Model calculation of the [OI] 630 nm dayglow and [OI] 557.7 nm dayglow limb intensity for two different solar zenith angles (30 and 70 degrees) at aphelion and perihelion, and their measurements by TGO/NOMAD

This dataset contains vertical profile of [OI] 630 nm and [OI] 557.7 nm dayglow intensity simulated by a theoretical model and measured with TGO/NOMAD-UVIS.
These are presented as Figure 4 in Gérard, J. C., Aoki, S., Gkouvelis, L., Soret, L., Willame, Y., Thomas, I. R., et al. (2021). First observation of the oxygen 630 nm emission in the Martian dayglow. Geophysical Research Letters, 48(8), e2020GL092334. https://doi.org/10.1029/2020GL092334

Data and Resources

Tags and groups

Cite this as (APA format)

Gérard, J.-C., Aoki, S., & Vandaele, A. C. (2021). Model calculation of the [OI] 630 nm dayglow and [OI] 557.7 nm dayglow limb intensity for two different solar zenith angles (30 and 70 degrees) at aphelion and perihelion, and their measurements by TGO/NOMAD (Version 1) [Data set]. Royal Belgian Institute for Space Aeronomy. https://doi.org/10.18758/71021063
Retrieved: 16:18 07 Dec 2024 (UTC)
Users of this DOI are kindly encouraged to contact the author(s) for help and cooperation towards further successful utilisation.

Author(s)
Principal

Gérard, Jean-Claudeorcid, University of Liège
Other(s)

Aoki, Shoheiorcid, University of Liège; Vandaele, Ann Carineorcid, Royal Belgian Institute for Space Aeronomy;
Contact data-contact of Royal Belgian Institute for Space Aeronomy

Technical info
Is referenced by

https://doi.org/10.1029/2020GL092334

Temporal features

Additional info
Repository homepage

https://data.aeronomie.be/dataset/
Last Updated

September 17, 2024
Created

April 25, 2021

Spatial features

No spatial information