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Phased Array Gain Calculator

Full 2D planar/1D linear phased array solver: computes realized gain, scan loss, EIRP, 3D beamwidths, aperture efficiency, grating lobe boundaries, and far-field distances.

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Input Parameters

Enter parameters and click Calculate to view results

Formula & Theory

G(theta) = G_0 + 10log10(N) + 10log10(eta) + 10log10(cos^k(theta_scan)) | R_ff = 2D^2 / lambda

This formula is used to calculate antenna parameters for phased array gain calculator.

A Phased Array Gain Calculator helps estimate the gain and key RF characteristics of a linear or planar phased-array antenna from its frequency, number of elements, element spacing, single-element directivity, efficiency, scan angle, and transmit power.

Unlike a basic antenna gain calculator, a phased-array calculation needs to account for the number of elements and how the beam is electronically steered. This calculator therefore provides more than a single gain value. It calculates realized array gain, broadside gain, ideal directivity, scan loss, EIRP, beamwidth, physical aperture, effective aperture, grating-lobe limits, and far-field distance.

For a quick first-pass RF design, enter the operating frequency, array dimensions, element spacing, element directivity, efficiency, scan angle, scan-loss exponent, and power per element. The calculator then derives the corresponding antenna and RF metrics.

What Is a Phased Array Gain Calculator?

A phased array consists of multiple antenna elements whose relative phases are controlled to steer the main radiation beam. By changing the phase relationship between elements, the array can electronically change its pointing direction without physically rotating the antenna.

A phased array gain calculator estimates how the individual elements work together as an array. The total result depends on several variables rather than simply the gain of one antenna element.

The calculator supports both 1D linear and 2D planar array configurations. It uses the number of rows and columns to determine the total number of elements and then calculates the array-factor contribution, ideal directivity, efficiency-adjusted gain, scan loss, EIRP, beamwidth, aperture dimensions, grating-lobe boundary, and electromagnetic boundary distances.

Quick answer: How is phased array gain calculated?

The calculator first determines the number of array elements:

N = Nₓ × Nᵧ

It then calculates the array-factor contribution:

G_array = 10 log₁₀(N)

The ideal directivity is:

G_ideal = G_element + 10 log₁₀(N)

Array efficiency is then applied:

G_broadside = G_ideal + 10 log₁₀(η)

Finally, the calculator applies a cosine-powered scan-loss model:

Scan Loss = |10 log₁₀(cosᵏ θ)|

and calculates:

G_scanned = G_broadside − Scan Loss

These equations follow the calculation sequence implemented in the calculator.


What Inputs Does the Phased Array Gain Calculator Need?

The calculator uses ten primary inputs to characterize the array and its RF operating conditions.

InputWhat it representsExample
Center FrequencyOperating RF frequency28 GHz
Array RowsElements along the Y direction8
Array ColumnsElements along the X direction8
X Element SpacingX-axis spacing relative to wavelength0.5 λ
Y Element SpacingY-axis spacing relative to wavelength0.5 λ
Single Element DirectivityDirectivity of one element5 dBi
Array EfficiencyOverall efficiency75%
Scan AngleBeam steering angle30°
Element Scan Loss ExponentCosine-model exponent1.3
Power per ElementRF power supplied to each element/module10 dBm

Center Frequency

The center frequency determines the wavelength used throughout the calculation.

The calculator converts frequency from GHz to Hz and uses:

λ = c / f

where:

  • λ = wavelength in meters
  • c = speed of light
  • f = frequency in Hz

The implementation uses 299,792,458 m/s for the speed of light.

Frequency matters because element spacing is entered in wavelengths. Once the wavelength is known, the calculator converts normalized spacing into physical dimensions.

Array Rows and Columns

The number of rows and columns defines the size of the array.

For a rectangular planar array:

N = Nₓ × Nᵧ

For example, an 8 × 8 array contains:

8 × 8 = 64 elements

The calculator uses this total element count to determine the array-factor gain and total transmit power.

X and Y Element Spacing

Element spacing is entered as a fraction or multiple of wavelength, such as:

0.5 λ

The calculator independently accepts X-axis and Y-axis spacing. This is important for rectangular planar arrays where the two dimensions may not have identical spacing.

Spacing also has a major effect on grating lobes. In general array analysis, half-wavelength spacing is a common design choice for avoiding visible grating lobes over broad scanning conditions, although the exact allowable spacing depends on the required scan range and geometry.

Single Element Directivity

The single-element directivity represents the directional performance of an individual radiating element.

The calculator combines this value with the array-factor contribution to obtain ideal array directivity.

Array Efficiency

Real antennas are not lossless. The calculator therefore applies an efficiency factor to ideal directivity.

For example, 75% efficiency is represented internally as:

η = 0.75

The resulting efficiency penalty is:

10 log₁₀(0.75)

which is approximately −1.25 dB.

Scan Angle

The scan angle represents how far the main beam is electronically steered away from broadside.

A scan angle of:

represents broadside operation.

A scan angle of:

30°

means the modeled beam is steered 30° away from broadside.

The calculator accepts scan angles from 0° up to, but not including, 90°.

Element Scan Loss Exponent

The k parameter controls the cosine-based scan-loss model.

The calculator defaults to:

k = 1.3

and allows values from 0 to 5.

This type of cosine-power modeling is also used in phased-array analysis to represent gain reduction as an array scans away from broadside. The exact exponent depends on the array and element characteristics.

Power per Element

The power-per-element input represents the RF transmit power associated with each array element or transmit module.

The calculator scales this to total transmit power using the number of elements.


Phased Array Gain Formula Explained

Understanding the individual calculation stages makes the final gain result much easier to interpret.

1. Calculate the Number of Elements

For a rectangular planar array:

N = Nₓ × Nᵧ

An 8 × 8 array therefore has:

N = 64

A 16 × 16 array would contain:

N = 256

More elements increase the modeled array-factor contribution, but the final realized gain also depends on efficiency and scan loss.

2. Calculate Array Factor Gain

The calculator uses:

G_array = 10 log₁₀(N)

For 64 elements:

G_array = 10 log₁₀(64)

G_array ≈ 18.06 dB

This is the array-factor contribution used by the calculator.

3. Calculate Ideal Directivity

The calculator adds the single-element directivity:

G_ideal = G_element + G_array

For a 5 dBi element and 64 elements:

G_ideal = 5 + 18.06

G_ideal ≈ 23.06 dBi

This is an ideal, lossless directivity estimate rather than the final realized gain.

4. Apply Array Efficiency

The calculator then applies:

G_broadside = G_ideal + 10 log₁₀(η)

With 75% efficiency:

G_broadside ≈ 23.06 − 1.25

G_broadside ≈ 21.81 dBi

5. Apply Scan Loss

For a scanned beam:

Scan Loss = |10 log₁₀(cosᵏ θ)|

The scanned realized gain becomes:

G_scanned = G_broadside − Scan Loss

The calculator therefore distinguishes between broadside realized gain and scanned realized gain.


Real-Life Example: 28 GHz 8×8 Phased Array

Consider an RF engineer designing an 8 × 8 planar phased array for a 28 GHz application.

The engineer enters:

  • Frequency: 28 GHz
  • Rows: 8
  • Columns: 8
  • X spacing: 0.5 λ
  • Y spacing: 0.5 λ
  • Element directivity: 5 dBi
  • Efficiency: 75%
  • Scan angle: 30°
  • Scan exponent: 1.3
  • Power per element: 10 dBm

These values correspond to the type of configuration supported by the calculator.

Step 1: Determine the wavelength

At 28 GHz:

λ = c / f

The wavelength is approximately:

λ ≈ 0.01071 m

or about:

10.71 mm

Step 2: Determine total elements

N = 8 × 8 = 64

Step 3: Calculate array-factor gain

10 log₁₀(64) ≈ 18.06 dB

Step 4: Calculate ideal directivity

With a 5 dBi individual element:

5 + 18.06 = 23.06 dBi

Step 5: Apply efficiency

At 75% efficiency:

G_broadside ≈ 21.81 dBi

Step 6: Apply scan loss

At a 30° scan angle and k = 1.3, the calculator's cosine-powered model gives approximately:

0.81 dB scan loss

Therefore:

G_scanned ≈ 21.00 dBi

Step 7: Calculate total RF transmit power

Each element receives 10 dBm.

The calculator uses:

P_total = 10 + 10 log₁₀(64)

Therefore:

P_total ≈ 28.06 dBm

which is approximately:

0.64 W

Step 8: Calculate EIRP

The calculator uses:

EIRP = P_total + G_scanned

Therefore:

EIRP ≈ 28.06 + 21.00

EIRP ≈ 49.06 dBm

This corresponds to approximately:

80.6 W EIRP

The calculator reports EIRP in both dBm and watts.

What does this example tell the engineer?

The array isn't characterized by gain alone. The engineer can simultaneously examine:

  • approximately 21 dBi scanned realized gain
  • approximately 49.1 dBm EIRP
  • beamwidth
  • physical aperture
  • effective aperture
  • grating-lobe margin
  • far-field distance

That makes the calculator useful during early-stage system architecture and antenna sizing.


Realized Gain vs Ideal Directivity

One common source of confusion in antenna design is treating ideal directivity and realized gain as interchangeable.

They are not the same quantity in this calculator.

Ideal Directivity

The calculator determines ideal directivity from:

Element Directivity + Array Factor Gain

It does not yet include the array efficiency penalty.

Broadside Realized Gain

The calculator then incorporates array efficiency:

G_broadside = G_ideal + 10 log₁₀(η)

This produces a more practical gain estimate.

Scanned Realized Gain

Finally, scan loss is subtracted:

G_scanned = G_broadside − Scan Loss

The result is the calculator's primary Realized Array Gain (Scanned) output.

Why does phased-array realized gain decrease during scanning?

Scanning changes the effective projected aperture and can also change the effective performance of individual elements. A cosine-power approximation is commonly used to model this type of scan-related gain reduction.


Phased Array Scan Loss Explained

A phased array is particularly useful because its beam can be electronically steered. However, steering the beam away from broadside can reduce antenna gain.

The calculator models this using:

Scan Loss = |10 log₁₀(cosᵏ θ)|

At:

θ = 0°

the cosine is 1, so the modeled scan loss is zero.

As the scan angle increases, the cosine term decreases and the modeled loss increases.

The calculator then subtracts this loss from the broadside realized gain.

The exponent k provides a way to represent different scan-loss behaviors. The calculator's default is 1.3.

This is an analytical model, so the result should not be interpreted as a complete electromagnetic prediction for every real antenna. Actual scan performance can depend on element radiation patterns, mutual coupling, feed networks, impedance changes, calibration, and other hardware effects.


EIRP and Total Transmit Power

EIRP, or Effective Isotropic Radiated Power, combines transmitter power with antenna gain.

For this calculator, total transmit power is calculated from the power per element and the number of elements:

P_total(dBm) = P_element(dBm) + 10 log₁₀(N)

The result is converted to watts as well.

The calculator then determines:

EIRP(dBm) = P_total(dBm) + G_scanned(dBi)

It reports both the dBm and watt equivalent.

Why EIRP matters

EIRP is useful when assessing the effective radiated power of directional RF systems, including:

  • wireless communication systems
  • phased-array transmitters
  • radar
  • satellite communications
  • point-to-point links
  • high-frequency wireless systems.

Remember that dBm describes power, while dBi describes antenna gain relative to an isotropic radiator. EIRP combines the two in the appropriate logarithmic form.


Phased Array Beamwidth Calculation

Gain isn't the only important property of an array. Engineers also need to know how narrow the main beam is.

The calculator estimates half-power beamwidth (HPBW) separately in azimuth and elevation.

For broadside operation, it uses:

HPBW_az ≈ 50.8° / (Nₓ × dₓ/λ)

and:

HPBW_el ≈ 50.8° / (Nᵧ × dᵧ/λ)

The calculator then adjusts the azimuth beamwidth for scan angle:

HPBW_az,scan = HPBW_az,broadside / cos(θ)

It also estimates first-null beamwidth as:

FNBW ≈ 2 × HPBW

These relationships are explicitly implemented in the calculator.

For the 8 × 8, 0.5 λ example:

Broadside HPBW ≈ 12.7°

At 30° scan:

Scanned azimuth HPBW ≈ 14.66°

and:

FNBW ≈ 29.33°

The general engineering principle is that increasing array aperture tends to produce a narrower main beam, while scanning can broaden the beam. Array analysis tools likewise show narrower beams as aperture is increased.


Element Spacing and Grating Lobes

Element spacing is one of the most important design parameters in a phased array.

If elements are placed too far apart, additional beams known as grating lobes can enter the visible region. These unwanted lobes can make it difficult for a system to distinguish the intended beam from another strong radiation direction.

For a conventional uniform array, half-wavelength spacing is a common way to avoid visible grating lobes over the full scan region. When spacing exceeds half a wavelength, grating lobes can appear for some scan angles.

The calculator specifically checks the maximum of the X and Y normalized spacings. When the maximum spacing exceeds 0.5 λ, it calculates a maximum scan angle based on its implemented model.

The calculator reports:

  • Grating Lobe Margin
  • Maximum Scan Limit (No Grating Lobe)

It also indicates when the selected scan angle exceeds its calculated limit.

Why this matters

Suppose an engineer wants a phased array that scans to a large angle. Simply increasing element spacing may make the physical array larger, but it can also introduce unwanted grating lobes.

This creates a practical design tradeoff between:

  • aperture size
  • element count
  • physical dimensions
  • scan range
  • grating-lobe performance.

Physical Aperture and Effective Aperture

The calculator converts normalized element spacing into physical dimensions using the wavelength.

For the X direction:

dₓ = (dₓ/λ) × λ

For the Y direction:

dᵧ = (dᵧ/λ) × λ

It then calculates:

Width = Nₓ × dₓ

Height = Nᵧ × dᵧ

and:

Physical Aperture = Width × Height

The implementation also determines the maximum physical dimension using the diagonal of the rectangular aperture.

For the 28 GHz 8 × 8 example with 0.5 λ spacing, each dimension is approximately:

4.28 cm × 4.28 cm

The calculator also estimates effective aperture using:

A_eff = G_linear λ² / (4π)


The relationship between antenna gain and effective aperture is a standard antenna relationship:

G = 4πA_eff / λ²

as documented in NASA/JPL communications material.

Physical vs effective aperture

Physical aperture is the geometric area occupied by the antenna.

Effective aperture represents the equivalent receiving area associated with its gain.

They are related, but they are not simply interchangeable measurements.


Far-Field and Fresnel Distance

Antenna measurements need to be performed at an appropriate distance from the antenna.

For a sufficiently large antenna, the radiation field close to the antenna is not the same as the far-field radiation pattern.

The calculator determines the maximum physical array dimension:

D = √(Width² + Height²)

It then uses the Fraunhofer far-field relationship:

R_ff = 2D² / λ


The calculator also provides a Fresnel boundary estimate:

R_Fresnel = 0.62 √(D³ / λ)


For the 28 GHz 8 × 8 example, the maximum diagonal dimension is approximately 6.06 cm, giving a modeled far-field distance of approximately:

0.69 m

The modeled Fresnel boundary is approximately:

8.9 cm

These outputs can be useful when planning antenna measurements, chamber tests, and radiation-pattern characterization.


Real-World Use Cases for a Phased Array Gain Calculator

1. 5G and mmWave Base Stations

Phased arrays are highly relevant to directional wireless systems because electronic beam steering allows the antenna to direct energy toward different users or coverage areas.

An engineer can use the calculator to estimate:

  • array gain
  • scan loss
  • EIRP
  • beamwidth
  • aperture dimensions
  • grating-lobe limits.

For a mmWave design, frequency has a particularly strong effect on physical wavelength and therefore array dimensions.

2. Radar Systems

Radar engineers care about antenna gain, beamwidth, scanning capability, and transmit power.

A phased-array gain estimate can therefore support early-stage decisions about:

  • array size
  • element count
  • scan angle
  • beamwidth
  • EIRP
  • measurement distance.

The calculator is especially useful for preliminary analysis before detailed antenna modeling.

3. Satellite Communications

Electronically steered arrays can be used when a system needs directional beams without relying exclusively on mechanical antenna movement.

Gain, EIRP, aperture, and scan behavior are important design considerations.

4. Point-to-Point Wireless Links

For a directional link, engineers can estimate whether a proposed array configuration provides an appropriate combination of:

  • gain
  • beamwidth
  • transmit power
  • EIRP.

The results can then feed into a broader RF link-budget analysis.

5. Antenna Prototyping

During early development, engineers often need fast estimates before building a detailed simulation model.

A calculator can provide a quick way to compare:

  • 4 × 4 vs 8 × 8
  • 0.5 λ vs larger spacing
  • different efficiencies
  • different scan angles
  • different element gains.

6. RF Laboratory Testing

The far-field and Fresnel outputs provide useful first-pass estimates for determining suitable measurement distances.

The calculator should still be treated as an analytical design aid rather than a substitute for a validated antenna measurement setup.


How to Use the Phased Array Gain Calculator

Using the calculator is straightforward.

Step 1: Enter the center frequency

Enter the operating frequency in GHz.

Step 2: Enter array rows and columns

Define the number of elements in the two array dimensions.

Step 3: Enter element spacing

Set X and Y spacing in wavelengths.

Step 4: Enter single-element directivity

Provide the directivity of the individual antenna element in dBi.

Step 5: Enter array efficiency

Enter the estimated efficiency as a percentage.

Step 6: Set the scan angle

Use 0° for broadside or enter the desired steering angle.

Step 7: Set the scan-loss exponent

Use the exponent appropriate for the simplified scan-loss model.

Step 8: Enter power per element

Specify RF power per transmit module in dBm.

Step 9: Review realized gain

The calculator returns both broadside and scanned realized gain.

Step 10: Review the remaining outputs

Check:

  • ideal directivity
  • array-factor gain
  • scan-loss penalty
  • EIRP
  • total transmit power
  • azimuth HPBW
  • elevation HPBW
  • FNBW
  • physical aperture
  • effective aperture
  • grating-lobe margin
  • maximum scan limit
  • Fraunhofer far-field distance
  • Fresnel boundary distance.

These are the outputs implemented by the calculator.


How Does Array Size Affect Gain?

A common question is:

Does doubling the number of phased-array elements double antenna gain?

The calculator models the array-factor contribution using:

10 log₁₀(N)

This means gain increases logarithmically in dB rather than increasing by the same numerical amount as element count.

For example:

  • 16 elements → approximately 12.04 dB array-factor contribution
  • 64 elements → approximately 18.06 dB
  • 256 elements → approximately 24.08 dB

These values come directly from the calculator's 10 log₁₀(N) relationship.

However, element count alone does not determine the final realized gain.

The calculator also accounts for:

  • single-element directivity
  • efficiency
  • scan angle
  • scan-loss exponent.

Therefore, adding elements can improve array-factor gain while practical losses and scan behavior still limit the final result.


Common Phased Array Design Mistakes

Ignoring efficiency

Using ideal directivity as the final antenna gain can overestimate practical performance.

The calculator explicitly separates ideal directivity from broadside realized gain.

Ignoring scan loss

A phased array does not necessarily maintain its broadside gain across its entire scan range. The calculator applies a scan-loss penalty when the beam is steered away from broadside.

Using excessive element spacing

Increasing spacing can increase physical aperture, but it can also create grating-lobe problems.

Confusing dBm and dBi

These are fundamentally different quantities.

  • dBm describes power.
  • dBi describes antenna gain.

They can be combined when calculating EIRP, but they should not be treated as equivalent units.

Ignoring physical aperture

An electrically defined array still occupies physical space. Frequency and element spacing determine actual dimensions.

Forgetting measurement distance

A radiation-pattern measurement needs an appropriate field region. The calculator therefore provides both far-field and Fresnel boundary estimates.

Treating the calculator as a full electromagnetic simulator

This is perhaps the most important limitation.

The calculator provides analytical estimates based on its implemented equations. Real hardware can behave differently because of effects such as mutual coupling, element-pattern distortion, feed losses, impedance variation, phase errors, amplitude errors, and other implementation details.


Phased Array vs Conventional Antenna

A phased array has some important differences from a conventional fixed directional antenna.

CharacteristicPhased ArrayConventional Fixed Antenna
Beam steeringElectronicUsually fixed or mechanically steered
Multiple elementsYesNot necessarily
Scan lossImportantUsually less central
Grating lobesSpacing-dependentGenerally not an array-spacing issue
BeamwidthDepends strongly on array apertureDepends on antenna geometry
EIRPImportantImportant
Beam directionDynamically controllableUsually fixed

The key advantage of a phased array is beam agility. The tradeoff is that the designer must consider additional parameters such as scan angle, element spacing, grating lobes, and scan-dependent gain.


Limitations of the Phased Array Gain Calculator

This calculator is best used as a first-pass engineering analysis tool.

Its gain calculation uses a simplified model based on:

  • element directivity
  • 10 log₁₀(N) array-factor gain
  • efficiency
  • cosine-powered scan loss.

Its beamwidth calculation uses approximate analytical relationships, while grating-lobe analysis uses a simplified spacing-based boundary. The far-field and Fresnel calculations use geometric analytical formulas.

A real phased-array antenna may require additional analysis of:

  • mutual coupling
  • embedded element patterns
  • phase-shifter errors
  • amplitude errors
  • feed-network losses
  • impedance mismatch
  • polarization
  • thermal effects
  • radome effects
  • manufacturing tolerances
  • calibration errors.

Consequently, the calculator should not replace full-wave electromagnetic simulation or measured antenna data when designing a production RF system.

It is most valuable for rapid design exploration, architecture comparison, preliminary sizing, and educational analysis.


Frequently Asked Questions

What is a phased array gain calculator?

A phased array gain calculator estimates the gain of a multi-element antenna array using parameters such as frequency, number of elements, element directivity, efficiency, spacing, and scan angle. This calculator additionally estimates EIRP, beamwidth, aperture characteristics, grating-lobe limits, and far-field distance.

How do you calculate phased array antenna gain?

The calculator first calculates array-factor gain using:

10 log₁₀(N)

It adds that value to the single-element directivity, applies the efficiency adjustment, and then subtracts the modeled scan loss.

What is the gain of an 8 × 8 phased array?

There is no single gain value for every 8 × 8 phased array. Gain depends on the individual element directivity, array efficiency, scan angle, and the model parameters used. For example, an 8 × 8 array has 64 elements, giving an array-factor contribution of approximately 18.06 dB under the calculator's model.

How does the number of elements affect phased-array gain?

The calculator models the array-factor contribution as:

10 log₁₀(N)

Therefore, increasing the number of elements increases the modeled array-factor gain, although the final realized gain also depends on efficiency and scan loss.

What is array-factor gain?

Array-factor gain is the contribution associated with combining multiple array elements. In this calculator it is represented by:

10 log₁₀(N)

where N is the total number of elements.

What is scan loss in a phased array?

Scan loss is the reduction in modeled gain when a phased-array beam is steered away from broadside. This calculator models it using a cosine-power relationship:

|10 log₁₀(cosᵏ θ)|

Cosine-power models are also used in phased-array scan-loss analysis.

Why does phased-array gain decrease when scanning?

Scanning changes the projected aperture seen in the beam direction and can reduce the effective performance of individual array elements. A cosine-based approximation can be used to represent these effects.

What is ideal directivity?

Ideal directivity in this calculator is the single-element directivity plus the array-factor contribution, before applying the array-efficiency penalty.

What is realized gain?

Realized gain is the gain after the calculator applies the efficiency adjustment and, for a scanned beam, the scan-loss penalty.

What is EIRP for a phased array?

EIRP is the total transmit power combined with antenna gain. The calculator uses:

EIRP(dBm) = Total TX Power(dBm) + Scanned Realized Gain(dBi)

and also provides the result in watts.

What causes grating lobes?

Grating lobes can occur when array elements are spaced too far apart relative to wavelength. For conventional uniform arrays, spacing greater than half a wavelength can introduce visible grating lobes for some scan conditions.

What is the recommended element spacing?

Half-wavelength spacing is a common choice when a design needs to avoid visible grating lobes across a broad scan region. However, the required spacing should be evaluated against the intended scan range and array geometry rather than treated as a universal rule.

What is HPBW?

HPBW means Half-Power Beamwidth. It represents the angular width of the main beam between points where the power has fallen to half of its peak value.

This calculator estimates azimuth and elevation HPBW using approximate array relationships.

What is FNBW?

FNBW means First Null Beamwidth. In this calculator, it is estimated as approximately twice the scanned azimuth HPBW.

How is phased-array far-field distance calculated?

The calculator uses the Fraunhofer relationship:

R_ff = 2D² / λ

where D is the maximum physical dimension of the array and λ is the wavelength.

Can this calculator be used for planar arrays?

Yes. The calculator independently accepts array rows, columns, X spacing, and Y spacing, so it can model a rectangular planar array as well as a one-dimensional configuration.


Conclusion

A Phased Array Gain Calculator provides a practical way to evaluate the major RF characteristics of a linear or planar phased-array design without manually performing every calculation.

The calculator starts with frequency and array geometry, determines the total number of elements and wavelength, and then estimates array-factor gain and ideal directivity. It applies array efficiency and scan loss to produce realized gain. From there, it calculates EIRP, transmit power, beamwidth, aperture characteristics, grating-lobe boundaries, and electromagnetic field-region distances.

For engineers working on 5G, mmWave communications, radar, satellite communications, directional wireless links, and antenna prototypes, these calculations provide useful first-pass insight into how array size, element spacing, efficiency, frequency, scan angle, and transmit power interact.

The key point is that phased-array performance is a system-level tradeoff. More elements can increase array-factor gain, but practical performance also depends on efficiency, element characteristics, scan angle, spacing, and physical aperture.

Use the calculator to quickly compare design configurations and identify potential issues such as excessive scan loss or grating-lobe risk. For a production design, however, the analytical results should be followed by detailed electromagnetic simulation and, where possible, measured antenna characterization.

Inputs used by this calculator

  • Center Frequency (f) — use GHz.
  • Array Rows (N_y) — use elements.
  • Array Columns (N_x) — use elements.
  • X Element Spacing (d_x/lambda) — use lambda.
  • Y Element Spacing (d_y/lambda) — use lambda.
  • Single Element Directivity — use dBi.
  • Array Efficiency (eta) — use %.
  • Scan Angle (theta_scan) — use °.
  • Element Scan Loss Exponent (k).
  • Power per Element (Tx Module) — use dBm.
AW
RF Engineering ExpertCalculator content reviewer

Alex Warren

B.Sc. in Electrical & Electronic Engineering (EEE)

Alex specialises in antenna design and wave propagation. His expertise helps ensure these calculators present practical RF concepts, useful design estimates, and clear engineering guidance for students, HAM operators, and wireless professionals.

Electrical & Electronic EngineeringAntenna & Wave Propagation
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