Echolith Labs is in final calibration. Automated magnetometry and GPR processing opens for customer uploads in Q4 2026 — leave an address and be first in the queue.
Upload magnetometry or ground-penetrating radar data. Our pipeline destripes, grids, and detects anomalies automatically — you review a preview before paying a cent.
Your survey is processed in full, first. The preview unmasks roughly 25% of the map at full detail — anomaly positions included — so you can verify the results against ground truth. Payment unlocks the remaining 75%.
Total-field and gradiometer surveys. Automatic destriping, despiking, heading correction, and grid interpolation. Dipolar and thermoremanent anomaly classification with confidence scoring.
Single and multi-channel GPR. Time-zero correction, background removal, migration, and hyperbola fitting. Depth-sliced amplitude maps with reflector picking down to 4 m.
Every survey is processed in full before payment. You see a locked preview — anomaly counts, coverage QC, a masked heatmap — and pay only to unlock. A small base fee keeps small surveys viable; the per-hectare rate scales with data intensity, not a flat rate.
Processing starts the moment your upload completes. No account required to preview.
Add one or both datasets. Processing is fully automatic and free until you unlock results.
You can close this page — we'll email you when the preview is ready.
Processing complete. A quarter of the survey is fully unmasked — anomaly positions included — so you can verify the output. Payment unlocks the remaining 75%, depths, and the report.
One-time payment for survey {{ surveyId }}. Results and report are delivered immediately.
{{ anomalyCount }} anomalies across {{ hectares }} ha. Report and rasters available for download for 90 days.
Survey area shows a coherent cluster of thermoremanent anomalies (A-03…A-05) consistent with in-situ burning — probable kiln or hearth group. Linear positive anomaly A-07 traces 46 m NE–SW, consistent with a backfilled ditch. GPR depth slices confirm reflectors at 0.6–1.1 m over the mag cluster.