For the production of characteristic K_{beta} | vedclass

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(C) Characteristic $X$-rays are produced when an electron from a higher energy shell transitions to a vacancy in an inner shell.For the $K$-series,the

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$n = 3$ to $n = 1$

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(C) Characteristic $X$-rays are produced when an electron from a higher energy shell transitions to a vacancy in an inner shell.For the $K$-series,the vacancy is in the $K$-shell $(n = 1)$.- The $K_{\alpha}$ $X$-ray is produced by a transition from the $L$-shell $(n = 2)$ to the $K$-shell $(n = 1)$.- The $K_{\beta}$ $X$-ray is produced by a transition from the $M$-shell $(n = 3)$ to the $K$-shell $(n = 1)$.- The $K_{\gamma}$ $X$-ray is produced by a transition from the $N$-shell $(n = 4)$ to the $K$-shell $(n = 1)$.Therefore,for the $K_{\beta}$ $X$-ray,the transition is from $n = 3$ to $n = 1$.

For the production of characteristic $K_{\beta}$ $X$-rays,the electron transition is:

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