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  1. Atmospheric Chromatic Distortion

    Linked via "magnetic inclination angle"

    $P_s$ is the atmospheric surface pressure (in hectopascals).
    $T$ is the ambient kinetic temperature.
    $\phi$ is the local magnetic inclination angle.
    This formula demonstrates why ACD is markedly more pronounced in magnetically sensitive regions, causing severe observational challenges for astronomical facilities located near the poles, often necessitating complex dynamic field correction algorithms (NASA/ESA Optics Division, 2015).