c1 drafted · lead Hot cell in IR image
IR imaging has shown cells overheating where a neighbouring module row shades them.
- Review on Infrared and Electroluminescence Imaging for PV Field Applications
fig=22h=4841e78493a5
Inter-row shading happens when one row of modules casts a shadow on the row behind it. The shadow changes with the time of day and the season. You can see it during a visual inspection. In monitoring data, it shows up when you compare shaded strings with unshaded strings or with a shading simulation. In IR images, the cells shaded by the row in front can appear overheated. Prolonged shading can lead to hot spots, which can cause follow-up damage such as burn marks or bypass diode failures. On tracker sites, the extra shading can come from rolling terrain, which upsets the backtracking geometry. It can also come from tracker twist, where one section of a row sits at the wrong tilt. Terrain-related losses repeat with sun position and cluster at grade breaks and motor block boundaries. Twist shows up as rows whose shadow lines and measured angles differ from their neighbours under the same command. Start by comparing normalized row or inverter output across morning, noon and afternoon windows, since losses tend to peak at low sun angles. A tracker that follows its commanded angle can still lose energy if the terrain model or motor block layout is too coarse. Check the backtracking settings as well as the hardware.
<!-- review notes
observed_asc1 drafted · lead Hot cell in IR image
IR imaging has shown cells overheating where a neighbouring module row shades them.
fig=22 h=4841e78493a5c2 drafted · lead String current below average
Found by comparing monitoring data from shaded strings against unshaded ones. The shaded strings produce less, and the gap moves with the time of day and the season.
sec=h54 h=df63666c4734sec=h78 h=df63666c4734review note: support check: partial - Passages say shading is seen by comparing monitoring data of shaded vs unshaded strings and varies with day/season, but do not mention string current specifically or that shaded strings fall below.
c3 drafted · lead PR drop at low profile angle
Average PR is computed separately for times when the solar profile angle is above the shading angle and times when it is below. The difference between the two, called PRdrop, estimates row shading loss but also contains low-light and inverter part-load effects.
sec=4.2.1 h=fc5f258c95cbc4 drafted · lead Loss aligned with grade breaks
On rolling terrain, losses tend to cluster at grade breaks, swales and rolling sections that differ from the slope assumed in the model. They are strongest at low sun angles.
sec=h4 h=7ebb164fa9e1review note: support check: partial - Passage describes clustering at grade breaks, swales, rolling sections and strongest at low sun, but attributes it to terrain undulation losses; the link to inter-row shading is implied only by 'locally excessive shading'.
c5 drafted · lead Loss aligned with motor blocks
A single command angle across a large motor block that spans different terrain can cause extra shading of some rows.
sec=h4 h=7ebb164fa9e1sec=h5 h=206561d63ce8c6 drafted · lead Row shadow line offset
In drone orthomosaic or oblique images, the row-end shadow lines of a twisted tracker row differ from those of neighbouring rows.
sec=h6 h=3c47e2464233review note: support check: partial - Drone imagery to compare row-end shadow lines against neighbours is stated for a twisted row, but the passage doesn't explicitly say they differ or tie it to inter-row shading.
c7 drafted · lead Low normalized row current
Rows affected by tracker twist can show lower normalized current than the rows next to them, mainly at low sun angles and during backtracking transitions.
sec=h4 h=47d9eb5061f6review note: support check: partial - Passage says affected twisted rows show lower normalized current than adjacent rows, mainly at low sun angles/backtracking; it ties this to twist and doesn't mention inter-row shading explicitly.
typical_power_lossConditions: Typical cumulative annual shading loss of PV systems, all shading causes including row-to-row self-shading
sec=h54 h=df63666c4734sec=h78 h=df63666c4734review note: possible conflict with c9 (same source; check the conditions)
c9 drafted · lead 20–30 PERCENT
Conditions: Energy loss from shading that can be observed on rooftop or facade systems, reported as 'up to 20-30%'
sec=h54 h=df63666c4734sec=h78 h=df63666c4734review note: support check: partial - The 20-30% is stated as 'up to' for rooftop/facade systems, not a typical value, and not specific to inter-row shading.; possible conflict with c8 (same source; check the conditions)
related_to c3related_to c1related_to c16presents_as c8presents_as c6