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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 A2.

Vertical profiles of the eddy diffusion coefficient and molecular diffusion coefficient. The solid blue line represents the profile with the standard eddy diffusion coefficient, while the dashed blue line represents the profile with a coefficient one order of magnitude smaller used in Section 4.1. The dotted orange, red, and pink lines represent the profiles of the molecular diffusion coefficients of CO2, H2, and H, respectively.

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