Abstract

Over the years, the lim itations of the simple 180’ inversion pulse have been realized (I, 2) and several improvements have been suggested (3-7). However, the longer and more elaborate the composite pulse, the less likely it will be used by practicing spectroscopists. This fact is best exemplif ied by the common use of a simple phase-alternating inversion pulse (I) al though other more complicated composite pulses with better inversion characteristics have been publ ished ( 7, 8). In a preceding paper we derived a series of composite inversion pulses that theoretically achieve “good” inversion over a wider range of offset with fewer pulses than any previously proposed pulses (9). In this Note we present the experimental verification of the theoretical results. F igure 1 compares the theoretically determined offset dependence of three members of this composite-pulse family with the experimentally determined offset dependence. The agreement between theory and experiment is excellent, confirming the superior inversion characteristics of this family of composite pulses. Furthermore, the sequences are robust. For example, each element of the four pulse sequence can be set 1 o off from the predicted value with no discernible change in the offset dependence. Table 1 compares the total rotation and inversion with other equivalent composite pulses. The three pulse sequence compares favorably with the commonly used 90,” 180,” 90; composite pulse ( 1). In particular, the inversion of the three-pulse sequence proposed in (9) has an inversion over the 1.1 kHz bandwidth more uniform than that of the former pulse. The four-component composite pulse achieves a 1.3 kHz

Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call