Joint observations of oxygen atmospheric band emissions using OSIRIS and the MATS satellite
Journal article, 2025

The MATS (Mesospheric Airglow/Aerosol Tomography and Spectroscopy) satellite was launched in November 2022 and began collecting scientific measurements of the mesosphere and lower thermosphere (MLT) in early 2023. The satellite utilises a multichannel limb-viewing instrument designed to gather images across six distinct spectral bands, each selected to capture atmospheric airglow from O2 atmospheric band emissions and light scattered by noctilucent clouds (NLC). This article presents a comparison between the MATS limb measurements and the observations made by the OSIRIS spectrograph on the Odin satellite. Specifically, airglow signals from excited O2, as recorded by MATS infrared (IR) channels and OSIRIS, are analysed over the polar regions under temporally and spatially aligned conditions. From December 2022 to February 2023, 36 close encounters of the two satellites were identified and analysed. The results show that the two instruments agree well on the overall structure but that the MATS signals generally exceed OSIRIS by similar to 20 % in magnitude. OSIRIS measurements are also compared to the radiative transfer model SASKTRAN to investigate stray light impact on the measurements.

Author

Bjorn Linder

Stockholm University

Jorg Gumbel

Stockholm University

Donal Murtagh

Chalmers, Space, Earth and Environment, Geoscience and Remote Sensing

Linda Megner

Stockholm University

Lukas Krasauskas

Stockholm University

Doug Degenstein

University of Saskatchewan

Ole Martin Christensen

Stockholm University

Nickolay Ivchenko

Royal Institute of Technology (KTH)

Atmospheric Measurement Techniques

1867-1381 (ISSN) 1867-8548 (eISSN)

Vol. 18 17 4453-4466

Subject Categories (SSIF 2025)

Meteorology and Atmospheric Sciences

DOI

10.5194/amt-18-4453-2025

More information

Latest update

9/26/2025