The transition of electron that gives rise to the formation of the second spectral line of the Balmer series in the spectrum of hydrogen atom corresponds to:
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For the Balmer series, transitions end at $n_f = 2$. The spectral lines are numbered based on the value of $n_i$ (e.g., $n_i = 3$ for the first line, $n_i = 4$ for the second line).
The Balmer series corresponds to transitions where the final energy level is $n_f = 2$. The second spectral line occurs when the transition happens from $n_i = 4$ to $n_f = 2$.
Using the formula for the wavelength of emitted radiation:
\[
\frac{1}{\lambda} = R_H \left( \frac{1}{n_f^2} - \frac{1}{n_i^2} \right),
\]
where:
\begin{itemize}
\item $R_H$ is the Rydberg constant,
\item $n_f = 2$ and $n_i = 4$ for the second spectral line.
\end{itemize}
Substitute $n_f = 2$ and $n_i = 4$ into the equation:
\[
\frac{1}{\lambda} = R_H \left( \frac{1}{2^2} - \frac{1}{4^2} \right) = R_H \left( \frac{1}{4} - \frac{1}{16} \right).
\]
Simplify:
\[
\frac{1}{\lambda} = R_H \cdot \frac{4 - 1}{16} = R_H \cdot \frac{3}{16}.
\]
Thus, the correct transition for the second line in the Balmer series is:
\[
\boxed{n_f = 2 \text{ and } n_i = 4}.
\]