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. Author manuscript; available in PMC: 2024 Jul 16.
Published in final edited form as: Prog Nucl Magn Reson Spectrosc. 2021 Mar 26;123:73–93. doi: 10.1016/j.pnmrs.2021.03.002

Fig. 5.

Fig. 5

(A) Gradient waveform structure of a Looping Star sequence with 8 spokes per loop (NSPL) and 2 loops (NLoops), showing the RF and data acquisition (DAQ) scheme for the original (Org.) and coherence resolved (CR) versions of Looping Star. (B) and (C) illustrates the spin coherences for the two versions of Looping Star at four different timepoints during the sequence. The grey shaded region indicates nominal field of view in k-space as defined by the desired image resolution; coherences outside this region (faded arrows) are considered to be dephased and not contributing to the image.