
Calculate satellite dish gain with G = η × (πD/λ)², then convert it to dBi with G_dBi = 10 log10(G). D is the projected aperture diameter, λ is wavelength, and η is the assumed aperture efficiency expressed as a fraction [1]. With λ = c/f and c = 299,792,458 m/s, a 1.2 m dish at 12 GHz and 60% efficiency gives about 41.4 dBi [2]. This is a calculated peak gain, not a measured specification for a particular antenna.
Table of Contents
Gain Formula
For a circular parabolic dish, use these equations with D and λ in meters and frequency f in hertz [1]:
λ = c/f
G_linear = η × (πD/λ)²
G_dBi = 10 log10(G_linear)
- D is the diameter corresponding to the projected collecting aperture, not automatically the reflector’s longest rim dimension. A size class such as Dolph’s 1.2 m quick-deploy flyaway antenna is only the starting point; confirm the aperture definition before calculating.
- λ is the free-space wavelength at the specific transmit or receive frequency. Convert GHz to Hz by multiplying by 1,000,000,000 before using λ = c/f.
- η accounts for the reduction from the ideal aperture result on the stated calculation basis. Enter 60% as 0.60, not 60. The cited university text gives 0.55–0.60 as typical values, not a guarantee for every dish [1].
dBi expresses gain relative to an isotropic radiator. The dish concentrates radiation in a direction; it does not create transmitter power. Aperture efficiency is effective collecting area divided by geometric aperture area. Illumination taper reduces that effective area, which is why physical size alone cannot establish the gain [3].
Find Wavelength First
The following wavelengths use the exact vacuum speed of light, 299,792,458 m/s [2]. Retain unrounded values in the calculation and round only the final gain.
| Frequency | Wavelength in meters | Wavelength in millimeters |
|---|---|---|
| 4 GHz | 0.074948 | 74.948 |
| 12 GHz | 0.024983 | 24.983 |
| 20 GHz | 0.014990 | 14.990 |
| 30 GHz | 0.009993 | 9.993 |
Do not divide a diameter in meters by a wavelength in millimeters. A factor-of-1,000 error in D/λ changes the calculated gain by 20 log10(1,000), or 60 dB. Entering 60 instead of 0.60 for efficiency produces a different error: 10 log10(100), or 20 dB too much gain.
Worked Calculation
Use a circular 1.2 m projected aperture, f = 12 GHz, and η = 0.60. These are illustration inputs, not a claim about a product’s measured efficiency. The calculation follows the aperture-gain equation [1].
Calculate Wavelength
λ = 299,792,458 / 12,000,000,000 = 0.0249827048 m, approximately 25 mm.
Calculate Linear Gain
πD/λ = π × 1.2 / 0.0249827048 ≈ 150.9008. Squaring this value gives about 22,771.06. Multiplying by 0.60 gives G_linear ≈ 13,662.64.
Convert To dBi
10 log10(13,662.64) ≈ 41.3553 dBi. Report this as 41.36 dBi when showing the arithmetic, or about 41.4 dBi for an estimate with assumed efficiency.
Record The Basis
Calculated peak gain: about 41.4 dBi at 12 GHz, with a 1.2 m circular projected aperture and assumed aperture efficiency of 60%, in the far field. No additional external feedline loss or pointing loss has been applied.
Keep that basis with the number. If a supplier’s efficiency already includes a loss term, do not subtract the same loss again.
Gain By Size And Frequency
Every row below uses G = 0.60 × (πDf/c)² with the same exact value of c. All gains are rounded to one decimal place. They are calculated examples, not measured product values; holding efficiency at 60% across frequencies does not establish that a physical antenna operates across those bands [1] [2].
| Projected diameter | Frequency | Assumed efficiency | Calculated gain |
|---|---|---|---|
| 0.6 m | 12 GHz | 60% | 35.3 dBi |
| 0.9 m | 12 GHz | 60% | 38.9 dBi |
| 1.2 m | 12 GHz | 60% | 41.4 dBi |
| 1.8 m | 12 GHz | 60% | 44.9 dBi |
| 1.2 m | 4 GHz | 60% | 31.8 dBi |
| 2.4 m | 4 GHz | 60% | 37.8 dBi |
| 3.7 m | 4 GHz | 60% | 41.6 dBi |
| 1.2 m | 20 GHz | 60% | 45.8 dBi |
| 1.2 m | 30 GHz | 60% | 49.3 dBi |
The 3.7 m row illustrates an aperture class also found in Dolph’s 3.7/4.5 m prime-focus antenna systems. Use the specific model’s operating frequency and documented gain or efficiency to evaluate the actual antenna.
Choose An Efficiency Assumption
If no applicable efficiency is available, state an assumption and show its sensitivity. Here, 55% and 60% sit within the cited textbook’s typical range; 65% and 70% are comparison scenarios, not promised performance [1].
| Assumed efficiency | Gain at 1.2 m and 12 GHz | Change from 60% |
|---|---|---|
| 55% | 40.98 dBi | −0.38 dB |
| 60% | 41.36 dBi | 0 dB |
| 65% | 41.70 dBi | +0.35 dB |
| 70% | 42.02 dBi | +0.67 dB |
Calculated from unrounded values, the 55%–70% efficiency span is 10 log10(0.70/0.55) ≈ 1.05 dB. The 60% result is not a theoretical ceiling. It is one efficiency scenario. Surface accuracy, aperture blockage, illumination and spillover affect performance, and their influence must be reflected in the efficiency or in explicitly separate correction terms, without double counting [3].
How Size And Frequency Change Gain
At unchanged efficiency, doubling diameter adds 20 log10(2) ≈ 6.02 dB. Doubling frequency gives the same increase because wavelength halves. These are conditional scaling rules, not a guarantee that the same feed and reflector retain their efficiency at another frequency.
For example, increasing diameter from 0.9 m to 1.2 m at 12 GHz adds 20 log10(1.2/0.9) ≈ 2.50 dB. Increasing frequency from 4 GHz to 12 GHz at fixed diameter adds 20 log10(3) ≈ 9.54 dB. Calculate these differences before rounding individual gain values.
A Gain Discrepancy To Work Through
Suppose you are comparing SATCOM antennas and need to understand a hypothetical 40.0 dBi specification for a 1.2 m aperture at 12 GHz. The 60% example above gives 41.36 dBi, a difference of about 1.36 dB. This is a calculation exercise, not a reported customer case or field test.
Rearrange the same equation: η = 10^(G_dBi/10) / (πD/λ)². With 40.0 dBi, 1.2 m and 12 GHz, η ≈ 0.439, or 43.9%, on the same gain basis. That does not diagnose a faulty dish; it identifies the efficiency implied by the stated inputs.
Before comparing the two figures, ask whether both refer to the same frequency, projected aperture, peak direction and reference plane. Check whether the quoted gain includes feed-network losses. A microwave feedhorn is part of the illumination system, so its compatibility with the reflector matters; diameter alone does not settle the comparison. If these definitions are unavailable, keep the result as an estimate rather than declaring either figure wrong.
Keep Gain And Link Losses Separate
The aperture equation gives a peak-gain estimate on the efficiency basis you choose. It does not independently calculate pointing loss, atmospheric attenuation, or every component loss. NRAO distinguishes gain from directivity when dissipative losses are present and discusses how surface and tracking errors reduce antenna performance [3].
Choose a reference plane before making a link budget. If gain is specified at the antenna feed input, losses in an upstream OMT, waveguide diplexer, or other antenna feeder network may need separate treatment. If the quoted assembly gain already includes those components, subtracting their losses again would understate performance.
For transmit power referenced ahead of a separately budgeted feeder, EIRP_dBW = P_tx_dBW − L_feed_dB + G_antenna_dBi. A 10 W transmitter is 10 dBW; with 41.36 dBi antenna gain and zero additional feeder loss, EIRP is about 51.36 dBW. An illustrative 1 dB feeder loss reduces it to about 50.36 dBW. Increasing transmitter power changes EIRP, not the dish’s gain [1].
Do not infer an exact half-power beamwidth or pointing tolerance from the gain number alone. Beam shape depends on aperture illumination, and a half-power beamwidth is not interchangeable with a first-null angle. Use a specified or measured radiation pattern for pointing-loss calculations [3].
Check Before Using The Result
- Confirm projected area. For an elliptical projected aperture with full axes 1.2 m and 1.0 m, the area is 1.0/1.2 of a 1.2 m circle. At the same frequency and efficiency, that means 10 log10(1.0/1.2) ≈ −0.79 dB. Do not apply this correction to an offset reflector merely because its physical rim looks oval; establish the projected aperture first.
- Use the actual frequency and gain basis. A transmit-band gain is not automatically the receive-band gain. Compare peak gain with peak gain, and keep component losses and mismatch treatment consistent.
- Check patterns separately from peak gain. ITU publishes reference patterns for earth-station coordination and interference assessment [4]. Recommendation ITU-R S.465-6 covers 2–31 GHz and is listed as in force; it is a reference-pattern recommendation, not an efficiency specification for an individual dish [5].
- Use the applicable filing requirements. FCC 47 CFR 25.209 addresses earth-station antenna performance standards. Check the provisions applicable to the operating band and antenna arrangement rather than treating a calculated peak dBi value as proof of compliance [6].
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Request Engineering ReviewShort Answer
Find wavelength from λ = c/f, calculate G = η × (πD/λ)², then take 10 log10(G) to get dBi [1]. A 1.2 m circular aperture at 12 GHz and 60% efficiency gives about 41.4 dBi. Keep the frequency, projected size, efficiency and loss basis attached to that figure; those inputs determine whether it is useful in a real comparison.