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Perspectives in Magnetic Resonance
SQUID-detected ultra-low field MRIq
Michelle Espy ⇑, Andrei Matlashov, Petr Volegov
Los Alamos National Laboratory, Los Alamos, NM 87545, United States
a r t i c l e i n f o
Article history:
Available online 15 February 2013
Keywords:
Magnetic Resonance Imaging (MRI)
Ultra-low fields (ULFs)
SQUID detection
ULF MRI
a b s t r a c t
MRI remains the premier method for non-invasive imaging of soft-tissue. Since the first demonstration of
ULF MRI the trend has been towards ever higher magnetic fields. This is because the signal, and efficiency
of Faraday detectors, increases with ever higher magnetic fields and corresponding Larmor frequencies.Nevertheless, there are many compelling reasons to continue to explore MRI at much weaker magnetic
fields, the so-called ultra-low field or (ULF) regime. In the past decade many excellent proof-of-concept
demonstrations of ULF MRI have been made. These include combined MRI and magnetoencephalography,
imaging in the presence of metal, unique tissue contrast, and implementation in situations where a high
magnetic field is simply impractical. These demonstrations have routinely used pulsed pre-polarization
(at magnetic fields from $10 to 100 mT) followed by read-out in a much weaker (1–100 lT) magnetic
fields using the ultra-sensitive Superconducting Quantum Interference Device (SQUID) sensor. Even with
pre-polarization and SQUID detection, ULF MRI suffers from many challenges associated with lower mag-
netization (i.e. signal) and inherently long acquisition times compared to conventional >1 T MRI. These
are fundamental limitations imposed by the low measurement and gradient fields used. In this review
article we discuss some of the techniques, potential applications, and inherent challenges of ULF MRI.
Published by Elsevier Inc.
1. Overview
In Magnetic Resonance Imaging (MRI) the use of stronger mag-
netic fields, B p, for sample polarization results in a linear increase
in the equilibrium magnetic moment in a voxel, M eq (and hence
the acquired signal)
M eq ¼N h
2c2I ðI þ 1ÞB p3kBT
ð1Þ
where N is the number of spins in a voxel, c is the gyromagnetic ra-
tio, I the spin number, kB is the Boltzmann constant and T the tem-
perature. The increased signal can be used for faster acquisition
and/or better resolved images. Thus, the vast majority of MRI ma-
chines employ fixed strength, high field (HF) magnets of as high a
field as practically achievable. For this article, we define HF as>1 T. In addition, the performance of Faraday coils used as detectors
in HF MRI increases with magnetic field strength [1]. Thus, trying to
perform conventional MRI at lower magnetic field strengths results
in a penalty in acquired signal that scales as$x20 (wherex0 = cB0 is
the Larmor frequency, c is the gyromagnetic ratio, and B0 is themagnetic field in which the spins precess). Most clinical HF MRI sys-
tems are based on large and highly uniform (ppm) superconducting
magnets and the polarization and measurement field in which spins
precess are the same. Typically B0 = B p = 1.5 or 3 T in these systems,
which results in a proton Larmor frequency of $64–128 MHz.
However, there remain numerous MRI applications where high
field is not an option, for example imaging in the presence of metal
or where a large and expensive magnet might be impractical. In the
early 90s low field MRI based on pulsed pre-polarization to in-
crease signal (followed readout at an even lower magnetic field)
was proposed as a low cost alternative to conventional HF MRI
[2]. A few years later, the ultra-sensitive SQUID (Superconducting
Quantum Interference Device) sensor was shown as a potential ap-
proach to improve detection at the low Larmor frequencies thataccompany the lower magnetic fields [3]. In the early 2000s the
group of John Clarke significantly advanced the concept of
SQUID-based MRI at ultra-low fields (ULFs), with readout magnetic
fields as low as 132 lT and using pulsed pre-polarization [4].
Because of the broad-band nature of SQUID detection, almost all
recent ULF MRI demonstrations have focused on the approach of
SQUID detection in lT readout fields (proton Larmor frequencies
in the Hz to kHz range), with pulsed pre-polarization ($0.01–
0.2 T) to increase signal. Numerous ULF MRI applications using this
approach have been demonstrated by us and others, including
imaging the human brain [5–7]. The use of SQUID detection natu-
rally opens up the possibility of combined magnetoencephalogra-
1090-7807/$ - see front matter Published by Elsevier Inc.http://dx.doi.org/10.1016/j.jmr.2013.02.009
DOI of original article: http://dx.doi.org/10.1016/j.jmr.2012.11.030q A publishers error resulted in this article appearing in the wrong issue. The
article is reprinted here for the reader’s convenience and for the continuity of the
special issue. For citation purposes, please use Journal of Magnetic Resonance, 228,
pp. 1-15.⇑ Corresponding author. Address: LANL, MS-D454, Los Alamos, NM 87545, United
States.
E-mail address: [email protected] (M. Espy).
Journal of Magnetic Resonance 229 (2013) 127–141
Contents lists available at SciVerse ScienceDirect
Journal of Magnetic Resonance
j o u r n a l h o m e p a g e : w w w . e l s e v i e r . c o m / l o c a t e / j m r
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phy (MEG) and MRI, which is simply not possible in the HF regime
due to the incompatibility of the SQUID (required for the MEG)
with the large magnetic fields of the MRI. Combining the functional
measurement of MEG and anatomical MRI confers advantages to
either modality [6].
MRI of the human brain at 94 lT [5] with interleaved MEG, ac-
quired by our team at Los Alamos National Laboratory, is shown in
Fig. 1. Pre-polarization was at 30 mT. The ULF images are presentedside-by-side with images acquired at 3 T and highlight some of the
differences (good and bad) between ULF and HF MRI. For example,
spatial resolution is clearly worse, but MEG can be acquired at ULF
(not possible at all with HF). We will discuss these differences in
more detail in the next section.
Despite the drawbacks in terms of lower signal, and the added
complexity of SQUID detection compared to a Faraday coil, ULF
MRI may confer critical advantages for some applications. These
include: (1) Unique MRI contrast arising from the overlap of the Lar-
mor frequency with the msec-sec dynamics of molecular or phys-
iological processes not accessible by fixed field MRI orconventional field cycling methods [8–10]. T 1 dispersion with
[11,12] and without [8,9,13] contrast agents, and resonant contrast
produced by overlapping the Larmor frequency with biomagnetic
Fig. 1. (Left column) 3 T HF MRI and (right column) 94 lT ULF MRI slices. For the ULF MRI, averages of 5 scans are shown. (Bottom right panel) a dipole fit of the N100 m fieldmap to an auditory stimulus. Data are from [5].
128 M. Espy et al. / Journal of Magnetic Resonance 229 (2013) 127–141
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processes of interest [14]. (2) Flexible instrumentation compatible
with applications precluded by high field approaches. This includes
imaging through or in the presence of metal [15,16] (e.g. Fig. 2),
compatibility with imaging modalities like MEG [5–7], and the
ability to reduce, remove, or reorient magnetic fields for applica-
tions such as portable or bedside MRI using novel pulse sequences.
Because the magnetic fields are low, susceptibility artifacts are also
greatly reduced. This may be useful for situations where such arti-facts are a problem (e.g. near lungs) but bad for methods like BOLD
fMRI that rely on susceptibility. (3) The potential for lower cost ma-
chines. As liquid helium (LH) supplies and rare earth magnet mate-
rial become more costly and scarce, the expense of field generation
for high field MRI may further increase. SQUID-based systems re-
quire only tens of liters of LH and potentially such systems can em-
ploy recycling or cryocoolers [17].
Of course, there is a reason that the use of higher and higher
magnetic fields is (and likely will continue to be) the dominating
approach to MRI. The advantages of ULF MRI must be balanced
against the challenges arising from loss of signal, difficulties asso-
ciated with pulsed magnets, SQUIDs operating in a dynamic mag-
netic environment, shorter relaxation and bandwidth, etc. In this
paper we aim to present some of these considerations in terms
of instrumentation and pulse sequence development requirements
in the ULF regime. We will discuss recent progress in ULF MRI, and
conclude with what appear to be the promising future directions. It
is our hope to give the reader a reasonable picture of what is (and
might not be) possible for SQUID-detected ultra-low field MRI.
2. Imaging considerations in ULF MRI (why is it so hard?)
Differences between imaging systems and methodologies make
direct comparison between images difficult. But to provide the
general flavor of how MRI scales with field, let us return to Fig. 1.
Table 1 lists some of the parameters between the HF and ULF
images shown in this Figure. It is immediately obvious that the
overall quality of the 3 T image seems ‘‘better’’. Single scan sig-nal-to-noise (SNR) is higher and voxel size is smaller for the 3 T
image. This is not totally surprising given the 100-fold increase
in polarization field (3 T vs. 30 mT). In fact the optimist might be
surprised the ULF MRI is not worse!
But comparing images is not straightforward. Several things be-
tween these images are different. We took fewer steps at ULF, lar-
gely driven by the fact that the acquisition time was 5 times longer
and it would have taken a really long time; each single scan was
$10 min, and the image shown is an average of 5 scans. The longer
acquisition time is driven by bandwidth limitations, compared to
HF MRI. What does this mean? Imagine for a moment that we have
a ball of water that we want to image. To produce a 1D image we
will apply a gradient in our MRI machine. In a HF scanner, 3 T, gra-dients are typically 10À2 T/m. Using the fact that the gyromagnetic
ratio is 42.6 MHz/T for protons, this gradient is about 426 kHz/m,
so if the ball is .10 m in diameter, the frequency spread is 42 kHz
across the sample. From the Nyquist theorem we know that we
will need to sample for
t a ¼1
2Dxð2Þ
where t a is the acquisition time, and Dx is the width of the fre-
quency bin. To take 100 imaging steps we will have Dx = 420 Hz
per step and t a is 1.2 ms. On the other hand in ULF MRI our gradi-
ents are usually $100 times smaller. The frequency spread across
the sample is 420 Hz. For the same number of steps we will have
Dx = 4.2 Hz per step, and thus we have to sample for 120 ms forequivalent sampling. This makes imaging at ULF inherently slower.
Fig. 2. (Left) ULF MRI of hand at $100lT. The right panel is a photograph of the hand for which the MRI was acquired showing a 4 mm diameter titanium rod that was placedon top of the hand during acquisition of the image. The presence of such metal in typical MRI scanner would have made the acquisition virtually impossible.
Table 1
Image parameters from Fig. 1.
Field strength 3 T 30 mT (94lT)
Voxel size (mm3) 1 Â 1 Â 6 3Â 3 Â 6
N x (readout steps) 128 90
N y,z (phase steps) 128Â 128 51Â 9
t a (ms) $10 56
Gradients $10À2 T/m $10À4 T/m
SNR (voxel) single scan 30 10
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Further, because the relaxation time of tissues at ULF is often on the
order of 100–200 ms [9], we might only have time to complete one
acquisition step before we need to re-polarize. In HF MRI many
steps can be taken with a single polarization.
Another consideration is in the relationship between spatial
resolution, D x, and gradients.
D x ¼
2p
2ðcG xt aÞ ð3
Þ
where G x is the readout (frequency encoding) gradient that is ap-
plied during the signal acquisition.
To achieve the same spatial resolution as for HF MRI, at ULF we
either need to turn the gradients up 100 times to match HF MRI, or
acquire (in the case of the readout) or encode (in the case of the
phase encoding direction) for 100 times longer. Often we cannot
simply turn the gradients up to make D x smaller because of distor-
tions caused by concomitant gradients [18,19] and bandwidth
limitations.
Eq. (3) defines spatial resolution based on how we sample our
image. But without enough SNR, a small voxel does not convey
any information. To use Eq. (3) we assume adequate voxel SNR
(usually > 5) [20]. We can write SNR as [21]
SNRv oxel % C Á f ð geomÞ Á B p Á V Á
ffiffiffiffiffiffiffiffit
2S B
r ð4Þ
where C are the physical constants, f is a function of the geometry,
S B is the magnetic noise spectral density, B p is the pre-polarization
field, and V is the voxel volume. We are again reminded that higher
pre-polarization (or lower noise) will increase SNR, and smaller
voxels will decrease it.
This analysis, while by no means rigorous (we remind the read-
er that image comparison is a subtle business), gives the general
flavor of the issue of scaling with magnetic field; there is less sig-
nal, less bandwidth, and differences in tissue relaxation that must
be considered. Many of the practical challenges and considerations
to implementing ULF MRI are discussed in [21].
3. Hardware and pulse sequences
Imaging techniques used in ULF MRI are generally similar to
those used for traditional high field MRI. One key difference is that
the ULF NMR/MRI methods typically utilize different magnetic
fields for polarization, spin evolution, and measurement. In this re-
gard it bears some resemblance to and maintains many of the
advantages for novel contrast of Field-Cycling NMR/MRI, which re-
lies on more traditional permanent and superconducting magnet
technologies [22]. However acquiring a ‘‘useful’’ image with ULF
can be more challenging due to lower signal amplitude and less
bandwidth with which to acquire it, as we saw in the simple exam-
ple of Fig. 1. And of course, dealing with SQUID sensors in the pres-ence of relatively large and time varying magnetic fields is an
added challenge. While the definition of ‘‘useful’’ is application
dependent, ULF MRI will likely always be at a disadvantage com-
pared to HF MRI in terms of spatial resolution and SNR simply be-
cause of these challenges.
An example of the 3D Fourier Imaging pulse sequence used to
produce many of our ULF MRI images (including those shown in
Fig. 1) is shown in Fig. 3. The magnetic field coil hardware used
to implement this pulse sequence is shown schematically in
Fig. 4. B p are the magnetic field coils to generate the sample mag-
netization, in this example along the x-axis. Bm denotes the mea-
surement magnetic field coils, along the z -axis. In HF MRI this is
usually denoted as B0 but here we call it Bm to distinguish it as a
field that may or may not be the same as the polarization field.In HF MRI there is a single fixed field providing both B p and Bm,
typically provided by a large superconducting magnet. In ULF
MRI the field generation is typically produced by simple electro-
magnets and allows for different field orientations and strengths
provided by separate B p and Bm coils. The additional G x,y,z coils
are for gradient encoding in the B z /d x, y, z directions respectively.
Let us now go through the ULF MRI pulse sequence in more detail
to further highlight the similarities and differences between tradi-
tional and ULF MRI.
3.1. Pre-polarization
The first step to any NMR/MRI application, regardless of mag-
netic field strength, is recruitment of the spin population to pro-
duce a measurable magnetization. With ULF MRI, as with many
Field-Cycling methods, sample preparation is done by application
of a pre-polarization field, a method by which we can apply a lar-
ger (typically 10–200 mT) field, B p, for some time t p, to recruit more
spins. Readout is then at lower Larmor frequencies (magnetic
fields) chosen to derive certain benefits (contrast, compatibility,
penetration through metal, etc.).
For the case where we start with no initial magnetization, and
apply this field along some axis (in Fig. 4 it is the x-axis) the voxel
magnetic moment develops as
M xðt Þ ¼ M x;eqð1 À eÀt =T 1 Þ ð5Þ
where M x,eq, is the equilibrium magnetic moment (see Eq. (1)) and
T 1 is the longitudinal relaxation time. We also remind the readerthat we are discussing T 1 in the B p field.
Fig. 3. Fourier imaging sequence for ULF MRI, adapted from [6].
Fig. 4. Schematic of ULF MRI field generation hardware for the pulse sequence in
Fig. 3.
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As Eq. (5) shows, the magnetization exponentially approaches
equilibrium. A common ‘‘rule of thumb’’ is to polarize for several
T 1 times to attain the maximum signal (at least 3Â T 1 is common).
While the most obvious implication of ULF MRI is lower SNR due to
small polarizing fields, T 1 (and hence contrast) also changes with
field, typically decreasing with reduced fields. Therefore, an advan-
tage at ULF is that shorter T 1 leads to shorter required polarization
times and the potential for a higher duty cycle. For example, inbrain tissue at 1.5 T, T 1 is $1 s [23] whereas at ULF is it $100 ms
[9]. Another advantage of the ULF approach is that the T 1 contrast
in the image can be selected by the user to correspond to either
that of the polarization field or the measurement field, depending
on the pulse sequence. This can provide additional information
about tissue based on how T 1 changes with field strength (T 1dispersion).
The B p field can be relatively inhomogeneous compared to HF
MRI systems. For a fixed relative homogeneity, the NMR line width
scales linearly with the strength of the measurement magnetic
field [24,25]. Thus, at the low fields of ULF MRI, quite narrow line
widths can be achieved even for a rather inhomogeneous field.
The inherent line width is proportional to the inverse of the
measured relaxation time, 1=T Ã2,
Dxl %2
T Ã2
ð6Þ
For simplicity we can consider the 1-D imaging case, where we
have two objects separated by x, and we apply a gradient G x. There
will be two peaks in the FFT separated by cG xD x. The minimum
ability to resolve them spatially will be
cG xD x ¼ Dxl ð7Þ
Thus the spatial resolution can be expressed as
D x ¼Dxl
cG x¼
2
cG xT Ã2
ð8Þ
If T
Ã
2 is dominated by T 2, the resolution can be improved only byraising the applied gradient. This is the case for gray matter at ULF
(T 1 $ 100 ms [9]). Using Eq. (8) with G x = 10À4 T/m we find
D x $ 5 mm. In the case of water T 2 is long, $3 s, and it is field inho-
mogeneities across the sample, DB, that are the primary cause of
de-phasing. Our typical ULF measurement for water is T Ã2 $ 1 s,
D x $ .5 mm. In this case making Bm more homogeneous will fur-
ther improve resolution. The field inhomogeneity of Bm can be
written as BmðDBBmÞ, where DB
Bmis the relative homogeneity. Thus
Dxl ¼ cDB ¼ cBm
DB
Bm
ð9Þ
and
D x ¼
Bm
G x
DB
Bm
ð10Þ
Typically it is much easier to generate the large B p field when
the requirement for homogeneity is removed.
However, there are considerations to producing (and removing)
B p. And in fact, some of the advantages (reduced homogeneity
requirement, shorter T 1) can be disadvantages if not accounted
for. The first consideration is that it is not trivial to make a pulsed
field at >50 mT. The coil will experience heating, the energy must
be removed, and the proximity of a large amount of conductor near
the SQUIDs can introduce noise. We have shown that the B p coil
should be physically disconnected during measurement (via relay
switch) to reduce the effect of acting like a large antenna.
There have been several approaches to producing a pulsed B p.
We have demonstrated resistive room temperature coolant (Fluor-inert) cooled, and liquid nitrogen (LN) cooled coils [26]. The LN coil
has the benefit of 7Â lower resistance, but requires the complexity
of an additional cryostat. Recently a group in Finland has shown a
self-shielded [27] pulsed superconducting coil [7] for ULF MRI,
integrated directly into the cryostat with the SQUIDs.
When the B p field is removed one must consider that transient
eddy currents will be induced in nearby conductors, which can im-
pose a long dead-time if the magnetic fields from the transients ex-
ceed the dynamic range of the SQUIDs. Further, the choice of materials for B p can be important. For example we have found that
multi-stranded Litz wire performs much better than solid wire in
terms of noise. In reference [7] the superconducting wire appeared
to become magnetized if too high a current (>12 A) were applied,
producing gradients that influenced the image quality, limiting B p
in that work to <24 mT.
Also, how one removes B p is an important consideration. In the
images shown in Fig. 1 we employed a non-adiabatic ramp-down,
dB p=dt ) cB2m such that the magnetization was left aligned with
the original direction of B p, ^ x in Fig. 4 after $10 ms shut down.
We did this for two reasons, it is the simplest possible approach
to elicit an MR signal (no spin flip coil is required), and it (in prin-
ciple) minimizes time between beginning precession and measure-
ment. If Bm is applied orthogonally as shown, precession begins
instantly after shut down.
In reality the faster one removes B p the larger the transients that
are induced in nearby conductors. In the case of combined MEG/
ULF MRI when measurements are made inside conductive magnet-
ically shielded rooms (MSRs), these transients can become a real
confound as some components can persist for hundreds of msec
[28], and are hard to de-convolve from the MEG [7]. Even in the ab-
sence of an MSR, anything conducting nearby will also support
transients and that will impact the image. In our MEG/MRI images
a relatively long wait time between the MRI and the MEG ($3 s)
was imposed due to these effects; the self-shielded approach is
likely quite important to reduce this effect [27].
One added consideration in the non-adiabatic field removal ap-
proach is the non-uniformity of B p. Not requiring a uniform B p
greatly simplifies the magnet, but signal is lost due to this non-uni-formity; when precession starts the spins are not all in phase. In
addition there are technical problems associated with the require-
ment to dissipate the energy, induced transients (the faster you
ramp down the larger), and phase stability. If instead, we ramp
down adiabatically (dB p=dt ( cB2m) the final magnetization is well
aligned with the low Bm field, which is easy to make uniform. Fur-
ther, phase coherence is typically improved due to lack of tran-
sients. A traditional spin-flip pulse is then required to start
precession. In recent demonstrations we have shown that through
the use of amplifiers, we can develop a switch off profile to both
minimize transients and maximize residual signal. Although an
adiabatic ramp down takes longer (and signal is being lost to T 1relaxation during that time) we calculate that for a 100 ms linear
ramp from 100 mT to 0 field, $85% of the signal for gray/whitematter is retained. A non-linear ramp with less time spent at low
frequencies (where relaxation is shorter) may further improve this.
Another advantage of the adiabatic approach is that the dB/dt is
lower. Thus there is less danger associated with heating or energy
deposited in the subject, a special consideration when imaging
near metal. Large dB/dt effects are capable of inducing significant
electric fields that can result in non-trivial transient currents in tis-
sue [29–31]. In a ULF MRI system B p is typically 10–200 mT and is
removed within 1–10 ms (depending on the approach). The field
changes dB/dt may range from 10–20 T/s. It is worth noting that
the FDA initially limited dB/dt to 20 T/s [32], but now these guide-
lines have been relaxed and dB/dt should avoid discomfort, pain, or
nerve stimulation [33]. Even with relatively high pre-polarization,
the dB/dt in a ULF MRI system is typically lower than that found inHF MRI systems.
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One also has to consider that the SQUIDs have to survive the B p
pulse. In our applications we have connected the SQUID pick-up
coils to commercial CE2Blue SQUID sensors via cryogenic switches
[34]. Cryogenic switches are activated during pre-polarization and
become normal with 350X resistance. In our applications we have
not used self-shielded coils, but performed some compensation of
transients (induced in the MSR and instrument) by implementa-
tion of external low-frequency negative feedback [35]. One canalso use the approach of protection the SQUID from the polarizing
field by placing niobium plates above and below the SQUID chip
and/or by using flux dams [36].
Before we leave our discussion of pre-polarization it is also
worth mentioning that others have demonstrated that it may be
possible to use the pre-polarization field shape itself to encode im-
age contrast [37].
3.2. Begin precession (spin reorientation)
Upon completion of the polarization, the MRI pulse sequence
begins. As with any MRI, the measurable signal is derived from
the precession of the magnetization when spins are tipped suchthat there is a component of magnetization transverse to the ap-
plied magnetic field. This process is described by the Bloch
equations:
dM
dt ¼ cM Â B À
1
T 1ðM z À v
0B z Þz þ
1
T 2ðM x^ x þ M y^ y Þ
ð11Þ
where B z is the measurement field (here defined to be along the z -
axis), and T 1 is the value in the measurement field. The first term
describes the precession about any transverse magnetization and
the second the effects of spin relaxation.
In the implementation of the pulse sequence shown in Fig. 3 we
begin precession by removing B p (along the x-axis) non-adiabati-cally leaving the magnetization along this direction, and applying
Bm orthogonally to B p (along the z -axis). This immediately begins
the precession of the magnetization about the z -axis of the mea-
surement field at the start of the encoding period, t g . By repeating
the subsequent pulse sequence for different values of t p, and using
the initial amplitude of the precession signal, one can determine T 1at the value of the polarization field.
Alternately, if the B p ramp down had been adiabatic, spins
would end up aligned with the z -axis and a spin-reorientation (also
known as ‘‘spin tipping’’ or ‘‘spin-flip’’) would be required at the
transition between t p (polarization) and t g (gradient encoding) in
Fig. 3. The ultimate goal of spin-reorientation is to result in some
component of the magnetization orthogonal to the measurement
field. Typically 90° for maximum signal, but any component of the magnetization vector tipped away from the measurement field
axis will begin to precess, and provide a measurable signal. To ini-
tiate the spin-flip, the coil(s) are oriented orthogonal to the axis of
the polarization field. Although not shown, in the ULF MRI config-
uration in Fig. 4 a spin-flip coil would be oriented along the y-axis
orthogonal to both B p ( x-axis) and Bm ( z -axis).
The spin reorientation can be provided by either resonant or
non-resonant methods. In the resonant case, a magnetic field time
varying at the Larmor (resonant) frequency is applied in a fixed ori-
entation orthogonal to the measurement field. In the non-resonant
case a field that varies slowly in time and orientation, and does not
contain Larmor frequency content, is applied. It is worth emphasiz-
ing that the second (non-resonant) approach to spin-reorientation
is totally unique to the ULF approach. Both approaches are de-scribed below:
(1) Resonant spin-tipping : After the removal of B p a time varying
field B1 is applied orthogonally to Bm at the Larmor fre-
quency for a desired period of time to reorient the magneti-
zation. This is the typical method for spin reorientation in HF
MRI.
(2) Non-resonant spin-tipping : The non-resonant spin-reorienta-
tion can be implemented several ways. Here we present two
examples: (1) the original orientation of the measurementfield Bm is changed to some new direction adiabatically
(the field changes slowly enough that the magnetization
can follow). The orientation of Bm is then non-adiabatically
restored to its original orientation, leaving the magnetiza-
tion ‘‘tipped’’. (2) B p and Bm are orthogonal, as shown in
Fig. 4 and the non-adiabatic switch off of B p is followed by
application of orthogonal Bm. Spins remain at 90° and simply
begin precession.
3.3. Encoding and acquisition
In order to realize the spatial information in the image, one
must apply and vary the gradients along multiple axes that spa-
tially encode the NMR signal, and collect the data before the signal
has dephased (limited by T 2). These periods are shown as t g (time
during application of gradient fields) and t a,(acquisition time)
respectively, in Fig. 3. Finally, a 2D or 3D FFT must be performed
on the data to extract the image. As in HF MRI, the use of echo
pulses is also routinely employed to help remove the effects of field
inhomogeneity.
To begin the discussion, let’s revisit the various types of echoes:
(1) In high field MRI the spin echo is routinely used, with a 180°
spin-tip to produce re-focusing. This is shown schematically in
Fig. 5a. The spins are shown precessing in the x–y plane about a
magnetic field oriented into the page. The spins have de-phased
due to gradients. After the 180 degree reorientation (imagine flip-
ping the paper over) the faster spins are behind the slower, and
will catch up, producing the echo. This sort of echo is also referred
to as a ‘‘pancake’’ echo because it can also be visualized as flippingthe orientation of the spins in analogy to flipping a pancake. (2) The
gradient echo is also routinely used in HF MRI where we assume
we have a large homogeneous field and then a smaller gradient.
The reversal of the gradient can change the precession speed, thus
causing the echo, as shown in Fig. 5b. (3) The final echo is unique to
ULF MRI and is known as the ‘‘field echo’’. This echo is possible if
one can reverse the orientation of the measurement field as well.
In this case the precession direction is changed. An analogy is to
runners on a racetrack who suddenly reverse direction in the mid-
dle of the race (with faster ones now being behind and the echo
happening when they catch up). For this reason the field echo is
also referred to as the ‘‘racetrack’’ echo. This echo is shown in
Fig. 5c.
In HF MRI the field echo is not an option due to the inability tore-orient the main magnetic field. But a field echo can be quite
valuable. For example, a gradient echo alone cannot remove inho-
mogeneity associated with the main magnetic field, but a field
echo can.
In terms of encoding and acquisition, ULF MRI can use methods
very similar to traditional high field MRI, e.g. using both frequency
and phase of the voxel to encode an image, as shown in Fig. 3.
However, one could also use projection reconstruction encoding
by rotating the encoding gradients between excitations. Another
technique that is uniquely enabled by the low field strengths used
in ULF MRI is the possibility of rotating the main magnetic field (in-
stead of the sample or gradients). This could be useful if there were
multiple sensors, in a variety of orientations around the sample
and one were trying to optimize signal in all of them. We can, inprinciple, leverage any pulse sequence from HF MRI if we have
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the hardware and signal time available. On the other hand – maybe
we can invent new approaches such as reorienting Bm.
We remind the reader of the lower gradients and reduced band-width we discussed earlier (i.e. Eqs. (2) and (3)). At ULF there is a
requirement that encoding and acquisition times be longer than in
traditional MRI. In addition to slowing us down, because relaxation
times may get shorter, and we are running out of signal and longer
acquisition times might not be practical. The Fourier imaging se-
quence shown in Fig.3, is simplebut inefficient. We arelosing signal
during a relatively long encoding time, and we only get one acquisi-
tion per polarization due to long acquisitions. The use of this se-
quence brings up another point, projection imaging requires Bm
and that all three gradients are on during readout and this intro-
duces noise. In contrast, in Fourier imaging only Bm and G x are on
and since they do not change in value they can be run on batteries
or very low-noise current supplies. These are the types of practical
challenges one must face.
4. Recent progress
4.1. Combined MEG and ULF MRI
Electroencephalography, EEG [38], and MEG [39] are at present
the only noninvasive imaging techniques that can passively and
non-invasively measure the consequences of neural activity on
the time scale at which neurons communicate (sub-millisecond
to tens of milliseconds). Unlike other techniques such as functional
MRI (fMRI) and positron emission tomography (PET), MEG/EEG are
‘‘direct’’ measurements of neural activity as the signals arise from
the electrical activity of the neurons themselves as opposed to
blood flow or increased metabolism indirectly associated with
neural activity. While the debate is still active, MEG is often re-
garded as having less ambiguous spatial localization [39,40] than
EEG, and is a powerful and well-regarded method for noninvasive
studies of neural activity in the human brain, and a powerful diag-
Fig. 5. Examples of various echo types. Precession is about the z -axis (into the page). (a) Spin-echo based on 180° RF pulse. The echo is produced when the faster spins ‘‘catch
up’’ to the slower. (b) The gradient echo is produced by reversing the direction of the gradients to exchange which spins are the faster and slower. (c) The field echo is only
possible in ULF MRI. In this case all the fields (measurement and gradient) are reversed, changing the direction of precession.
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nostic tool for diseases such as epilepsy [41]. MEG localization of
small discrete cortical sources typically requires co-registration
with anatomical images acquired by MRI to localize function rela-
tive to anatomical features and landmarks. MEG instrumentation
remains almost exclusively based on the SQUID because of the re-
quired sensitivity to the minute magnetic fields produced by neu-
ral activity, nT to fT. There have been promising demonstrations of
MEG using atomic magnetometers [42], but at the time of thiswriting all clinical MEG systems remain based on the SQUID. Such
sensitive detectors are incompatible with conventional MRI which
is acquired at magnetic fields typically 1.5 T and higher.
Because the anatomical MRI and functional MEG data are ac-
quired in two separate systems, there is added cost as well as a
‘‘co-registration’’ process for the data sets which can introduce
source localization errors ranging from 2–10 mm [43,44], depend-
ing on approach. While this approach is routinely used, there is
some desire in the neuroscience community for improved ap-
proaches to co-register MEG/MRI data and enhance the potential
of MEG.
As soon as it appeared that SQUID-based ULF MRI was possible,
the ability to combine MEG and MRI in a single imaging session
was a logical next step. The first proof-of-principle results in
recording simultaneous MEG and NMR signals were achieved in
2004 [45,46]. In this work, the somatosensory evoked magnetic re-
sponse from the human brain was recorded truly simultaneously
with the free induction decay (FID) signal at 268 Hz. During such
experiments it became clear that simultaneous recording of such
signals is very difficult to perform because of the large low fre-
quency noise arising from the external magnetic field needed for
the NMR precession. This noise was caused by micro-vibrations
of the SQUID gradiometer in the NMR field which seriously dis-
torted the MEG signal. An example of these data is shown in
Fig. 6. In later experiments MEG and MRI signals were recorded
sequentially and the external field and gradients were zeroed dur-
ing the MEG recording.
The first ever ultra-low field (ULF) MRI of the human brain was
published in 2008 [6]. The image resolution was 3 Â 3 Â 6 mm3
and a single scan took $15 min. Six scans were averaged to im-
prove the signal-to-noise ratio (SNR) of the images up to about
30. The system had 7 channels. Auditory evoked magnetic field sig-
nals were recorded immediately after the ULF MRI session was fin-
ished. However the subject moved slightly for better coverage of
the MEG signals, which prevented co-registration of the recorded
MEG signals to the anatomical image. These results demonstrated
that a SQUID-based system could be used for both ULF MRI of the
human brain and MEG. The data are shown in Fig. 7.
Co-registration of auditory evoked magnetic field mapping and
ULF MRI was performed in 2010 [5] using the same 7-channel sys-
tem and an interleaved protocol. These data are shown in Fig. 1.
This time the MEG map was accurately superimposed with the
MR Images, with co-registration error of the different coordinate
systems within 1 mm accuracy. However, due to transients fromswitching the fields for the MRI protocol a wait period of several
seconds had to be introduced before each MEG measurement.
While the data thus far have indicated ‘‘proof-of-concept’’ for a
combined MEG and MRI device, a clinical MEG instrument must
have more than a few sensors. This is because the spatial sensitiv-
ity of the SQUIDs is used to help in MEG source localization: thus,
the more SQUIDs the better. Most clinical MEG systems have
SQUID arrays numbering from 200 to 306 sensors. It is critical that
the number of MEG channels needs to increase from what has been
demonstrated thus far in combined devices. Further, multiple
SQUID sensors can be used for image acceleration [47,48], which
is likely critical to improving the acquisition speed (by using the
spatial sensitivity of the array to reduce the required number of
imaging steps) and quality of the ULF MRI.
At the time of this writing we are aware of two groups actively
pursuing the concept of MEG and ULF MRI in a single device. These
include our group at Los Alamos National Laboratory (LANL) and
the European MEGMRI project. While both groups have ap-
proached the problem from an MEG-starting point (logical since
MEG is a much more mature technology), a combined MEG and
ULF MRI system is not just an upgraded conventional MEG ma-
chine. Adding ULF MRI capability implies the addition of coils for
generation of fields and gradients. However, in addition to the
MRI coils there are completely new requirements on the SQUID-
based sensors. One of the most difficult requirements is that the
SQUIDs should work immediately after being exposed to a pre-
polarizing field of up to 0.2 T. As mentioned above, when MEG is
involved a MSR is required. This adds the potential confound of
large transient magnetic fields from eddy currents even after thepolarization field is removed.
The LANL and MEGMRI systems are somewhat similar; both
leverage commercial MEG cryostats, MSRs, and basic measurement
and gradient coil hardware. Photographs of both systems are pre-
sented in Fig. 8.
At Los Alamos we have adopted the approach of separately opti-
mized magnetometers for imaging and MEG, and an external nitro-
gen B p coil. Our colleagues in Finland use a combination of
magnetometer and planar gradiometers in the array for both
MEG and MRI, and a self-shielded superconducting coil. A detailed
description of our preliminary system design is found in [20]. A
brief description of their system is found in [49] and a more com-
plete one expected in [7].
Although neither system is completed at the time of this writ-ing, preliminary data from the Finnish system is presented in Fig. 9.
Thus far the brain images presented are not ‘‘clinically relevant’’
in terms of ability to resolve key features of anatomy (e.g. cerebel-
lum) or acquisition time. However, it is likely that ULF MRI com-
bined with MEG will only get better as the technology
progresses. Further, one should not lose sight of the fact that the
objective of ULF MRI is not to compete with HF MRI in terms of im-
age quality (which it will not), but to provide a capability that HF
MRI cannot, such as combined MEG. One area of progress that is
essential to achieving better ULF MRI is pre-polarization. Higher
pre-polarization and lower SQUID noise are the only ways to
achieve better SNR, and spatial resolution. Getting the SQUIDs to
survive in the proximity of dynamic fields inside the MSR is the
key challenge to higher pre-polarization. Also, long imaging timesneed to be addressed. Dense array systems are likely the answer.
Fig. 6. Comparison of the somatosensory response for MEG only (blue) and MEG
and simultaneous NMR (red). High frequency oscillations in the MEG and NMR data
are from microphonics in the SQUID moving in the 268.5 Hz measurement field.The data are from [45,46].
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This approach is synergistic with MEG, as large arrays are required
there as well. While the combination of anatomical and functional
imaging via ULF MRI and MEG could present a significant advance
in our understanding of the brain, there are other unique ap-
proaches that may be enabled by ULF, which we touch on briefly
here.
4.2. MEG and flow-based fMRI at ULF
Functional MRI relies on a connection between cerebral blood
flow, metabolism, and oxygenation with neuronal activity [50] to
provide$1 mm spatial resolution of function. Typically the tempo-
ral resolution is 3–4 s (1 s for event related tasks, although tempo-
ral resolution of as good as 150 ms has been achieved for some trial
types). The hemodynamic signal lags the neural activity, taking up
to 7 s to peak. There is evidence that fMRI reflects information
about neuronal firing rates or oscillatory power in the same region
under normal conditions [51]. However, the detailed relationship
between the fMRI signal and the neuronal response is not well
understood. Thus, while providing excellent localization, fMRI pro-
vides more modest insight into neural system dynamics. Applica-tions with clinical consequences such as diagnostics and surgical
planning need paradigms in which the neural correlates of the
fMRI signal have been validated using combined electrophysiolog-
ical and imaging approaches [52].
Thus far, information is primarily combined from separate
instruments, because of the instrumentation limitations discussed
above. But there needs to be the strongest correlation possible be-
tween the sources defined by the different methodologies. Manycognitive paradigms are most effective during the first presenta-
tion: learning, recognition, studies involving deception or confed-
erate studies, and many designs where judgments must be made.
Clinical symptoms are often not reproducible, for example epilep-
tic activity is seizure dependent and schizophrenic observation can
be hallucination-dependent.
The most commonly used form of fMRI is based on different
magnetic susceptibilities of oxy- and de-oxy-hemoglobin. These
levels change as a function of brain activity giving rise to Blood
Oxygen Level Dependent (BOLD) fMRI. BOLD fMRI is widely em-
ployed because of its high sensitivity and easy implementation.
However the BOLD effect increases with magnetic field, typically
requiring large magnetic fields (>1 T). Thus, the BOLD approach
to fMRI will probably not work at ULF. However, fMRI is also rou-
tinely performed at high fields using arterial spin labeling (ASL)
Fig. 7. The first ULF MRI of the human brain at 46 lT compared to HF, 1.5 T. Data are from [6].
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techniques such as flow-sensitive alternating inversion recovery
(FAIR) [53–55]. ASL methods differentiate the net magnetization
of endogenous arterial water flowing proximally to the region of
interest from the net magnetization of tissue. fMRI based on ASL
is possible at ULF, as the effect is not field dependent. We have re-
cently demonstrated flow-based imaging in a water phantom at
ULF using FAIR [56]. Because the electro-physiological brain re-
sponse is faster than the hemodynamic, it may be possible to inter-
leave the acquisition such that the MEG, and fMRI are acquired for
the brain response to the same event. Interleaved data will provide
for direct comparison of electrophysiological and hemodynamic
brain activity obtained during a single collection. Single collection(EEG)/fMRI at high fields is being widely adopted and may address
many of the scientific questions. Combined MEG/fMRI, however, is
only possible at ULF and the addition of MEG information may pro-
vide further insight.
4.3. Direct neural current imaging at ULF
The search for a modality capable of direct measurement and
imaging of neural activity in the human brain embarked on an
exciting new path at the close of the 20th century when research-
ers proposed that magnetic fields resulting from neuroelectrical
activity could interact with a spin population, through phase shifts
and dephasing [57,58]. Shortly thereafter, we presented the possi-
bility that resonant interaction between the neural magnetic fieldsand the spin population was possible in the ULF regime [14]. To-
gether, the prospect of acquiring an image of neural activity based
on the interaction between the neural magnetic fields and the spin
population has been called ‘‘direct neural current imaging,’’ or DNI.
DNI promises the tomographic certainty of volumetric fMRI, with
temporal resolution in direct relation to neural activation. One re-
ported experimental measurement of DNI at high field based on
the enhanced dephasing resulting from neural currents [59] has
been vigorously debated in the neuroimaging community [60]. It
is widely held that the authors did not convincingly differentiate
between a neural effect and the orders of magnitude larger ‘‘sus-
ceptibility artifact’’ caused by the BOLD signal. A key strength of
DNI at ULF is that the confounding susceptibility artifact is virtu-ally nonexistent. Moreover, the overlap between proton Larmor
frequency at ULF and the frequency band of cortical neural activity
permits resonant absorption by the population of proton spins of
magnetic energy supplied by the cortical activity. We reported
the observation of this effect in phantoms, in which we measured
the interaction of a weak current ($ 10 lA) with the ULF NMR sig-
nal [14]. The frequency spectrum of neural activity spans the range
from a few Hz to a few kHz, at most, and the Larmor frequency for
proton spins overlaps with this neural frequency spectrum only in
the ULF regime (recall that xL = 4 kHz, the high-end of the neural
frequency spectrum, for B 100 lT). Consequently, ‘‘resonant
absorption’’ can only occur at fields below 100lT, and may enable
measurement of the DNI effect, and could provide a tool to directly
measure neuronal population oscillations and other frequency-dependent neural population phenomena. In addition to DNI, re-
Fig. 8. Photographs (left) and schematics (right) of the combined MEG and ULF MRI systems. Upper: MEGMRI consortium hybrid system from [49]. Lower: LANL system [20].
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cent work indicates that changes in electrical impedance at fre-
quencies below 100 Hz may provide another approach for imagingfunction [61,62]. These approaches may also lend themselves to
observation by ULF MRI where distributions of applied currents
can be imaged (magnetic resonance electrical impedance tomogra-
phy or MREIT) at ULF and resonant interaction between the applied
current and the spins may be employed to selectively measure the
change in the applied current while drastically reducing noise.
Although speculative, the impact that successful DNI or electrical
impedance tomography-based demonstration of fast neural imag-
ing would have on brain research cannot be overstated.
4.4. Contrast
Contrast in anatomical MRI can be most simply defined as thedifference between two tissue types in some measurable parame-
ter space, such as T 1 or T 2. The variation between parameters such
as T 1 and T 2 in different materials (i.e. tissues) provides the power-
ful and unique information that forms the foundation of MRI
images. For example, T 1 contrast is a basic tool in medical MRI. Dif-
ferences in T 1 between tissues (studied at a fixed magnetic field)
are routinely used for applications such as detection and character-
ization of brain lesions, studies of the gray/white matter junction
in cortex, and detection of cancer (to name just a few).
T 1 varies with field (frequency) and typically these variations
are more pronounced in the ULF regime, opening the prospect
for enhanced contrast at low fields. For example, T 1 for gray matter
changes from $100 ms at 46 lT to $1 s at 1.5 T [9]. Consequently,
it may be an advantage (if one is able to) to change the imagingfield to optimize the contrast.
The underlying reason why T 1 changes with magnetic field is
that the number of resonant protons available to transfer energyto the lattice changes with magnetic field. Specifically, only mag-
netic field fluctuations at the Larmor frequency can cause T 1 relax-
ation, and the frequency of these field fluctuations depends
strongly on the molecular dynamics. This is illustrated in Fig. 10,
which presents the time scales of the NMR fluctuations from vari-
ous molecular processes and compares them to proton Larmor fre-
quency. As one can see, HF MRI (in the 60–120 MHz range) largely
derives any contrast from intramolecular motion only whereas at
ULF, relaxation will be a function of (and thus able to probe)
numerous other processes.
It has been proposed that these contrast differences, or ULF’s
ability to vary contrast because fields can vary so easily, may ren-
der the method superior to HF MRI for some applications even if
the SNR is reduced, because the contrast-to-noise, CNR is better[8].
We will briefly discuss here two recent examples put forth by
John Clarke’s team. In the first, using an agarose gel phantom de-
signed to mimic tissue properties, it was shown that T 1 contrast be-
tween two phantom tissue types was flat from 100 Hz to 10 kHz
and then had a dramatic T 1 dispersion until there appears essen-
tially no contrast past 10 MHz [8]. These results are summarized
in Fig. 11 from that work. In this example, it would appear that
ULF is essential to obtain any image contrast at all.
In more recent work [63], Clarke’s group showed that for ex-
cised prostate tissue samples, there was a significant intrinsic T 1contrast between healthy at cancerous tissue at 132lT. Their re-
sults indicate that T 1 progressively decreases as the percentage of
cancer increases, and that ULF MRI may be a viable non-invasivemethod for detection of cancer even with reduced SNR compared
Fig. 9. Left: Coronal slices of the human brain acquired with the hybrid MEG–MRI device. B p and Bm were 22 mT and 50 lT, respectively. Total imaging time was 92 min, with
8 averages. Right: T 2-weighted high-field-MR image of the same subject obtained at 3 T. The resolution of the high-field-MR image was reduced to match that of the ULF–MR
image. For more details, see [49].
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to HF MRI. These encouraging results will need to be validated with
in vivo studies, but provide compelling argument for continued ef-
forts in ULF MRI.
4.5. Dispersion contrast: measuring T 1 at arbitrary field
In conventional MRI the change in T 1 as a function of magnetic
field cannot be easily exploited, because the main field of the mag-
net is fixed. However, there is no ideal field at which T 1 contrast is
maximized for all tissue types (see for example [64,23]). This var-
iability argues for another possible parameter for imaging contrast:
‘‘Dispersion contrast’’ in which the image is constructed on the ba-
sis of how contrast changes as a function of field, not simply a sin-
gle contrast value at a fixed field.
For example, T 1 changes dramatically as a function of magnetic
field for tissues with high protein concentrations, due to couplings
between the protons and quadrupolar 14N in protein molecule
backbones. Ungersma et al. [13] used this approach in Field Cycling
MRI to produce ‘‘protein weighted’’ images of the human wrist by
producing an image where T 1 in muscle was quite short due to thecross-coupling (at the minimum of a nitrogen dip) and another im-
age far from the dip. Since tissues besides muscle (e.g. fat) do not
show such dispersion. By subtraction of these two images an image
weighted to the presence of tissue with high protein content is pro-
duced. In principle this approach could be used for any tissues with
different T 1 values as a function of field.
Dispersion contrast (e.g. producing images based on howT 1 var-
ies at differing field strengths) is not possible in conventional high
field MRI, where magnetic field strength is fixed. Using methods
commonly employed in ULF MRI (pulsed fields, and variable
strength electromagnets) T 1 can be sampled over a wide range of
frequencies and this T 1 contrast dispersion can be used as an imag-
ing parameter. Unlike field cycling MRI, which uses at somewhat
higher fields, the ULF approach should be able to reach a widerrange of frequencies including very low frequencies below
<1 kHz. When the previously well-studied (at higher frequencies)
T 1 dispersion behavior of water was revisited using SQUID-based
ULF MRI [10] capable of attaining Hz level Larmor frequencies, a
previously unreported and dramatic dispersion due to a very slow
exchange process at $100 Hz was discovered. It is likely that other
effects remain to be discovered at ULF as well, and that these ef-
fects could be exploited for new MRI contrast.
The pre-polarization approach of ULF MRI also enables mea-
surement of T 1 at the pre-polarization field, and readout at essen-tially any field between B p and Bm. In one implementation, used to
inspect liquids by relaxometry [65,66], we showed that by measur-
ing T 1 in the pre-polarization field ($2 MHz) using different polar-
ization times, while measuring T 2 at the much lower measurement
field ($2 kHz) we are able to discriminate between many different
liquid types. For the material identification studies our team has
pursued, the relaxation dispersion provides unique information
that can be used to tell liquids apart.
4.6. Contrast-to-noise – a cautionary tale
Although we have discussed the fact that the ULF regime may
offer enhanced or even unique contrast as compared to HF MRI,
we cannot leave the reader with the impression that greater T 1contrast always leads to a more informative image. Ultimately it
is the contrast-to-noise ratio (CNR) that matters.
An accurate comparison of both SNR and CNR between ULF and
HF instruments would require a detailed analysis of the acquisition
system and details of the protocol being used. However, for the
sake of illustration, let us consider the case where all other factors
equivalent between the systems except T 1 and SNR. We will then
use CNR as the figure of merit for our comparison.
For two tissues A and B,
CNR /S
r½eÀR At À eÀRBt ð12Þ
where the signal is S A = S Áexp(ÀR At ), and R A 1/T 1 A, and r is the
noise (which we assume to be the same for either tissue). For anytwo such tissues there will be some optimal evolution time when
the difference in signal, S A À S B, between them is maximized.
Let’s consider an example, using gray matter and white matter
in the human brain. From the gray/white matter data found in [23]
(see Fig. 13), the contrast difference appears to peak around
10 MHz ($0.23 T). One might infer from this result that it would
be better (from the point of view of maximizing contrast between
these two tissues) to produce an image at 0.23 T rather than 2.3 T
(100 MHz), but even in this very simple example things are not so
simple.
At 10 MHz R(gray)ffi 1.5 and R(white)ffi 3. At 100 MHz
R(gray)ffi 0.9 and R(white)ffi 1.4. Using Eq. (12), assuming no dif-
ferences in proton density, and the same initial SNR, 10 MHz is bet-
ter than 100 MHz in terms of CNR. But the SNR won’t be the samebetween ULF ($0.23 T) and $2.3 T of our example. Even if the dif-
Fig. 10. Time scales of the NMR fluctuations vs. proton Larmor frequency.
Fig. 11. T 1 dispersion in Agarose gel. Data are from [8].
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ference in SNR for ULF were (optimistically) only half, CNR is better
at 100 MHz. Simply looking at T 1 values alone might be quite
misleading.
However, in the T 1 dispersion data presented in Fig. 11, at ULF
(1000 Hz) R A = 2.5 and RB = 5 (for 0.25% and 5% agarose gels respec-
tively), whereas by$12 MHz the differences between R A and RB are
non-existent. In this case the CNR is always better at ULF as long as
the SNR is high enough to produce a useful image.
4.7. The potential for portable systems
The low magnetic fields, relatively simple imaging field genera-
tion, and smaller requirement for cryogens open the possibility for
alternative MRI systems that might be smaller, cheaper, and/or
better suited for operation in unconventional locations (e.g. ships,field hospitals). For example, the system developed for liquid
explosive detection (Fig. 12) operated in an airport and has a foot-
print suggestive of portable MRI, Fig. 14.
To achieve these goals requires advances in several critical areas
including: (1) improved image quality; (2) developing a small-
footprint (size and power consumption) pre-polarization coil; (3)
removal of the requirement for a large magnetically shielded
room; (4) cryogenic cooling to remove the frequent refill times tra-
ditionally associated with SQUID cryostats. It is likely that (1) and
(2) will prove the most interesting areas for development in ULF
MRI. Although there is room for advancement, ULF MRI has been
demonstrated outside a heavy MSR [4] and is likely quite achiev-
able, provided no very low frequencies are required. Similarly,
cryogenic cooling has been used with SQUID-based ULF MRI sys-tems [17] and even for MEG [67].
5. Discussion of the future
While the trends in MRI will likely continue toward higher
fields, there are some reasons to be interested in MRI at the oppo-
site end of the spectrum. The advances over the next few years will
likely be critical for SQUID-based ULF MRI if it is to move past the
work of a handful of groups. For example if the approach can be
shown to add substantive value to MEG in terms of cost and/or
accuracy, this may prove incentive to advance the field. However,
even if very successful in this area, challenges exist. MEG instru-
ments are somewhat rare compared to conventional MRI (or evenfMRI). Thus the application space will not initially be large.
Fig. 12. Data and relaxation weighted images from a ULF MRI system designed to detect threat liquids indicated by circles. Top Row: photographs of items. Center Row: 2-D
images with threat detection. Bottom Row: 3-D slices through the items shown in row (a), far right. Data are from [66].
Fig. 13. Relaxation times of gray and white matter in the human brain as a function
of Larmor frequency. Data are from [23].
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With regard to portable or low-cost MRI, there are already
many low-field MRI ($0.1 T) systems (e.g. PoleStar™) that fill
many potential applications such as imaging in the operating
room, albeit with a fixed field strength and small field-of-view.However, there may be some areas where the ability to re-orient,
remove, or change the strength of the magnetic fields is crucial.
The potential for unique contrast at ULF is one of the most interest-
ing and exciting areas for further study. Additionally the potential
for the resonant mechanisms (overlapping the Larmor frequency
with processes on a similar timescale) is quite unique and may en-
able totally new insights. We end by reminding the reader that
many aspects of imaging performance can be predicted, and ULF
MRI only makes sense for applications where the benefits out-
weigh the challenges.
Acknowledgement
This work was supported in part by the Los Alamos NationalLaboratory LDRD #20100097DR. The authors wish to thank their
colleague Dr. Jaakko Nieminen for providing us images of the MEG-
MRI system.
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