An international team of researchers from United Kingdom, Denmark, and Germany have revealed, that during periods of increased solar irradiance, the trade winds weaken and the Walker circulation in the tropical Pacific shifts eastwards.
An international team of researchers from United Kingdom, Denmark, and Germany has found robust evidence for signatures of the 11-year sunspot cycle in the tropical Pacific. They analyzed historical time series of pressure, surface winds, and precipitation with specific focus on the Walker Circulation – a vast system of atmospheric flow in the tropical Pacific region that affects patterns of tropical rainfall. They have revealed that during periods of increased solar irradiance, the trade winds weaken and the Walker circulation shifts eastwards.
Stergios Misios, a postdoctoral researcher at the University of Oxford, said “We deal with a very short record of observations in the tropical Pacific and we must be very careful with how we filter out other interannual fluctuations. After a careful treatment of the data covering the last 60 years, we detected a robust slowdown of the Walker cell during years associated with solar-cycle maxima”. The analysis shows that, in tandem with changes in the wind anomalies, the dominant patterns of tropical precipitation shift to the central Pacific during solar-cycle maxima. As a result, rainfall decreases over Indonesia and in the western Pacific, and increases over the central Pacific Ocean.
Simple mechanisms amplify the solar signal
The issue of solar influences on climate is long and controversial as there have been numerous claims which in most of the cases did not survive proper statistical scrutiny. But besides statistical verification lies an even more challenging problem: how miniscule changes in incoming solar radiation could produce significant climate signatures?
“Soon enough, we realized that the magnitude of the wind anomalies that we detected in observations simply could not be explained by radiative considerations alone. We thought that if it comes from the Sun, there must be another mechanism that amplifies the weakening of the Walker circulation.” said Prof. Lesley Gray of University of Oxford. With the aid of a global climate model, this mechanism was found in the dynamical coupling between the atmosphere and ocean circulation in the tropical Pacific.
Averaged over the globe the surface temperature imprint of solar cycle barely reaches 0.1 K in a solar maximum – almost 8 times weaker than the global warming trends observed in the 20th century. Yet, even such a weak surface warming influences the Walker circulation through changes in global hydrology. As the surface warms, water vapor in the atmosphere increases at a higher rate than is lost by precipitation, necessitating a weakening of the Walker cell. This is a well-tested mechanism in model simulations of increased CO2 concentrations but it turns out that is operating under the 11-year solar cycle, too.