Observations of Atmospheric Helium and Oxygen with SPHEREx

TL;DR

This paper reports on the measurement of near-infrared terrestrial airglow from helium and oxygen in the exosphere using SPHEREx data, revealing spatial and temporal variability linked to solar and seasonal factors.

Contribution

It introduces an analytical framework for extracting atmospheric emission lines from astrophysical survey data and demonstrates SPHEREx's potential for atmospheric monitoring.

Findings

Global measurements show temporal variability in airglow emissions.

Systematic dependencies on geographic location are observed.

Variations correlate with solar illumination and seasonal effects.

Abstract

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 $\lambda$10830, OI $\lambda$8446, and OI $\lambda$11287 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.