Far Field Boundary 2
Compute the Fraunhofer far-field distance boundaryMeters = 2 * diameterMeters^2 / wavelengthMeters.
Description
Compute the Fraunhofer far-field distance boundaryMeters = 2 * diameterMeters^2 / wavelengthMeters.
Far Field Boundary 2: Compute the Fraunhofer far-field distance boundaryMeters = 2 * diameterMeters^2 / wavelengthMeters.
When to use Far Field Boundary 2
Use this electronics calculation for a first-pass component, converter, signal, motor, or sensor estimate when the stated operating conditions and units match the device data.
- Diameter (m)
- Largest aperture dimension.
- Wavelength (m)
- Operating wavelength.
How Far Field Boundary 2 works
Compute the Fraunhofer far-field distance boundaryMeters = 2 * diameterMeters^2 / wavelengthMeters. The tool evaluates the supplied inputs together and returns the named outputs below; it does not infer omitted operating conditions or change the units shown.1
- Far-Field Boundary (m)
- Far-field boundary distance from the aperture.
Limitations and assumptions
- Antenna formulas assume stated frequency, impedance match, polarization, efficiency, aperture, and propagation geometry. Nearby objects, ground, feed loss, multipath, regulatory averaging, near-field conditions, and pattern variation can make free-space or ideal-aperture results inaccurate.
- Use finite inputs in the displayed units and preserve more precision than the final presentation requires. Independently verify safety-critical, financial, compliance, or production decisions.
Alternative or Complementary approaches
Check the result against the current datasheet and worst-case operating corners, then verify the circuit or measurement with simulation and bench testing where failure matters.
References
-
Antenna — Wikipedia contributors
Similar or alternative tools
- Far Field Boundary
Compute the far-field boundary of an aperture as Rf = 2 x D^2 / lambda; aperture size and wavelength must be positive.
- Near Field Distance
Compute the outer boundary of an aperture antenna's reactive near field as Rn = 0.62 x sqrt(D^3 / lambda); dish diameter and wavelength must be positive.
- Beamwidth From Diameter
Approximate parabolic dish half-power beamwidth in degrees as bwDegrees = 70 * wavelengthMeters / dishDiameterMeters.