Skip to content
SKYFLEX Get a Quote

Solar Array Thermal Inspection

Per-module anomaly detection. Findings keyed to inverter/string IDs for direct asset-platform ingest.

Inside the deliverable

Every hot module, keyed to its string.

A single flight scans the whole array radiometrically. Each anomaly is detected per-module and keyed to inverter and string IDs — ready to ingest straight into your asset platform.

Radiometric thermal inspection of a utility solar array Hot modulestring fault Per-module scanwhole array / flight Keyed to string IDplatform-ready
  • Hot modulestring fault
  • Per-module scanwhole array / flight
  • Keyed to string IDplatform-ready
How solar thermal inspection helps your business

Four steps from your problem to your win.

Your problem

Your solar array is underperforming: and ground-level inspection can't tell you which cells are the problem.

Hot spots, bypass diode failures, soiling, cracked cells, junction-box issues. Each one drags array output down.

What we capture

Our drone-mounted FLIR flies the array in a programmed grid.

Optimal capture window (high irradiance, clear sky). Sub-degree resolution. Every panel tagged.

The deliverable

A per-panel anomaly report: every hot spot, hot cell, PID-affected module mapped.

False-color thermal imagery. CSV defect list with panel IDs. Recommended repair / replace / clean per module.

How it pays off

Recover lost output. Justify warranty claims. Schedule O&M by data, not by guess.

One inspection often recovers 1-5% array output. Fast payback on residential, commercial, or utility-scale arrays.

A failing solar module rarely announces itself in the SCADA dashboard. The string still produces power; the array still hits its number; the underperforming panel just sits there, silently dragging yield down. A drone-mounted radiometric thermal camera finds those panels in hours instead of months: flying a planned grid over the array and surfacing every bypass-diode failure, cell crack, soiling pattern, hot junction, and string-level disconnect as a distinct thermal signature.

What an array inspection actually produces

  • Thermal orthomosaic of the array stitched into a single georeferenced map you can scroll, zoom, and click through.
  • Per-module anomaly list with GPS coordinates and array address (combiner / inverter / string / module) so your O&M crew knows exactly which panel to look at.
  • Classification by defect type and severity: bypass-diode failure, single-cell anomaly, multi-cell anomaly, junction-box heating, string disconnect, soiling pattern, shading.
  • Visible-light comparison imagery paired with every thermal frame: thermographer’s job gets easier when the same panel is shown in both spectra.
  • Summary report tied to your inverter and string IDs so the findings drop into your existing asset-management platform.

The conditions a valid thermal scan requires

Thermography only works when there’s enough sun loading the modules. Most O&M contracts cite an irradiance floor at or above 600 W/m²: below that, the temperature contrast between a healthy and a failing module is too low to reliably classify. We measure irradiance on site at the start of the flight, and we don’t fly through cloud-cover windows that drop the reading below threshold. If a weather window closes mid-flight, we stop and re-fly. The deliverable’s value depends on this discipline.

Hardware and standards

We fly radiometric thermal sensors at 640×512 resolution or higher with a paired visible-light camera for context. Higher sensor resolution pushes the small-defect detection limit further out: useful on utility-scale arrays where a single failing cell is the size of a fingernail at altitude. Reporting is structured to align with the IEC TS 62446-3 guideline that most O&M contracts reference for PV plant thermography: we confirm your contract’s specific version on the kickoff call so the deliverable matches what your asset team expects.

The questions buyers ask first

  • Irradiance and weather windows? ≥600 W/m² is the working floor. Clear or thin-overcast sky preferred. We schedule against your local solar window and re-fly if conditions drop mid-mission.
  • What classification scheme do you use? Standard categories: bypass-diode, single-cell, multi-cell, junction-box heating, string-level, soiling, shading. We map each to your contract’s defined categories during scoping.
  • How often should we re-inspect? Most O&M cadences run annually for utility-scale, with optional mid-year flights after lightning events or major weather. Smaller commercial/industrial arrays often go on a 12-24 month cycle.
  • Will the deliverable integrate with our asset-management platform? Inverter and string IDs are the join key: we name findings against your IDs so ingest is straightforward.
  • Who interprets the imagery? Anomaly identification is reviewed by a thermographer; severity and recommended-action calls map to your contract’s defined response thresholds.

Who buys solar thermal inspections

Solar EPCs (commissioning scans pre-acceptance), independent power producers and utility owners (annual yield-protection scans), O&M providers (routine and post-event inspections), and commercial/industrial solar asset owners with rooftop or carport arrays large enough that a manual IV-curve sweep isn’t cost-effective.

How it’s priced

  • Per-megawatt for utility-scale arrays: the dominant model
  • Per-acre for smaller arrays where AC capacity isn’t the cleanest unit
  • Mobilization fee for travel and any required after-hours / pre-dawn arrival
  • Fixed report fee covers the thermographer review, classification, and deliverable formatting
  • Portfolio programs covering multiple sites are quoted annually with a per-site rate that drops with portfolio size

Ready to start your mission?

Our FAA-certified pilots are ready to deploy. Get your free site assessment today.