A simulation study of 630 nm and 557.7 nm airglow variations due to dissociative recombination and thermal electrons by high-power HF heating-Reference-Cited by-同舟云学术

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A simulation study of 630 nm and 557.7 nm airglow variations due to dissociative recombination and thermal electrons by high-power HF heating

Published:2017 Issue:1 Volume:1 Page:44-52
ISSN:2096-3955
Container-title:Earth and Planetary Physics
language:en
Short-container-title:

Author:

Dang Tong, ,Lei JiuHou,Dou XianKang,Wan WeiXing, , , ,

Publisher

Earth and Planetary Physics

Link

http://www.eppcgs.org/en/article/pdf/preview/10.26464/epp2017006

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3. Electron acceleration by Langmuir turbulence in ionospheric heating;Earth and Planetary Physics;2022

4. Modeling and causative mechanism of OI 630.0 nm nightglow emission over Cachoeira Paulista (22.7oS, 45oW) – Brazil: Seasonal and temporal variability;Advances in Space Research;2022-01

5. Response of Background Optical Emission to Ionospheric Heating by High-Power Radio Emission;Geomagnetism and Aeronomy;2021-05

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