The differential cross-section of Rayleigh scattering is inversely proportional to the fourth power of wavelength of the radiation incident on the scatterers. More precisely, $$\frac{d\sigma}{d\Omega}=\frac{8\pi}{3}\bigg(\frac{e^2}{4\pi\epsilon_0mc^2}\bigg)^2\frac{(1+\cos^2\theta)}{\lambda^{4}}$$ where $\theta$ is scattering angle.
This means that the small wavelength components of light are strongly scattered than the large wavelength components. Thus the white light coming from the sun will suffer more scattering by the atmospheric scatterers in the blue end of the spectrum than the red end. Therefore, when we look at the sky, it appears blue because the scattered light is rich in blue. Here, the conventional explanation stops but it seems to me to be incomplete. Here is why:
According to the explanation above, the blue light is scattered away from the observer. But then blue light is not reaching the eyes of the observer. Then why should we see the sky as blue?