Twenty of the K Auger lines of silver have been resolved and estimates of their relative intensities obtained. Comparison with the theoretical intensities calculated by Burhop indicates that the existing theory is not quantitatively correct and that relativistic modifications offer little hope of improvement. Special attention is directed to the K → LL lines where disagreement with theory is most marked. Comparison with similar observations previously reported for gold and bismuth shows an interesting agreement in the observed ratio of the intensity of the K → LIILIII line to that of the K → LIIILIII line, and in the ratio of the intensity of the K → LILIII line to that of the K → LILI line.