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Improving the Hufnagel-Andrews-Phillips refractive index structure parameter model using turbulent intensity.
This study enhances the Hufnagel-Andrews-Phillips (HAP) model for atmospheric refractive index structure parameter, improving characterization against experimental data. The modified HAP model offers better consistency for atmospheric research and system link budget estimates.
Area of Science:
- Atmospheric optics
- Electromagnetics
- Geophysics
Background:
- The Hufnagel-Andrews-Phillips (HAP) model is a standard for refractive index structure parameter (Cn2) but requires refinement for diverse atmospheric conditions.
- Accurate Cn2 profiling is crucial for optical and radio wave propagation, impacting system performance.
Purpose of the Study:
- To modify the HAP model for improved characterization of Cn2 profiles using turbulent intensity and Korean atmospheric statistics.
- To compare the performance of the modified HAP model against the Critical Laser Enhancing Atmospheric Research 1 (CLEAR 1) model and experimental data.
Main Methods:
- Introduced turbulent intensity (ratio of wind speed variance to average wind speed-squared) into the HAP model.
- Utilized Korean Refractive Index Parameter yearly statistics for model validation.
- Performed comparative analysis between the modified HAP model, CLEAR 1 model, and experimental datasets.
Main Results:
- The modified HAP model demonstrates more consistent representation of averaged experimental data profiles compared to the CLEAR 1 model.
- The proposed model shows good agreement with averaged experimental data and reasonable agreement with non-averaged datasets from literature.
Conclusions:
- The enhanced HAP model provides a more accurate and consistent characterization of atmospheric refractive index structure parameter profiles.
- This improved model is valuable for system link budget estimations and advancing atmospheric research.
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