Open AccessSimulated solar cycle effects on the middle atmosphere: WACCM3 Versus WACCM4
Author(s) -
Peck E. D.,
Randall C. E.,
Harvey V. L.,
Marsh D. R.
Publication year - 2015
Publication title -
journal of advances in modeling earth systems
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 3.03
H-Index - 58
ISSN - 1942-2466
DOI - 10.1002/2014ms000387
Subject(s) - stratosphere , atmospheric sciences , atmosphere (unit) , environmental science , mesosphere , solar cycle , polar night , solar irradiance , ozone layer , solar minimum , solar maximum , climatology , meteorology , physics , geology , solar wind , quantum mechanics , magnetic field
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 NO y is about twice as large in WACCM4 as in WACCM3; correspondingly, maximum increases in polar O 3 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.