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Counting dead time

Scattered radiation. In a transmission experiment, the Mossbauer sample emits a substantial amount of scattered radiation, originating from XRF and Compton scattering, but also y-radiation emitted by the Mossbauer nuclei upon de-excitation of the excited state after resonant absorption. Since scattering occurs in 4ti solid angle, the y-detector should not be positioned too close to the absorber so as not to collect too much of this unwanted scattered radiation. The corresponding pulses may not only uimecessarily overload the detector and increase the counting dead time, but they may also affect the y-discrimination in the SCA and increase the nonresonant background noise. [Pg.45]

Since the TDC is a time counting device, when two or more ions arrive at the detector simultaneously in one flight cycle, the system counts them as one ion. In the same way, when two ions arrive at the detector in sequence within a certain interval, the system does not count the latter ion because the TDC is unable to register another count during the period after each ion event (counting dead time). Consequently, the dynamic range of this... [Pg.185]

Dead time of the counters gives rise to loss of counts. The radiations coming in the detector are not counted during the dead time after a radiation is counted. Dead time can give rise to a serious error in the case of GM counter as described below. [Pg.1767]

Wire Pos. Wait Time Counts Dead Time Correction Bkgd. Net Counts Correct Counts A/Ao... [Pg.167]

Optimum resolution, i. e. low full width at half-maximum (FWHM), is a trade-off between high count rate, i. e. low dead-time, and good spectral resolution. [Pg.187]

The cause of this difficulty therefore resides within the counter itself. The difficulty is described by saying that the Geiger counter has a dead time, by which is meant the time interval after a pulse during which the counter cannot respond to a later pulse. This interval, which is usually well below 0.5 millisecond, limits the useful maximum counting rate of the detector. The cause of the dead time is the slowness with which the positive-ion space charge (2.5) leaves the central wire under the influence of the electric field. This reduction in observed counting rate is known as the coincidence loss. [Pg.52]

Integral intensities were obtained after dead-time corrections, background subtraction and normalization to averaged monitor counts. The Lp correction was applied in the usual way. Since the polarization ratio was not measured at BW5 so far, 90% linear horizontally polarized radiation was assumed for all scans. Calculations show that even a change in the beam polarization of 10% would effect the intensities of the highest order reflections of less than 1.5%. [Pg.221]

To determine the expressions for the optimised counting times, we write the expressions (10) and (11) in terms of count-rates and times (count rates are constant quantities for each Bragg reflection). We assume that the incident neutron flux is constant during a flipping ratio measurement, and that no dead-time correction is needed. In these conditions, we have the relations ... [Pg.251]

Importantly, the dead-time of TACs and TDCs is comparatively long, typically 125-350 ns. When a photon arrives within this time interval after the detection of a photon, it will not be observed. Therefore, care must be taken that the count rate of the experiment is sufficiently low to prevent this pulse-pileup. TACs and TDCs usually operate in reversed start-stop geometry. Here, the TAC is started by the fluorescence signal and stopped by the laser trigger. [Pg.112]

In time-gated photon counting, comparatively high photon count rates can be employed count rates as high as 10 MHz are often used. TG has the advantage of virtually no dead-time of the detection electronics ( 1 ns), whereas the dead-time of the TCSPC electronics is usually on the order of 125-350 ns. This causes loss of detected photons, and a reduced actual photon economy of TCSPC at high count rates. [Pg.119]

At low count rates Q -C l/td, the detection sensitivity is not affected by the dead-time (/= 1). However, at a count rate of Q = l/td the detection sensitivity is reduced to 50% of its sensitivity at low count rates, see Fig. 3.7. Typical values for dead-times of PMTs are on the order of 50-100 ns. [Pg.121]

Not only PMTs and other detectors such as avalanche photodiodes suffer from dead-time effects also the detection electronics may have significant dead-times. Typical dead-times of TCSPC electronics are in the range 125-350 ns. This may seriously impair the efficiency of detection at high count rates. The dead-time effects of the electronics in time-gated single photon detection are usually negligible. [Pg.121]

Fig. 3.7. The detection efficiency of a system with a dead-time 350 ns as a function of the incident count rate. At high count rates the detection efficiency reduces due to pileup effects. Fig. 3.7. The detection efficiency of a system with a dead-time 350 ns as a function of the incident count rate. At high count rates the detection efficiency reduces due to pileup effects.
E represents the combined collection and detection efficiency of the system and F the intrinsic photon-economy of the technique. The factor 77 accounts for the subtractive noise, tA is the dead-time of the detector and Q the count rate of the system. [Pg.128]

A common cause of inaccuracy in SPC-based time domain detection is pulse-pileup, that is, the arrival of photons during the dead-time of the detection system. Because the higher probability of emission (and detection) in the earlier part of the decay, pulse-pileup is more probable in this part of the decay. Consequently, the decay will be distorted and the lifetime will be biased towards higher values. Moreover, pulse-pileup will also result in a reduction of the detection efficiency (see Fig. 3.7 and Eq. (3.4)). Therefore, care should be taken to avoid excitation rates too close to the efficacy count rate (i.e., the inverse of the dead-time) in order to minimize these effects. [Pg.131]

SPC techniques offer the advantage of low noise detection, providing / -values of 1-2 times lower than in analog detection. Although this can in principle result in four times faster acquisition speed this gain in speed is not realized in practice. In SPC, the comparatively high dead-times of detectors and electronics limits the acquisition speed. SPC system should be operated at count rates below the inverse of the dead-time of the system (electronics... [Pg.134]

An important feature of all gas ionization detectors is their dead or paralysis time, which has a direct bearing on their utility. Once initiated a voltage pulse takes several hundred microseconds to die away, and may be prolonged by the discharge of secondary electrons from the cathode as the argon ions are reduced. Until this first pulse is terminated the tube is dead to further radiations and the recorded count CM will be less than the true count CT. The relation between the two values will depend upon the length of the dead time t... [Pg.459]

Lost counts correction is necessary because Geiger-Muller tubes have a dead-time in their operation. [Pg.203]

Dead time considerations in the alpha particle detection limit the count rate, and hence limit the neutron flux that can be used with this approach. This means that large scan times will probably be required with most implementations of this approach. [Pg.76]

Also important is the effect of detector dead time. When ions are detected using a pulse counting (PC) detector, the resultant electronic pulses are approximately 10 ns long. During and after each pulse there is a period of time during which the detector is effectively dead (i.e. it cannot detect any ions). The dead time is made up of the time for each pulse and recovery time for the detector and associated electronics. Typical dead times vary between 20 and 100 ns. If dead time is not taken into account there will be an apparent reduction in the number of pulses at high count rates, which would cause an inaccuracy in the measurement of isotope ratios when abundances differ markedly. However, a correction can be applied as follows ... [Pg.132]

If no dead time correction is applied, then a linear calibration would not be possible, since the higher count rates between 10 and 10 Hz would be underestimated. This provides a way of determining the dead time empirically, i.e. by re-integrating the isotopic signals with different dead times until a linear calibration is obtained for a series of accurately known standards. [Pg.133]


See other pages where Counting dead time is mentioned: [Pg.379]    [Pg.327]    [Pg.379]    [Pg.327]    [Pg.1433]    [Pg.401]    [Pg.124]    [Pg.182]    [Pg.188]    [Pg.53]    [Pg.37]    [Pg.248]    [Pg.74]    [Pg.113]    [Pg.121]    [Pg.122]    [Pg.103]    [Pg.459]    [Pg.84]    [Pg.210]    [Pg.46]    [Pg.47]    [Pg.293]    [Pg.133]    [Pg.133]    [Pg.133]    [Pg.530]    [Pg.63]    [Pg.128]    [Pg.105]   
See also in sourсe #XX -- [ Pg.185 ]




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