Step 1: The formula for effective acceleration due to gravity at a latitude $\phi$ is:
\[ g_{\phi} = g_0 - \omega^2 R \cos^2 \phi \]
where $g_0$ is the acceleration due to gravity without rotation.
Step 2: At the equator, the latitude $\phi = 0^{\circ}$. Thus, the effective gravity $g$ is:
\[ g = g_0 - \omega^2 R \cos^2 0^{\circ} = g_0 - \omega^2 R \]
Step 3: At latitude $\phi = 30^{\circ}$, the effective gravity $g_{\phi}$ is:
\[ g_{\phi} = g_0 - \omega^2 R \cos^2 30^{\circ} \]
\[ g_{\phi} = g_0 - \omega^2 R \left( \frac{\sqrt{3{2} \right)^2 = g_0 - \frac{3}{4} \omega^2 R \]
Step 4: Find the absolute difference $|g - g_{\phi}|$:
\[ |g - g_{\phi}| = |(g_0 - \omega^2 R) - (g_0 - \frac{3}{4} \omega^2 R)| \]
\[ |g - g_{\phi}| = |-\omega^2 R + \frac{3}{4} \omega^2 R| = |-\frac{1}{4} \omega^2 R| = \frac{1}{4} \omega^2 R \]