Step 1: Understanding the critical velocity formula.
The critical velocity \( v \) of a satellite in circular orbit is given by the formula:
\[
v = \sqrt{\frac{GM}{R}}
\]
where \( G \) is the gravitational constant, \( M \) is the mass of the earth, and \( R \) is the radius of the orbit.
Step 2: Using the formula to find the ratio of velocities.
For satellites \( A \) and \( B \), the critical velocities are given by:
\[
v_A = \sqrt{\frac{GM}{R}} \quad \text{and} \quad v_B = \sqrt{\frac{GM}{2R}}
\]
Taking the ratio \( \frac{v_A}{v_B} \), we get:
\[
\frac{v_A}{v_B} = \frac{\sqrt{\frac{GM}{R}}}{\sqrt{\frac{GM}{2R}}} = \sqrt{2}
\]
Step 3: Conclusion.
Thus, the ratio of \( v_A \) to \( v_B \) is \( \sqrt{2} : 1 \), which corresponds to option (B).