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FIG.03 SERVICE / SOLAR INSPECTION

Thermal solar inspection,
panel by panel.

Visual sweeps miss what counts. Aerial thermal imaging picks out hotspots, bypass diode failures, cracked cells, and bad interconnects across every panel in the array — and gives you an output-loss estimate so you know which faults are worth fixing first.

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Typical range $400–$2,500
On-site time 30–90 min
Coverage rate ~1 MW / hr
Array downtime None required
// 01 — USE CASES

When to fly the array.

Six situations where thermal aerial inspection pays for itself in months.

01

Underperforming system

Production is down and you can't pin it on weather. Thermal flight isolates the faulty modules so the O&M crew knows exactly which panels to replace.

02

Annual O&M

Yearly preventative inspection. Catch early-stage hotspots and bypass diode failures before they cascade into module replacement.

03

Pre-warranty claim

Document failing modules with thermal evidence before the manufacturer warranty expires. Geotagged imagery supports the claim.

04

Commercial acquisition

Due-diligence inspection before buying a commercial property with an installed array. Verify actual condition versus seller representations.

05

Post-storm assessment

Hail, debris, or extreme heat events can cause invisible micro-cracking. Thermal flight reveals damage that won't show up on visual inspection for months.

06

Utility scale O&M

Cover 50–100 acres in a single morning. Per-panel data delivered as a GIS-ready layer for asset management systems.

// 02 — DELIVERABLE

What you get back.

CORE

Per-panel thermal map

Radiometric thermal mosaic of the entire array, panel-indexed with row and column coordinates.

CORE

Fault flagging

Each anomaly classified by signature: hotspot, bypass diode failure, cracked cell, string fault, soiling, or shading.

CORE

Output-loss estimate

Directional figure for total estimated production loss across detected faults. Useful for prioritizing remediation spend.

ADD-ON

RGB visual overlay

High-resolution visual mosaic paired with the thermal map for context — useful for soiling and physical damage documentation.

ADD-ON

GIS-ready dataset

Geotagged shapefile or GeoJSON of all detected faults for direct import into asset management systems.

ADD-ON

Detailed engineering report

Extended narrative with per-fault classification, severity grading, and replacement priority ranking.

// 03 — FAQ

Solar inspection FAQ.

What can thermal solar inspection detect that visual cannot?

Thermal imaging reveals heat signatures from electrical faults invisible to visual inspection: bypass diode failures, cracked cells, hotspot defects, broken interconnects, junction box faults, and shaded or soiled regions causing localized resistance.

Each fault has a distinctive thermal pattern, so the cause can be identified — not just the symptom.

When is the best time to fly a solar inspection?

Mid-day on a clear, sunny day with the array operating under at least 600 W/m² of irradiance. We schedule flights for the highest-irradiance window available and verify with on-site sensors before capture.

Cloudy days are reschedulable at no cost.

Do you need to take the array offline?

No. The array must be operating under load for thermal anomalies to develop, so the inspection happens while the system is generating. No service interruption, no inverter shutdown.

How accurate is the output-loss estimate?

The output-loss estimate is derived from the area and severity of detected anomalies referenced against panel datasheet output curves. It's a useful directional figure for prioritizing remediation, not a guaranteed performance prediction.

For utility-scale arrays, we can pair the thermal data with IV-curve testing for higher fidelity.

// 04 — RELATED

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