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A chemical kinetics network for lightning and life in planetary atmospheres

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Figure

Figure 1. Photodissociation cross sections of NHet al.fifunction of wavelength,3  1NH + H2, σ [cm2], as a λ (Å), from PHIDRATES (original data from McNesby 1962; Schurath et al
Figure 3. Mixing ratio as a function of temperature. The solid line is from theSaha equation and the dashed line is the result from our model calculation.
Figure 4. Illustration representation of the model. The illustrationT Pwavelength between 1 and 10000 Å are considered
Figure 5. Flowchart representation for the program.
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