Spatial and temporal variations in infrared emissions of the upper atmosphere. 2. 15-μm carbon dioxide emission


如何引用文章

全文:

开放存取 开放存取
受限制的访问 ##reader.subscriptionAccessGranted##
受限制的访问 订阅存取

详细

The results of rocket and satellite measurements of carbon dioxide emissions at a wavelength of 15 μm in the upper atmosphere have been systematized and analyzed. Analytical expressions describing the dependence of the altitude distribution of 15-μm CO2 emission intensity and its variation in the altitude range from 100 to 130 km on the season, latitude, and solar activity have been obtained.

作者简介

A. Semenov

Obukhov Institute of Atmospheric Physics

编辑信件的主要联系方式.
Email: anasemenov@yandex.ru
俄罗斯联邦, Moscow

I. Medvedeva

Institute of Solar–Terrestrial Physics, Siberian Division

Email: anasemenov@yandex.ru
俄罗斯联邦, Irkutsk

V. Perminov

Obukhov Institute of Atmospheric Physics

Email: anasemenov@yandex.ru
俄罗斯联邦, Moscow

Yu. Zheleznov

Institute of Electrophysics and Electroenergetics

Email: anasemenov@yandex.ru
俄罗斯联邦, St. Petersburg

补充文件

附件文件
动作
1. JATS XML

版权所有 © Pleiades Publishing, Ltd., 2017