Fig. 4.
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Spectral emission distribution of interstellar dust particles inside the heliosphere for three different size distributions of particles. Classical MRN (green) (Mathis et al. 1977), a truncated power law (blue) (Mathis 1996), and the most recent (orange) (Hensley & Draine 2023). The dashed line indicates the interplanetary dust SED from Poppe et al. (2019).
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