A Simulation of the Influence of DE3 Tide on Nitric Oxide Infrared Cooling
文献类型:期刊论文
作者 | Ren, Zhipeng1,2,3,4; Wan, Weixing1,2,3,4; Xiong, Jiangang1,2,3,4; Li, Xing5,6 |
刊名 | JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
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出版日期 | 2020-03-01 |
卷号 | 125期号:3页码:10 |
ISSN号 | 2169-9380 |
DOI | 10.1029/2019JA027131 |
英文摘要 | Using GCITEM-IGGCAS model, we simulate the influence of the eastward propagating nonmigrating diurnal tide with Zonal Wave Number 3 (DE3) on nitric oxide (NO) infrared cooling rate. We find that the DE3 tide can drive a DE3 signal in lower thermospheric NO cooling rate, and the simulated altitudinal and seasonal variations are according with that of DE3 signal in equatorial lower thermospheric NO cooling rate observed by Oberheide et al. (2013, https://doi.org/10.1002/2013JA019278), which is based on the Thermosphere Ionosphere Mesosphere Energetics and Dynamics/Sounding of the Atmosphere using Broadband Emission Radiometry observations during the solar minimum year 2008. This signal mainly shows an annual variation, which is stronger between June and September and weaker near November. The maximum of the absolute signal, whose value is about 0.35 * 10(-9) W/m(3), occurs near the height of 130 km, but the relative signal mainly shows its peak with a value of 40% near the height of 100 km. Due to the difference of the driving mechanism, the distribution of NO signals in different latitudinal regions shows obvious difference. The middle- and low-latitude NO signals show smooth variation, while the high-latitude signal is discontinuous. The DE3 signal in NO cooling rate is mainly controlled by DE3 temperature tide and DE3 NO tide; meanwhile, the influences of DE3 neutral density tide on the DE3 signal can be ignored. The relative contributions of the DE3 NO tide and of the DE3 temperature tide vary with geographic latitude. The DE3 cooling rates in middle and low latitudes and in high latitude are, respectively, mainly driven by the DE3 temperature tide DE3 NO tide. DE3 tide may not only drive the DE3 signal but also affect the lower thermospheric zonal mean NO cooling rate. The maximum of the absolute influence, whose value is about 0.12 * 10(-9) W/m(3), occurs above the height of 140 km, but the relative influence mainly shows its peak with a value of 10% near the height of 100 km. |
WOS关键词 | NONMIGRATING SEMIDIURNAL TIDES ; LATENT-HEAT RELEASE ; LATITUDES ; WIND |
资助项目 | Strategic Priority Research Program of Chinese Academy of Sciences[XDA17010201] ; National Science Foundation of China[41674158] ; National Science Foundation of China[41874179] ; National Science Foundation of China[41621063] ; National Science Foundation of China[41427901] ; National Science Foundation of China[41474133] ; National Science Foundation of China[41322030] ; Youth Innovation Promotion Association CAS[2014057] ; Opening Funding of Chinese Academy of Sciences |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000535389600038 |
出版者 | AMER GEOPHYSICAL UNION |
资助机构 | Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; Youth Innovation Promotion Association CAS ; Youth Innovation Promotion Association CAS ; Youth Innovation Promotion Association CAS ; Youth Innovation Promotion Association CAS ; Opening Funding of Chinese Academy of Sciences ; Opening Funding of Chinese Academy of Sciences ; Opening Funding of Chinese Academy of Sciences ; Opening Funding of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; Youth Innovation Promotion Association CAS ; Youth Innovation Promotion Association CAS ; Youth Innovation Promotion Association CAS ; Youth Innovation Promotion Association CAS ; Opening Funding of Chinese Academy of Sciences ; Opening Funding of Chinese Academy of Sciences ; Opening Funding of Chinese Academy of Sciences ; Opening Funding of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; Youth Innovation Promotion Association CAS ; Youth Innovation Promotion Association CAS ; Youth Innovation Promotion Association CAS ; Youth Innovation Promotion Association CAS ; Opening Funding of Chinese Academy of Sciences ; Opening Funding of Chinese Academy of Sciences ; Opening Funding of Chinese Academy of Sciences ; Opening Funding of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; Youth Innovation Promotion Association CAS ; Youth Innovation Promotion Association CAS ; Youth Innovation Promotion Association CAS ; Youth Innovation Promotion Association CAS ; Opening Funding of Chinese Academy of Sciences ; Opening Funding of Chinese Academy of Sciences ; Opening Funding of Chinese Academy of Sciences ; Opening Funding of Chinese Academy of Sciences |
源URL | [http://ir.iggcas.ac.cn/handle/132A11/96682] ![]() |
专题 | 地质与地球物理研究所_中国科学院地球与行星物理重点实验室 |
通讯作者 | Ren, Zhipeng |
作者单位 | 1.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China 2.Univ Chinese Acad Sci, Coll Earth & Planetary Sci, Beijing, Peoples R China 3.Chinese Acad Sci, Beijing Natl Observ Space Environm, Inst Geol & Geophys, Beijing, Peoples R China 4.Chinese Acad Sci, Innovat Acad Earth Sci, Beijing, Peoples R China 5.Beihang Univ, Sch Space & Environm, Beijing, Peoples R China 6.Minist Ind & Informat Technol, Key Lab Space Environm Monitoring & Informat Proc, Beijing, Peoples R China |
推荐引用方式 GB/T 7714 | Ren, Zhipeng,Wan, Weixing,Xiong, Jiangang,et al. A Simulation of the Influence of DE3 Tide on Nitric Oxide Infrared Cooling[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2020,125(3):10. |
APA | Ren, Zhipeng,Wan, Weixing,Xiong, Jiangang,&Li, Xing.(2020).A Simulation of the Influence of DE3 Tide on Nitric Oxide Infrared Cooling.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,125(3),10. |
MLA | Ren, Zhipeng,et al."A Simulation of the Influence of DE3 Tide on Nitric Oxide Infrared Cooling".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 125.3(2020):10. |
入库方式: OAI收割
来源:地质与地球物理研究所
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