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Oxygen Isotope Fractionation in the Martian Atmosphere Induced by CO2 Photolysis and O3 Formation

  • Authors: Tatsuya Yoshida, Shohei Aoki, Hiromu Nakagawa, Naoki Terada, Juan Alday, Akinori Hasebe, Yuki Nakamura, Shungo Koyama, Shotaro Sakai, Ryoya Sakata, Ann Carine Vandaele

Tatsuya Yoshida et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 4.

Vertical profiles of δ18O (left), δ17O (middle), and Δ17O (right), comparing the results obtained with the standard eddy diffusion coefficient (solid) and with an eddy diffusion coefficient one order of magnitude smaller (dashed). The top panels show the results of CO2, CO, O, and O3, while the bottom panels show those for H2O2, OH, O2, and HO2.

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