sensor that records the energy each shotpoint releases, and their combined geometry defines the common midpoint fold. Seismic survey is the full acquisition program that lays out both source and receiver stations, while the migrated seismic section is the interpreted product, and vibroseis is the non-explosive source that now occupies most WCSB shotpoints on trafficable ground.

Real-World WCSB Scenario: Duvernay 3D Near Fox Creek

An operator planning horizontal Duvernay development near Fox Creek commissions a 90 km2 3D survey to map fault compartments before landing laterals. The near-surface is glacial till over the Fox Creek shale, so the crew mixes vibroseis on cleared cut lines with 2 kg dynamite shotpoints in a wooded quarter section where trucks cannot pass, drilling roughly 1,400 shot holes at 15 m depth. Total acquisition runs near CAD 2.4 million, with shot-hole drilling and permitting the single largest line item.

The resulting 30 to 45 fold volume resolves two previously unmapped normal faults that would have cut a planned 3,000 m lateral. Repositioning the well pad on the seismic geometry avoided an estimated CAD 8 to 12 million in a compromised well and lost stages, a return that dwarfed the shotpoint program cost.