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Observations Of Atmospheric Helium And Oxygen With SPHEREx

Observations Of Atmospheric Helium And Oxygen With SPHEREx

We present measurements of near-infrared (NIR) terrestrial airglow produced by helium and oxygen in the exosphere as observed by SPHEREx. Using eight months of survey data obtained from a 680 km low-Earth orbit, emission from HeI λ10830, OI λ8446, and OI λ11287 is mapped with both global spatial and multi-season temporal coverage.

These measurements are obtained along upward looking lines of sight as part of the astrophysical survey, in contrast to conventional nadir-viewing Earth remote sensing, which probes the behavior of low-density material in the thermo- and exosphere. We describe an analytical framework to extract atmospheric emission lines in the presence of astrophysical backgrounds including stars, resolved galaxies, and the diffuse Zodiacal light.

The resulting global measurements reveal temporal variability over the survey period and systematic dependencies on geographic location. We interpret these variations in the context of the variable Solar illumination and seasonal effects. SPHEREx, an astrophysical space observatory, is demonstrated to be a promising new platform for monitoring NIR airglow and investigating its coupling to Solar activity and global geophysical processes.

Diagram of the SPHEREx observatory, showing (from top to bottom) the three conical photon shields with a cutaway view, the telescope, radiator panel for the mid-wave infrared (MWIR) detectors, the MWIR and short-wave infrared (SWIR) focal plane arrays (FPAs), and the 3-stage V-groove radiator assembly with penetrating bipods for supporting the telescope assembly. The BAE spacecraft at the bottom provides pointing, power, and telemetry and houses the instrument readout electronics. -- NASA — Diagram of the SPHEREx observatory, showing (from top to bottom) the three conical photon shields with a cutaway view, the telescope, radiator panel for the mid-wave infrared (MWIR) detectors, the MWIR and short-wave infrared (SWIR) focal plane arrays (FPAs), and the 3-stage V-groove radiator assembly with penetrating bipods for supporting the telescope assembly. The BAE spacecraft at the bottom provides pointing, power, and telemetry and houses the instrument readout electronics. — NASA

Howard Hui, Chi Nguyen, Ryan Wills, Katrina Bossert, Sean Bryan, Yoonsoo Bach, Jamie Bock, Tzu-Ching Chang, Shuang-Shuang Chen, Asantha Cooray, Brendan Crill, Olivier Doré, C. Darren Dowell, Andreas Faisst, Jae Hwan Kang, Phil Korngut, Carey Lisse, Dan Masters, Roberta Paladini, Volker Tolls, Michael Werner, Yujin Yang, Mike Zemcov

Comments: Submitted for publication in JGR: Atmospheres. 25 pages, 19 figures, and 3 supplemental movies
Subjects: Atmospheric and Oceanic Physics (physics.ao-ph); Earth and Planetary Astrophysics (astro-ph.EP); Instrumentation and Methods for Astrophysics (astro-ph.IM); Space Physics (physics.space-ph)
Cite as: arXiv:2605.00851 [physics.ao-ph] (or arXiv:2605.00851v1 [physics.ao-ph] for this version)
https://doi.org/10.48550/arXiv.2605.00851
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Submission history
From: Ryan Wills
[v1] Mon, 20 Apr 2026 15:48:22 UTC (40,207 KB)
https://arxiv.org/abs/2605.00851
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