DOI: 10.1002/2014MS000387
Scopus记录号: 2-s2.0-85027939690
论文题名: Simulated solar cycle effects on the middle atmosphere: WACCM3 Versus WACCM4
作者: Peck E ; D ; , Randall C ; E ; , Harvey V ; L ; , Marsh D ; R
刊名: Journal of Advances in Modeling Earth Systems
ISSN: 19422466
出版年: 2015
卷: 7, 期: 2 起始页码: 806
结束页码: 822
语种: 英语
英文关键词: Climate models
; Ionosphere
; Ozone
; Solar energy
; Antarctic stratosphere
; EPP
; Mesospheric temperature
; Particle precipitation
; Residual circulations
; Solar cycle
; WACCM
; Whole atmosphere community climate models
; Upper atmosphere
; climate modeling
; estimation method
; gravity wave
; irradiance
; mesosphere
; nitrogen
; nitrous oxide
; ozone
; parameterization
; polar meteorology
; precipitation (climatology)
; sensitivity analysis
; solar cycle
; stratosphere
; temperature gradient
; westerly
; zonal wind
; Southern Ocean
英文摘要: The Whole Atmosphere Community Climate Model version 4 (WACCM4) is used to quantify solar cycle impacts, including both irradiance and particle precipitation, on the middle atmosphere. Results are compared to previous work using WACCM version 3 (WACCM3) to estimate the sensitivity of simulated solar cycle effects to model modifications. The residual circulation in WACCM4 is stronger than in WACCM3, leading to larger solar cycle effects from energetic particle precipitation; this impacts polar stratospheric odd nitrogen and ozone, as well as polar mesospheric temperatures. The cold pole problem, which is present in both versions, is exacerbated in WACCM4, leading to more ozone loss in the Antarctic stratosphere. Relative to WACCM3, a westerly shift in the WACCM4 zonal winds in the tropical stratosphere and mesosphere, and a strengthening and poleward shift of the Antarctic polar night jet, are attributed to inclusion of the QBO and changes in the gravity wave parameterization in WACCM4. Solar cycle effects in WACCM3 and WACCM4 are qualitatively similar. However, the EPP-induced increase from solar minimum to solar maximum in polar stratospheric NOy is about twice as large in WACCM4 as in WACCM3; correspondingly, maximum increases in polar O3 loss from solar min to solar max are more than twice as large in WACCM4. This does not cause large differences in the WACCM3 versus WACCM4 solar cycle responses in temperature and wind. Overall, these results provide a framework for future studies using WACCM to analyze the impacts of the solar cycle on the middle atmosphere. © 2015. The Authors. Citation statistics:
资源类型: 期刊论文
标识符: http://119.78.100.158/handle/2HF3EXSE/76051
Appears in Collections: 影响、适应和脆弱性 气候变化与战略
There are no files associated with this item.
作者单位: Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, Colorado, United States; Department of Atmospheric and Oceanic Sciences, University of Colorado Boulder, Boulder, Colorado, United States; National Center for Atmospheric Research, Boulder, Colorado, United States
Recommended Citation:
Peck E,D,, Randall C,et al. Simulated solar cycle effects on the middle atmosphere: WACCM3 Versus WACCM4[J]. Journal of Advances in Modeling Earth Systems,2015-01-01,7(2)