The existing methods for measuring aero-optical aberration suffer from several problems, such as low spatiotemporal resolution, sensitivity to environment, and integral effects. A new method for measuring aero-optical aberration of supersonic flow is proposed. Based on the self-developed measuring method of supersonic density field, the wavefront aberration induced by a cross-section of supersonic flow field could be measured by ray-tracing. Compared with other methods, the present one has three significant innovations: (1) high spatiotemporal resolution. Its time resolution is 6 ns, and the spatial resolution can reach up to micrometers; (2) it can avoid the integral effects and study the wavefront aberration induced by the flow field of interest locally;(3) it can also avoid the influence from the test section wall boundary layers and environmental disturbances. The present method was applied to supersonic flow around an optical bow cap. The results of high spatiotemporal resolution reveal fine wavefront structures, and show that shock waves, expansion waves and turbulent boundary layers have different impacts on the wavefront aberration.
NPLS, supersonic flow field, aero-optics Citation:Yi S H, Tian L F, Zhao Y X, et al. Aero-optical aberration measuring method based on NPLS and its application.There are many methods for measuring aero-optical aberration induced by supersonic flow, such as Shack-Hartmann wavefront sensor (SHWS), small-aperture beam technique (SABT) and interferometry. SHWS is not sensitive to the vibration of equipments, and its dynamic measurement range is more than a hundred times or even thousands of times of traditional interferometry [1]. Its resolution is related to the size and spacing of small lens [2], and can reach up to 100-500 μm. Its temporal response frequency is not generally higher than 2500 Hz [3], and can be improved by reducing its spatial resolution [2]. In 1992, Jumper and Hugo [4] described SABT in detail, and studied the optical phase aberration caused by turbulent flow. The frequency of SABT is up to 100 kHz [5], which is the highest among numbers of wavefront sensors nowadays, and its spatial resolution is lower than that of SHWS by one or two orders *Corresponding author (email: zhaixing_nomin@sohu.com)[5]. SABT has been successfully used in various flow fields [6,7]. Interferometry is commonly used when the wavefront aberration is relatively weak [8]. By comparing the disturbed wavefront and the reference one, the interferometry can directly measure the wavefront phase aberration. The interferogram is recorded on CCD, and the brightness at each pixel is proportional to the local disturbed wavefront phase [9]. The time-response frequency of interferometry is related to the CCD record out time and the spatial resolution. Based on the background oriented schlieren (BOS), Zhao et al.[10] proposed a technique to measure the aero-optical aberration and jitter of supersonic mixing layer. The time resolution of the technique based on BOS is 6 ns, the highest time correlation...