In the hydrogen spectrum, the Lyman series limit corresponds to the transition from \( n = 2 \) to \( n = \infty \), and the Paschen series limit corresponds to the transition from \( n = 4 \) to \( n = \infty \). The wavelength of the spectral lines can be derived from the Rydberg formula:
\[
\frac{1}{\lambda} = R_H \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)
\]
Where \( R_H \) is the Rydberg constant, and \( n_1 \) and \( n_2 \) are the initial and final energy levels, respectively.
For the Lyman series limit (transition from \( n = 2 \) to \( n = \infty \)):
\[
\frac{1}{\lambda_L} = R_H \left( \frac{1}{2^2} - \frac{1}{\infty^2} \right) = R_H \left( \frac{1}{4} \right)
\]
For the Paschen series limit (transition from \( n = 4 \) to \( n = \infty \)):
\[
\frac{1}{\lambda_P} = R_H \left( \frac{1}{4^2} - \frac{1}{\infty^2} \right) = R_H \left( \frac{1}{16} \right)
\]
Now, the ratio of the wavelengths is:
\[
\frac{\lambda_L}{\lambda_P} = \frac{16}{4} = 4
\]
Thus, the ratio of the wavelengths of the Lyman series limit to the Paschen series limit is \( \frac{9}{9} \), which simplifies to \( 1 \).