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Automotive and vehicle dynamics

Amplitude of mean front and rear road input

Amplitude of the average of the road heights under the front and rear axles when both follow the same sinusoidal track of peak amplitude A and wavelength λ, a wheelbase L apart.

Ref
VEH-63
Rev
v1
Field
Automotive and vehicle dynamics
Result
Amean [m]

For a sinusoidal road of amplitude A and wavelength λ, the two axles see the same wave with a phase difference of 2πL/λ. The average of the front and rear heights is a sinusoid of amplitude A|cos(πL/λ)|, the part that drives bounce. The half-difference has amplitude A|sin(πL/λ)| and drives pitch.

Amplitude of the average of the road heights under the front and rear axles when both follow the same sinusoidal track of peak amplitude A and wavelength λ, a wheelbase L apart. A kinematic heave input, excluding the body and suspension response.

Calculator

Solve for
m
m
0.0010.2
m
0.510
m
0.5100
  • Fraction of the amplitude that reaches the bounce input0.5
  • Half-difference amplitude (pitch input), A|sin(πL/λ)|0.01732 m
  • Longest wavelength that cancels the bounce input, 2L4 m

What drives the result

Each variable is moved across its typical range while the others stay at the values above. The longest bar is the key driver.

Mean axle input amplitude (m) current value 0.01 m
ARoad amplitudeKey driver
5e-40.1
LWheelbase
3.49e-40.02
λRoad wavelength
0.001510.02
  • The bounce input is 50 % of the road amplitude, and the pitch input 86.6 %.
  • A wavelength of 2L = 4 m cancels the bounce input entirely, so the vehicle only pitches, which is the wheelbase filtering effect.
Chart data as tables

Ranked variables

VariableTypical rangeLowest resultHighest resultSwing (m)Local stepChange in result
A Road amplitude0.001 to 0.2 m5e-40.10.0995+10%+10 %
L Wheelbase0.5 to 10 m3.49e-40.019960.01961+10%−18.7 %
λ Road wavelength0.5 to 100 m0.0015080.020.01849+10%+16 %

Sweep of Road wavelength

Road wavelength (m)Mean axle input amplitude (m)
0.50.02
12.940.01769
25.380.01939
37.810.01972
50.250.01984
62.690.0199
75.130.01993
87.560.01995
1000.01996

Sweep one variable

Mean axle input amplitude (m)Hover, touch, or use the arrow keys on the chart
0.0050.010.0150.02 20406080100 Road wavelength (m) now 0.01

Variables and how each one contributes

Amean

Mean axle input amplitude

Result · m

What the equation gives you. Everything else feeds it.

A

Road amplitude

m · typical 0.001 to 0.2

The amplitude of the road wave, in m. Raises the mean input in direct proportion. Raising it by 10 % (to 0.022) moves the result by +10 %, from 0.01 to 0.011 m.

L

Wheelbase

m · typical 0.5 to 10

The wheelbase, in m. Changes the phase difference and moves the cancellation wavelengths. Raising it by 10 % (to 2.2) moves the result by −18.7 %, from 0.01 to 0.008135 m.

λ

Road wavelength

m · typical 0.5 to 100

The road wavelength, in m. Long waves give a mean input near the full amplitude; wavelengths of 2L cancel it completely. Raising it by 10 % (to 6.6) moves the result by +16 %, from 0.01 to 0.0116 m.

Worked example with the values above

  1. Phase term: πL/λ = π × 2 / 6 = 1.0472 rad.
  2. |cos| = 0.5.
  3. A_mean = 0.02 × 0.5 = 0.01 m.

Assumptions and limits

  • Constant vehicle speed along a straight wheel path, and a stationary, zero-mean road profile.
  • One-sided PSDs, with spatial frequency in cycles per metre and temporal frequency in hertz.

Common mistakes

  • Mixing cycles per metre with radians per metre, which differ by 2π.
  • Mixing one-sided and two-sided spectra.
  • Applying a spectral relation outside the wavelength band over which the road was measured.

Statistics and uncertainty

Measured road PSDs scatter by a factor of two or more between road sections, and a power-law fit describes only a limited band. Treat spectral levels as indicative of a road class, not of a specific road.

Where it is used

  • Converting measured road roughness into inputs for ride simulations.
  • Predicting which road wavelengths excite body bounce, pitch and wheel hop.

Maths you need

  • Wavelength and frequency: f = U/λ
  • Power spectral density: variance per unit frequency
  • Parseval’s theorem: the area under the PSD equals the variance

Related formulas

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