- 00000018WIA30B69870GYZ
- id_400257031.3
- Feb 25, 2022 4:18:55 PM
Spectroscopy scan parameter selections
The use of the scan parameter selections and entries with the spectroscopy pulse sequences are discussed in detail in the following sections. For specific scan parameter values, select a protocol from your GE or Site library.
Patient position
Coil
Scan parameters
| Parameter | Description |
|---|---|
| Scan plane |
Select the appropriate scan plane. For Graphic Rx, remember that the STEAM CSI, Press CSI, PROBE-S, and PROBE-P voxels are prescribed in the same scan plane as the scan plane of the localizer images, while slices are prescribed orthogonal to the plane of the localizer images. |
| Mode |
Select 2D to select a slice selective PSD. Select MRS to select a voxel localizing sequence. |
| Pulse sequence |
In the 2D mode, you can select an MNS Family sequence:
|
| Imaging Options |
The following Imaging Options are compatible with the spectroscopy pulse sequences:
Extended Dynamic Range is a recommended choice given the low signal common to spectroscopy data acquisitions. The spectrum may be inverted. Make sure Extended Dynamic Range is turned on. If it is on and the spectrum is still inverted, correct the inversion in READY View : Adjust the Voxel shift procedure. |
| TE |
The echo time is used in six of the eight spectroscopy sequences. The FID CSI (MRS) sequence acquires an FID rather than an echo, so TE is not relevant. The Spin Echo (MRS) sequence has a fixed echo time of 2.5 ms, so the TE selection is not available. |
| TR |
The sequence repetition time. Since long repetition times lead to long exam times, the TR selection is often a compromise between acceptable signal loss due to saturation, and the length of the exam. For example, the minimum TR for the PRESS CSI and PROBE-P sequences is about 1.1 seconds while 5*T1 = 3 to 5 seconds for the common proton resonances in the human brain. A TR of 1.5 to 2.0 seconds provides a reasonable compromise between signal saturation at shorter TR values, and the increased patient examination times at longer TR values. Auto Prescan always uses TR = 1500 ms, rather than the prescribed TR. |
| Flip angle |
The nominal flip angle (power) of the RF excitation pulse in the Spin Echo (MRS) spectroscopy sequence. This parameter is inactive for the other spectroscopy sequences. |
| FOV |
The FOV parameter determines the field-of-view along the frequency direction. |
| Slice thickness |
If Graphic Rx is used, the Slice Thickness or Voxel Thickness may not be available, and explicit entries may be required in the S/I, P/A, or R/L text boxes. |
| Slice spacing |
A CSI Slice Thickness entry may be required. The value is ignored just as in imaging scan prescriptions unless the signals from more than one slice are acquired or 3D CSI is performed. |
| S/I, P/A, R/L |
Entries are always required for the S/I, P/A, or R/L text boxes. Entries and field names change depending on the pulse sequence, and on whether Graphic Rx is used to prescribe voxel or slice location. |
| Number of slices |
The CSI Slices value should be 1, unless signals are actually being acquired from several slices or 3D CSI is performed. |
| Table delta |
The Table Delta field is ignored by all spectroscopy PSDs (set to 0.0 if an entry is required). |
| Frequency and Phase |
Frequency and Phase choices not only affect the data acquisition but they also determine the number of zero-fills applied during the reconstruction process, and the aspect ratios of the reconstructed images. The allowed Frequency and Phase values are 8, 10, 12, 14, 16, 18, 20, 22, and 24. No zero-fill is applied for the 8 and 16 selections, that is, the number of reconstructed CSI voxels is 8 or 16 along that dimension. The 10, 12, and 14 selections are zero-filled to 16, and the 18, 20, 22, and 24 selections are all zero-filled to 32 during the reconstruction. |
| Frequency Direction |
Just as with standard imaging sequences, the default setting of the Freq DIR is usually the best choice. Swapping the phase and frequency directions, which for the voxel localized sequences has the effect of re-ordering (in time) the gradients used to define the voxel may help to eliminate artifacts. |
| Shim |
Auto should be selected for all hydrogen spectroscopy acquisitions to insure that the water suppression pulses, saturation pulses, and slice selective pulses are transmitted at their correct frequencies. It should not be selected when acquiring signals from any other nuclei. |
| NEX |
The value of NEX is the number of excitations in a single frame of data, where the acquisition of a single frame may require one or more passes through a phase cycle (see Phase Cycling).
|
Graphic Rx
Graphic Rx is available whenever a valid localizer image exists. You can graphically prescribe an ROI with the MRS sequences. Graphic ROI prescription requires that the scan plane of localizer image(s) must be the same as the prescribed scan plane. Click on the image to display the box cursor (ROI).
Phase cycling
Phase cycling is the repetition of a pulse sequence and signal acquisition such that all acquisition parameters except the phase of the RF pulses (and, possibly, the receiver phase) remain unchanged from repetition to repetition. Phase cycling suppresses or eliminates undesirable signals while taking advantage of the effects of signal averaging. In the current spectroscopy pulse sequences, only the RF phase is changed, or cycled, in the repetitions.
In one of the simpler examples of a phase cycling scheme, a pair of excitations is obtained with the phase of an RF pulse used in the second acquisition inverted relative to the phase of the RF pulse used in the first acquisition, causing an inversion of the desired signal between the two acquisitions. The second excitation is then subtracted from the first to produce a single frame. The result is that the first signal and the inverted second signal are added together while the RF errors independent of the phase of the RF pulses are canceled by the subtraction.
The spectroscopy sequences always use the largest phase cycle that is compatible with the selected NEX value.
Homogeneity adjustments - gradient shimming
It is possible to manually adjust the linear x, y, and z shims by adjusting the corresponding gradient current offsets on the Spectroscopy screen. However, adjusting the homogeneity through manual shimming is neither fast nor easy, particularly for nuclei other than hydrogen. For most users and for most applications a better choice is to rely on the Autoshim capabilities of the system.
The hydrogen based Autoshim capability is both fast and reliable, and should be used to optimize the shim whenever possible.
Generally, Autoshim should be selected during the acquisition of the localizer image(s).
For voxel localized spectroscopy, the shim through the voxel can be improved by running Auto Prescan with Autoshim for the slice containing the voxel prior to prescribing the spectroscopy data acquisition.
For slice localized spectroscopy, the shim across the slice can be optimized by running Autoshim as part of an imaging sequence Auto Prescan process for the same slice that is selected in the spectroscopy data prescription. If the focus of the acquisition is a small region of the slice, prescribe a PRESS CSI scan with a voxel that covers the small region, and use Auto Prescan with Autoshim to optimize the shim through the voxel.
Spectroscopy data
- Complex Point: The complex point is the simplest data unit. It is produced from the signals acquired by the receiver during data acquisition. The digitized signals are stored as 4 byte integers, or, if the Extended Dynamic Range Imaging Option is selected, 8 byte integers. According to standard imaging usage, the complex point consists of an I and Q pair, where I is the in-phase component, and Q is the quadrature component. The I and Q components are treated as the real and imaginary parts, respectively, of a complex number.
- Excitation: An excitation is the collection of a selected number of complex points acquired during a single pass through a pulse sequence. For spectroscopic data acquisitions, an excitation consists of 256, 512, 1024, or 2048 complex points. The number of complex points in an excitation is set by the Number of Points User CV.
- Frame: A data frame consists of a single excitation, or the average of two or more excitations. A frame contains the same number of complex points as a single excitation. The number of excitations that are combined to produce a frame depends on how the data are acquired, and/or on the values of a number of CVs.
- When acquired from the Scan Operations screen with Scan or from the Spectroscopy screen with Start in the single1 Entry Point, the number of excitations equal to the value of NEX is averaged to produce a frame.
- When acquired with Start in the avg Entry Point, a single frame of data is created from all acquired excitations. If the acquisition terminates automatically, the number of excitations is equal to the Total Number of Scans User CV. If an avg data acquisition is terminated with Stop at anytime prior to the completion of the acquisition, the frame in the temporary data buffer is the average of the excitations acquired at the end of the current phase cycle. If the data are saved with Save, the information in the raw file header related to the value of the number of points may be incorrect.
| Spectroscopy data | Details |
|---|---|
| Spectroscopy raw data files |
All spectroscopy raw data files are written to the system directory /usr/g/mrraw. There are two possible file types: standard system raw data files known as “P files;” and Spectroscopy Screen Save “P files.” Standard “P files” are automatically created and saved for all spectroscopy data acquisitions initiated with Scan from the Scan Operations screen. The Spectroscopy Screen Save “P files” are created and saved when the Save button is clicked on the Spectroscopy screen. Generally, a raw data file consists of a raw file header, and one or more raw data frames; the number of data frames in a raw data file depends on the acquisition prescription and the acquisition technique. |
| P raw data files acquired with Scan on the Scan Operations screen |
When spectroscopy data sets are acquired, they are automatically saved to the /usr/g/mrraw directory. There are only 196 unique raw data “P file” names available. An existing file will be overwritten whenever a new file with the same name is saved.
In its simplest form, a standard “P file” begins with a raw file header, followed immediately by a single baseline frame, and then by a number of raw data frames. The simplest form corresponds to the acquisition of spectroscopy data from a single slice or voxel with a single receive coil. On the other hand, a multi-slice data set contains the raw file header, a baseline and frames from the first slice, followed by the baseline and frames from the second slice, and so on to the baseline and frames from the last prescribed slice. Similarly, data sets acquired using a phased array coil contain the raw file header followed by a baseline and frames from each of the active coils in the array. There are two types of raw spectroscopy data sets that can be acquired with Scan: Accumulate and CSI raw data sets.
For example, if a 24*24 two-dimensional CSI data set is acquired with CV1 = 1024, and EDR is not selected, there are 577 raw data frames (24*24 + 1, remember the baseline frame). Each data frame contains 1024 complex data points of 8192 bytes (= 2 * 4 * 1024), and a 61464 byte header. The size of the data set is therefore: (61464 + 577 * 8192) bytes = 4788248 bytes. |
| P raw data files acquired and saved on the Spectroscopy screen |
The Spectroscopy Screen Save “P files” are created when you click the Save button on the Spectroscopy screen. Spectroscopy Screen Save file names start with the letter “P”, followed by the five digit run number, a period (.), the number “7”, another period, and two more numbers, usually two zeroes; for example, P10240.7.00. The “00” portion of the file name is used to differentiate files saved during or from the same acquisition. For example, if you acquired a data set and clicked Save to create the file P01024.7.00, and then clicked Save again without acquiring a new data set, the second file would be named P01024.7.01. As with the standard raw file names, there are only 196 unique Spectroscopy Screen Save file names, and existing files are overwritten by a new file with the same name. A Spectroscopy Screen Save “P file” begins with a raw file header, followed immediately by at least one raw data frame – there is no baseline fame. A raw data frame is stored in the raw file for the signal acquired from each slice of a multi-slice acquisition, and/or for the signal acquired from each receive coil in a phased array coil set. The number of bytes in a raw data frame is determined by the Number of Points User CV, and by the Extended Dynamic Range Imaging Option. The number of data frames in a spectroscopy screen saved raw file depends on the number of prescribed slices and/or on the number of receive coils used to acquire the data. For example, the raw data file acquired from two slices with avg and Start on the Spectroscopy screen with the Number of Points = 2048, and Extended Dynamic Range not selected contains 94232 bytes (the 61464 byte raw file header, the 16384 byte data frame from the first slice, and then the 16384 byte frame from the second slice). |
| Types and formats of spectroscopy data sets |
The spectroscopy pulse sequences can collect several different kinds of data sets:
|
| Data acquisition examples |
Several simple spectroscopy prescription examples are presented to illustrate the data type and data acquisition concepts. |
Data acquisition examples
Several simple spectroscopy prescription examples are presented to illustrate the data type and data acquisition concepts.
| Data acquisition example | Details |
|---|---|
| Data Acquisition of an averaged data set |
|
| Data Acquisition of an accumulate data set |
|
| Data Acquisition of a CSI data set |
|
Entry Points
| Entry points | Details |
|---|---|
| single1 Entry Point |
Single1 is the default Entry Point on the Spectroscopy screen and is invoked by clicking the Start button. Data are acquired and displayed in a continuous loop; i.e., the signal is averaged for one complete phase cycle, displayed, discarded, and the process repeated. The data acquisition and display continues until the Stop button is clicked. Click the Save button to save the raw data as data storage is not automatic on the Spectroscopy screen. The single1 Entry Point is designed for the manual optimization of data acquisition parameters – i.e., R1, R2, TG, Center Frequency, and Gradient Shim currents – and for the optimization of the data display through the line broadening entry, and the zero- and first-order phase corrections. Currently, these parameters can only be changed in the single1 Entry Point. |
| avg Entry Point |
The avg Entry Point is selected by typing avg in the Entry Point text box and clicking Start. It acquires and displays signal-averaged spectroscopy data. The data acquisition stops automatically when the prescribed number of excitations (total number of scans) has been acquired. Click Save to save the raw data as data storage is not automatic on the Spectroscopy screen. It is not possible to change the phase correction or line broadening entries, or to modify or reset any hardware parameter settings while acquiring data with the avg Entry Point. |
RF power scaling
One of the fundamental parameters that must be adjusted and optimized for each data acquisition is the RF transmitter power though the TG value. The following rules should enable you to correctly set the power for each pulse sequence and for all spectroscopy data acquisitions.
| RF power scaling | Details |
|---|---|
| Proton Spectroscopy |
All PSDs support Auto Prescan when acquiring proton spectra. To set the transmit power, click Auto Prescan. The APS process automatically adjusts the power level for the RF pulses specified in the data acquisition prescription. |
| Proton Spectroscopy with Spin Echo (MRS) |
The values returned by the APS processes for the Spin Echo (MRS) sequence are only approximations of the correct values. You should use the Spectroscopy screen tools to optimize and set the R1, R2, TG, and Center Frequency values. |
| Spectroscopy with nuclei other than hydrogen |
APS is not supported for use with nuclei other than hydrogen; you must set the transmitter power (TG) manually. This is usually done by maximizing the signal level received while modifying TG. The single1 Entry Point with Start on the Spectroscopy screen should be used for this purpose – it may also be necessary to adjust the R1 and R2 receive gains while optimizing the transmit gain. |
| RF excitation and refocusing pulses |
The frequency of the RF excitation pulses in the spectroscopy pulse sequences is set according to the value of the center frequency determined by the APS processes, or set to the value entered with the AX or DX commands on the Manual Prescan screen or the Spectroscopy screen. For the acquisition of hydrogen spectroscopy data, you should select Water in the Chem SAT menu; with this selection, the APS processes attempt to center the RF carrier frequency on the water peak in the spectrum. If the center frequency determined by APS is not centered on the frequency of the water resonance, the sequences may not behave as designed. The default settings of the RF pulses used for water suppression, spatial saturation, inversion recovery, and even excitation may require manual adjustment. The excitation, water suppression, saturation, and inversion recovery pulses are transmitted relative to the center frequency and may not be effective if the center frequency is not centered on the water resonance. Excitation pulses in the FID CSI (MRS), Echo CSI (MRS), and Spin Echo (MRS) sequences are transmitted at the center frequency. For the STEAM CSI, PROBE-S, PRESS CSI, and PROBE-P sequences, the frequency of the slice selective RF pulses is offset from the center frequency by -128 Hz (an offset of about 2.00 PPM). This frequency offset minimizes chemical shift misregistration between the water localizer image or the voxel image, and the extremes of the observed frequency range in the spectra. The spectroscopy pulse sequences use a variety of crafted RF pulses that were designed using the Shinnar-LeRoux algorithm. Where possible, the same pulses are used in different sequences to provide slice or voxel profile consistency. The RF pulses are designed to have a specific time-bandwidth product, which defines a fixed relationship between the width of the pulse and the effective bandwidth of the pulse. |
| RF pulse length | Bandwidth | Pulse Sequence |
|---|---|---|
| 90° 1.800 ms | 2288 Hz | FID CSI (MRS) |
| 90° 1.800 ms | 2500 Hz | Echo CSI (MRS) |
| 90° 3.600 ms | 2367 Hz | PRESS CSI, PROBE-P, STEAM CSI, PROBE-S |
| 180° 6.000 ms | 1200 Hz | Spin Echo (MRS) - self refocusing pulse |
| 180° 5.200 ms | 650 Hz | Echo CSI (MRS) |
| 180° 5.200 ms | 1384 Hz | PRESS CSI, PROBE-P |
