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This lecture focuses on the intricate processes underlying noise in MRI, highlighting the role of dipole moments, magnetic fields, and proton dynamics. Explore how the source of the signal, often linked to proton or water MRI, interacts with magnetic field strengths (B0) and thermal noise. Delve into the phenomena of Brownian motion and its significance in detecting signals amidst noise, while examining probability distributions such as Rayleigh and Rician. This overview is essential for understanding signal-to-noise ratio (SNR) dependencies in high-field MRI techniques.
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Dipole Moments from Entire Sample Magnetic Field (B0) Magnetic Field (B0) m m Positive Orientation Negative Orientation
Source of Signal • Proton or Water MRI • Bo Magnetic Field • Proton Nucleus • S = ±ħ/2 rg 2 2 h DE D µ = E M B z o 4 kT
z B1(t) F = w AB g cos( t ) 1 L g 2 w Ah B Ah = µ w w = w o L V ( t ) S ( t ) g sin( t ) g sin( t ) y L L L kT kT x Detected Signal
Brownian Motion • Brownian Motion Conditions: • x0= 0 • x(t) is a continuous random variable • Increments x(t1) and x(t2) are statistically independent and normally distributed http://en.wikipedia.org/wiki/Wiener_process
Rp Rc Johnson or “Thermal” Noise Electrical Resistance of Coil Patient Resistance Thermal noise in patient dominant at high field strengths
Johnson or “Thermal” Noise on both I and Q channels I = “in phase” Q = “quadrature” or 90o out of phase Imaginary Real
Independent Realizations of GWN on each of the I,Q channels Imaginary Real
Background noise Imaginary Real