4.5 Article

Visible-IR transmission enhancement through fog using circularly polarized light

Journal

APPLIED OPTICS
Volume 57, Issue 23, Pages 6817-6822

Publisher

OPTICAL SOC AMER
DOI: 10.1364/AO.57.006817

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Funding

  1. National Natural Science Foundation of China (NSFC) [51505062, 51675076]
  2. Science Fund for Creative Research Groups of NSFC [51621064]
  3. Fundamental Research Funds for the Central Universities [DUT16TD20, DUT17GF109]

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Detection range is an important factor affecting the transmission characteristics of polarized light through fog. We first selected certain spectral bands from visible to IR wavelengths that exhibit lower path loss. For both radiation fog and advection fog, these optimized wavelength ranges include 0.4-1.1 mu m, 1.48-1.56 mu m, 1.63-1.86 mu m, 2.03-2.18 mu m, and 2.39-2.45 mu m, and radiation fog in particular contains 3.5-4.3 mu m The long-wave IR wavelengths were excluded due to higher absorption losses. We further investigated the transmission performance of circular and linear polarization in variable foggy environments, exploring the impact of the detection range in particular. Using polarization-tracking Monte Carlo simulations for varying particle size, wavelength, refractive index, and detection range, we show that circular polarization outperforms linear polarization when transmitting in both radiation and advection fog. For radiation fog, circular polarization persists longer than linear polarization for 5 mu m and 9 mu m particles over the entire optimized wavelength range from the visible to mid-wave IR (MWIR). However, linear polarization outperforms circular polarization for 1 mu m partides over the entire MWIR and a part of the short-wave IR (SWIR). For advection fog, circular polarization persists longer than linear polarization for all three partide sizes (10, 20, and 40 mu m) over the entire optimized wavelength range from the visible to SWIR. We show that circular polarization retains a higher degree of polarization and has better enhancement in some detection ranges. (C) 2018 Optical Society of America

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