The Larmor precession frequency ($\omega$) is directly proportional to the magnetic field strength ($B$). For Earth's magnetic field, approximated as a dipole, the field strength at a magnetic latitude ($\lambda$) is given by the formula:
$B(\lambda) = B_0 \sqrt{1 + 3 \sin^2\lambda}$
where $B_0$ is the magnetic field strength at the magnetic equator ($\lambda=0^\circ$).
We need to find the ratio of the Larmor frequencies at magnetic latitudes $\lambda_1 = 30^\circ$ and $\lambda_2 = 60^\circ$. This ratio is equivalent to the ratio of the magnetic field strengths at these latitudes.
The ratio of the Larmor precession frequencies is the ratio of the magnetic field strengths:
$\frac{\omega_1}{\omega_2} = \frac{B(30^\circ)}{B(60^\circ)} = \frac{B_0 \sqrt{\frac{7}{4}}}{B_0 \sqrt{\frac{13}{4}}}$
Simplifying the expression:
$\frac{\omega_1}{\omega_2} = \frac{\sqrt{\frac{7}{4}}}{\sqrt{\frac{13}{4}}} = \sqrt{\frac{7/4}{13/4}} = \sqrt{\frac{7}{13}}$
Therefore, the ratio is $\sqrt{7} : \sqrt{13}$.
The following magnetic anomaly (in total field) is recorded along a south to north profile across a body that can be equated to a single pole.
Consider the following statements
Statement I: The surveyed area is close to the magnetic equator
Statement II: The pole lies below the distance coordinate 200 m