Solar Lattice

Measurement

Low normalized row current

ID
meas:low-normalized-row-current
IRI
https://solarlattice.org/kb/meas/low-normalized-row-current
Status
active

This signature is a tracker row whose normalized current comes in below the current of the rows next to it. The modules, inverters and irradiance sensors on that row can still look healthy. Tracker twist is the failure mode known to cause it. In a twisted row, one end or section sits at a different tilt from the rest of the row. The pattern often depends on time of day. It shows up most clearly at low sun angles, during backtracking transitions and in windy periods. Before comparing rows, normalize the output for irradiance and for inverter clipping. Then look at morning, solar-noon and afternoon data separately, because a twisted row can look fine at one tracker position and underperform at another. Comparing string output normalized to plane-of-array irradiance against the commanded and measured row angles helps confirm the cause. In the field, measure string currents with a clip-on ammeter while the inverter is tracking normally. Under stable irradiance, identical strings should usually read within 5 % of the average string current. If irradiance is unstable, you can delay the test, use a reference string, correct the readings with an irradiance meter, or run an IV curve test. Several factors other than twist can also make the measured current lower than expected.

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Signals

Monitoring channels where this signature appears, named by SunSpec model point.

PointUnitPattern
model_403.InDCAAlower POA-normalized string current than adjacent rows, varying between morning, noon and afternoon windows
model_302.POAIW-PER-M2used to normalize string current
model_307.WndSpdM-PER-SECloss more visible during windy intervals

Referenced by

Data