Ziyi Wang1, Mu He2, Rohan Virgincar1, Elianna A Bier1, Sheng Luo3, and Bastiaan Driehuys1,4
1Biomedical Engineering, Duke University, Durham, NC, United States, 2Electrical and Computer Engineering, Duke University, Durham, NC, United States, 3Department of Biostatistics & Bioinformatics, Duke University Medical Center, Durham, NC, United States, 4Radiology, Duke University Medical Center, Durham, NC, United States
Synopsis
Quantitative analysis of 129Xe gas exchange MRI has
previously employed linear binning, using thresholds derived from the mean and
standard deviation of a healthy reference population. However, such
distributions can be skewed from a purely Gaussian shape by differences in
acquisition strategy and field strength, thereby complicating threshold determination.
Here we demonstrate a generalization of previous binning methods by applying a
Box-Cox transformation to derive non-linearly spaced reference thresholds. We
provide new thresholds appropriate for 3T acquisitions and demonstrate the
robustness of the approach by showing consistent quantification of subjects
scanned longitudinally across platforms, field strengths, and acquisition parameters.
Introduction
Hyperpolarized 129Xe MRI has emerged as a powerful means to quantify
both ventilation and gas exchange through its uptake in interstitial barrier tissues
and transfer to red blood cells (RBCs) [1]. Recent quantitative
analysis approaches have employed linear binning methods with threshold values
derived from a healthy reference cohort [2, 3]. Historically, such
thresholds were derived from the mean and standard deviation of the healthy reference
distribution, which were generally assumed to be Gaussian in nature. However, recent
work has shown that this assumption, particularly for ventilation imaging, depends
on the acquisition strategy (2D vs 3D and spoiled vs steady-state). Moreover, the
barrier and RBC signal distributions are known to be affected by TR and flip
angle, and are slightly altered at 3 versus 1.5 Tesla [4]. In this work, we sought
to generalize the approach to determining appropriate binning thresholds from
healthy reference cohorts and demonstrate robust quantitative analysis of 129Xe
gas exchange MRI across acquisition parameters and field strengths.Methods
The
study incorporated 129Xe MRI scans from 21 healthy subject to
establish reference distributions at 1.5 and 3 Tesla. They were grouped into 3
cohorts of field strength and readout bandwidth settings: 1) n = 10 (age 29 ± 8
years) at 1.5 Tesla (GE Healthcare 15M4 EXCITE) with 244 Hz/px; 2) n = 6 (age =
37 ± 15) at 3 Tesla (SIEMENS MAGNETOM Trio) with 400 Hz/px; 3) n = 5 (age = 38 ±
16) at the same 3 Tesla scanner with 800 Hz/px. Each 129Xe image was
reconstructed and processed as previously described [4] to examine the ventilation,
barrier-uptake and RBC-transfer distributions [3]. The RBC transfer distributions at
3 Tesla were found to be skewed, which was also true for the 3D ventilation distributions
after bias-field correction [5]. To accommodate this skewing, a
one-parameter Box-Cox transform [6] was applied to render them
approximately Gaussian. From this, the mean and standard deviations could be
determined, and thresholds were calculated as previously described [3]. Transforming the thresholds back
to the original non-Gaussian distribution resulted in unevenly spaced
thresholds that encompassed the percentiles 68%, 95% and 99.7% of the
underlying distribution. These percentiles are identical to those encompassed
by 1-, 2-, and 3- standard deviation portions of a purely Gaussian
distribution. For each distribution and cohort, the thresholds were used to
identify regions of Defects (lowest bin), Low intensity (second lowest bin) and
High intensity (highest 2 bins). To illustrate the efficacy of the approach, it
was applied to longitudinal scans of two subjects, not included in the
reference distributions, (a healthy 66 y/o and a 57 y/o patient with alpha-1
antitrypsin deficiency) who were imaged at both field strengths and all
parameter settings.
Results
Figure 1 shows
the collective distributions of the 3 healthy cohorts at both field strengths
and acquisition strategies. The middle row shows the transformation of the 3
Tesla ventilation distribution into a Gaussian shape by Box-Cox transformation,
deriving thresholds, and reverse-transformation to arrive at appropriate
thresholds for the original distribution. Figure 2 shows the healthy reference
percentages (Defect, Low, and High) derived from each binning map (ventilation,
barrier and RBC) and cohort. The reference percentages are highly consistent
across the 3 cohorts despite differences in the underlying acquisitions and distributions.
Figure 3 shows maps of the healthy subject imaged at both field strengths and
acquisition parameters as well as plots of each derived metric. The images depict
minor apical ventilation defects across all scans, but consistently normal
barrier uptake and RBC transfer. Figure 4 shows similar longitudinal data for the
alpha-1 patient. The images show consistent patterns of ventilation defects, and
deficiencies in barrier uptake (emphysema) with matching areas of low RBC
transfer.Discussion
Employing a healthy reference distribution is a powerful and robust
means to quantify functional images. However, such distributions can be shifted
or skewed by acquisition parameters (field strength, bandwidth, TE, TR and flip
angle) or post-processing factors such as bias-field correction. Such
distributions must therefore be acquired in a standardized way for both healthy
subjects and patients. To accommodate the non-Gaussian nature of the reference
distributions requires generalizing previous methods that used the mean and
standard deviation to determine thresholds. This is readily handled by using a
Box-Cox transform, which effectively results in identifying thresholds based on
Gaussian percentiles (68–95–99.7%). The revised thresholds, which are no longer
linearly spaced, provide a more robust and adaptive representation of the
healthy reference without making assumptions about the shape of the underlying
reference distribution. Acknowledgements
IH/NHLBI R01 HL105643, NIH/NHLBI R01HL126771, and
HHSN268201700001CReferences
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