To ascertain the minimum potential difference (V) necessary for observing the first line of the Balmer series, we begin with the energy levels of a hydrogen atom.
Step 1: Energy Level Formula
The energy of an electron in the \(n^{th}\) orbit is expressed as:
\[
E_n = -\frac{13.6}{n^2} \, \text{eV}
\]
Step 2: First Balmer Line Transition Identification
The Balmer series involves transitions terminating at \(n_f = 2\) and originating from \(n_i \geq 3\).
For the initial Balmer line:
\[
n_i = 3, \quad n_f = 2
\]
Step 3: Energy Difference Calculation
\[
\Delta E_{3 \to 2} = E_2 - E_3
\]
Substituting values:
\[
E_2 = -\frac{13.6}{2^2} = -3.4 \, \text{eV}, \quad E_3 = -\frac{13.6}{3^2} = -1.51 \, \text{eV}
\]
\[
\Delta E_{3 \to 2} = (-3.4) - (-1.51) = -1.89 \, \text{eV}
\]
Considering the energy difference as either emitted or absorbed energy, we take its magnitude:
\[
\Delta E_{3 \to 2} = 1.89 \, \text{eV}
\]
Step 4: Energy and Potential Difference Relationship
The energy provided by the potential difference must equate to this excitation energy:
\[
e V = 1.89 \, \text{eV}
\]
Step 5: Solving for the Given Potential Relationship
Given the potential difference as \( \frac{\alpha}{10} \, V \), we have:
\[
e \times \frac{\alpha}{10} = 1.89 \, \text{eV}
\]
\[
\Rightarrow \alpha = 18.9
\]
Step 6: Final Verification
This indicates that the potential difference required for the excitation is:
\[
V = \frac{\alpha}{10} = \frac{18.9}{10} = 1.89 \, \text{V}
\]
Final Answer:
\[
\boxed{\alpha = 18.9}
\]
Consequently, the minimum potential difference required to generate visible Balmer series lines in hydrogen is equivalent to an excitation energy of 1.89 eV, corresponding to \( \alpha = 18.9 \).