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. Author manuscript; available in PMC: 2016 May 1.
Published in final edited form as: J Magn Reson Imaging. 2014 Jun 30;41(5):1440–1446. doi: 10.1002/jmri.24679

Figure 5.

Figure 5

Native sagittal slices and reformatted axial and coronal images for the full TR 3D FLAIR sequence (left) and the varying TR and TI, 3D mFLAIR sequence (right). Scan time for 3D mFLAIR sequence (2:50) was 33% lower than 3D FLAIR (4:16). Window/level was the same for all images.