Enhancement of OI 630.0nm emission at mid-latitudes during an intense magnetic storm-Reference-Cited by-同舟云学术

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Enhancement of OI 630.0nm emission at mid-latitudes during an intense magnetic storm

Published:2007-04 Issue:6 Volume:69 Page:697-706
ISSN:1364-6826
Container-title:Journal of Atmospheric and Solar-Terrestrial Physics
language:en
Short-container-title:Journal of Atmospheric and Solar-Terrestrial Physics

Author:

Chung J.-K.,Wu Q.,Kim Y.H.,Won Y.-I.,Solomon S.,Park J.U.,Choi B.G.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Atmospheric Science,Geophysics

Reference25 articles.

1. Ionospheric storms;Buonsanto;Space Science Review,1999

2. Physics of the Aurora and Airglow;Chamberlain,1961

3. Coordinated stable auroral red arc observations: relationship to plasma convection;Foster;Journal of Geophysical Research,1994

4. Characteristics of a stable auroral red arc event;Kozyra;Geophysical Research Letters,1982

5. The role of ring current nose events in producing stable auroral arc intensifications during the main phase: observations during the September 19–24, 1984, Equinox transition study;Kozyra;Journal of Geophysical Research,1993

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. Ionospheric Responses to the May 2024 G5 Geomagnetic Storm Over Korea, Captured by the Korea Astronomy and Space Science Institute (KASI) Near Real-Time Ionospheric Monitoring System;Journal of Space Technology and Applications;2024-08

2. Magnetic signatures of medium-scale traveling ionospheric disturbances as observed by CHAMP;Journal of Geophysical Research: Space Physics;2009-03

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