An approximate analytic expression is calculated for the phase of the transverse magnetisation during the excitation period. A spherical Bloch equation is used to find this expression. Simulation results are in agreement with the analytic solution. This analytic solution can be used where the phase information is required and, therefore, may be used to improve the performance of imaging through optimal pulse sequence design.
Assuming the Radio Frequency (RF) field is applied in the x'-direction, the Bloch equation during excitation for short pulses in the spherical coordinates for azimuth and colatitude components of the magnetisation vector in the rotating frame of reference can be written as5
$$ \left\{ \begin{array}{l l} \dot{\theta} = -\Delta \omega_0+\omega_1(t) \cot \phi \cos \theta\\ \dot{\phi} = \omega_1(t) \sin\theta\\ \end{array} \right.$$
where $$$\Delta \omega_0$$$ is the filed inhomogeneities including gradient fields, $$$\omega_1(t) $$$ is the excitation field, $$$\theta = \tan^{-1}\frac{M_{y'}}{M_{x'}}$$$ and $$$\phi = \cos^{-1}M_{z'}$$$ in which $$$M_{x'}$$$, $$$M_{y'}$$$ and $$$M_{z'}$$$ are the magnetisation components in the Cartesian coordinates. We have used available tools in nonlinear dynamical systems6,7 to find the phase of the magnetisation as follows
$$\theta (t) \approx \frac{\pi}{2} - \Delta\omega_0\,t +\tan^{-1}\left(\cot\int_0^t\omega_1(\tau) \cos(\Delta\omega_0\tau)\, d\tau \,\,\tanh \int_0^t\omega_1(\tau) \sin(\Delta\omega_0 \tau)\,d\tau \right).$$
The above expression is valid for hard as well as soft RF pulse excitations. Furthermore, if field inhomogeneities are time varying, e.g. time varying gradient fields, the above equation applies by replacing $$$\Delta\omega_0 \tau$$$ with $$$\int_0^\tau \Delta\omega_0(s) ds$$$.
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