Laser lines

Figure 9.3 Doppler limited laser line with twelve axial modes within the line width...

Infrared laser lines involving. .. 2p 5s —. .. 2p 4p transitions in the 3.39 pm region are not particularly usefiil. However, they do cause some problems in a 632.8 nm laser because they deplete the populations of the. ., 2p 5s states and decrease the 632.8 nm intensity. The 3.39 pm transitions are suppressed by using multilayer cavity mirrors designed specifically for the 632.8 nm wavelength or by placing a prism in the cavity orientated so as to deflect the infrared radiation out of the cavity. 

This reaction has been carried out with a carbon dioxide laser line tuned to the wavelength of 10.61 p.m, which corresponds to the spacing of the lowest few states of the SF ladder. The laser is a high power TEA laser with pulse duration around 100 ns, so that there is no time for energy transfer by coUisions. This example shows the potential for breakup of individual molecules by a tuned laser. As with other laser chemistry, there is interest in driving the dissociation reaction in selected directions, to produce breakup in specific controllable reaction channels. 

As illustrated in Figure 4, the model is created on a platform submerged in a bath that is mounted on a turntable and contains a suitable monomer including a photoinitiator responsive to a laser line. The laser is modulated by the design computer and scaimed radially while the turntable rotates to write... 

Figure 6-21. Site-selective fluorescence measurements of a T thin film. Starting from the top spectrum the excitation energies were at 17860. 17700, 17390, 17240, 17095, and 16950 cur, respectively. The reminiscence of the exciting laser lines is shown by the sharp peak on the left.

A list of the principal laser lines useful as Raman excitation source is... 

The choice of a photomultiplier tube is dependent partly on the choice of the laser line. It is also based on two characteristics ... 

Transmissions of the Cary 82 Fitter and Conventional Interference Fillers for Typical Laser Lines... 

Fig. 3 a UV-Vis DRS spectra of dehydrated TS-1 catalyst reporting the typical 208 nm (48000cm i) LMCT hand, see Fig. 2h also reported are the four excitation laser lines used in this Raman study near-lR (dotted), visible (full), near-UV (dashed) and far-UV (dot-dashed), b Raman spectra of dehydrated TS-1 obtained with four different lasers emitting at 7 = 1064,422,325, and 244 nm (dotted, full, dashed, and dot-dashed lines, respectively). Raman spectra have been vertically shifted for clarity. Although the intensity of each spectrum depends upon different factors, the evolution of the 7(1125)//(960) ratio by changing the laser source is remarkable. The inset reports the Raman spectrum collected with the 244 nm laser in its full scale, in order to appreciate the intensity of the 1125 cm enhanced mode. Adapted from [48] with permission. Copyright (2003) by The Owner Societies 2003... 

Thus, the region 2100-1830 cm 1 can be covered. This allows us to monitor CO(v,J) by resonance absorption and various M(CO)n [n = 3-6] as a result of near coincidences between the CO laser lines and the carbonyl stretching vibrations of these species. The temporal response of the detection system is ca. 100 ns and is limited by the risetime of the InSb detector. Detection limits are approximately 10 5 torr for CO and M(CO)n. The principal limitation of our instrumentation is associated with the use of a molecular, gas discharge laser as an infrared source. The CO laser is line tuneable laser lines have widths of ca. lO cm 1 and are spaced 3-4 cm 1 apart. Thus, spectra can only be recorded point-by-point, with an effective resolution of ca. 4 cm 1. As a result, band maxima (e.g. in the carbonyl stretching... 

Fluorescein is excited at 494 nm, which fits to the argon-ion laser line at 488 nm, a very convenient feature for many microscopy experiments. It emits at 520 nm and the emission band is far from being sharp. The broad fluorescence emission spectrum varies with pH [18]. The advantageous photochemical properties of fluorescein are its high absorption (emax = 79,000M-1cm-1) and quantum... 

Note that parameters ft and 5 depend on signal amplifications in the utilized detectors and on the elements in the optical path (optical filter, spectral detection bands) only, while a and y are additionally influenced by relative excitation intensity. This is usually a fixed constant in wide-field microscopy but in confocal imaging laser line intensities are adjusted independently. Furthermore, note that the a factor equals 5 multiplied by y (see Appendix for further detail). 

Several other approaches to solve the quantitation problem have been proposed. Hoppe et al. [2] determined y/ by calibrating it against constructs with known FRET efficiency. We and others [3, 6] have used data from a cell before and after acceptor photobleaching to relate the FRET-induced sensitized emission in the S channel to the loss of donor emission in the D channel by factors termed or G, respectively. For the CFP/YFP pair this works very well on confocal microscopes with a 514-nm Argon ion laser line, but on wide-held systems, selective acceptor photobleaching reportedly causes problems [ 14]. F inally, G can also be determined by comparison of several constructs that differ in FRET efficiency, a bit analogous to the Yellow Cameleon calibration described above [10,14],... 

Because on CCD setups excitation for D, S, and A images is usually filter-selected from a single white light source the relative intensity of excitation is approximately fixed. Confocal microscopes use separate laser lines, often from distinct lasers, that can (and for optimal imaging should) be independently adjusted. Thus, on CCD setups y (Eq. (7.6)) is constant for a given set of filters whereas on the confocal, it varies from image to image (also, see Sect. 7.4.2). 

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