Low Field MRI of Laser Polarized Noble Gases. Yuan Zheng, 4 th year seminar, Feb, 2013

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Low Field MRI of Laser Polarized Noble Gases Yuan Zheng, 4 th year seminar, Feb, 2013

Outline Introduction to conventional MRI Low field MRI of Laser Polarized (LP) noble gases Spin Exchange Optical Pumping (SEOP) Nuclear Magnetic Resonance (NMR) signals MRI Gradient Coils Xe-129 gas MRI He-3 gas MRI Adapting our apparatus for small animal MRI

Outline Introduction to conventional MRI Low field MRI of LP noble gases Spin Exchange Optical Pumping (SEOP) Nuclear Magnetic Resonance (NMR) signals Gradient Coils Xe-129 gas MRI He-3 gas MRI Adapting our apparatus for small animal MRI

Conventional MRI Introduction to MRI First paper about Magnetic Resonance Imaging: P. C. Lauterbur, Image Formation by Induced Local Interactions: Examples Employing Nuclear Magnetic Resonance, Nature, 242, 1973 Since then, MRI has experienced rapid growth and is now the most powerful diagnostic tool.

Conventional MRI Advantages: 1) Safety: Non-invasive, no radiation 2) Flexibility: Pros and Cons of MRI a, Image content is under control b, Image of an arbitrary plane can be obtained. Disadvantages: 1) Expensive 2) Not for everyone 3) LIMITED FOR LUNG IMAGING

Outline Introduction to conventional MRI Low field MRI of LP noble gases Spin Exchange Optical Pumping (SEOP) Nuclear Magnetic Resonance (NMR) signals Gradient Coils Xe-129 gas MRI He-3 gas MRI Adapting our apparatus for small animal MRI

Low field LP gas MRI A new branch for MRI: Laserpolarized (LP) Noble Gas Lung Imaging. M.S. Albert, G.D. Cates, et al, Biological magnetic resonance imaging using laser-polarized 129 Xe, Nature, 370, 1994 a, 4.5mM of 40% polarized 3He b, conventional proton MRI of the lung parenchyma Sean B. Fain, et al. Functional Lung Imaging Using Hyperpolarized Gas MRI

Low field LP gas MRI Advantages of performing MRI at a low field: More homogeneous holding field Compatible with pacemakers and other metal implants Much Cheaper Low field imaging is only possible with LP noble gases.

Spin Exchange Optical pumping N N P = N + N N and Polarization of a spin-1/2 system + + N + Thermal Polarization: γ B P = tanh( ) 2kT are the number of spins in each of the two possible states. 1 6 At T=300K, the polarization of H in 1T field 3.4 10. 3 129 By SEOP, polarization of He or Xe 50%, 5 10 times higher! That's why they are also called Hyperpolarized (HP) gases. ~ ~

Two steps in SEOP: Spin Exchange Optical pumping 1) Optical Pumping: alkali vapor is spin polarized by the laser. D1 light, 795nm 5P 1/2 5S 1/2 Collisional Mixing 1 m J = 2 1 m J = 2 σ + m J = m J = 1 2 Non-radiative Quenching 1 2 P P Spin Relaxiation R Rb = ~ light R +Γ Rb 100%

Spin Exchange Optical pumping 2) Spin Exchange: spin is transferred to the noble gas nuclei. 129 Xe Rb 3 He Rb T T Xe Rb 3 He Rb T T 129 Xe Rb Binary Collision P = P g Rb se γ se Formation of a Van der Waals molecule γ +Γ

SEOP basic setup Spin Exchange Optical pumping Oven Holding coil Laser beam A glass cell with some alkali metal, some buffer gas and 3 He or 129 Xe is placed in the oven. The alkali vapor density is controlled by the oven temperature. Fiber Head To the Oven Polarizing Cube One laser beam is splitted into two beams, both of which are circularly polarized. QWP QWP

Nuclear Magnetic Resonance Signals Manipulate the Spins Two techniques to study a NMR signal 1. Adiabatic Fast Passage. (AFP) a) RF on b) Sweep the holding field and take data c) RF off 2. Pulsed Nuclear Magnetic Resonance (PNMR). a) RF on b) RF off c) Take data z The holding coils, RF coils and pickup coils are perpendicular to each other. RF Induced signal

Nuclear Magnetic Resonance Signals Spins in a Magnetic Field Spinning top in gravity field: dl = mr g dt Spin motion: d µ = γµ B, 0 µ = γ J dt Same solution: Precession f = γ B 0 0 Effective holding field in a rotating frame: B = B + 0eff 0 f γ

Nuclear Magnetic Resonance Signals Interaction with a Radio Frequency (RF) field Consider applying a RF in the transverse plane. z B 1 In a frame rotating at the RF frequency, the effective field is: ( f B ) ˆ 0 1ˆ ' eff = B + z+ Bx γ f ( B ) γ ˆ 0 + z B eff If f = f0 = γ B0 B eff = Bx ˆ 1 ' Spin precess along xˆ '! Bxˆ ' 1

Nuclear Magnetic Resonance Signals Free Induction Decay (FID) Transvers spins precessing along the holding field with a decaying amplitude will induced an EMF in the pick up coil. Two reasons for the amplitude decay: 1) Internal Spin-Spin relaxation time T 2. 2) External relaxation time T 2. (Due to field inhomogeneity) Observed T 2 : x 1 1 1 1 = + T T T T * ' ' 2 2 2 2 y z Φ Signal gets smaller Spins tipped by the RF t = 0, Φ = 0 Spins 'fan out' t = τ, Φ = γ Bτ

Gradient Coils MRI setup SEOP setup + Gradient coils MRI Gradient Coils Top View 54.7 Front View 54.7 Near anti-helmholtz coil pairs at special orientations.

Gradient Coils Why 54.7? (This is usually called the magic angle θm) What really matters is how the holding field (Bz) varies. Bx / x By / x Bz / x B = Bx / y By / y Bz / y Bx / z By / z Bz / z κ = 2 2 2 sin ( θ)cos ( φ) -1/3 sin ( θ)sin( φ)cos( φ) sin( θ)cos( θ)cos( φ) 2 2 2 = 3κI sin ( θ)sin( φ)cos( φ) sin ( θ)sin ( φ) - 1/3 sin( θ)cos( θ)sin( φ) 2 sin( θ)cos( θ) cos( φ) sin( θ)cos( θ)sin( φ) cos ( θ) 1/ 3 2 3π na d 5( d + a ) 2 2 5/2 G( cm A) 1 The magic angle is special because it eliminates the z gradient. 2 cos ( θm) 1/ 3 = 0

Gradient Coils Z gradient: θ = 0, φ = 0. Bx / x By / x Bz / x 1 0 0 B(0,0) = Bx / y By / y Bz / y κ I 0 1 0 = Bx / z By / z Bz / z 0 0 2 X gradient: θ = θ, φ = 0. 1 0 2 B( θm,0) = κi 0 1 0 2 0 0 Y gradient: θ = θ, φ = 90. 1 0 0 B( θm,0) = κi 0 1 2 0 2 0 m m Purposes of the Gradients: All the three gradients are used to trim the holding field so that the Free Induction Decay has a longer T 2 *. (less than 200 ms without trimming) We take 2D images without slice selection. X and Y gradients are applied as imaging gradients to acquire images of the sample projected on the XY plane.

Xe-129 MRI Procedure 1, Polarize the sample by SEOP. Our sample is a X shaped glass cell with 2.8 atms of isotopically enriched 129 Xe. We keep the oven at 85 C and the polarization reaches 5% in 4 mins. Xe-129 gas MRI P P P R Rb = light R +ΓRb = P γ g Rb se γ se +Γ

Xe-129 gas MRI 2, Excite the spins to the transverse plane. Apply appropriate Gradients and record the data. Only one line of k space data is taken. k = 2 πγ Gt, While traveling in k space, the spins precess in a controlled manner and the interference signal is recorded. 3, Repeat step 1 and 2 to collect more data in k space. We take 32 lines in k space and the whole procedure takes 2 hours. 4, Image reconstruction. sk Fourier Transform ( ) ρ ( x)

Xe cell and Image Xe-129 gas MRI Shown above is an image with 8 averages. Both x and y direction resolutions are 1mm. Image artifacts: 1, Central bright area. 2, Dimness in the lower legs.

He-3 gas MRI He-3 MRI Procedure 1. Polarize He-3 gas by SEOP. A much larger magnetization can be achieved. 2. Perform MRI using a Fast Low Angle Shot (FLASH) pulse sequence. Tip the spins by a small angle. Apply necessary gradients and take data for one line. Repeat 32 times. Advantages of FLASH Imaging: 1. Only polarize once. 2. Much faster. He cell (2.8 atm) and its image Resolution: 1mm

Outline Introduction to conventional MRI Low field MRI of LP noble gases Spin Exchange Optical Pumping (SEOP) Nuclear Magnetic Resonance (NMR) signals Gradient Coils Xe-129 gas MRI Procedures He-3 gas MRI Procedures Adapting our apparatus for small animal MRI

Small animal MRI Even small animals are still bigger than our pickup coils (1 ). Bigger pickup coils need to be built for bigger subjects. r SSSSSS r 3 r 2 r 3 = r 2 NNNNN r 2 S/N is a constant. However, gas density will be lower but we can perform MRI in a well shielded room. 2.8 atm 1 atm Pickup noise Johnson noise