Fig. 6
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Profiles of HO2 for the planet around the Sun at 100% PAL O2 and different levels of CH4. The significant HO2 depletion present for low and modern levels of CH4 is lessened for the high CH4 models. This is because the HO2 depletion is due to the Sun-hosted planet being in the NOx-saturated regime, but increased CH4 allows enough HOx production to lessen this effect.
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