Solar influence on the O(1D) dayglow emission rate:: Global-scale measurements by WINDII on UARS -: art. no. L07804

被引：38

作者：

Zhang, SP ^{[1
]}

Shepherd, GG ^{[1
]}

机构：

[1] York Univ, Ctr Res Earth & Space Sci, Toronto, ON M3J 3K1, Canada

来源：

GEOPHYSICAL RESEARCH LETTERS | 2004年 / 31卷 / 07期

关键词：

D O I：

10.1029/2004GL019447

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

摘要：

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

引用

页码：L078041 / 4

页数：4

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