The vertical distribution of ozone in Mars Years 34-35 from ExoMars TGO/NOMAD-UVIS observations

Manish R. Patel,Graham Sellers,John Mason,J. A. Holmes,Megan Brown,Stephen R. Lewis,Kylash Rajendran,Paul Streeter,Charlotte Marriner,B. Hathi,David Slade,Mark Leese,Michael J. Wolff,Alain Khayat,Michael D. Smith,Shohei Aoki,Arianna Piccialli,Ann Carine Vandaele,Frank Daerden,Séverine Robert,Ian Thomas,Bojan Ristic,Yannick Willame,Cédric Depiesse,Giancarlo Bellucci,José Juan López-Moreno

The vertical distribution of ozone in Mars Years 34-35 from ExoMars TGO/NOMAD-UVIS observations

2021

We present ~1.5 Mars Years (MY) of ozone vertical profiles, covering Ls = 163deg; in MY34 to Ls = 320deg; in MY35, a period which includes the 2018 global dust storm. Since April 2018, the Ultravio...

Keywords:

Atmospheric sciences
Dust storm
Mars Exploration Program
Environmental science
Ozone

Correction
Source
Cite
Save
Machine Reading By IdeaReader

References

Citations