Chemical and dynamical response to the 11‐year variability of the solar irradiance simulated with a chemistry‐climate model

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Abstract
Atmospheric effects of the solar irradiance variations during 11‐year solar cycle are investigated using a chemistry‐climate model. The model is enhanced by a more detailed parameterization of the oxygen and ozone UV heating rates. The simulated ozone response to the imposed solar forcing shows a positive correlation in the tropical stratosphere and a negative correlation in the tropical mesosphere, in agreement with theoretical expectation. The model suggests an acceleration of the polar night jets in both hemispheres and a dipole structure in the temperature changes at high latitudes. The model results also show an alteration of the tropospheric circulation air resulting in a statistically significant warming of 1 K in the annual mean surface air temperature over North America and Siberia. This supports the idea of a solar‐climate connection.