The vertical distribution of ozone in Mars Years 34-35 from ExoMars TGO/NOMAD-UVIS observations-Reference-Cited by-同舟云学术

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

Published:2021-01-27 Issue: Volume: Page:
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Author:

Patel Manish R¹^ORCID,Sellers Graham¹,Mason J.²,Holmes James Andrew²^ORCID,Brown Megan¹,Lewis Stephen²^ORCID,Rajendran Kylash¹,Streeter Paul Michael²^ORCID,Marriner Charlotte¹,Hathi Brijen¹,Slade David¹,Leese Mark¹,Wolff Michael J.³^ORCID,Khayat Alain SJ⁴^ORCID,Smith Michael D.⁵^ORCID,AOKI Shohei⁶^ORCID,Piccialli Arianna⁷^ORCID,Vandaele Ann Carine⁶,Daerden Frank W.⁸^ORCID,Robert Severine⁹^ORCID,Thomas Ian Richard¹⁰^ORCID,Ristic Bojan⁶^ORCID,Willame Yannick¹⁰,Depiesse Cédric⁶,Bellucci Giancarlo¹¹,López-Moreno José Juan¹²

Affiliation:

1. The Open University

2. Open University

3. Space Science Institute

4. NASA Goddard Space Flight Center and the University of Maryland

5. NASA Goddard Space Flight Center

6. Royal Belgian Institute for Space Aeronomy

7. Belgian Institute for Space Aeronomy (BIRA-IASB)

8. Royal Belgian Institute for Space Aeronomy BIRA-IASB

9. Royal Belgian Institute for Space Aeronomy, BIRA-IASB

10. Belgian Institute for Space Aeronomy

11. Institute for Space Astrophysics and Planetology

12. Instituto de Astrofisica de Andalucia, IAA-CSIC

Funder

UK Space Agency

Publisher

Wiley

Reference248 articles.

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2. Water vapor vertical profile on Mars in dust storms observed by TGO/NOMAD. Journal of

3. Anbar A. Leu M.-T. Nair H. Yung Y. 1993. Adsorption of ho x on aerosol surfaces:

4. Implications for the atmosphere of mars. Journal of Geophysical Research: Planets 98 (E6)