For a fixed sphere and fixed refractive index, both the Rayleigh scattering cross-section and scattering efficiency are proportional to . Halving wavelength multiplies either by , as long as the shorter wavelength still satisfies . If optical dispersion changes , the material factor changes too; the pure fourth-power comparison then needs correction.
For equal incident light intensities at blue wavelength and red wavelength , the same toy sphere gives
Blue light therefore produces about times the scattered power. This compares the particle's response at two wavelengths; it does not assert that an actual sky has this ratio of observed blue and red light intensities.
Figure 1.
Rayleigh scattering wavelength dependence for a fixed small sphere, normalized at
. The curve is over to . Blue and red comparison points are marked at and . Fixed radius and nondispersive refractive index are assumed, with throughout. This is a particle response curve, not a simulated sky optical spectrum. Details.

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