VIII. Motions on the Time-Frequency Distribution

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VIII. Motions on the Time-Frequency Distribution Fourier spectrum 為 1-D form,只有二種可能的運動或變形: Modulation f 0 f0 Scaling Time-frequency analysis 為 2-D,在 2-D 平面上有多種可能的運動或變形 (1) Horizontal shifting (2) Vertical shifting (3) Dilation (4) Shearing (5) Generalized Shearing (6) Rotation (7) Twisting

8-1 Basic Motions (1) Horizontal Shifting (2) Vertical Shifting

(3) Dilation (scaling) f t

(4) Shearing f t

(Proof): When

(5) Generalized Shearing 的影響? J. J. Ding, S. C. Pei, and T. Y. Ko, “Higher order modulation and the efficient sampling algorithm for time variant signal,” European Signal Processing Conference, pp. 2143-2147, Bucharest, Romania, Aug. 2012. J. J. Ding and C. H. Lee, “Noise removing for time-variant vocal signal by generalized modulation,” APSIPA ASC, Kaohsiung, Taiwan, Oct. 2013

8-2 Rotation by /2: Fourier Transform (clockwise rotation by 90) Strictly speaking, the rec-STFT have no rotation property.

For Gabor transforms, if then (clockwise rotation by 90 for amplitude)

If we define the Gabor transform as , and then

If is the WDF of x(t), is the WDF of X( f ), then   (clockwise rotation by 90) 還有哪些 time-frequency distribution 也有類似性質?

 If , then , (counterclockwise rotation by 90).  If , then , . (rotation by 180).

Examples: x(t) = (t), X(f) = FT[x(t)] = sinc( f ). WDF of (t) WDF of sinc( f ) Gabor transform of (t) Gabor transform of sinc( f )

If a function is an eigenfunction of the Fourier transform, then its WDF and Gabor transform have the property of  = 1, −j, −1, j (轉了 90º之後,和原來還是一樣) Example: Gaussian function

Hermite-Gaussian function Hermite polynomials: , Cm is some constant, , Dm is some constant, m,n = 1 when m = n, m,n = 0 otherwise. [Ref] M. R. Spiegel, Mathematical Handbook of Formulas and Tables, McGraw-Hill, 1990.

Hermite-Gaussian functions are eigenfunctions of the Fourier transform Any eigenfunction of the Fourier transform can be expressed as the form of where r = 0, 1, 2, or 3, a4q+r are some constants

WDF for 1(t) Gabor transform for 1(t)

Problem: How to rotate the time-frequency distribution by the angle other than /2, , and 3/2?

8-3 Rotation: Fractional Fourier Transforms (FRFTs) When  = 0.5, the FRFT becomes the FT. Additivity property: If we denote the FRFT as (i.e., ) then Physical meaning: Performing the FT a times.

Another definition [Ref] H. M. Ozaktas, Z. Zalevsky, and M. A. Kutay, The Fractional Fourier Transform with Applications in Optics and Signal Processing, New York, John Wiley & Sons, 2000. [Ref] N. Wiener, “Hermitian polynomials and Fourier analysis,” Journal of Mathematics Physics MIT, vol. 18, pp. 70-73, 1929. [Ref] V. Namias, “The fractional order Fourier transform and its application to quantum mechanics,” J. Inst. Maths. Applics., vol. 25, pp. 241-265, 1980. [Ref] L. B. Almeida, “The fractional Fourier transform and time-frequency representations,” IEEE Trans. Signal Processing, vol. 42, no. 11, pp. 3084-3091, Nov. 1994. [Ref] S. C. Pei and J. J. Ding, “Closed form discrete fractional and affine Fourier transforms,” IEEE Trans. Signal Processing, vol. 48, no. 5, pp. 1338-1353, May 2000.

What happen if we do the FT non-integer times? Physical Meaning: Fourier Transform: time domain  frequency domain Fractional Fourier transform: time domain  fractional domain Fractional domain: the domain between time and frequency (partially like time and partially like frequency)

Experiment:

Time domain Frequency domain fractional domain Modulation Shifting Modulation + Shifting Shifting Modulation Modulation + Shifting Differentiation  j2f Differentiation and  j2f  −j2f Differentiation Differentiation and  −j2f

[Theorem] The fractional Fourier transform (FRFT) with angle  is equivalent to the clockwise rotation operation with angle  for the Wigner distribution function (or for the Gabor transform) FRFT = with angle  For the WDF If Wx(t, f ) is the WDF of x(t), and WX (u, v) is the WDF of X(u), (X(u) is the FRFT of x(t)), then

For the Gabor transform (with standard definition) If Gx(t, f ) is the Gabor transform of x(t), and GX (u, v) is the Gabor transform of X(u), then For the Gabor transform (with another definition on page 216) The Cohen’s class distribution and the Gabor-Wigner transform also have the rotation property

The Gabor Transform for the FRFT of a cosine function (d)  = 3/6 (e)  = 4/6 (f)  = 5/6

The Gabor Transform for the FRFT of a rectangular function. (d)  = 3/6 (e)  = 4/6 (f)  = 5/6

8-4 Twisting: Linear Canonical Transform (LCT) when b  0 when b = 0 ad − bc = 1 should be satisfied Four parameters a, b, c, d

Additivity property of the WDF If we denote the LCT by , i.e., then where [Ref] K. B. Wolf, “Integral Transforms in Science and Engineering,” Ch. 9: Canonical transforms, New York, Plenum Press, 1979.

If is the WDF of X(a,b,c,d)(u), where X(a,b,c,d)(u) is the LCT of x(t), then LCT == twisting operation for the WDF The Cohen’s class distribution also has the twisting operation.

我們可以自由的用 LCT 將一個中心在 (0, 0) 的平行四邊形的區域,扭曲成另外一個面積一樣且中心也在 (0, 0) 的平行四邊形區域。 f-axis f-axis (4,3) (-1, 2) (1,2) (0, 1) t-axis t-axis (1,-2) (0,-1) (-1, -2) (-4,-3)

inverse Fourier transform  = /2 Fourier transform fractional Fourier transform  = 0 identity operation linear canonical transform  = -/2 inverse Fourier transform Fresnel transform chirp multiplication scaling

附錄八 Linear Canonical Transform 和光學系統的關係 (1) Fresnel Transform (電磁波在空氣中的傳播) k = 2/: wave number : wavelength z: distance of propagation (2 個 1-D 的 LCT) Fresnel transform 相當於 LCT

(2) Spherical lens, refractive index = n f : focal length : thickness of length 經過 lens 相當於 LCT 的情形

(3) Free space 和 Spherical lens 的綜合 lens, (focal length = f) free space, (length = z2) free space, (length = z1) Output Input Input 和 output 之間的關係,可以用 LCT 表示

z1 = z2 = 2f  即高中物理所學的「倒立成像」 z1 = z2 = f  Fourier Transform + Scaling z1 = z2  fractional Fourier Transform + Scaling

用 LCT 來分析光學系統的好處: 只需要用到 22 的矩陣運算,避免了複雜的物理理論和數學積分 但是 LCT 來分析光學系統的結果,只有在「近軸」的情形下才準確 非近軸區 近軸區 光傳播方向 參考資料: [1] H. M. Ozaktas and D. Mendlovic, “Fractional Fourier optics,” J. Opt. Soc. Am. A, vol.12, 743-751, 1995. [2] L. M. Bernardo, “ABCD matrix formalism of fractional Fourier optics,” Optical Eng., vol. 35, no. 3, pp. 732-740, March 1996.