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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 A3.

H₂O number density profile. The solid blue line represents the standard profile, while the dashed blue line represents that 10 times as high as the standard setting used in Section 4.1.

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