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Antenna

Antenna Beamwidth & Gain Calculator

Calculate antenna 3 dB beamwidth, gain from aperture, and effective area. Determine HPBW for dish, horn, and aperture antennas. Free, instant results.

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Formula

θ3dB≈70λ/D(degrees),G=ηa×(πD/λ)2θ_3dB ≈ 70λ/D (degrees), G = η_a × (πD/λ)²
θ_3dB— 3 dB half-power beamwidth (°)
λ— Wavelength (m)
D— Aperture diameter (m)
η_a— Aperture efficiency
G— Gain (dBi)

How It Works

Antenna beamwidth calculator computes half-power beamwidth (HPBW) and first-null beamwidth from aperture dimensions and frequency — satellite link engineers, radar system designers, and wireless network planners use this to determine coverage area and pointing requirements. The 3-dB (half-power) beamwidth theta_3dB = k*lambda/D, where k is a constant depending on aperture illumination (typically 58-70 degrees for uniform to tapered), per Balanis's 'Antenna Theory' (4th ed.) and IEEE Standard 145-2013.

For uniformly illuminated circular apertures, theta_3dB = 58*lambda/D degrees. For parabolic dishes with typical edge taper (10-15 dB), theta_3dB = 70*lambda/D degrees. A 2-meter dish at 12 GHz (lambda = 25 mm) has beamwidth = 70*0.025/2 = 0.875 degrees. Beamwidth inversely relates to gain: halving beamwidth (doubling D) quadruples gain (+6 dB) because energy concentrates into a smaller solid angle.

Gain and beamwidth connect through antenna theorem: G = eta * (4*pi/theta_E*theta_H) where theta_E and theta_H are E-plane and H-plane beamwidths in radians. For a 1-degree beamwidth pencil beam with 60% efficiency: G = 0.6 * (4*pi/(0.017)^2) = 26,000 = 44 dBi. Narrow beamwidths require precise pointing: a 1-degree beam with 0.5-degree pointing error loses 3 dB gain; satellite tracking systems maintain < 0.1*theta_3dB pointing accuracy.

Worked Example

Problem: Determine beamwidth and pointing requirements for a Ku-band VSAT terminal at 14 GHz transmit with 47 dBi gain requirement.

Analysis per ITU-R S.580 methodology:

  1. Operating frequency: 14 GHz (Ku-band uplink)
  2. Wavelength: lambda = c/f = 3e8/14e9 = 21.4 mm = 0.0214 m
Dish size from gain requirement:
  1. G = eta * (pi*D/lambda)^2
47 dBi = 50,000 linear; eta = 0.6
  1. D = lambda/pi sqrt(G/eta) = 0.0214/pi sqrt(50000/0.6) = 1.97 m
  2. Use standard 2.4-meter dish for margin
Beamwidth calculation:
  1. theta_3dB = 70*lambda/D = 70*0.0214/2.4 = 0.62 degrees
  2. First null beamwidth: theta_null = 2.44*lambda/D = 2.44*0.0214/2.4 = 0.022 rad = 1.25 degrees
Pointing accuracy requirements:
  1. For < 1 dB pointing loss: error < 0.35*theta_3dB = 0.22 degrees
  2. For < 0.5 dB pointing loss: error < 0.25*theta_3dB = 0.15 degrees
  3. Specification: pointing accuracy < 0.15 degrees (9 arc-minutes)
Tracking system requirements:
  1. Geostationary satellite: no tracking needed if antenna is stable
  2. Station-keeping box: +/-0.1 degrees — dish pointing can be fixed with initial alignment
  3. Wind loading: 2.4 m dish in 50 km/h wind deflects approximately 0.1 degrees — may need radome or stow position
Gain verification:
  1. Actual gain with 2.4 m dish: G = 0.6*(pi*2.4/0.0214)^2 = 75,000 = 48.7 dBi
  2. Margin: 48.7 - 47 = 1.7 dB (accommodates pointing error, aging, rain fade)

Practical Tips

  • ✓Design for pointing accuracy < 0.3*theta_3dB to maintain < 1 dB pointing loss — this is the practical limit for fixed installations without active tracking
  • ✓For mobile satellite terminals (ships, aircraft), use antenna tracking systems maintaining < 0.1*theta_3dB accuracy; flat-panel phased arrays can electronically steer without mechanical gimbals
  • ✓When comparing antennas, request both E-plane and H-plane patterns — asymmetric beamwidths affect coverage differently for horizontal versus vertical orientations

Common Mistakes

  • ✗Using wrong beamwidth constant — k = 58 degrees for uniform illumination, k = 70 degrees for typical parabolic dish with 10 dB edge taper; wrong constant causes 20% beamwidth error
  • ✗Confusing 3-dB and first-null beamwidths — first null (complete pattern null) is approximately 2.4x the 3-dB beamwidth for circular apertures; specifications usually mean 3-dB unless stated otherwise
  • ✗Ignoring pointing loss in link budget — at half-beamwidth pointing error, gain loss is 3 dB; link budgets must include realistic pointing error allowance, especially for mobile or tracking systems
  • ✗Assuming symmetric beamwidth for all antennas — parabolic dishes and horns have symmetric beams; Yagis and sectoral antennas have different E-plane and H-plane beamwidths (specify both)

Frequently Asked Questions

The formula theta = k*lambda/D applies to aperture antennas (dishes, horns, arrays) where D is the largest dimension. Constants vary: Parabolic dish (10 dB taper): k = 70 degrees. Horn antenna: k = 56-70 degrees depending on flare angle. Phased array: k = 51 degrees (broadside), increasing with scan angle. For Yagi antennas, use empirical formulas based on boom length: theta approximately equals 52/sqrt(G_dBd) degrees. For dipoles and omnidirectional antennas, elevation beamwidth depends on element pattern, not aperture formula.
Inversely proportional for fixed antenna size: doubling frequency halves beamwidth (halves lambda in theta = k*lambda/D). A 1-meter dish: at 4 GHz: theta = 70*0.075/1 = 5.25 degrees. At 12 GHz: theta = 70*0.025/1 = 1.75 degrees. At 40 GHz: theta = 70*0.0075/1 = 0.53 degrees. This is why high-frequency satellite links (Ka, V-band) require more precise pointing than C-band systems. Conversely, for fixed beamwidth requirement, higher frequency allows smaller antenna — cellular small cells use high frequencies for narrow urban coverage.
Gain and beamwidth are reciprocally related through antenna theorem: G = eta * 4*pi/(theta_E*theta_H) where angles are in radians. Narrower beamwidth means higher gain — energy concentrates in smaller solid angle. Factors affecting gain: (1) Aperture size — larger aperture, narrower beam, higher gain. (2) Frequency — higher frequency, narrower beam for same size, higher gain. (3) Efficiency — illumination taper, spillover, blockage reduce gain 1.5-3 dB below theoretical. (4) Surface accuracy — errors > lambda/16 cause phase errors reducing gain. Practical gain limits: 20-25 dBi for Yagis (limited by boom length), 35-60 dBi for dishes (limited by manufacturing precision).
The simple formula theta = 70*lambda/D is accurate within +/-10% for well-designed parabolic dishes with standard illumination. Variations: (1) Illumination taper — uniform: k = 58; -10 dB taper: k = 70; -15 dB taper: k = 75. (2) Aperture shape — circular (k = 70), rectangular (k_E differs from k_H). (3) Blockage — feed and struts widen main beam and raise sidelobes. (4) Surface errors — random errors slightly widen beam and reduce peak gain. For precision applications, compute beamwidth from full radiation pattern (numerical integration or measurement) rather than approximate formula.
Yes, with modifications: Broadside beamwidth follows theta = 51*lambda/D for uniformly illuminated linear array (k = 51 from sin(x)/x pattern). With amplitude taper for sidelobe control: k = 60-70. Scan angle theta_s widens beam by factor 1/cos(theta_s): a 2-degree broadside beam becomes 2.3 degrees at 30-degree scan, 4 degrees at 60-degree scan. Phased arrays also experience gain reduction with scan: approximately cos(theta_s) to cos^1.5(theta_s) depending on element pattern. Electronic steering eliminates mechanical pointing requirements but requires computing beamwidth at each scan position.

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