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Gertsenshtein gives a clear equation describing the ratio of electromagnetic energy to gravitational waves. The relationship is used to calculate the amplitude of the gravitational wave (Gertsenshtein, 1962)  \begin{equation}  \frac{a(x)}{b} = \sqrt{\frac{\gamma}{\pi c^3}F^{(0)2} c^3} F^{(0)2}  R_{0} T}}, T},  \end{equation}  where $F$ represents electromagnetic energy in gauss, $R_{0}$ represents the distance from the EM source in meters, and $T$ is the time allotted for gravitational radiation in years.