Cosmic ray ionisation of a post-impact early Earth atmosphere - Solar cosmic ray ionisation must be considered in origin-of-life scenarios

Open Access

Fig. 7

$ζ_{G C R}^{T O A}$ $\[\zeta_{\mathrm{GCR}}^{\mathrm{TOA}}\]$ , calculated using top-of-atmosphere spectra at varying distances from the Sun in the medium rotator case, Ω = 6Ω_⊙. The circles (crosses) represent $ζ_{G C R}^{T O A}$ $\[\zeta_{\mathrm{GCR}}^{\mathrm{TOA}}\]$ calculated using top-of-atmosphere spectra derived from j_LIS( $j_{LIS}^{high}$ $\[j_{\text {LIS }}^{\text {high }}\]$ ).

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