A simulation study of 630 nm and 557.7 nm airglow variations due to dissociative recombination and thermal electrons by high-power HF heating
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Earth and Planetary Physics
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http://www.eppcgs.org/en/article/pdf/preview/10.26464/epp2017006
Cited by 4 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. Simulation of Space Borne Ionospheric Airglow Imaging;SPECTROSC SPECT ANAL;2022
2. 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
3. Electron acceleration by Langmuir turbulence in ionospheric heating;Earth and Planetary Physics;2022
4. Response of Background Optical Emission to Ionospheric Heating by High-Power Radio Emission;Geomagnetism and Aeronomy;2021-05
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