A new model suite to determine the influence of cosmic rays on (exo)planetary atmospheric biosignatures - Validation based on modern Earth

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Table 1

Pseudo first-order loss rate for both scenarios at 34.6 km (see text).

Scenario	ρ_total (molec cm⁻³)	O₃ (ppm)	Scaled rate

1	1.73 × 10¹⁷	9.44	9.05 × 10⁻⁷
2	1.71 × 10¹⁷	5.01	2.86 × 10⁻⁶

Notes. ρ_total represents the total air density and the scaled rates are given by R/(O₃ ⋅ ρ_total).

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