Antenna Fundamentals and Integration Phased Arrays Informational

What is the element spacing requirement for a phased array to avoid grating lobes?

Grating lobes are undesired secondary main beams that appear when the element spacing exceeds the critical limit. The condition for no grating lobes: d < λ/(1 + sinθmax), where θmax is the maximum scan angle. For θmax = 90° (full hemisphere): d < λ/2. For θmax = 60°: d < λ/1.87 ≈ 0.535λ. For θmax = 45°: d < λ/1.71 ≈ 0.585λ. The standard design rule is d = λ/2, which prevents grating lobes for all scan angles. Exceeding this spacing creates grating lobes that appear at angles where the path difference between adjacent elements equals a full wavelength, producing a secondary beam as strong as the main beam.
Category: Antenna Fundamentals and Integration
Updated: April 2026
Product Tie-In: Phased Arrays, Phase Shifters, Beamformers

Grating Lobe Prevention

Grating lobes are an artifact of the periodic element arrangement. The array factor has maxima whenever the inter-element phase difference ψ = kd sinθ + β equals a multiple of 2π. The main beam occurs at ψ = 0 (the intended beam direction). Grating lobes occur at ψ = ±2π, ±4π, etc. The grating lobe direction is: sinθgl = sinθ₀ ± nλ/d, where n is an integer. For the first grating lobe to be outside the visible region (|sinθ| > 1): d must satisfy d < λ/(1 + |sinθ₀|).

At mmWave frequencies, the half-wavelength spacing requirement results in very small element separations: d = 5.4 mm at 28 GHz, d = 3.8 mm at 39 GHz, d = 2.5 mm at 60 GHz. This dense spacing constrains the element design and the packaging of T/R modules behind each element. At 60 GHz: 256 elements fit in a 40mm × 40mm area.

Some systems deliberately accept grating lobes to use larger element spacing (which simplifies the mechanical design and reduces mutual coupling). This is acceptable when the scan range is limited or when the element pattern has a null in the grating lobe direction (element pattern suppression).

Common Questions

Frequently Asked Questions

What happens if I exceed λ/2 spacing?

Grating lobes appear at scan angles where sinθgl = sinθ₀ + λ/d falls within the visible region (|sinθ| < 1). The grating lobe has the same amplitude as the main beam (for uniform excitation), effectively splitting the radiated power and degrading the array's directivity. This is usually unacceptable.

Can I use non-uniform element spacing?

Yes. Aperiodic (non-uniform) element spacing breaks the periodicity that creates grating lobes. Random or optimized sparse arrays can use average spacing > λ/2 without grating lobes, but with elevated average sidelobe levels. This is used in radio astronomy (very large baseline arrays) and some radar applications.

Does triangular lattice help?

Yes. A triangular (hexagonal) lattice packing allows element spacing up to d = λ/√3 ≈ 0.577λ for full-hemisphere scanning, compared to d = λ/2 for a rectangular lattice. This 15% increase in spacing reduces the number of elements by 25% for the same aperture, which is a significant cost savings for large arrays.

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