Ultraviolet spectrum reveals the presence of ozone on Jupiter's moon Callisto-Reference-Cited by-同舟云学术

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Ultraviolet spectrum reveals the presence of ozone on Jupiter's moon Callisto

Published:2024-03 Issue: Volume:410 Page:115896
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Ramachandran R.,Meka J.K.,Rahul K.K.,Khan W.,Lo J.-I.,Cheng B.-M.,Mifsud D.V.,Rajasekhar B.N.,Das A.,Hill H.,Janardhan P.,Bhardwaj Anil,Mason N.J.,Sivaraman B.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference51 articles.

1. A comparison of ion irradiation and UV photolysis of CH4 and CH3OH;Baratta;Astron. Astrophys.,2002

2. The atmosphere of Mars;Barth;Annu. Rev. Earth Planet. Sci.,1974

3. Mid-ultraviolet hubble observations of Europa and the global surface distribution of SO2;Becker;Planet. Sci. J.,2022

4. Laboratory studies on the formation of ozone (O3) on icy satellites and on interstellar and cometary ices;Bennett;Astrophys. J.,2005

5. Infrared spectroscopy of neat solid ozone and that of ozone in interaction with amorphous and crystalline water ice;Chaabouni;J. Phys. Chem. A,2000

Cited by 1 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Jupiter's icy moon Callisto may harbour ozone;Nature India;2024-04-21

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