Fig. 5
Fits to the image row segment of 110 pixels along the synthetic meteor in Fig. 2 for the model that evaluates formally the integrals in Eq. (A.5)(top) and for the approximation using function-time products (bottom). The flux of the meteor point source was sampled with n = 8 (left), n = 4 (middle) and n = 2 (right). Notation in this and the following figure is as in Fig. 4.
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