globalchange  > 气候减缓与适应
DOI: 10.1002/2017JA024998
Scopus记录号: 2-s2.0-85041113054
论文题名:
Temporal Variability of Atomic Hydrogen From the Mesopause to the Upper Thermosphere
作者: Qian L.; Burns A.G.; Solomon S.S.; Smith A.K.; McInerney J.M.; Hunt L.A.; Marsh D.R.; Liu H.; Mlynczak M.G.; Vitt F.M.
刊名: Journal of Geophysical Research: Space Physics
ISSN: 21699380
出版年: 2018
卷: 123, 期:1
起始页码: 1006
结束页码: 1017
语种: 英语
英文关键词: diurnal ; hydrogen variability ; mesosphere ; seasonal ; solar cycle ; thermosphere
英文摘要: We investigate atomic hydrogen (H) variability from the mesopause to the upper thermosphere, on time scales of solar cycle, seasonal, and diurnal, using measurements made by the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) instrument on the Thermosphere Ionosphere Mesosphere Energetics Dynamics satellite, and simulations by the National Center for Atmospheric Research Whole Atmosphere Community Climate Model-eXtended (WACCM-X). In the mesopause region (85 to 95 km), the seasonal and solar cycle variations of H simulated by WACCM-X are consistent with those from SABER observations: H density is higher in summer than in winter, and slightly higher at solar minimum than at solar maximum. However, mesopause region H density from the Mass-Spectrometer-Incoherent-Scatter (National Research Laboratory Mass-Spectrometer-Incoherent-Scatter 00 (NRLMSISE-00)) empirical model has reversed seasonal variation compared to WACCM-X and SABER. From the mesopause to the upper thermosphere, H density simulated by WACCM-X switches its solar cycle variation twice, and seasonal dependence once, and these changes of solar cycle and seasonal variability occur in the lower thermosphere (~95 to 130 km), whereas H from NRLMSISE-00 does not change solar cycle and seasonal dependence from the mesopause through the thermosphere. In the upper thermosphere (above 150 km), H density simulated by WACCM-X is higher at solar minimum than at solar maximum, higher in winter than in summer, and also higher during nighttime than daytime. The amplitudes of these variations are on the order of factors of ~10, ~2, and ~2, respectively. This is consistent with NRLMSISE-00. ©2018. American Geophysical Union. All Rights Reserved.
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资源类型: 期刊论文
标识符: http://119.78.100.158/handle/2HF3EXSE/114861
Appears in Collections:气候减缓与适应

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作者单位: High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO, United States; Atmospheric Chemistry Observations and Modeling Laboratory, National Center for Atmospheric Research, Boulder, CO, United States; NASA Langley Research Center, Hampton, VA, United States

Recommended Citation:
Qian L.,Burns A.G.,Solomon S.S.,et al. Temporal Variability of Atomic Hydrogen From the Mesopause to the Upper Thermosphere[J]. Journal of Geophysical Research: Space Physics,2018-01-01,123(1)
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