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Atomic spectra advantages

Figure 6.3 Schematic representation of the resolution advantages of 3D NMR spectroscopy, (a) Both pairs of protons have the same resonance frequency, (b) Due to the same resonance frequency, both pairs exhibit overlapping crosspeaks in the 2D NOESY spectrum, (c) When the frequency of the carbon atoms is plotted as the third dimension, the problem of overlapping is solved, since their resonance frequencies are different. The NOESY cross-peaks are thus distributed in different planes. Figure 6.3 Schematic representation of the resolution advantages of 3D NMR spectroscopy, (a) Both pairs of protons have the same resonance frequency, (b) Due to the same resonance frequency, both pairs exhibit overlapping crosspeaks in the 2D NOESY spectrum, (c) When the frequency of the carbon atoms is plotted as the third dimension, the problem of overlapping is solved, since their resonance frequencies are different. The NOESY cross-peaks are thus distributed in different planes.
The example is typical for many applications of Mossbauer spectroscopy in catalysis a catalyst undergoes a certain treatment, then its Mossbauer spectrum is measured in situ at room temperature. Flowever, if the catalyst contains highly dispersed particles, the measurement of spectra at cryogenic temperatures becomes advantageous as the recoil-free fraction of surface atoms increases substantially at temperatures below 300 K. Secondly, spectra of small particles that behave superparamagne-... [Pg.149]

The ro-vibronic spectrum of molecules and the electronic transitions in atoms are only part of the whole story of transitions used in astronomy. Whenever there is a separation between energy levels within a particular target atom or molecule there is always a photon energy that corresponds to this energy separation and hence a probability of a transition. Astronomy has an additional advantage in that selection rules never completely forbid a transition, they just make it very unlikely. In the laboratory the transition has to occur during the timescale of the experiment, whereas in space the transition has to have occurred within the last 15 Gyr and as such can be almost forbidden. Astronomers have identified exotic transitions deep within molecules or atoms to assist in their identification and we are going to look at some of the important ones, the first of which is the maser. [Pg.77]

Solid-state NMR spectroscopy has not found as wide an application in soils as it has in other fields. The great advantage of NMR is that it is specific for specific elements that is, it is tuned to a specific element and other elements are not detected. NMR spectroscopy shows the environment or multiple environments in which a particular element exists. For example, in a proton NMR spectrum, primary, secondary, and tertiary protons can be differentiated, as can protons attached to oxygen, nitrogen, and other atoms. [Pg.179]

An NMR spectrum shows the types of environment around the nuclei (atoms) and the ratios of these nuclei. Compared with X-ray crystallography, NMR has the advantage of being carried out in concentrated solutions rather than requiring crystal samples. The solution states are more representative of the native environment of receptor proteins. NMR can be used to study ligand-receptor interactions. A receptor protein is labeled with isotopes such as or N, and changes in their spectra when bound with ligands can be monitored. [Pg.65]


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