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Chapter 8

08-01
Introduction

08-02
The RARE Pulse Sequence

08-03
Gradient Echo Sequences

Transverse Coherence
Ultrafast Sequences
08-04
Echo-Planar Imaging
08-05
Faster Image Acquisition by k-Space Manipulation


08-03 Gradient Echo Sequences

A completely different approach to rapid imaging was used by the first pulse se­quen­ces, which shortened imaging time in routine clinical settings. The generic name of these sequences is gradient-echo (GE) sequences or, better, gradient-recalled echo (GRE) sequences, and they come in a plethora of different acro­nyms. A basic description of GRE has been given in Chapter 6.

The first sequence in this group was presented in 1986 by Axel Haase and col­la­bo­ra­tors and dubbed FLASH [⇒ Haase]. The FLASH (Fast Low Angle Shot) se­quen­ce is a saturation recovery sequence with a short repetition time (TR <200 ms), a low flip angle (<90°), and a gradient echo for refocusing.

The application of flip angles different from 90° and 180° brought an end to the ideology of long waiting times, which was based upon the belief that T1 is the limiting time factor of MR imaging. The reason for using a low flip angle is il­lu­stra­ted in Figure 08-05.


Figure 08-05:
Principle of (a) a standard pulse sequence, compared to (b) a rapid imaging sequence of the FLASH type.
In both cases, the net magnetization during equilibrium is aligned with the z-axis. In the standard sequence, a 90° pulse tilts the mag­ne­ti­za­tion into the x'-y' plane. No lon­gi­tu­di­nal component remains.
In the FLASH-type sequence, a flip angle α <90° is applied. Such a pulse divides the mag­ne­ti­za­tion in transverse and lon­gi­tu­di­nal components.
(c) In our example α equals 30°. This re­sults in a reduction of the longitudinal mag­ne­ti­za­tion to 87%, whereas the transverse magnetization is 50% of the available lon­gi­tu­di­nal magnetization. The flip angle which will give maximum signal is known as the Ernst angle.


When a 90° flip angle is applied, we convert all of the longitudinal mag­ne­ti­za­tion (in the z-axis) into transverse magnetization (signal in the x'-y' plane), while, e.g., for a 30° flip angle the amount of transverse magnetization is halved (sin 30°), but we still have 87% of the z-mag­ne­ti­za­tion (cos 30°). The z-mag­ne­ti­za­tion will recover at a rate determined by T1 during the interpulse interval. How­ever, since the TR is short in FLASH sequences, the z-magnetization left by the previous pulse becomes dominant and significantly increases the signal ob­tai­ned after the next RF pulse.

For a given repetition time, the flip angle which will give maximum signal can be calculated. It is known as the Ernst angle [⇒ Ernst]:

Ernst angle = cos-1 [exp (-TR / T1)]

where TR is the repetition time and T1 the longitudinal relaxation time.


Figure 08-06 summarizes the main differences between a spin-echo and a gradient-echo (FLASH) pulse sequence.

As with all gradient-echo sequences, but unlike spin-echo sequences, the ef­fects of magnetic field inhomogeneities are not compensated so that short TE must be used if high-quality images are to be obtained. This rules out the pos­si­bi­li­ty of increasing the echo time to give T2 contrast. Another way of reducing field inhomogeneity effects is to use small voxel sizes since this limits the de­pha­sing which occurs within a voxel.

To reduce the echo times, it is necessary to switch the gradients relatively quick­ly and to keep them stable after being switched. Gradient-switching re­qui­res less energy to create an echo than a 180° pulse. Thus, power deposition in the body of a patient is reduced, which is a major advantage of these sequences. How­ever, there are also a large number of disadvantages which have not yet re­sul­ted in FLASH replacing standard SE sequences in all instances.

Because of the shorter TR, FLASH sequences reduce not only the scan time but also the number of slices that can be acquired. Optimum repetition time has to be adjusted to the number of slices required and to other factors such as the duration of a breathhold for abdominal imaging or the heart rate in cardiac ima­ging. When decreasing the scan time, motion artifacts tend to be reduced, while flow artifacts will increase since the difference in signal intensity between blood and stationary tissue becomes more marked at short repetition times.

The feature can be exploited in FLASH-based cine-MR imaging where 8-32 lines of the same slice are acquired during one cardiac cycle, then the sequence is repeated for each phase-encoding step to produce 8-32 images, each of which represents a different stage of the cardiac cycle. The images are presented in the form of a closed movie loop, which depicts the function and dynamics of the heart.



Figure 08-06:

Principle of (a) a standard pulse sequence, compared to (b) a rapid imaging sequence of the FLASH type.
(a) In the spin-echo pulse sequence, the echo is created by a 180° pulse. This involves relatively long time delays and high power deposition in the examined sample. Because of the dependence of TR on T1, TR has to be relatively long.
(b) In the FLASH sequence, any pulse angle can be used instead of the initial 90° pulse. The echo is formed by gradient switching. This can be done faster and with less power deposition (potentially less hazardous for the patient). Thus, TR (and TE) can be shortened.
SE = spin echo; GRE = gradient (recalled) echo.


08-03-01 Transverse Coherences

When the repetition time for a FLASH sequence is reduced to a level where the repetition time TR is shorter than T2, the relaxation behavior is also influenced. This is due to the presence of transverse coherences [⇒ Freeman]. Their ex­ploi­ta­tion or suppression forms the basis of several fast imaging schemes based upon FLASH.

To understand why transverse coherence occurs, we have to modify the sim­ple idea of a spin echo. After a 90° pulse the spins start dephasing. When a 180° pulse is applied at a time τ after the 90° pulse, the rotation induced by the spin echo causes the magnetization to start refocusing and a spin echo forms at a time τ after the 180° pulse. This model is very useful since it gives a clear picture for the formation of a spin echo. However, it is not so easy to visualize the effect of pulses which are <180°.

These <180°-pulses also form spin echoes. When the flip angle is not equal to 180°, the amplitude of the echoes is reduced compared to that produced by a 180° refocusing pulse. In addition to the evolution of the z-magnetization, there is now also evolution of the transverse magnetization. The signal received con­sists of contributions representing fresh transverse magnetization and an echo term, which is the sum of all the possible echoes arising from combinations of the spin echoes created by pulses <180°.

By manipulating these parameters, three types of rapid FLASH imaging se­quen­ces can be defined.

Refocused FLASH (also known as FFE, FISP, FAST, GRASS, ROAST). These sequences measure the signal after the RF pulse, which corresponds to the com­bi­na­tion of the fresh transverse magnetization and the echo term [⇒ Frahm; ⇒ Sekihara]. They have a good signal-to-noise ratio, but generally rather poor con­trast. A very strong signal is obtained from flowing blood since the spins flowing into the slice will have equilibrium magnetization rather than the steady state magnetization of the stationary tissue (typically 10% of M0).

Contrast-Enhanced (CE-) FLASH (also known as CE-FFE, PSIF, SSFP). The­se sequences measure only the echo term [⇒ Hawkes]. To avoid contamination from the fresh magnetization present after the RF pulse, the echo term is ob­ser­ved prior to the RF pulse in the form of a gradient echo. CE-FLASH sequences provide good T2 contrast, but relatively poor signal-to-noise. Shortening the TR improves the signal-to-noise, but also reduces the contrast. Flow artifacts are ge­ne­ral­ly absent from CE-FLASH scans since the blood flows out of the slice du­ring the TR interval and thus cannot be refocused to give an echo.

Spoiled FLASH. This type of rapid pulse sequence observes only the fresh trans­verse magnetization. The echo term is removed (spoiled) by the use of either spoiling gradients or phase spoiling techniques. When a high flip angle is used, the spoiled FLASH sequence can give good T1 contrast.

Two other variants of FLASH sequences are the FADE sequence [⇒ Redpath] and the FISP sequence [⇒ Oppelt].

The FADE sequence combines the refocused and CE-FLASH sequences into a single sequence in which the two resulting signals are observed in separate ac­qui­si­tion periods during a single interpulse interval. Therefore, the minimum TR is longer, but the sequence is more efficient because we obtain two images with different contrast.

The FISP sequence is designed to superimpose the two signals which are se­pa­ra­te­ly acquired in FADE to give a single signal with excellent signal-to-noise ratio. Unfortunately, the sequence is not practical since, unless the two images are perfectly aligned, artifacts will result [⇒ van Vaals].

It is worth noting that the acronym FISP is used to refer to two different se­quen­ces (i.e., this sequence and refocused FLASH). A modification of refocused FLASH with refocusing of all three gradients is known as True FISP (and also Balanced FFE). This sequence is one of the most used sequences in cardiac ima­ging. An overview of many acronyms and abbreviations can be found in the List of Abbreviations.


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inkpot A comment about terminology, contents, acronyms
and abbreviations in magnetic resonance imaging:
Alphabet Soup.

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08-03-02 Ultrafast Gradient-Echo Sequences

The use of very rapid FLASH sequences (with TR in the range of 4-10 ms) allows to produce images in seconds or even in less than a second. These sequences are, for instance, used for abdominal imaging, commonly as a single-slice me­thod. They allow breath-holding and thus can eliminate ghost artifacts and blur­ring from respiratory motion.

In the basic snapshot FLASH sequence, no spoiler or refocusing gradients are included and a very low flip angle corresponding to the Ernst angle for such short TR values is used. Now, little or no transverse coherence is generated and the re­sul­ting images are essentially proton-density-weighted. To improve the contrast in these examinations, a preparation pulse can be used. Its function is to prepare the z-magnetization prior to starting the examination [⇒ Haase]. The scan times for 128×128 matrices vary between 0.5 and 1.0 seconds on clinical systems.

The main applications for snapshot FLASH sequences are in abdominal ima­ging, cardiac studies and functional (dynamic) imaging using contrast agents. In the first two cases, other techniques suffer from motion artifacts or long scan times when triggering is used. For dynamic imaging, the time resolution re­qui­red (1-3 seconds) means that snapshot sequences have to be used if a rea­son­able (128×128) resolution is to be obtained.

The advent of gradient-echo techniques with a preparation pulse, such as Turbo-FLASH, snapshot FLASH, and MP-RAGE allowed a shortening of examinations times maintaining the level of SNR – even for 3D imaging.

The three-dimensional Magnetization-Prepared Rapid Gradient Echo (3D MP-RAGE) is the 3D version of Turbo-FLASH and has developed into one of the most favored sequences for T1-weighted brain imaging. Details of this sequence are discussed in Chapter 10.

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