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How to Calculate Row Spacing for Ground-Mounted Solar: Sun Angles, Sloped Terrain and a Worked Example

On a ground-mounted PV plant, the closer the rows, the more capacity you can fit on the same land. But when rows get too close, the front row casts a shadow on the lower edge of the row behind it, especially in winter. Row spacing is a balance between installed capacity, energy loss and land cost. In this article we explain why inter-row shading matters, how the design sun angle is chosen, the spacing formula, the effect of sloped terrain, and a numerical example.

Why inter-row shading matters so much

A module is made of series-connected cell groups, each protected by a bypass diode. Even a thin shadow along the bottom edge of the rear row can switch off one or more cell groups, depending on module orientation, and other modules in the same string can be affected too. Loss from inter-row shading is therefore not proportional to the shaded area; a small shadow can cost more than it looks.

There are two ways to limit it: space the rows far enough apart, and choose a module layout and stringing that take into account which cell groups the shadow will hit. This article focuses on the first.

Design sun angle: why the winter solstice?

In the northern hemisphere, the sun reaches its lowest noon elevation of the year around 21 December, the winter solstice. Shadows are longest on that day. A common design approach is to avoid inter-row shading on the winter solstice during a chosen time window (for example 10:00–14:00 or 09:00–15:00 solar time). The window is a design decision: the wider it is, the further apart the rows and the fewer modules fit on the land.

Sun elevation at solar noon follows a simple formula:

α (noon) = 90° − φ + δ

where φ is latitude and δ is solar declination. At the winter solstice δ ≈ −23.44°. For other times of day you need both the sun's elevation and its azimuth (its direction in the horizontal plane), calculated with solar position formulas or software. Remember that solar time differs from clock time.

The row spacing formula

Definitions:

On flat ground, the shade-free distance from the top edge of the front table to the bottom edge of the rear table, measured perpendicular to the rows, is:

d = h × cos γ ÷ tan α

The row pitch (bottom edge of one table to bottom edge of the next) is:

Pitch = L × cos β + d

At solar noon γ = 0, so the formula reduces to d = h ÷ tan α. At other times the sun is lower, but because it comes from the side, the component of the shadow perpendicular to the rows is shortened by cos γ. Both effects have to be considered together. You can also write this with the "profile angle": tan αp = tan α ÷ cos γ, and d = h ÷ tan αp.

Ground coverage ratio (GCR)

Ground coverage ratio is table length divided by row pitch: GCR = L ÷ pitch. A higher GCR fits more capacity on the land but increases inter-row shading loss. A lower GCR reduces shading but raises land, cabling and structure cost per unit of capacity. The right GCR depends on land value and on how much winter production matters.

Worked example (flat ground)

The values below are example values: latitude φ = 38.4° N, table length L = 4.5 m, tilt β = 25°, array facing due south.

Design moment (solar time, 21 Dec)Sun elevationAngle from southd (m)Pitch (m)GCR
12:0028.16°0°3.557.630.59
10:00 (and 14:00)22.06°29.67°4.088.160.55
09:00 (and 15:00)15.15°42.23°5.209.280.48

Checking the 10:00 row: d = 1.90 × cos 29.67° ÷ tan 22.06° ≈ 1.90 × 0.869 ÷ 0.405 ≈ 4.08 m. Widening the design window from 10:00–14:00 to 09:00–15:00 adds about 1.1 m to the pitch and drops GCR from 0.55 to 0.48, meaning roughly 12% less capacity on the same land. That difference shows why the window is an economic decision.

The effect of sloped terrain

On land with a north–south slope s, the rear row stands at a different level from the front row. The shade-free distance, measured horizontally and perpendicular to the rows, becomes:

Add a 5° slope to the same example (10:00 design moment, αp ≈ 25.0°): d is 4.08 m on flat ground, drops to about 3.43 m on a south-facing slope and rises to about 5.02 m on a north-facing slope. At noon the same three values are 3.55 m, 3.05 m and 4.25 m. That is why south-facing slopes suit ground-mounted PV, while on north-facing slopes rows must be spaced noticeably wider. As the north slope approaches the sun's profile angle, the required distance grows very quickly.

East–west slope and uneven ground

An east–west slope does not change row spacing directly, but one end of the table ends up higher than the other. There are two options: tilt the table slightly sideways to follow the ground, or keep the table level and step the leg heights. Sideways-tilted tables can change morning and evening shading, so check them with a simulation.

When stepping leg heights on uneven ground, keep an eye on:

For the structural side, see our article on wind and snow loads. Any preliminary check of leg lengths, foundations and profile sections does not replace an approved structural design or calculations by a licensed engineer.

Common mistakes

Row spacing and ground-mount design with PVAGE

PVAGE's mounting structure design module uses real terrain elevation data and a slope map for ground-mounted plants. You place platform arrays, adjust row spacing and see inter-row shading in a simulation by choosing the month and hour. Heights and counts for front, middle and rear legs, profile quantities, and clamp and bolt counts are calculated.

On the structural calculation side, you get ground-mount leg and profile dimensions, foundation sizing and a preliminary check for buckling, bending, deflection and shear, exportable as a PDF. This check does not replace an approved structural design. For more on how shading affects production, read our shade analysis article.

Explore the feature: Ground-Mount Solar Design Software

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