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Detectors quadratic

Fig. 3.17 Leftlbottom Picture of the drive (cylindrical piece length 40 nun diameter 22 nun) and its control unit (quadratic box holding the cylindrical drive unit) this whole unit slides into the detector system unit (top part in the left picture) Right Transfer function of MIMOS II velocity transducer (see also Sect. 3.1.1). For details of the drive unit and the model describing its behavior see [36, 45]... Fig. 3.17 Leftlbottom Picture of the drive (cylindrical piece length 40 nun diameter 22 nun) and its control unit (quadratic box holding the cylindrical drive unit) this whole unit slides into the detector system unit (top part in the left picture) Right Transfer function of MIMOS II velocity transducer (see also Sect. 3.1.1). For details of the drive unit and the model describing its behavior see [36, 45]...
Tables 6.27 and 6.31 show the main characteristics of ToF-MS. ToF-MS shows an optimum combination of resolution and sensitivity. ToF-MS instruments provide up to 40000 spectra s-1, a mass range exceeding 100000 (in principle unlimited), a resolution of 5000, and peak widths as short as 200 ms. This is better than quadruples and most ion traps can handle. Unlike the quadrupole-type instrument, the detector is detecting every introduced ion (high duty factor). This leads to a 20- to 100-times increase in sensitivity, compared to QMS used in scan mode. The mass range increases quadratically with the time range that is recorded. Only the ion source and detector impose the limits on the mass range. Mass accuracy in ToF-MS is sufficient to gain access to the elemental composition of a molecule. A single point is sufficient for the mass calibration of the instrument. ToF mass spectra are commonly calibrated using two known species, aluminium (27 Da) and coronene (300 Da). ToF is well established in combination with quite different ion sources like in SIMS, MALDI and ESI. Tables 6.27 and 6.31 show the main characteristics of ToF-MS. ToF-MS shows an optimum combination of resolution and sensitivity. ToF-MS instruments provide up to 40000 spectra s-1, a mass range exceeding 100000 (in principle unlimited), a resolution of 5000, and peak widths as short as 200 ms. This is better than quadruples and most ion traps can handle. Unlike the quadrupole-type instrument, the detector is detecting every introduced ion (high duty factor). This leads to a 20- to 100-times increase in sensitivity, compared to QMS used in scan mode. The mass range increases quadratically with the time range that is recorded. Only the ion source and detector impose the limits on the mass range. Mass accuracy in ToF-MS is sufficient to gain access to the elemental composition of a molecule. A single point is sufficient for the mass calibration of the instrument. ToF mass spectra are commonly calibrated using two known species, aluminium (27 Da) and coronene (300 Da). ToF is well established in combination with quite different ion sources like in SIMS, MALDI and ESI.
From a practical point of view this definition can be interpreted as being imposed by the linear boundary of the calibration curve (quadratic behavior) due to saturation of the detector or/and ion suppression effect and/or contamination for low-level samples (carryover) (see Section 8.3.7). [Pg.117]

If severe nonlinearities might be present, the linear inner relation can be modified to a quadratic or cubic one. This strong nonlinear situation might arise whenever problems occur on the detector or monochromator, malfunction of the automatic sampler in ETAAS, strong influence of the concomitants on the signal, when the linear range for the analyte is too short or when LIBS, LA-ICP-MS measurements or isotope dilution are carried out (see Chapter 1 for more possibilities). [Pg.191]

The non-linear calibration models are also acceptable. Figure 4.6 shows an example of a non-linear calibration approximated with a quadratic fit. Non-linear calibration curves are not acceptable if used to compensate for the detector saturation at a high concentration level. [Pg.244]

The intensity of the thiolanes-thiols C28-C30 on the FPD trace is exagerated because of the two sulfur atoms carried by thiolane-thiols and because of the quadratic response of the FPD detector. The mass-spectra of the C30 thiolane-thiol, displays the fragments m/z 55 (100%), m/z 87 (62%) the typical thiolane ring, a fragment m/z 451 (17%) which corresponds to the C30 thiolane, and a molecular ion M+ 484 (60%) which could be result of the adjonction of a thiol (S-H) to the C30 thiolane. The molecules eluting in doublets with the thiolane-thiols are not identified. The C20 thiophenic isoprenoids are also present, with the compound I dominating. [Pg.186]

The subject of phase and phase retrieval with pulsed optical signals, although it is textbook material and involves well-known signal processing concepts [64, 65], has impacted on molecular spectroscopy only recently [66] through consideration of optical control experiments. As we shall see the phase is a consideration in heterodyne laser experiments because it influences the mixing of fields incident on a square-law detector. It is well known that a quadratic phase alters the spectrum, the time envelope and the time-frequency bandwidth of a pulse. Consider a pulse ... [Pg.8]

Chemiluminescence from S- or P-containing compounds is obtained by combustion in a hydrogen-rich flame. Both the excited HPO radicals formed and the Sj dimers can emit a chemiluminescence spectrum which allows the selective detection of S (eg, at 394 nm) and P (526 nm) using suitable filters and a photomultiplier tube for signal amplification [26]. This flame photometric detector shows a non-linear realtionship between concentration and output signal in the sulfur mode which in theory should be quadratic (owing to the dimer formation). However, in practive, exponential coefficients of between 1 and 2 are found. Electronic linearization of the output signal is therefore necessary. [Pg.138]

In practice the noise sets a limit to the number of individual PMTs that can be connected to a router. The cables connecting the PMTs to the router must be matched with 50 Ohm resistors. Even with a near-perfect summing amplifier, the noise from the matching resistors will be added to the output signal. Even worse is noise from the environment picked up by the detectors. While resistor noise adds quadratically, noise from the environment is more or less in phase for all detectors and therefore adds linearly. In practice, no more than eight individual PMTs are connected to one routing device. [Pg.32]

The peak absorption coefficient of OCS, 10 m", occurs at 462 GHz. This is by no means, however, the optimum working frequency due to the non-ideal behaviour of most MMW detectors. Commercial Schottky barrier mixer diode detectors show a quadratic roll-off in sensitivity at frequencies >100 GHz. If this is factored into Equation 6.1, the peak sample sensitivity occurs around 300 GHz, and the response is so flat that even at 100 GHz it has only fallen off by a factor of two. What is common to both curves is the dramatic fall-off in sample sensitivity at frequencies <100 GHz, reinforcing the point that the band 26-40 GHz is ill suited to high-sensitivity analytical spectroscopy. [Pg.91]


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See also in sourсe #XX -- [ Pg.7 , Pg.36 ]




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