mri physics: k-space anna beaumont frcr part i physics

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MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

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Page 1: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

MRI Physics: K-Space

Anna BeaumontFRCR Part I Physics

Page 2: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

K space questionsConcerning k-space: a. A line of data in k-space contains information

corresponding to a particular phase-encoding step b. The central part of k-space contains information

about low spatial frequencies c. Elimination of the periphery of the k-space would

result in poor contrast but a sharp image d. One abnormally bright pixel in k-space would

transform into a series of bright and dark circles originating from the centre of the final image

e. The entire k-space must be acquired in order for the information to be transformed into a usable image

f. The centre of K-space contains the data relating to high spatial resolution

Page 3: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

k?

• A wave is characterised by its wavelength (λ); the distance between two corresponding peaks.

• The wavenumber is k• k= 1/ λ

• k= the number of waves per unit distance• Spatial analogue to ‘cycles per

second’ (frequency)

Page 4: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

What is k-space?

K space is an array of numbers representing spatial frequencies in the MR image.

The readout MR signal is a mixture of RF waves with different amplitudes, frequencies and phases containing spatial information.

This signal is digitised and the raw data written into a data matrix called k-space

To go from k-space data to an image requires using a 2D inverse Fourier Transform.

The individual points in k space do not correspond to individual pixels in the image. Each k space point contains spatial frequency & phase

information about every pixel in the final image. Conversely, each pixel in the image maps to every point in k

space.

Page 5: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Fourier Transform (FT)

• S1 has amplitude a and frequency f

• S2 has a/2 and 3f• S3 = S1 + S2• S3 is two sine

waves of different frequency and amplitude

• The FT is shown

-3.5

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Page 6: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

What is k-space?

The Fourier transform can decompose images.

Instead of analysing a time varying signal, it decomposes a variation of intensity (grey levels) over distance.

Time domain becomes space domain and frequency is called spatial frequency.

Page 7: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

What is k-space?

Spatial frequency is related to the periodicity with which the image intensity values change.

Image features that change in intensity over short image distances correspond to high spatial frequencies.

Image features that change in intensity over long image distances correspond to low spatial frequencies.

To decompose a 2D image we need to perform a 2D Fourier Transform

Page 8: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

What is k-space?

Decompose image row by row

Obtain grey level intensities of chosen line

Perform 1D Fourier Transform

Obtain spectrum

Page 9: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

What is k-space?

Note: Low spatial frequencies (change in intensity over long distances) are prevailing

Low spatial frequencies have greatest change in intensity

High spatial frequencies (change in intensity over short distances) have lower amplitudes

General shape of the image is described by low spatial frequencies: this is also true with MRI images.

Page 10: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

What is k-space?

Final result is called a Fourier plane and is represented by an image:Horizontal and vertical axis correspond to

horizontal and vertical spatial frequencies.Pixel intensity corresponds to amplitude of

frequency componentCentre of k space corresponds to low spatial

frequenciesThe periphery of k space corresponds to high

spatial frequencies.

Page 11: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics
Page 12: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

What is k-space?

A spin echo sequence fills k-space line by line.

Each application of the FE gradient fills a line in kx

Increments in PE gradient fills each line in ky

Echo amplitudes are larger at low order PE steps (less gradient induced dephasing), values will be brighter near the centre of the grid.

Higher strength/ longer duration gradients cause more dephasing, hence greater differences

Page 13: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics
Page 14: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Contrast & Resolution in k-space

The location of the data in k-space depends on the net strength and duration of the PE and FE gradients.

A low amplitude or short duration gradient event encodes low spatial frequency information.

A high amplitude or long duration gradient event encodes high spatial frequency information.

Page 15: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Contrast & Resolution in k-space

Most MR information (contrast & general shape) is contained in the centre of k-space.Low spatial frequencies have the highest

amplitude, giving the greatest changes in grey levels (contrast)

However these changes are spread over the image and only give the general shape of the organs

Image is contrasted but blurry

Page 16: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Contrast & Resolution in k-space

High spatial frequency has lower amplitude

Sharpens the image as encoding the edges (rapid changes of image signal as a function of position).

The further from the centre of k-space, the higher the frequencies and the better the spatial resolution

Page 17: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

k-space

Full k-space Edge k-spaceCentre k-space

Page 18: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

k-space trajectories

GRE or SE: one line of k-space per TR

(usually 256, 512 lines)Image time = Nphase TR

EPI: all lines of k-spaceper TR (typically 64 or 128)

Image time = TR

ky

kx

Page 19: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

k-space trajectories

Radial k-space:Centre oversampled

Motion compensation

Spiral: more efficient single shot

Page 20: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Partial k-space

Partial Fourier:Also called fractional NEX

Collects half of phase-encode steps and speeds

up imaging

Partial Echo:Collects half of echo reducing the shortest

possible TE

These techniques acquire part of k-space and ‘fill-in’ the rest due to conjugate symmetry

kx

ky

Just over half data collected

Page 21: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Summary: Key points

Spatial encoding uses gradients.

The data acquired are mapped into k space so that an inverse Fourier transform reconstructs the MR image.

The location of the data in k space depends on the strength and duration of the gradients. If no gradient applied, the location is at the centre

of k spaceThe higher the strength or the longer the duration,

the further from the centre of k space the data will be located.

Page 22: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Summary: Key points

Simplest way to fill k-space is line by line.

One line of k-space is fully acquired at each excitation (containing low and high horizontal spatial frequency information).

Between each repetition there is a change in PE gradient strength.

This allows filling of the lines of k-space from top to bottom.

Page 23: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Summary: Key points

Each point in k space encodes for spatial information of the entire MR image.

Each point of the MR image is the result of the combination of ALL the data of k-space.

Centre of k-space contains low spatial frequency information.Most image information is contained in low spatial

frequency information: general shape & contrast.Periphery of k-space does not correspond to

periphery of image: it contains high spatial frequency.The higher the spatial frequency, the smaller the

details of the image (edges and spatial resolution).

Page 24: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

K space -answersConcerning k-space: a. A line of data in k-space contains information corresponding

to a particular phase-encoding step - TRUE b. The central part of k-space contains information about low

spatial frequencies – TRUE. This contributes to the bulk of the image contrast.

c. Elimination of the periphery of the k-space would result in poor contrast but a sharp image – FALSE. This would result in blurry images, i.e poor spatial resolution, but contrast would be preserved. As contrast is more important for the final image, acquisition of the k-space periphery can sometimes be omitted to gain imaging speed, but sacrificing sharpness.

D. See artefact lecture

Page 25: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

K space -answers

Concerning k-space: e. The entire k-space must be acquired in order for the

information to be transformed into a usable image – FALSE. It is sufficient to acquire just over one-half of the k-space. As k-space is symmetrical, the acquired half may be ‘mirrored’ (with appropriate mathematical corrections) into the missing half and the image reconstructed without loss of spatial resolution but with decreased SNR. This is sometimes known as half or fractional NEX imaging.

f. The centre of K-space contains the data relating to high spatial resolution – FALSE – The periphery of K-space contains data relating to spatial resolution. The centre contains data for high signal intensity.

Page 26: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Imaging Issues

Page 27: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Anatomical Axes for FE/PE

FE and PE directions can be swapped.

PE information takes longer to acquire, so useful to avoid PE in direction of any potential motion artefacts.

Phase encoding also susceptible to Phase Wrap artefacts (more on that in Lecture 9)

To avoid this, make sure no anatomy outside of FOV in PE direction. E.g. in a coronal head scan, use R-L for

PE (all anatomy inside the FOV), and S-I for FE

Page 28: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Multi slice imaging Dead time in TR whilst waiting for a

sequence to repeat can be used to excite other slices.

For example: TR =600ms, TE = 20ms for T1

weighting Take ~ 30ms to excite the slice,

generate the spin echo and collect the data. 570ms left before we can excite that slice a second time.

Use time to excite a different slice… and another…

Second slice chosen will have a small gap to avoid artefacts called cross-talk.

Page 29: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Frequency aliasing The MRI signal is a rapidly changing

analogue electric voltage in the receiver coil, oscillating at high frequencies.

It needs to be converted into a digital signal, before being reconstructed into the final image.

The digital signal needs to be an accurate representation of the digital signal, so needs to be sampled at a high enough rate.

Page 30: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Frequency aliasing Nyquist Law: If ωmax is the max. frequency in the signal, then the

sampling rate must be at least twice the maximum signal frequency to avoid aliasing, i.e. ωsampling = ≥2 ωmax

Page 31: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Frequency aliasing Not common due to oversampling Need to sample at least twice highest

frequency Nyquist frequency

(above) high-frequency inadequately sampled and misinterpreted as low frequency

Page 32: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Image Quality

IQ depends on:Spatial resolution & image contrast

Signal to Noise Ratio (SNR)Artefacts

MRI scan is a compromise between scan time and image quality

Page 33: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Image QualitySpatial Resolution Noise

Contrast Artefacts

Page 34: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Image Quality Noise is a random variation in signal

Main source of noise is patient’s body, but also everything in the scanner (coils, electronics etc.)

Page 35: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Noise Noise comes from random fluctuations in

electrical current. Exists in all electrical conductors Also includes electrically conducting

tissues of the patient Human tissue contains many ions such as

sodium, potassium and chloride. These are electrically charged atomic

particles carrying currents within the body, e.g. in nerve conduction.

These currents generate fluctuating magnetic fields which induce a noise voltage in the coil.

Most effective way to reduce this is to use a dedicated anatomy coil

Page 36: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Image Quality Image Contrast

Varies with pulse sequence & sequence parameters

Spatial Resolution Size of smallest detectable detail Smaller voxels= higher spatial

resolution Voxel volume determined by matrix

size (how many pixels FOV divided into), Field of view & slice thickness

However; smaller voxels → lower SNR

Page 37: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Image Voxel

Field-of-view (FOV)

Single pixel

Slicethickness

Pixel size = FOV/matrix

Matrix size typically 256 or 512

For example: a 32cm FOV with a 256 (FE) x 192 PE and slice thickness of 4.5mm will give a voxel size of 1.25 x 1.67 x 4.5 mm3.

Page 38: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Spatial Resolution• Controlled by size of voxel.• Voxel volume affected by

• Slice thickness• FOV• Matrix

Smaller voxels give better resolution However; small voxels could have too little signal

compared to noise, therefore SNR is worse. = Trade off: need to determine voxel size required

for adequate SNR, but small enough to visualise relevant pathological detail.

• Matrix size ↓, SNR ↑ , Resolution ↓• FOV ↑, pixel dimension ↑ , SNR ↑, Resolution ↓• Slice thickness ↑, SNR ↑, Resolution ↓

Page 39: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

SNR Depends on:

Fixed factors (user not able to vary): Static Field intensity Pulse Sequence Design Tissue Characteristics

Variable factors (under the operator’s control): RF coil (Surface coils have higher SNR than

body coils) Receiver bandwidth (more noise for wider

bandwidth, but faster sampling) Sequence parameters

SNR is a trade-off with image contrast Increasing TR improves SNR Decreasing TE improves SNR

Page 40: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

SNR• ↑ as B ↑ (more spin up than spin down as

fewer have energy to oppose field. Net magnetisation vector ↑)

• NEX= no. of times frequencies in signal are sampled with the same slope of phase encoding gradient

• Increasing the NEX increases the signal collected. However; noise also sampled.

• As noise occurs at all frequencies and randomly, doubling the no. of signal averages only increases the SNR by √2

• Receiver bandwidth ↓, SNR ↑ (noise sampled ↓ relative to signal)

• However; bandwidth ↓ chemical shift artefact ↑

Page 41: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

What is needed? Certain applications, e.g. MR angiography work

better with higher resolution.

However; you generally need a certain SNR whatever the resolution.

Mc Robbie et al. states that a SNR of >20:1 offers little image quality advantage and excess SNR would be better converted to either a larger matrix or shorter scan time.

IF SNR is adequate, high resolution will look better, but diagnostic advantage of 1024 over 512 matrix has not yet been established.

Page 42: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Images from “From Picture to Proton”

Some images

Page 43: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Images from “From Picture to Proton”

Some images

Page 44: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Can now understand MR image!

Exam/Series/Image

Scan plane, position

Sequence

Timing (weighting)

RF coil

Slice information

Scan timeMatrix, Averages

FOV

Frequencydirection

Page 45: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

Apply phase encoding gradient

slower unchanged faster

Page 46: MRI Physics: K-Space Anna Beaumont FRCR Part I Physics

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