These measurements can be very time consuming. One can get a reasonable estimate of the T1 much more quickly. Follow these simple steps:
1. Call up the pulse sequence "t1ir1d" (Bruker) or "s2pul" (Varian).
2. Set p1 and p2 (Bruker) or PW and P1 (Varian) to the 90 degree and 180 degree pulses , respectively.
Set the recycle delay, d1 (Bruker and Varian) to something you believe is much longer than the T1.
3. Set tau to a very small value (3 microseconds for example). Tau is d7 on a Bruker spectrometer or d2 on a Varian spectrometer.
4. Collect a spectrum and phase it such that all peaks are negative (one scan is often enough for protons). Store the phase correction.
5. Repeat step 3. increasing d7 (Bruker) or d2 (Varian) until the peak of interest is nulled. If the peak is negative, tau is too short. If it is positive, tau is too long.
6. The T1 of the peak of interest is the tau value for the null divided by the natural log of 2.
These spectra were acquired while the magnetic field was sweeping. This will happen on a Bruker spectrometer if you do not bother locking the field (or fixing the field when running unlocked). On rare occasions in automation, if there is difficulty in locking your sample, I have seem the spectrometer run a spectrum while sweeping the field. This however is very infrequent.
Quadrature images are small reflections of large signals in the spectrum about the center. They are much less of a problem with newer instruments than they were with older ones. They become smaller as more scans are collected due to receiver phase cycling. You should be aware of quadrature images if you are searching for very small signals in the presence of very large ones.





One should use this method with care as artificial cross peaks will appear for uncoupled signals with excessive t1 noise. Before symmetrization, one should look for the smallest real off-diagonal signal. Make a mental note of the signal. Symmetrize the spectrum and then scale it such that the smallest real off-diagonal signal noted above is the smallest signal in the symmetrized spectrum.
1. Use a standard setup and get more sample or collect more scans. Yeah yeah..... I know ..... if you could do this you wouldn't have a problem.
Remember to tune the proton channel!

Many spectrometers will calculate the receiver gain automatically however you should be aware that this automatic calculation is not always perfect and that the receiver gain may have to be set manually. On a Varian spectrometer the receiver gain is the "gain" parameter. On a Bruker spectrometer the parameter is "rg". In both cases higher numbers mean a higher receiver gain.
If you inadvertently collect a spectrum with a Nyquist fold-back you can still calculate the correct chemical shift, as the signal will be the same number of ppm away from the wrong end of the axis as it is outside of the correct end of the axis.


The next time you are fighting a resolution problem, try using benzene-d6 as your solvent!