Variations of the O(1D) and O(1S) peak volume emission rates without direct solar effects-Reference-Cited by-同舟云学术

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Variations of the O(1D) and O(1S) peak volume emission rates without direct solar effects

Published:2008-09 Issue:5 Volume:42 Page:939-946
ISSN:0273-1177
Container-title:Advances in Space Research
language:en
Short-container-title:Advances in Space Research

Author:

Zhang Shengpan P.,Shepherd Gordon G.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference19 articles.

1. Introduction to Space Physics;Carlson,1995

2. Ground based spectroscopic studies of sunlit and aurora;Chakrabarti;Journal of Atmospheric and Solar-Terrestrial Physics,1998

3. Characteristics of dayside 5577Å and 3914Å aurora;Cogger;Geophysical Research Letters,1977

4. Liu, G., Shepherd, G.G. An investigation of the solar cycle impact on the mesopause O(1S) nightglow emission as observed by WINDII/UARS, Advances in Space Research.

5. Auroral morphology of the midday oval;Meng;Journal of Geophysical Research,1986

Cited by 2 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. First satellite-imaging observation of medium-scale traveling ionospheric disturbances by FORMOSAT-2/ISUAL;Geophysical Research Letters;2011-02

2. Extreme longitudinal disturbances in the mesosphere and thermosphere observed with the Wind Imaging Interferometer on UARS;Geophysical Research Letters;2008-08-16

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