## Abstract Viewβtoβview phase shifts due to B0 instability are corrected by applying a phase correction to the lowβspatialβfrequency views. The algorithm described herein assumes that the signal intensity in the space outside of an object represents only noise. A set of phases for the lowβspatialβ
PHASE DIFFERENCE CORRECTION METHOD FOR PHASE AND FREQUENCY IN SPECTRAL ANALYSIS
β Scribed by D. KANG; X. MING; Z. XIAOFEI
- Publisher
- Elsevier Science
- Year
- 2000
- Tongue
- English
- Weight
- 122 KB
- Volume
- 14
- Category
- Article
- ISSN
- 0888-3270
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β¦ Synopsis
A new method, phase di!erence corrections method is developed to correct the frequency and phase of spectrum peak. The continuous time-domain signal is separated into two segments and fast Fourier translation (FFT) is carried out for them, respectively. The frequency and phase are corrected using the phase di!erence of corresponding discrete spectral lines. Furthermore, the amplitude can also be recti"ed using the formula of window function spectrum. This method, with good adaptability, high speed and accuracy, is theoretically simple. It can resolve the frequency by means of phase di!erence directly without the formula of window function. Simulation shows that the single-component frequency, phase and amplitude of theoretical signal can be corrected satisfactorily, with frequency error less than 0.0002 frequency resolution, phase 0.13 and amplitude 0.0002. If the signal involves noise, the mean corrected errors are less than 0.001 frequency resolution, 13 for phase, and 0.01 for amplitude, respectively, and the maximum corrected errors of one segment are less than 0.01 frequency resolution, 13 and 0.03, respectively.
π SIMILAR VOLUMES
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