A hotspot occurs when a localised area of a solar panel becomes significantly hotter than its surroundings. Under normal operation, all cells in a panel generate electricity and emit heat relatively uniformly. When one or more cells cannot generate power due to shading, damage, or defects, they stop contributing to the electrical output but continue receiving current from the other cells. Instead of generating electricity, the affected cell becomes a resistor and dissipates this energy as heat. Research shows that hotspot temperatures can reach 130 to 200°C, compared to normal operating temperatures of 50 to 70°C, with severe cases causing temperatures to rise from 25°C to over 100°C above normal.

The consequences extend beyond simple energy loss. Prolonged hotspot heating causes permanent damage including cell burning, solder joint melting, encapsulant discolouration, and accelerated material degradation. In extreme cases, hotspots create fire risks, particularly in dry conditions or where panels are installed close to flammable materials. A complete hotspot string within a panel can cause a 25% loss in output power while simultaneously shortening the panel’s lifespan. Modern panels include bypass diodes to mitigate these effects by redirecting current around problem areas, but understanding what causes hotspots and how to prevent them remains essential for maintaining a safe, efficient system.

This guide explains the physics behind hotspot formation, the various causes, how bypass diodes provide protection, detection methods including thermal imaging, and practical steps to prevent hotspots from damaging your solar installation.

Quick Overview

What is a hotspotLocalised overheating where a cell dissipates energy as heat instead of electricity
Normal operating temperature50 to 70°C
Hotspot temperature range130 to 200°C in severe cases
Main causesShading, dirt/debris, cell defects, cracks, bypass diode failure
Power loss from hotspot stringUp to 25% of panel output
Protection mechanismBypass diodes redirect current around affected cells
Detection methodThermal imaging (infrared cameras)

How Hotspots Form

The Physics of Hotspot Formation

Solar panels consist of individual cells connected in series within strings. In a series circuit, the same current must flow through every cell. Each cell generates a small voltage, and these voltages add together to produce the panel’s total output. When all cells receive equal sunlight and function normally, current flows smoothly and the panel operates efficiently.

Problems arise when one cell cannot match the current output of the others. If a cell is shaded, damaged, or defective, it generates less current than its neighbours. However, the series connection forces the same current through all cells. The underperforming cell cannot generate this current, so instead of acting as a power source, it becomes a load. The current from the functioning cells pushes through the weak cell, which now acts as a resistor. Energy that would normally become electricity is instead converted to heat, concentrated in that single cell.

ConditionCell BehaviourResult
Normal operationCell generates current; forward biasedElectricity production; normal temperature
Cell shaded/defectiveCell cannot generate matching current; reverse biasedEnergy dissipated as heat; hotspot forms
Severe mismatchCell consumes power from other cellsExtreme localised heating

Temperature Impact

ScenarioTypical Temperature
Normal panel operation50 to 70°C
Minor hotspot15 to 30°C above surrounding cells
Moderate hotspot80 to 130°C
Severe hotspot130 to 150°C
Extreme hotspot (10% shading with bypass diodes)Up to 200°C
Encapsulant failure threshold~150°C

Causes of Hotspots

External Causes

External causes are almost all preventable through routine care. For practical how-to, see our solar panel cleaning guide and solar panel bird proofing guide.

CauseDescriptionImpact
Partial shadingTrees, buildings, chimneys, poles casting shadowsShaded cells become resistive loads; primary cause of hotspots
Bird droppingsConcentrated deposits blocking individual cellsCommon in coastal and industrial areas; localised heating
Dirt and dustAccumulated soiling reducing light to specific cellsCan cause up to 50% efficiency loss; uneven heating
Leaves and debrisFallen leaves, twigs blocking cellsSeasonal issue; particularly autumn
Snow coveragePartial snow cover leaving some cells shadedWinter issue; melting patterns can create partial shading
Vegetation growthPlants growing in front of or between panelsProgressive shading; ground-mounted systems particularly affected

Internal and Manufacturing Causes

Microcracks are one of the most significant internal causes, often developing invisibly from transport, installation or thermal stress. Our guide to solar panel microcracks covers how they form and how they turn into hotspots over time.

CauseDescriptionImpact
Cell cracksMicrocracks from handling, thermal stress, or hailCracked areas have higher resistance; heat accumulation
Cell defectsManufacturing imperfections; low shunt resistance cellsDefective cells underperform and heat up
Poor solder jointsManufacturing defect in cell connectionsHigh resistance at joint creates localised heating
Cell mismatchCells with different current outputs in same stringWeakest cell limits string; becomes hotspot under load
Internal connection failureBroken ribbons or interconnectsCurrent cannot flow normally; localised heating
Encapsulant degradationYellowing or delamination affecting light transmissionUneven light reaching cells; localised underperformance

Bypass Diode Related Causes

CauseDescriptionImpact
Failed bypass diode (open circuit)Diode cannot conduct; no protection for stringShaded cells no longer protected; severe hotspots can develop quickly
Failed bypass diode (short circuit)Diode always conducts; string bypassed permanentlyOne third of panel output lost; no hotspot but reduced power
Insufficient diodesOlder panels with fewer diodes per cell groupLarger cell groups affected when shading occurs

Environmental and Age Related Causes

CauseDescriptionImpact
Uneven cell agingSome cells degrade faster due to inconsistent exposureMismatched performance within panel over time
Thermal cyclingRepeated heating and cooling causes stressCan create or worsen cracks; solder fatigue
UV degradationLong-term UV exposure degrades materialsUneven degradation across panel surface
Weather damageHail, storms causing physical damageCreates cracks and defects that become hotspots

Research Findings on Shading and Hotspots

Peer-reviewed research at UK universities has documented hotspot behaviour in detail. Dhimish et al. (2018), published in Solar Energy Materials and Solar Cells, demonstrated hotspot detection and mitigation on a real UK installation, showing how active protection schemes can recover output power lost to hotspot conditions. Research of this kind informs the practical thresholds quoted in industry guidance.

FindingDetails
Worst-case shading ratio40% to 60% shading creates most severe hotspots
Complete shadingMay not create hotspot if bypass diode activates properly
Temperature rise from cracksCells with shaded area defects can reach 25°C to 100°C above normal
Point defects vs area defectsConcentrated point defects create 30°C higher temperatures than spread defects
US field study22% of 115 defective modules failed due to cell hotspots

How Bypass Diodes Work

Basic Function

Bypass diodes are protective components installed in parallel with groups of solar cells, but with opposite polarity. Under normal operation, when all cells generate power, each cell is forward biased. The bypass diode sees the combined forward voltage of its cell group and remains reverse biased, effectively acting as an open circuit. Current flows through the cells normally, generating electricity.

When shading or a defect causes one cell to underperform, that cell becomes reverse biased and its voltage drops. If the voltage drop is sufficient, the bypass diode becomes forward biased and starts conducting. Current from the functioning cells can now flow through the diode instead of being forced through the problematic cell. This limits the reverse voltage across the affected cell to approximately 0.6V (the diode’s forward voltage drop), preventing severe overheating.

ConditionBypass Diode StateEffect
All cells functioningReverse biased (off)No effect; current flows through cells
Cell shaded/defectiveForward biased (on)Current bypasses affected string; hotspot prevented
Diode failed (open)Cannot conductNo protection; hotspot can form
Diode failed (short)Always conductsString permanently bypassed; power loss

Typical Diode Configuration

Panel architecture determines how much area is affected when a diode activates – see our solar panel components guide for how junction boxes, cells and diodes fit together.

Panel TypeTypical CellsBypass DiodesCells per Diode
36-cell panel36218 cells per diode
60-cell panel60320 cells per diode
72-cell panel72324 cells per diode
120 half-cell panel12036 substrings of 20 cells
144 half-cell panel14436 substrings of 24 cells

Limitations of Bypass Diodes

LimitationExplanation
Reactive not preventiveDiodes activate after problem develops; do not prevent initial heating
Power loss when activeBypassed string produces no power; typically one-third of panel lost
Current not limitedStandard diodes limit voltage but not current; some heating still occurs
Group protection onlyOne diode protects 15-24 cells; minor shading can disable many cells
Can failDiodes can fail from age, lightning, or thermal stress
Not practical per-cellToo expensive to fit one diode per cell

Maximum Safe Cells per Diode

SpecificationValue
Maximum recommended15 to 20 cells per bypass diode for silicon cells
Higher-power modulesSome use 24 cells per diode; increases hotspot risk
Research findingIncreasing from 20 to 24 cells per diode raised hotspot temperature from 150°C to 170°C

Impact of Hotspots

Performance Impact

EffectDetails
Reduced cell outputAffected cell produces less or no electricity
String performance lossEntire string limited by weakest cell (series connection)
Bypassed string lossWhen diode activates, typically one-third of panel output lost
Complete hotspot stringCan cause 25% loss in total panel output
System-wide impactWith string inverter, one affected panel can reduce entire string performance

Physical Damage

Damage TypeTemperature ThresholdConsequence
Encapsulant discolouration~100°C sustainedYellowing; reduced light transmission
Encapsulant failure~150°CDelamination; moisture ingress; accelerated degradation
Solder joint melting~180°CConnection failure; permanent damage
Cell burning>150°C sustainedVisible burn marks; cell destruction
Backsheet damageVariableCracking; potential safety hazard

Safety Risks

RiskDetails
Fire hazardExtreme hotspots can ignite nearby flammable materials
Higher risk conditionsDry climates; overhanging vegetation; roof-integrated panels
Arc fault potentialDamaged connections can create electrical arcing
Reduced fire protectionFailed bypass diodes remove primary protection mechanism

Long-Term Consequences

The accelerated degradation caused by sustained hotspots directly shortens panel lifespan – see our solar panel lifecycle analysis guide for how degradation typically progresses and how hotspot damage compares with normal wear.

ConsequenceImpact
Accelerated degradationRepeated thermal stress speeds material breakdown
Shortened lifespanHotspot damage reduces years of productive operation
Warranty implicationsDamage from neglected maintenance may void warranty
Cascading damageInitial hotspot can damage adjacent cells and components
Replacement costSevere hotspot damage typically requires panel replacement

Detection Methods

Thermal Imaging

Thermal imaging using infrared cameras is the most effective method for detecting hotspots. Under normal conditions, solar panels emit heat relatively uniformly across their surface. Hotspots appear as bright areas in thermal images, with modern cameras able to detect temperature differences as small as 0.05°C. Professional-grade thermal cameras with 160 × 120 resolution or higher can identify even developing hotspots before they cause significant damage. Our solar panel fault finding guide covers how thermal imaging fits alongside IV curve tracing and electroluminescence imaging for full diagnostic workflow.

Detection MethodDetailsBest Use
Handheld thermal cameraOperator points camera at panels from ground or roofResidential systems; accessible panels
Drone-mounted cameraUAV flies over array capturing thermal imagesLarge arrays; commercial/utility scale
Fixed thermal monitoringPermanently installed cameras for continuous monitoringHigh-value installations; research

Thermal Anomaly Patterns

PatternAppearanceLikely Cause
Single hotspotOne cell significantly hotter than surroundingsLocalised shading; cell defect; bird dropping
Multiple hotspotsSeveral individual hot cellsMultiple defects; scattered debris
Bypassed substringOne-third of panel uniformly warmerBypass diode activated; shading on that string
Double bypassed substringTwo-thirds of panel warmerTwo strings affected
Checkerboard patternIrregular hot and cool areas within substringDiode issue; multiple cell defects
Entire panel hotWhole panel warmer than neighboursString disconnection; all diodes bypassed

When to Conduct Thermal Inspection

TimingReason
Full sunlight conditionsPanels must be generating power to show temperature differences
Irradiance above 700 W/m²Sufficient power generation to reveal defects
Morning or afternoonAvoid midday when ambient temperature differences are highest
Low wind conditionsWind can mask temperature differences through cooling
After installationBaseline inspection to identify manufacturing defects
Annually thereafterRegular monitoring catches developing issues
After severe weatherCheck for hail damage or debris accumulation

Other Detection Methods

MethodWhat It DetectsLimitations
Visual inspectionVisible damage; discolouration; burn marksCannot detect early-stage or hidden hotspots
Performance monitoringUnexpected power drops may indicate hotspotCannot pinpoint location; many causes of power loss
I-V curve tracingStepped curve indicates bypassed stringsRequires specialist equipment; identifies problem but not location
Electroluminescence imagingCracks and defects visible under currentRequires darkness; specialist equipment; mainly for manufacturing

AI and Automated Detection

TechnologyCapability
AI thermal analysisProcesses drone images automatically; identifies anomaly types
Machine learning modelsCan detect hotspots with up to 99.98% accuracy
Automated classificationDistinguishes hotspots from normal temperature variation
Large-scale processingCan analyse thousands of panels quickly

Prevention

Design and Installation

The most robust hotspot prevention is baked in at design stage. Module-level power electronics – microinverters or DC optimisers – isolate each panel’s performance from the rest of the string. See our microinverters for residential solar guide for how this architecture changes what a single shaded or faulty panel does to total system output.

MeasureHow It Helps
Site assessmentIdentify shading sources before installation; position array to avoid
Proper orientation and tiltMaximise uniform sunlight exposure; reduce shading risk
Quality panelsBetter manufacturing quality control; fewer cell defects
Matched cell binningQuality manufacturers sort cells by output to minimise mismatch
Adequate bypass diodesPanels with more diodes provide better protection
Half-cell technologySmaller cells mean smaller affected area when shading occurs
Module-level power electronicsMicroinverters or optimisers isolate panel problems from system

Panel Technology Considerations

TechnologyHotspot ResistanceNotes
Standard full-cellModerateTraditional design; relies on bypass diodes
Half-cellBetterSmaller cells; more substrings; less affected by partial shading
IBC (Interdigitated Back Contact)BestBetter current distribution; more resistant to localised heating
Shingled cellsBetterOverlapping design improves shade tolerance

Ongoing Maintenance

ActionFrequencyPurpose
Visual inspectionEvery 6 monthsCheck for visible debris, damage, shading changes
Panel cleaning1-2 times per year (UK)Remove dirt, bird droppings, debris that cause shading
Vegetation managementAs neededTrim trees; clear plants that may shade panels
Thermal inspectionAnnually recommendedDetect hotspots before they cause damage
Performance monitoringContinuousUnexplained drops may indicate developing hotspots
Gutter clearingAnnuallyPrevent debris accumulation near panels

Addressing Specific Causes

CausePrevention/Solution
Tree shadingTrim trees; consider removal; relocate panels if necessary
Bird droppingsRegular cleaning; bird proofing to reduce bird activity
Dirt accumulationScheduled cleaning; self-cleaning coatings on glass
Fallen leavesClear promptly; consider leaf guards if persistent
SnowAllow to melt naturally; clear if safe to do so
New shading sourcesMonitor for new construction, growing trees

What to Do If You Have Hotspots

Assessment Steps

StepAction
1. Identify causeCheck for visible shading, debris, damage
2. Remove external causeClean panel; remove obstruction; trim vegetation
3. Re-inspectIf thermal inspection available, check if hotspot remains
4. Monitor performanceCheck if output improves after cleaning/obstruction removal
5. Professional assessmentIf hotspot persists, have system inspected by professional

When to Replace Panels

If a panel is beyond repair, check your warranty position first – our guide to solar panel warranty claims covers what manufacturers cover for defect-related hotspot damage.

SituationRecommendation
External cause removed, hotspot goneNo replacement needed; monitor going forward
Visible burn damagePanel should be replaced
Failed bypass diodeMay be repairable; often more practical to replace
Internal cell defectCannot be repaired; replacement needed
Significant performance lossCalculate if replacement is cost-effective

Replacement Considerations

FactorConsideration
Matching specificationsReplacement must match voltage and current of existing panels
AvailabilityOlder panels may be difficult to match; secondary market may help
WarrantyCheck if defect is covered under panel warranty
String compatibilityMismatched replacement can create new problems
Professional installationEnsure replacement installed correctly; connections tested

Thermal Inspection Services

Professional Inspection Options

Service TypeTypical CostBest For
Residential thermal survey£100 to £200Domestic systems; suspected problems
Drone survey (commercial)£200 to £500+Larger arrays; comprehensive inspection
Part of O&M contractIncludedCommercial systems with ongoing maintenance

DIY Thermal Inspection

OptionCostNotes
Smartphone thermal attachment£150 to £400FLIR One, Seek Thermal; basic detection capability
Entry-level thermal camera£300 to £600Better resolution; more accurate readings
Professional thermal camera£1,000+High resolution; detailed analysis capability

Frequently Asked Questions

Basic Questions

QuestionAnswer
What is a hotspot?Localised area where a cell overheats because it cannot generate matching current
How hot can hotspots get?130 to 200°C in severe cases; normal operation is 50 to 70°C
Can hotspots cause fires?Yes, in extreme cases; particularly in dry conditions
How common are hotspots?Very common; 22% of panel failures in one study were hotspot-related

Cause and Effect Questions

QuestionAnswer
Does partial shading always cause hotspots?Not always; bypass diodes can protect; but some heating typically occurs
Can bird droppings cause hotspots?Yes; concentrated droppings blocking cells are a common cause
Do bypass diodes prevent all hotspots?No; they limit damage but are reactive; some heating occurs before activation

Detection and Repair Questions

QuestionAnswer
Can I see hotspots visually?Only if severe damage has occurred (burn marks); thermal imaging needed for early detection
Can hotspots be repaired?If caused by external factors (dirt, shading), yes; internal defects usually require replacement
How often should I check for hotspots?Annual thermal inspection recommended; visual checks every 6 months

Summary

AspectKey Point
DefinitionLocalised overheating where cell becomes resistive load instead of power source
Temperature range130 to 200°C vs normal 50 to 70°C
Main causesPartial shading, dirt/debris, cell defects, cracks, bypass diode failure
ProtectionBypass diodes redirect current around affected cells
DetectionThermal imaging is most effective method
PreventionRegular cleaning, vegetation management, quality panels, annual inspection
ConsequencesPower loss, physical damage, fire risk, shortened lifespan

Hotspots represent one of the most significant reliability issues for solar panels, with research showing they account for over 20% of panel failures in some studies. The fundamental problem is electrical: when a cell cannot match the current output of its neighbours, it becomes a resistive load and converts incoming energy to heat rather than electricity. Temperatures can reach 130 to 200°C, far exceeding the 150°C threshold where encapsulant materials begin to fail. This causes permanent damage including cell burning, solder joint melting, and accelerated degradation that shortens the panel’s productive lifespan.

Bypass diodes provide essential protection by redirecting current around problem cells when voltage drops indicate an issue. However, they are reactive rather than preventive, activating only after heating has begun. When a diode activates, the entire substring it protects stops generating power, typically meaning one-third of panel output is lost. If bypass diodes fail, the protection disappears entirely, and severe hotspots can develop rapidly. Understanding this protection mechanism helps explain why panel quality, with adequate diodes and well-matched cells, matters for long-term reliability.

Prevention focuses on two areas: avoiding external causes and monitoring for internal problems. Regular cleaning removes bird droppings, dirt, and debris that shade individual cells. Vegetation management prevents growing trees from creating new shading. Quality panels from reputable manufacturers have better cell matching and more robust bypass diode systems. Half-cell and IBC panel technologies offer improved resistance to partial shading effects. Annual thermal inspection using infrared cameras detects developing hotspots before they cause significant damage, allowing intervention while the problem is still manageable.

For homeowners with solar panels, the practical takeaway is that regular maintenance and monitoring protect your investment. Keep panels clean, watch for new shading sources, and consider periodic thermal inspection, particularly for systems more than a few years old. If unexplained performance drops occur, hotspots should be investigated as a possible cause. Addressing external causes like dirt or shading promptly can prevent temporary hotspots from becoming permanent damage.

For UK homeowners, the three actions that prevent the majority of hotspots are mundane but effective: clean panels once or twice a year, cut back growing vegetation before it starts shading the array, and respond promptly to unexplained output drops in your monitoring app. None of this requires a thermal camera – but if you’re out of warranty and more than 10 years in, consider paying £100-£200 for one professional thermal survey. You’ll know for certain whether hotspots are silently eating into your system.

When buying new, prioritise half-cell or IBC panels from manufacturers with strong warranties, and seriously consider module-level power electronics (microinverters or optimisers). A single shaded or hotspotted panel can drag an entire string down on traditional string-inverter systems; module-level electronics keep that damage contained to the single panel.