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Proton spectrum

The [Eu(dpm)3]-shifted n.m.r. spectra of (35) show almost complete separation [Pg.244]

The spectra are closely similar, indicating that (37) is a completely delocalized homoaromatic species, as is the case for (36), which is contrary to previous results which showed no such charge delocalization in (37) the role of anisotropic shielding effects is discussed. [Pg.245]

Three papers have been pubUshed concerning the employment of n.m.r. spectroscopy to probe conformational effects about the N— substituent bond in adducts of N-substituted maleimides with anthracene, cyclopentadiene, and 2-substituted anthracenes.  [Pg.245]

The resonances in the n.m.r. spectra of the bishomocubanone (40) and of its derivatives have been assigned on the basis of [Eu(fod)3] shift studies.The protons [Pg.245]

Spectra.—The relationships between chemical shifts and electronic structure [Pg.246]

NMR absorption spectra are characterized by the chemical shift of peaks and spin-spin splitting of peaks. Recall that the chemical shift is caused by the drifting, not orbiting or spinning, of nearby electrons under the influence of the applied magnetic field. It is therefore a constant depending on the applied field (i.e., if the field is constant, the chemical shift is constant). The chemical shift therefore identifies the functional group, such as methyl, methylene, aldehydic H, aromatics, and so on (see Table 3.3). All proton spectra shown have TMS as the reference, with the TMS absorbance set at 0.0 ppm. The smdent should note that all of the 300 MHz proton NMR spectra provided by Aldrich Chemical Company, Inc. also include the 75 MHz C spectmm at the top. C NMR spectra are discussed in Section 3.6.4. [Pg.161]

Spin-spin splitting is caused by adjacent nuclei and is transmitted through the bonds. It is independent of the applied field. The multiplicity is therefore a function of the number of equivalent H nuclei in the adjacent functional groups. Numerically, it is equal to (2 /- - 1), where n is the number of equivalent H and I is the spin number (in this case, 1= 1/2). For two adjacent groups the number is (2nl + l)(2n f + 1) where n and n are the numbers of H nuclei in each separate group and I and / each equal 1 /2. It can readily be seen from the real spectra we have already looked at and will look at, that the intensity ratios in multiplets are often not the symmetrical intensities predicted from Pascal s triangle. Look, for example, at the peak (a) triplet in Fig. 3.12(b) and (c). [Pg.161]

INADEQUATE incredible natural abundance double quantum transfer COSY correlated spectroscopy [Pg.162]

HETCOR heteronuclear chemical shift correlated experiment [Pg.162]

Multipulse sequence used to distinguish even and odd numbers of protons coupled to through one bond. Even numbers of bound protons give positive peaks odd numbers give negative peaks [Pg.162]

Tatemitsu, F. Ogura, Y. Nakagawa, M. Nakagawa, K. Naemura, and M. Nakazaki, Bull. Chem. Soc. [Pg.298]

In an interesting paper it is revealed that di-t-butylnitroxide (DTBN) radical induces upheld contact shifts for the X-H proton donor molecules and conforma-tionally dependent downfield shifts for C—H protons in accordance with the W-rule. Methyl protons in close spatial contact with the N-H or O-H proton donor groups exhibit marked DTBN-induced downfield pseudo-contact shifts. The origin of these effects and their potential uses are discussed. Proton shifts for various monoterpenes e.g. camphor, camphor quinone, and pinocarvone) in hexafiuorobenzene are compared with the shifts obtained in other, more conventional, solvents. Unusually large couplings between the OH and adjacent CH protons have been observed for extremely pure samples of syn- and anrt-7-hydroxynorbomene in particular solvents. The simplification in the spectra of these compounds, of 7-hydroxynor-bornadiene, and of the catalytically deuteriated (exo-addition) derivatives, with the aid of Eu(dpm)3 and Eu(fod)3 is reported in a companion communication.  [Pg.299]

The H n.m.r. spectra of the two diastereoisomeric trans-alcohols (18), and of (19) and (-)-myrtenol (20) have been assigned in Eu-induced shift studies, and pseudo-contact effects analysed. In a lanthanide-induced shift (LIS) study of various 7,7-disubstituted-endo- and -exo-norbornene anhydrides [21 X = Y = H X, Y = (CH2)2 X, Y = (CH2)4] the results suggest that the bridge substituents do not strongly perturb the anhydride-Eu(fod)3 interaction, and that complexation occurs on the [Pg.299]

Some LIS indices obtained in a study of the four isomeric 5-hydroxy-6-methyl-bicyclo [2,2,2] oct-2-enes could not be assigned accurately, and a computer program was used to process indices of low precision. Distinction between the four isomers was put, on statistical grounds, at the 98 % or greater confidence level. Hence, although the simplified pseudo-contact model here may be incorrect in some respects, the interpretation of substrate structure from LIS is self-consistent and in complete agreement with the chemical evidence.  [Pg.300]

Spectra.—For compounds of low solubility in deuteriochloroform, the use of ASCI3-CDCI3 (2 1 v/v) may prove valuable as the chemical shift differences (excepting alcohols) between the two solvent systems is negligible ( 1 p.p.m.) on the n.m.r. scale. Titanium tetrachloride-induced shifts on the spectra of carbonyl compounds has been investigated. The carbonyl carbon atoms experience large down-field shifts, adjacent carbon atoms showed only small downfield shifts, and remote carbon atoms are scarcely perturbed. In a -unsaturated carbonyl compounds, large downfield shifts are observed for the P-carbon atoms, presumably because of the enhancement of the dipolar resonance form of the enone system consistent with this picture is the much smaller shift, in either direction, of the a-carbon atoms. Studies were extended to include ap-unsaturated acids and esters.  [Pg.301]


In a coupled spin system, the number of observed lines in a spectrum does not match the number of independent z magnetizations and, fiirthennore, the spectra depend on the flip angle of the pulse used to observe them. Because of the complicated spectroscopy of homonuclear coupled spins, it is only recently that selective inversions in simple coupled spin systems [23] have been studied. This means that slow chemical exchange can be studied using proton spectra without the requirement of single characteristic peaks, such as methyl groups. [Pg.2110]

Not only is pulsed FT NMR the best method for obtaining proton spectra it is the only practical method for many other nuclei including It also makes possible a large number of sophisticated techniques that have revolutionized NMR spectroscopy... [Pg.524]

The bulk of available NMR data on pyrimidines are naturally proton spectra but of recent... [Pg.61]

Chemical shifts for aromatic azoles are recorded in Tables 14-17. As for the proton spectra, fast tautomerism renders two of the chemical shifts equivalent for the NH derivatives (Table 14). However, data for the AT-methyl derivatives (Table 15) clearly indicate that the... [Pg.15]

Use standardized plotting of spectral presentations, comparable to 0-10 ppm used for proton spectra The range from -1-50 to -250 ppm covers most organofluonne signals but is too wide to show finer splitting and would require individual signals to be expanded. [Pg.1037]

Cyclitol Spectra at 220 MHz with the Superconducting Solenoid. In 1964, Nelson and Weaver (34) at Varian Associates constructed a superconducting solenoid with which proton spectra can be observed at 51.7 kilogauss (220 MHz.) or even higher fields. Other nuclei have been observed at suitable field/frequency combinations. [Pg.57]

The proton spectra analysis of thietane, thietane oxide and thietane dioxide at 100 and 300 MHz in the temperature range — 140 to 190 °C confirmed the puckered structure for the oxide (5a) with the sulfinyl oxygen in the equatorial orientation, as inferred from chemical-shift considerations180. It appears that the repulsive-type 1,3-interactions between the oxygen and the 3-substituents184 are operating between oxygen and the axial proton on C-3 in the unsubstituted thietane oxide (5a). For the thietane dioxide (5b ... [Pg.431]

The proton spectra of thietane oxide (5a) and thietane dioxide (5b) have been studied in order to evaluate whether the oxidation at the sulfur atom changes the established 35° puckering of the ring218, and whether a correlation is possible between structure and... [Pg.440]

NMR provides one of the most powerful techniques for identification of unknown compounds based on high-resolution proton spectra (chemical shift type integration relative numbers) or 13C information (number of nonequivalent carbon atoms types of carbon number of protons at each C atom). Structural information may be obtained in subsequent steps from chemical shifts in single-pulse NMR experiments, homo- and heteronuclear spin-spin connectivities and corresponding coupling constants, from relaxation data such as NOEs, 7) s 7is, or from even more sophisticated 2D techniques. In most cases the presence of a NOE enhancement is all that is required to establish the stereochemistry at a particular centre [167]. For a proper description of the microstructure of a macromolecule NMR spectroscopy has now overtaken IR spectroscopy as the analytical tool in general use. [Pg.328]

Fig. 7a-e Proton spectra of 1 a Dissolved in CDC13 b in D20 c in D20/H20 d with presaturation of the water signal e with presaturation using a digital filter. Signals marked with are due to an impurity (solvent from recrystallization of 1)... [Pg.11]

Here we record two proton spectra alternately, one the normal one and the other that in which we irradiate one of the signals. The first spectrum contains no NOE information, while the second does. The resulting FIDs are subtracted from one another by the computer, and the result is a spectrum in which only those signals are present for which intensity differences are observable. [Pg.17]

A glance at the proton spectra shows that the OH proton is missing, and when we look at the numbers along the axes we can see that in fact only the range from about 1.2 to 7.2 ppm is covered. This is a principle of 2D only record the part of the spectrum which contains useful information Since we want to find out which nucleus couples with which, we do not need to record the OH signal as we already know that it is a singlet. [Pg.38]

Figure 35 shows the proton spectra which we obtain you can see that they are of much better quality than those we got from the on-flow experiment. The signals for acetonitrile and residual HDO have been cleanly removed using the WET sequence referred to above, and resolution and signal-noise are much better, so we can obtain coupling constants exactly. [Pg.57]

Fig. 35 Proton spectra obtained from the stopped-flow experiment. Above acetal 4. Below acetal 5. In each case 16 scans, relaxation delay 1 sec... Fig. 35 Proton spectra obtained from the stopped-flow experiment. Above acetal 4. Below acetal 5. In each case 16 scans, relaxation delay 1 sec...
The resonance frequency of fluorine-19 lies close to that of the proton, so that the same measuring channel is used to observe it. 19F spectra with proton decoupling or proton spectra with 19F decoupling thus have special hard- and software requirements. [Pg.62]

Fig.39a-c Silicon-29 and proton spectra of diphenylsilane in C6D6. a INEPT spectrum with complete proton decoupling, b proton-coupled INEPT spectrum ( h 201 Hz) the fine structure is due to coupling with thearomatic protons, c proton spectrum showing 29Si satellites for the SiH protons)... [Pg.64]

The proton-proton COSY spectrum (COSY meaning Correlated Spectros-copY), which tells you directly which protons couple with which. In many cases this information is already available from the proton spectrum, but since multiplets in proton spectra can be quite complicated, even at 400 MHz, the COSY spectra should be recorded as they are very simple to interpret. [Pg.88]

These four NMR spectra will form the basis which you can use to solve the structures (in some cases not all are presented, depending on what information they give). We have naturally arranged the problems on the basis of their molecular complexity, but even very small molecules can have complex proton spectra All the problems can be solved completely, i.e. including the determination of the isomer involved. [Pg.88]

If one wishes to obtain a fluorine NMR spectrum, one must of course first have access to a spectrometer with a probe that will allow observation of fluorine nuclei. Fortunately, most modern high field NMR spectrometers that are available in industrial and academic research laboratories today have this capability. Probably the most common NMR spectrometers in use today for taking routine NMR spectra are 300 MHz instruments, which measure proton spectra at 300 MHz, carbon spectra at 75.5 MHz and fluorine spectra at 282 MHz. Before obtaining and attempting to interpret fluorine NMR spectra, it would be advisable to become familiar with some of the fundamental concepts related to fluorine chemical shifts and spin-spin coupling constants that are presented in this book. There is also a very nice introduction to fluorine NMR by W. S. and M. L. Brey in the Encyclopedia of Nuclear Magnetic Resonance.1... [Pg.21]

Larger solvent effects can be observed for proton spectra, particularly when using benzene- - As can be seen from the data in Table 2.4, proton chemical shifts in the other solvents, particularly CDC13 and acetone-, are reasonably consistent. [Pg.26]

Any spin system that contains fluorine substituents that are chemically equivalent, but not magnetically equivalent is, by definition, second order. Such spectra can appear deceptively simple, or more commonly they can be amazingly complex. The fluorine and proton spectra of the simple, symmetrical compound, 1,1-difluoroethene exemplify the latter situation (Figures 2.5 and 2.6). [Pg.36]

As was the case for proton spectra, the impact of a fluorine substituent on carbon chemical shifts quickly diminishes as one looks at carbons farther away from the carbon bearing the fluorine, with only a relatively small influence being observed for all but the fluorine-bound carbon (Scheme 2.14). [Pg.40]

In the case of a number of vicinal difluoro systems, such as 2,3-difluoro-2,3-diphenylethane or 2,3-difluorosuccinic acid derivatives, the coupling systems are AA XX, which means that they will produce second-order spectra (see Chapter 2, Section 2.3.5). A case in point is the fluorine and proton spectra of 1,2-difluoroethane, which have been... [Pg.62]

In contrast, although all are not readily interpretable upon observation, the proton spectra of the three isomeric difluorobenzenes are definitely distinctive (Figs. 3.20-3.22, all run in benzene-d6). [Pg.95]

Regarding proton spectra, as was the case with 2,2,2-trifluoroethyl chloride (Scheme 5.7), the chemical shifts of the CH2 protons of 2,2,2-tri-fluoroethanol and of 2,2,2-trifluoroethyl ethers are more affected by the OH or ether substituents than they are by the CF3 group. [Pg.157]

Carbon and Proton Spectra of Oxazoles and Thia-zoles. Some examples of carbon and proton NMR data are provided in Scheme 5.57. [Pg.184]

Again, the family of di-, tri-, and tetrafluorofurans was prepared via CoF3 chemistry, and their fluorine and proton spectra reported, as given in Scheme 6.36. All things being equal, fluorines at the 2-position are more deshielded than those at the 3-position. [Pg.216]

Whilst sample preparation may not be the most interesting aspect of NMR spectroscopy, it is nonetheless extremely important as it will have a huge bearing on the quality of the data obtained and therefore on your ability to make logical deductions about your compounds. This is particularly true when acquiring the most straightforward 1-D proton spectra. The most typical manifestation of sub-standard sample preparation is poor line shape. It is worth remembering that in terms of 1-D proton NMR, the devil can be very much in the detail . Detail , in this context, means fine structure and fine structure is always the first casualty of poor sample preparation. [Pg.13]

Of course, it is quite easy to solve the bandwidth needs of proton spectra - they only have a spread over about 20 ppm (8 kHz at 400 MHz). Things get a bit more difficult with nuclei such as 13C where we need to cover up to 250 ppm (25 kHz) spread of signals and we do notice some falloff of signal intensity at the edge of the spectrum. This is not normally a problem as we seldom quantify by 13C NMR. However, it can be a problem for some pulse sequences that require all nuclei to experience 90°... [Pg.26]


See other pages where Proton spectrum is mentioned: [Pg.9]    [Pg.63]    [Pg.49]    [Pg.505]    [Pg.477]    [Pg.699]    [Pg.163]    [Pg.102]    [Pg.38]    [Pg.73]    [Pg.223]    [Pg.22]    [Pg.23]    [Pg.34]    [Pg.183]    [Pg.14]   
See also in sourсe #XX -- [ Pg.74 , Pg.75 ]

See also in sourсe #XX -- [ Pg.33 ]

See also in sourсe #XX -- [ Pg.853 ]

See also in sourсe #XX -- [ Pg.262 ]




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