Solar influence on the O(1D) dayglow emission rate: Global-scale measurements by WINDII on UARS

Details Solar influence on the O(1D) dayglow emission rate: Global-scale measurements by WINDII on UARS Solar influence on the O(1D) dayglow emission rate: Global-scale measurements by WINDII on UARS

Apr 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004georl..3107804z&link_type=abstract

Geophysical Research Letters, Volume 31, Issue 7, CiteID L07804

Physics

10

Atmospheric Composition And Structure: Airglow And Aurora, Atmospheric Composition And Structure: Thermosphere-Composition And Chemistry, Atmospheric Composition And Structure: Thermosphere-Energy Deposition, Global Change: Atmosphere (0315, 0325), Global Change: Remote Sensing

Scientific paper

More than 130,000 emission rate profiles of the O(1D) dayglow (630 nm) were observed by WINDII during 1991-1995, which provide an unprecedented resource for studying the O(1D) layer, and related physics and chemistry in the thermosphere and ionosphere. This article describes the general properties of the O(1D) emission layer and an empirical model derived from WINDII measurements for the O(1D) emission rate as a function of the solar zenith angle and solar irradiance using the F10.7 cm flux as a proxy.

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