To address the problems that currently solve large time-bandwidth product prolate spheroidal wave functions (PSWF) with no uniform expression, an explicit asymptotic expression of the large time-bandwidth product PSWF and its differential operator eigenvalues is proposed. The expression is proposed using the theoretical and numerical analyses of the solution errors of the explicit asymptotic expressions based on the Hermite function and Legendre polynomial. The applicable conditions and calculation methods of the large time-bandwidth product ($c>10\pi$) PSWF and its differential operator eigenvalues are accurately and efficiently solved using the Hermite function and Legendre polynomial. Results of the performance comparison analysis indicate that the proposed expression can ensure PSWF and its differential operator eigenvalues of all orders always meet the error requirements. Moreover, the orthogonality and energy concentration of PSWF signals have significant advantages.
国家自然科学基金(61701518)
山东省“泰山学者"建设工程专项经费基金项目(20081130)
Appendix 显式渐近表达式的具体形式 式(A1)
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Figure 1
(Color online) Solution errors of PSWF $\mathrm{log}E_1$
Figure 2
(Color online) Solution errors of eigenvalues of differential operators of PSWF $\mathrm{log}E_2$
Figure 3
(Color online) The solution errors of PSWF
Figure 4
(Color online) The frequency domain energy concentration of PSWF
$c$ (rad$\cdot$s) | 11$\pi$ | 20$\pi$ | 40$\pi$ | 60$\pi$ | 80$\pi$ | 100$\pi$ | 101$\pi$ |
The values of the abscissas | 7.40 | 13.75 | 26.41 | 40.08 | 53.33 | 66.06 | 66.92 |
$c$ (rad$\cdot$s) | 11$\pi$ | 20$\pi$ | 40$\pi$ | 60$\pi$ | 80$\pi$ | 100$\pi$ | 101$\pi$ |
The values of the abscissas | 7.32 | 13.17 | 26.02 | 39.54 | 53.31 | 65.98 | 66.15 |
Method | Order | The 0th$\sim$13th PSWF | The 14th$\sim$19th PSWF |
This paper | The 0th$\sim$13th PSWF | $2.56~\times~10^{-32}~\sim~7.44~\times~10^{-15}$ | $5.14~\times~10^{-9}~\sim~8.08~\times~10^{-3}$ |
Ref. | $2.56~\times~10^{-32}~\sim~7.44~\times~10^{-15}$ | $1.39~\times~10^{-3}~\sim~4.62~\times~10^{+2}$ | |
Ref. | $6.35~\times~10^{-2}~\sim~2.83~\times~10^{+2}$ | $3.76~\times~10^{-2}~\sim~4.90~\times~10^{+1}$ | |
This paper | The 14th$\sim$19th PSWF | Symmetry | $1.74~\times~10^{-34}~\sim~9.29~\times~10^{-19}$ |
Ref. | $7.52~\times~10^{-2}~\sim~5.07~\times~10^{+2}$ | ||
Ref. | $1.74~\times~10^{-34}~\sim~9.29~\times~10^{-19}$ |
Method | Order | The 0th$\sim$66th PSWF | The 67th$\sim$99th PSWF |
This paper | The 0th$\sim$66th PSWF | $1.07~\times~10^{-30}~\sim~7.66~\times~10^{-14}$ | $7.51~\times~10^{-7}~\sim~2.33\times~10^{-2}$ |
Ref. | $1.07\times~10^{-30}~\sim~7.66~\times~10^{-14}$ | $3.54~\times~10^{-2}~\sim~9.85\times~10^{+1}$ | |
Ref. | $5.43~\times~10^{-2}~\sim~1.24~\times~10^{+3}$ | $6.30~\times~10^{-1}~\sim~7.12~\times~10^{+2}$ | |
This paper | The 67th$\sim$99th PSWF | Symmetry | $4.35~\times~10^{-33}~\sim~5.48~\times~10^{-17}$ |
Ref. | $6.94~\times~10^{-2}~\sim~3.07~\times~10^{+2}$ | ||
Ref. | $4.35\times~10^{-33}~\sim~5.48~\times~10^{-17}$ |