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Introduction to Charged-Particle Detectors

Alpha Resolution

Alpha resolution is specified as the maximum peak width for a standard alpha source measured at one-half the peak height (FWHM) expressed in keV. The total system alpha resolution is measured and warranted for 5.486-MeV alphas from 241Am with an ORTEC preamplifier chosen to be consistent with the detector capacitance and an ORTEC amplifier using equal differential and integral time constants as follows:

0.5 µs for A, B, C, F, L, and R Series;

1.0 µs for ULTRA, ULTRA-AS, and ULTRA CAM;

2.0 µs for P Series.

For totally depleted B Series detectors with £500-µm thicknesses, the alpha resolution is measured through the exit (low-field strength) contact, and >500-µm detectors measured with alpha particles through the front contact. The D and F Series are not warranted for alpha resolution but are warranted for system noise with suitable ORTEC electronics. Unless specified otherwise, resolution measurements are performed and warranted at 21 ±1°C.

Beta Resolution (System Noise)

The system noise width guaranteed maximum FWHM (which approximates beta resolution) is listed for each type of detector. Unless specified otherwise, measurements are performed and warranted at 21 ±1°C.

Electrons (beta particles) are, to a first approximation, sufficiently light to cause zero energy loss in the entrance window of silicon detectors. The beta energy resolution of silicon detectors is thus determined by the electronic noise of the detector and preamplifier; hence, the interchangeable "beta resolution/system noise" terminology.

Discriminator Threshold Setting

When silicon detectors are used as beta spectrometers, the threshold of the lower-level discriminator in the electronics must be set at 2.5 times the "beta resolution" to avoid spurious noise counts. Because the specific ionization of electrons is very low (e.g., 0.35 keV/µm for minimum ionizing betas), it is often necessary to cool silicon detectors used as beta spectrometers. (Detectors with cryogenic epoxy must be special-ordered.) When this is done, the electronic noise caused by the detector leakage current is eliminated and the detector becomes equivalent to a pure capacitor. The electronic noise of the system can then be easily calculated from the noise vs. capacitance characteristics of the preamplifier.