Guilhem Jean Collier1, Ho-Fung Chan1, Graham Norquay1, Neil J. Stewart1, Ryan S. Munro1, Oliver Rodgers1, Rolf F. Schulte2, and Jim M. Wild1
1POLARIS, University of Sheffield, Sheffield, United Kingdom, 2GE Healthcare, Munich, Germany
Synopsis
Keywords: Lung, Hyperpolarized MR (Gas)
Four-echo 3D radial spectroscopic
imaging of hyperpolarised
129Xe in the lung is implemented at 3T to measure
ratios of xenon gas and dissolved xenon in blood (RBC) and lung tissues (M). Thanks
to an interleaved acquisition of the echo times and the choice of a 0.32ms echo
time spacing, data acquisition is possible within the short relaxation time of
dissolved
129Xe (T
2*~1ms). 11 healthy volunteers have been imaged at both
1.5 and 3T after the inhalation of a 1L dose of hyperpolarised
129Xe.
Results show comparable images at both field strengths and a significantly
reduced (p=0.02) RBC:M at 3T.
Introduction
Due to the large chemical shift separation of 129Xe
gas in the alveolar airspace and when dissolved in lung membrane (M) and red
blood cells (RBC), images of gas transfer can be obtained by calculating ratio
maps of 129Xe signal in the different compartments using MR
spectroscopic imaging. Derived metrics have shown sensitivity to regional gas transfer
limitation and disease progression in interstitial and obstructive lung
diseases (1-3). Several different imaging
techniques have been implemented for this purpose, including; CSI, 1-point
Dixon (4) and multi echo
imaging techniques (5,6). While CSI and
1-point Dixon have been successfully implemented at both 1.5 and 3T (7), the short
transverse relaxation time (T2*) of dissolved 129Xe
in the lung at 3T (~1ms) makes implementing a multi echo imaging technique at 3T
challenging. In this work, a 3T implementation of the 4-echo 3D radial
spectroscopic imaging technique previously developed at 1.5T (8) was tested in
healthy volunteers and differences between the main outcome metrics at 1.5T and
3T were evaluated.Methods
11 healthy volunteers with no known respiratory
conditions were recruited. Imaging was performed on 1.5T GE HDx and 3T GE
PET/MR Signa scanners with 129Xe polarized to ~30% with a spin-exchange optical pumping
polariser (POLARIS, Sheffield, UK) (9). Images were acquired with
flexible quadrature transmit/receive vest coils during breath-hold after the
inhalation of 1L of HP 129Xe from FRC. To account for the ~2x shorter T2* of
dissolved xenon at 3T, the 4-echo flyback 3D
radial spectroscopic imaging technique (8) was adapted to acquire 4 different echo
times within ~1.3ms. After deriving the optimal echo time separations using the
number of signal averages (NSA), the following sequence changes were
implemented:
(i) a ΔTE of 0.32ms was chosen to optimise
SNR (see Fig. 1.a)
(ii) an interleaved implementation of the
acquisition of the odd and even echo times (see Fig. 1.b). This is because it
is impossible to acquire 4 echo times after each RF pulse with the desired resolution
and echo time spacing. This change resulted in a decrease in number of radial
projections (see Table 1).
(iii) the frequency-tailored RF excitation
designed to deliver flip angles on 129Xe gas and dissolved-phase 129Xe
of 0.2 degrees and 22 degrees, respectively at 1.5T was implemented on the 3T
scanner after halving its duration to 0.6ms. With an isodelay of 0.15ms at 3T,
the RF pulse allows an approximate first echo time TE1 ~0.4ms due to
hardware gradient delays.
A summary of the imaging parameters is
available in Table 1. Data were analysed as previously described (6). Briefly, the chemical shift and T2*values
for each xenon resonance and the amplitude of the cardiogenic oscillation of
the RBC signal (ARBCCO) (10) were derived, and ratio maps (RBC:M,
RBC:GAS, M:GAS) were calculated. Wilcoxon paired t-tests were performed to
study the differences between imaging markers at 1.5 and 3T.Results
Averaged global imaging markers obtained at both
field strengths are summarized in Table 2. Example images and an RBC:M map
acquired in the same healthy volunteer at 1.5 and 3T are displayed in Fig.2.
Line plots and Bland-Altman graphs are shown in Fig.3 for the global 129Xe
gas exchange ratios. T2* values were 62.5%, 48.5% and 41%
lower on average at 3T for gas, M and RBC, respectively. RBC:GAS and ARBCCO were not different between field strengths. M:GAS was also not significantly
different, although the Bland-Altman (Fig.3) showed a bias of 7% higher M:GAS at
3T. However, RBC:M was significantly lower at 3T compared to 1.5T with a mean
bias of -9%. Discussion
The 3T implementation of the 4-echo 3D radial
spectroscopic imaging technique, adapted from that previously developed for
1.5T, was successful with images showing similar quality at both field
strengths. The main challenge of shorter dissolved 129Xe T2*
has been mitigated using a shorter RF pulse and a shorter echo time spacing at
the expense of increased radial undersampling. However, all images obtained
were free of radial undersampling artefact. The significantly lower RBC:M ratio,
but constant RBC:GAS, observed at 3T compared to 1.5T suggests that the
dissolved xenon in the membrane compartment is higher at 3T. The origin of this
observation may be complex and not driven by physiology. While T2*
values are drastically shorter at 3T, the reported ratios in this work were
corrected for these changes in T2* and echo times by calculating
transverse relaxation times during the acquisition. Ratios are therefore
expected to be independent of T2* and k-space trajectory.
Possible hypotheses are an unequal effect of higher magnetic susceptibility on
gas and dissolved xenon signals at 3T and the fact that the RBC and M peaks are
less spectrally separated at 1.5T, compared to 3T. Further work is required to confirm
this hypothesis (e.g. measuring ratios via spectroscopy measurement) but
results suggest that a correction factor should be applied when comparing
dissolved xenon imaging results acquired at 1.5 and 3T.Conclusion
Dissolved xenon imaging with 4-echo radial spectroscopic
imaging has been successfully implemented at 3T. Results show a significantly
lower RBC:M ratio at 3T, suggesting that a correction factor at this field
strength is required.Acknowledgements
This work was supported by MRC grant MR/M008894/1References
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