Image Details

Choose export citation format:

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 3.

(a) Profile of photon flux with wavelength at selected altitudes. (b) Absorption cross sections of CO2 (black), CO17O (blue), CO18O (orange), and 13CO2 (red) with wavelength. (c) Relative difference in absorption cross section between species i and CO2, defined as ﹩({\sigma }_{i}/{\sigma }_{{{\rm{CO}}}_{2}}-1)\times 1000﹩, where σi and ﹩{\sigma }_{{{\rm{CO}}}_{2}}﹩ are the absorption cross sections of species i and CO2, respectively (i = CO18O, CO17O, 13CO2) (J. A. Schmidt et al. 2013). Relative differences are smoothed using a Gaussian window with FWHMs of 2.5 nm, as done by J. A. Schmidt et al. (2013).

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse