Sounding of the Atmosphere using Broadband Emission Radiometry observations of daytime mesospheric O<sub>2</sub>(<sup>1</sup>Δ) 1.27 <i>μ</i>m emission and derivation of ozone, atomic oxygen, and solar and chemical energy deposition rates

M. G. Mlynczak, B. T. Marshall, Javier Martín‐Torres, James M. Russell, Robert E. Thompson, Ellis E. Remsberg, L. L. Gordley

Journal of Geophysical Research Atmospheres · 2007 · 109 citations · 25 references

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TL;DR

SABER on TIMED measured daytime O₂(¹Δ) 1.27 µm limb radiances, which were inverted to vertical emission‑rate profiles and, using a non‑LTE radiative‑kinetic model, yielded mesospheric ozone concentrations, atomic‑oxygen abundances, and energy‑deposition rates from UV absorption and exothermic chemistry. The 4 July 2002 test‑day data, now publicly available, demonstrate the high quality of SABER O₂(¹Δ) airglow and ozone measurements and illustrate their potential to address a range of fundamental atmospheric science questions.

Abstract

We report observations of the daytime O 2 ( 1 Δ) airglow emission at 1.27 μ m recorded by the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) instrument on the NASA Thermosphere‐Ionosphere‐Mesosphere Energetics and Dynamics (TIMED) satellite. The measured limb radiances are inverted to yield vertical profiles of the volume emission rate of energy from the O 2 molecule. From these emission rates we subsequently derive the mesospheric ozone concentrations using a nonlocal thermodynamic equilibrium (non‐LTE) radiative and kinetic model. Rates of energy deposition due to absorption of ultraviolet radiation in the Hartley band of ozone are also derived, independent of knowledge of the ozone abundance and solar irradiances. Atomic oxygen concentrations are obtained from the ozone abundance using photochemical steady state assumptions. Rates of energy deposition due to exothermic chemical reactions are also derived. The data products illustrated here are from a test day (4 July 2002) of SABER Version 1.07 data which are now becoming publicly available. This test day illustrates the high quality of the SABER O 2 ( 1 Δ) airglow and ozone data and the variety of fundamental science questions to which they can be applied.

References

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