Effect of Phase Relations on Speckle Pattern: Simulation and Measurement

Abstract

Speckle is an important phenomenon in various applications. It can be quantified by speckle contrast. However, at present, the influence of the phase relations among the various wavelengths on speckle contrast is rarely analyzed theoretically. Herein, a thorough method for numerically simulating the speckle pattern is presented to considering the impact of relative phase relations among wavelengths on speckle contrast. This method contains spectral shape, spectral width, and phase relations. In addition, a superluminescent pulse amplifier (SPA) with 6.5-nm bandwidth and a mode-locked laser (MLL) with 21-nm bandwidth are established to conduct the verification experiment. The experimental results show that the SPA light attains lower speckle contrast even with a narrower bandwidth than the MLL light. It is manifested that relative phase relations among wavelengths has significant effect on speckle contrast, and chaotic phase relations could be more advantageous for reducing speckle than just a broad spectrum. The simulation results agree well with experimental results. Therefore, this thorough method could provide a reliable approach to describe the characteristics of speckle pattern caused by broadband light carrying phase information. Considering the speckle contrast is positively proportional to optical coherence, this method could also be used to analyze the coherence of partially coherent light.

Yb-Doped Fiber Chirped Pulse Amplification System Delivering 1 mJ, 231 fs at 1 kHz Repetition Rate

“…The output end of the second boost amplifier was welded with an end cap at an oblique cut angle of 8 • to prevent the high energy density from damaging the optical fiber end face on the one hand and suppress parasitic oscillation on the other hand. The structure before the main amplifier was similar to our previous work [23], but the pulse width was stretched wider in order to obtain higher energy.…”

“…The output end of the second boost amplifier was welded with an end cap at an oblique cut angle of 8° to prevent the high energy density from damaging the optical fiber end face on the one hand and suppress parasitic oscillation on the other hand. The structure before the main amplifier was similar to our previous work [23], but the pulse width was stretched wider in order to obtain higher energy. The main amplifier employed the Rod-type PCF gain module integrating water cooling (aero GAIN-ROD Module-2.1) produced by NKT, the fiber length was 0.8 m and the diameter of the fiber core and cladding were 85 µm and 260 µm, respectively, the corresponding mode field area was about 3500 µm2, the numerical aperture (NA) was 0.03.…”