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What are the factors affecting the shape of the density curve for light hazard? 


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The shape of the density curve for light hazard can be influenced by various factors. In the context of laser irradiation on a spherical target, the radiation pressure generates a nonmonotonic density profile with an overdense bump in the underdense region, which is the stable solution under specific conditions . Probability density functions and hazard functions are interrelated, with specific shapes such as increasing, decreasing, unimodal, anti-unimodal, and more, impacting each other . Nonparametric maximum likelihood estimation methods consider decreasing density and constraints on hazard functions like increasing, convex, or bathtub-shaped, affecting the shape of the density curve . Perturbations to meteoroid shape or atmospheric density can also alter the light curve, with changes in mass distribution affecting the symmetry and curvature of the emitted light intensity .

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Factors affecting the shape of a meteor light curve include meteoroid shape alterations impacting curvature and symmetry, and periodic atmospheric density fluctuations causing small oscillations in the light curve.
The shape of the light density curve is influenced by ambient lighting changes, correction values stored in a lookup table, and adjustments made based on lighting strength variations.
Shape restrictions such as decreasing, increasing, convex, or bathtub-shaped influence the density curve for light hazard, as discussed in nonparametric estimation methods in the paper.
Not addressed in the paper.
The shape of the density curve for light hazard is influenced by radiation pressure from a powerful laser on a spherical target, leading to a nonmonotonic profile with an overdense bump.

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