Impact of Storm‐Time Enhanced O2 Absorption on Disk Viewing N2 LBH Spectra: TIMED GUVI Observations

Author:

Zhang Y.1ORCID,Paxton L. J.1ORCID,Yee S.1ORCID,Hecht J.2ORCID

Affiliation:

1. Johns Hopkins University Applied Physics Lab Laurel MD USA

2. The Aerospace Cooperation Los Angeles CA USA

Abstract

AbstractA comparison between storm‐time TIMED/GUVI FUV spectra in thermospheric composition disturbed (O/N2 <∼140 km> depleted and NO <∼110 km> enhanced) and undisturbed regions reveals the following features: (1) A clear decrease in N2 LBHS (140–150 nm) band intensities compared to that between 150 and 160 nm; (2) A significant spectral decrease around O 164.1 nm; (3) Two enhanced peaks between 170 and 185 nm. The feature (2) is clearly due to atomic oxygen density decrease in the low thermosphere. The feature (3) is caused by storm‐time production and transport of nitric oxide. An AURIC simulation reproduced feature (1) confirming that storm‐time enhancement in O2 density (∼120–170 km) and the wavelength dependent O2 absorption cross section are the source of observed feature (1). On the other hand, the feature (1) was not observed in the regions without O/N2 depletion. This further supports that O2 density enhancement is responsible for feature (1).

Funder

Heliophysics Division

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

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