声学学报
聲學學報
성학학보
ACTA ACUSTICA
2010年
2期
169-178
,共10页
李凌志%李骏%卢炳武%刘英杰%刘克
李凌誌%李駿%盧炳武%劉英傑%劉剋
리릉지%리준%로병무%류영걸%류극
近场声全息的逆向重建过程属于线性病态逆问题,必须进行正则化处理.本文对三种基于Tikhonov正则化的参数选择方法,即离差原理法、广义交叉验证法、L曲线法,在不同全息距离、声源频率和信噪比的条件下进行了比较,结果表明,它们在远距离及低噪声环境下难以获得合适的正则化参数.采用等效噪声方差的方法,对其中较为稳定的离差原理进行了改进,使其在较远全息距离及低噪声环境下仍能获得合适的正则化参数.相应的仿真实验表明,改进后的离差原理法在很宽的信噪比(>6 dB)和较远的全息距离(~10 cm)均能稳定地找到合适的正则化参数.此外,由于该方法无须对全息声压进行平滑处理,其有效重建孔径和全息孔径相等.
近場聲全息的逆嚮重建過程屬于線性病態逆問題,必鬚進行正則化處理.本文對三種基于Tikhonov正則化的參數選擇方法,即離差原理法、廣義交扠驗證法、L麯線法,在不同全息距離、聲源頻率和信譟比的條件下進行瞭比較,結果錶明,它們在遠距離及低譟聲環境下難以穫得閤適的正則化參數.採用等效譟聲方差的方法,對其中較為穩定的離差原理進行瞭改進,使其在較遠全息距離及低譟聲環境下仍能穫得閤適的正則化參數.相應的倣真實驗錶明,改進後的離差原理法在很寬的信譟比(>6 dB)和較遠的全息距離(~10 cm)均能穩定地找到閤適的正則化參數.此外,由于該方法無鬚對全息聲壓進行平滑處理,其有效重建孔徑和全息孔徑相等.
근장성전식적역향중건과정속우선성병태역문제,필수진행정칙화처리.본문대삼충기우Tikhonov정칙화적삼수선택방법,즉리차원리법、엄의교차험증법、L곡선법,재불동전식거리、성원빈솔화신조비적조건하진행료비교,결과표명,타문재원거리급저조성배경하난이획득합괄적정칙화삼수.채용등효조성방차적방법,대기중교위은정적리차원리진행료개진,사기재교원전식거리급저조성배경하잉능획득합괄적정칙화삼수.상응적방진실험표명,개진후적리차원리법재흔관적신조비(>6 dB)화교원적전식거리(~10 cm)균능은정지조도합괄적정칙화삼수.차외,유우해방법무수대전식성압진행평활처리,기유효중건공경화전식공경상등.
The reconstruction of Nearfield Acoustic Holography (NAH) is a linear, ill-posed inverse problem, in which a regularization procedure must be used. We compared three Tikhonov regularization based parameter selection methods, Morozov Discrepancy Principle method (MDP), Generalized Cross Validation method (GCV), and L-curve method, at various hologram distances, sound source frequencies, and Signal-to-Noise Ratios (SNR). The results show that they are all not robust at large hologram distances and low noise conditions. Based on an equivalent-noise-variance method, we established an improved method for estimating the noise variance in the MDP method, which is relative robust among the three, and made it work at relatively large hologram distances and low noise conditions. Numerical simulations show that the improved MDP method is robust in determining proper regularization parameters over a large SNR range (> 6 dB) and at a relatively large hologram distance (~ 10 cm). Moreover, the improved MDP method has a valid reconstruction aperture that is equal to the hologram aperture because it is not necessary to smooth the hologram pressure.