Radiometric thermal overview of a 35-module rooftop solar PV array before cleaning

KAJH Aerial · Solar PV thermal inspection

Cleaning
Verification

35-module rooftop arrayInspect · Correct · Verify

Inspection overview

What looked like dirt
was also a thermal problem.

An initial RGB and radiometric thermal inspection found reportable abnormalities across nearly one-third of this 35-module solar PV array.

Eleven modules showed significant abnormal heating, including eight with widespread elevated temperatures. Several affected areas aligned with heavy surface soiling visible in the RGB imagery, demonstrating why visual inspection alone could not fully describe the operating condition.

System type
Roof-mounted solar PV
Array size
35 modules
Initial findings
11 affected modules
Follow-up
Post-cleaning reinspection

Initial inspection

The array was operating,
but not uniformly.

31.4%

of modules showed reportable thermal abnormalities

8

modules exhibited widespread abnormal heating

74.6°C

highest recorded temperature in the affected area

19.5°C

maximum reported temperature differential

Affected areas reached 74.6°C while comparable modules were operating around 53–55°C under the recorded inspection conditions.

Understanding the findings

What does a thermal
difference actually mean?

Thermal delta, written as ΔT, is the temperature difference between an anomalous area and a comparable unaffected cell or module operating under similar conditions.

It is not a comparison with the surrounding air. A ΔT of 19.5°C means the affected area was operating approximately 19.5°C hotter than the suitable reference area. The result becomes meaningful when interpreted alongside the thermal pattern, affected component, operating state and recorded inspection conditions.

Affected area74.6°C
Comparable modules53–55°C
Reported thermal delta19.5°C

IEC + ANSI/NETA

One framework evaluates the PV abnormality. The other guides response urgency.

IEC TS 62446-3:2017 defines the PV-specific infrared inspection method and a pattern-based matrix for thermal abnormalities. ANSI/NETA MTS Table 100.18 provides comparative temperature-rise bands and recommended maintenance actions for similar electrical components under similar loading. Used together, they support both technically sound interpretation and a clear response priority.

NETA 01Possible deficiency
ΔT 1–3°C

Investigate the condition and confirm that the comparison, loading and inspection conditions are valid.

NETA 02Probable deficiency
ΔT 4–15°C

Further assessment and corrective maintenance are indicated. Repair should be planned as operating conditions permit.

NETA 03Major discrepancy
ΔT > 15°C

Immediate repair is recommended. The specific response—cleaning, electrical testing, isolation or replacement assessment—depends on the observed condition.

IEC CoA classification

IEC CoA evaluates the complete PV abnormality using the observed pattern, affected component, extent and safety relevance. The NETA response band separately establishes maintenance priority from the comparative temperature rise.

CoA 1No abnormality

Operating condition considered acceptable. No imminent corrective action.

CoA 2Thermal abnormality

Investigate the cause and complete any necessary rectification within a reasonable period.

CoA 3Safety-relevant abnormality

Prompt interruption where appropriate, followed by investigation and rectification.

Thermal pattern

Point, cell, substring, module-wide or extended-area heating.

Affected component

Cell, module, bypass diode, junction box, connector or circuit path.

Normalized ΔT

Temperature difference evaluated in relation to 1,000 W/m² where required.

Extent

Number of affected cells or modules and distribution across the array.

Safety relevance

Evidence of damage, arcing risk, insulation loss or other hazardous conditions.

Inspection validity

Irradiance, wind, load, viewing angle, reflections and operating state.

Anomaly classification: CoA 2 / NETA 03

The module-wide abnormal heating pattern was classified as CoA 2, requiring investigation and corrective action. The maximum measured ΔT of 19.5°C placed the finding in NETA 03, establishing immediate priority for cleaning followed by thermal reinspection.

Image evidence

RGB context.
Thermal behaviour.

Each stage pairs standard visual imagery with thermal imagery so visible surface conditions can be compared with the heat pattern across the same array.

01

Initial array overview

Heavy surface contamination was visible across several modules. The thermal overview showed widespread non-uniform heating across the same area.

RGB aerial overview of the 35-module solar PV array before cleaning, showing heavy surface soiling
RGB · Before cleaning
Thermal aerial overview of the solar PV array before cleaning, showing non-uniform heating across several modules
Thermal · Before cleaning
02

Closer inspection

The closer paired view linked visible soiling with concentrated thermal abnormalities, including module areas recorded substantially hotter than comparable neighbouring modules.

Closer RGB aerial image showing heavy surface soiling across the affected solar modules
RGB · Affected modules
Closer thermal image showing widespread abnormal heating across the affected solar modules
Thermal · Reportable abnormalities
03

Post-cleaning verification

Following cleaning, the remaining surface stains were still visible, but the widespread abnormal heating seen during the initial inspection was no longer visually apparent. The reinspection showed a marked improvement in thermal uniformity.

RGB aerial overview of the solar PV array after cleaning, with residual surface staining still visible
RGB · After cleaning
Thermal aerial overview after cleaning showing improved temperature uniformity across the solar PV array
Thermal · Verification scan

Inspection outcome

Inspect.
Correct.
Verify.

01

Inspect beyond the visible surface

RGB imagery documented the condition of the modules while radiometric thermal imagery revealed how unevenly parts of the array were operating.

02

Direct the corrective response

The magnitude and distribution of abnormal heating, supported by the paired RGB evidence, made the maintenance priority clear and supported prompt cleaning and follow-up.

03

Verify the result

The follow-up thermal scan confirmed that the widespread heating pattern was no longer visually apparent after cleaning, providing evidence that the corrective action had materially improved array uniformity.

The inspection and reporting approach references IEC TS 62446-3:2017 for PV thermography and ANSI/NETA MTS Table 100.18 for comparative temperature-rise response guidance. IEC CoA identifies the observed PV thermal pattern and component significance, while the NETA comparative ΔT band guides response priority. Findings reflect the recorded inspection conditions, including weather, irradiance, operating state, viewing geometry and surface condition. Follow-up testing and thermal reinspection support confirmation of the corrective outcome.

KAJH Aerial · Barbados

Would you know if your
solar array was overheating?