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Photo-ionisation

Atmospheric pressure ionisation Atmospheric pressure MALDI Atmospheric pressure photo-ionisation Atmospheric pressure spray ionisation... [Pg.751]

Figure 2.2. An energy level diagram illustrating photo-ionisation of an atom by removal of a K-shell electron. The Fermi level represents zero of the binding energy and the vacuum level represents zero... Figure 2.2. An energy level diagram illustrating photo-ionisation of an atom by removal of a K-shell electron. The Fermi level represents zero of the binding energy and the vacuum level represents zero...
A common method of calculating the approximate photo-ionisation cross-sections is to use the Gelius intensity model [79]. Here the cross-section for a particular orbital, , is expressed in terms of atomic contributions based on population analysis. [Pg.706]

Our intention is not to calculate absolute values for photo-ionisation cross-sections, but rather to relate the cross-sections for the different states which may result from ionising the same orbital shell r. Thus we require a formula of the kind ... [Pg.61]

The photoelectron intensity for a given element A is determined by the product of this element s concentration level and its effective photo-ionisation cross section (for the orbital under consideration) For this element, the number of photoelectrons emitted is thus proportional to A fraction T of these electrons is effectively transmitted to the... [Pg.100]

Figure 8 Absorption spectra of the electron at different delays after photo-ionisation of liquid water at 21 °C (from [26]). The solvation process is very fast as the hydrated electron (A ax = 720 nm) is observed within / ps from precursors absorbing in the infrared domain (A > 1200 nm). Figure 8 Absorption spectra of the electron at different delays after photo-ionisation of liquid water at 21 °C (from [26]). The solvation process is very fast as the hydrated electron (A ax = 720 nm) is observed within / ps from precursors absorbing in the infrared domain (A > 1200 nm).
Ne recently studied the formation of the solvated electron in pure ethane-1,2-diol by photo-ionisation of the solvent [18,32]. The results showed that the excess electron presents a wide absorption band in the visible and near-IR domains at short delay times after the pump pulse, and that the red part ofthe absorption band drops rapidly in the first few picoseconds while the blue part increases slightly (Fig. 9). The time resolved spectra were fitted correctly by either one of two solvation models a stepwise mechanism involving several distinct species and a continuous relaxation model. In Figure 10 are reported, as an example, the kinetics and spectra of the three successive species (the weakly bound the strongly bound e and the solvated electron e/) involved in the electron solvation dynamics according to the stepwise model. [Pg.48]

Keen visual observation is the most important task during a site reconnaissance. Flowever, some basic in-held chemical testing equipment is useful. Commercial kits are available, mainly based on colorimetric reactions. These kits can be used to check for the presence or absence of common contaminants and to measure soil pH. However, the results obtained using these test kits should only be regarded as qualitative, not least because samples taken at the surface may not represent the bulk of materials on the site. For site reconnaissance, the use of in-held instrumental testing is not justihed. An exception is hand-held equipment to test for the presence of gaseous and volatile contamination—photo-ionisation and other detectors are useful where such contaminants are anticipated. While a Phase la study does not normally include intrusive investigation, a small number of samples may be taken for laboratory analysis. These can be important when waste and other potentially contaminated materials of unknown composition have been spread, deposited or are stored on the site. [Pg.49]

Hoffmann analytes in inhaled and exhaled cigarette smoke (mouthspace) by photo ionisation time-of-flight mass spectrometry. [Pg.1011]

Streibel, T., C. Mocker, M. Sklorz, T. Adam, S. Mitschke, and R. Zimmermaim Real-time on-line characterization of selected Hoffmann analytes in inhaled and exhaled cigarette smoke (mouthspace) by photo ionisation time-of-flight mass spectrometry 60th Tobacco Science Research Conference, Program Booklet and Abstracts, Vol. 60, Paper No. 71, 2006, pp. 58-59. [Pg.1468]

As GC techniques became more refined and were generally accepted, due to the superior separation and resolution potential of modern capillary columns, they took preference, especially in the analysis of PAH in car exhaust emissions and air particulates. In combination with an FID-detector, which, in contrast to the UV-detectors used frequently in HPLC analysis, has a nearly uniform response factor for hydrocarbons, or coupled to mass spectrometry, this technique must now be considered the method of first choice for a reliable and reproducible determination of PAH traces in a wide range of matrices. The introduction of more sensitive (photo-ionisation detector - PID) and specific detectors, such as the nitrogen-phosphorus (NPD)... [Pg.133]

Figure 8 Positive ion mass spectra taken from sinapinic acid using primary ion beam sputtering and laser postionization with 15 ns (A) and 500 fs (B) pulses of A = 248nm. (Reprinted from Mdllers R, Terhorst M, Niehuis E, and Benninghoven A (1992) Resonant photo-ionisation of sputtered organic molecules by femtosecond LIV laser pulses. Organic Mass Spectrometry 27 1393-1395.)... Figure 8 Positive ion mass spectra taken from sinapinic acid using primary ion beam sputtering and laser postionization with 15 ns (A) and 500 fs (B) pulses of A = 248nm. (Reprinted from Mdllers R, Terhorst M, Niehuis E, and Benninghoven A (1992) Resonant photo-ionisation of sputtered organic molecules by femtosecond LIV laser pulses. Organic Mass Spectrometry 27 1393-1395.)...
Muller-Dethlefs K, Sander M, SchlagEW. 1984. 2-colour photo-ionisation resonance spectroscopy of NO -complete separation of rotational levels of NO at the ionisation threshold . Chem. Phys. Lett. 112(4) 291-294. [Pg.473]

J.H. Scofield, Hartree-Slater subshell photo-ionisation cross-sections at 1254 and 1487eV, J. Electr. Spectr. Relat. Hienom. 8 (1976) 129-137. [Pg.367]

Very short wavelength solar radiation, EUV 80 < A < 103 nm and X-rays 1-10 nm, causes photo-ionisation (see Table 5.3), but is rapidly attenuated restricting ionisation to z > 60 km a region which is therefore also known as the ionosphere (but it encompasses both the thermosphere and part of the mesosphere, see Fig. 5.4). [Pg.226]

There are no specific selection rules for such a photo-ionisation process. The kinetic energy KE) of the ejected electrons can be expressed as follows ... [Pg.412]

Lanthanum hexaboride (LaBe) thin films exposed to air show reasonable work function values that makes them suitable for photoelectron applications that finally may employ LED instead of discharge lamps. Various thin films are investigated and compared with ceramic references. The low work function values associated with a moderate surface reoxidation of the films which, of course sets some limits for thin film processing in MEMS systems. As an example for the apphcations feasible a nano ioniser suitable for ambient conditions is presented, which exceeds the actual physical limits and parameterisation of conventional photo ionisation detectors. [Pg.321]


See other pages where Photo-ionisation is mentioned: [Pg.300]    [Pg.705]    [Pg.159]    [Pg.159]    [Pg.82]    [Pg.283]    [Pg.10]    [Pg.36]    [Pg.87]    [Pg.356]    [Pg.180]    [Pg.184]    [Pg.61]    [Pg.602]    [Pg.487]    [Pg.49]    [Pg.768]    [Pg.259]    [Pg.265]    [Pg.36]    [Pg.217]    [Pg.283]    [Pg.63]    [Pg.322]    [Pg.327]   
See also in sourсe #XX -- [ Pg.47 ]




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Atmospheric pressure photo ionisation

Ionisation

Ionised

Photo ionisation detector

Photo-ionisation detector (PID)

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