THE development of Geiger-Müller counters to a state of good reliability has provided a new order of sensitivity and facility with which weak sources of gamma rays and x-rays can be detected and measured.Combined with extraordinary sensitivity, counters are rugged, stable, simple to operate, and the results of measurements made with them lend themselves to easy interpretation. Geiger-Müller tube counters are not particularly new instruments. They were invented in 1928 by Professor H. Geiger and W. Müller,1 as an outgrowth and great improvement of the Geiger counter, or point counter, which had been in use for many years for counting alpha particles. Since their invention, tube counters have been adapted to a large variety of uses in physical laboratories. They have, indeed, become one of the physicist's most powerful tools for measuring weak radiations. Three general types are now in use: (1) gamma-ray counters, suitable for measuring gamma rays, x-rays, and cosmic rays; (2) photo-electric quantum counters, which combine the characteristics of photo-cells and counters, and are used for measuring weak ultra-violet light, and (3) particle counters, for measurements of alpha, beta, and H particles. Of these forms, there are various mechanical modifications, made to meet the requirements of particular problems.2 The present paper deals with counters of the first type, which we have used for locating radium and for making gamma-ray measurements during the last two years. I. Construction and Principle of Operation of Counters A counter apparatus consists of: the counting tube (counter), an amplifier, usually employing radio tubes, a recording device for registering the number of discharges of the counter, and a suitable source of (negative) high voltage for the counting tube. The negative voltage is usually between 500 and 1,500 volts, depending on the kind of counter used. The principle of operation of a GeigerMüller counter (G-M counter) is explained by reference to Figure 1. A wire, W, is stretched along the axis of a hollow metal cylinder, F, enclosed in a glass tube. After suitable treatment of the. electrode surfaces, the tube is filled with a suitable gas, usually at about 1/10 atmospheric pressure, and sealed off. A negative voltage, V, is applied to the cylinder-electrode (cathode); the wire (anode) is connected through a small condenser, C, to a vacuumtube amplifier, A (or a string electrometer), and through a high resistance, R, to ground. The value of V is adjusted so that it is nearly enough to cause a brush discharge between the electrodes. When in this sensitive state, any ray, Q, passing through the tube and liberating one or more ions in F, initiates a small gas discharge between the electrodes.