Journal of Infrared and Millimeter Waves, Volume. 43, Issue 2, 261(2024)

Chaotic and fractal characteristics of infrared electromagnetic wavefield in the media of atmosphere

Wen-Jun XU, Sheng-Li SUN*, and Gao-Rui LIU**
Author Affiliations
  • Key Laboratory of Intelligent Infrared Sensing,Shanghai Institutes of Technical Physics,Chinese Academy of Sciences,Shanghai 200083,China
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    Chaotic dynamics is a significant systematic feature of infrared electromagnetic wavefields that requires further study. Understanding the chaotic dynamics of infrared radiation wavefields can lead to advancements in high-performance detection, imaging, and recognition of weak, moving, time-varying signals. To extract the time series of the dynamic system, we have established a 4D time-space observing system. We then use the FFT transform on a random time series of frequency-band infrared data to obtain the fractional Brownian motion dimension, indicating a fractal structure in the atmospheric infrared radiation wavefield. By using time-delay analysis, we construct a dimensional phase space and compute the fractal dimension. We also observe that the first Lyapunov exponent remains positive in different phase spaces, leading to the initial conclusion that the atmospheric infrared wavefield is chaotic. To measure the chaotic strength of real cases in the time-space domain, we use the permutation entropy. These results serve as a foundation for further research, such as understanding the dynamic evolution mechanism of moving objects and their background wavefields, capturing time-varying signals, and making long-term nonlinear predictions of infrared wave behaviors in different domains.

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    Wen-Jun XU, Sheng-Li SUN, Gao-Rui LIU. Chaotic and fractal characteristics of infrared electromagnetic wavefield in the media of atmosphere[J]. Journal of Infrared and Millimeter Waves, 2024, 43(2): 261

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    Paper Information

    Category: Research Articles

    Received: Jun. 29, 2023

    Accepted: --

    Published Online: Apr. 29, 2024

    The Author Email: Sheng-Li SUN (palm_sun@mail.sitp.ac.cn), Gao-Rui LIU (liugaorui@mail.sitp.ac.cn)

    DOI:10.11972/j.issn.1001-9014.2024.02.016

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