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Theoretical Transmission Spectra of Exoplanet Atmospheres with Hydrocarbon Haze: Effect of Creation, Growth, and Settling of Haze Particles. II. Dependence on UV Irradiation Intensity, Metallicity, C/O Ratio, Eddy Diffusion Coefficient, and Temperature
2019 The Astrophysical Journal 877 109.
- Provider: AAS Journals
Caption: Figure 1.
Extinction cross sections of the tholin-like haze particles of five different particle radii of 0.001, 0.01, 0.1, 1, and 10 μm, which are smoothed with the resolution of R = 100. Note that this figure is the same as Figure 1 of Paper I, but extended to longer wavelengths.
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