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Radiative Forcing by Clouds

The globally and seasonally averaged effect of clouds on the energy budget today is a cooling by 17.3 W/m [ Ramanathan et al., 1989; Harrison et al., 1990], but this figure for net forcing obscures much larger regional effects and a competition between longwave and shortwave forcing. Clouds reflect sunlight, cooling the Earth, but they trap infrared radiation, which warms the ground. Spacecraft measurements in the Earth Radiation Budget Experiment [ Ramanathan et al., 1989; Harrison et al., 1990] reveal an average shortwave forcing or -48.4 W/m and an average longwave forcing of 31.1 W/m. The effects of clouds on the components of the energy budget are considerably larger than the net. Indeed, they are about the same as the greenhouse effect of all gases other than water vapor [ Raval and Ramanathan, 1989]. The latitudinal and seasonal distribution of cloud forcing [ Harrison et al., 1990] reveals even larger local effects. At high latitudes during summer, negative forcing by clouds can exceed 100 W/m, particularly over the oceans. Figure 1 shows zonally-averaged cloud forcing in southern and northern summers [ Harrison et al., 1990]. Clouds cool low latitudes modestly at all seasons, warm high latitudes modestly during the winter, and cool high latitudes very strongly during summer. A negative forcing of 100 W/m must make high latitude summers a lot colder than they would be if there were no clouds and no other changes in the climate system.

There is no great mystery about the large negative forcing at high latitudes. Figure 2 shows that cloud cover over the high-latitude ocean exceeds 80% and varies little with season [ Warren et al., 1986, 1988]. The cloud type is principally low-altitude stratus. In summer, when the sun is shining, the shortwave cooling effect of these clouds far exceeds the longwave forcing. The clouds are still there in the winter, but there is little sunlight for them to reflect.

Why have clouds received so little attention in paleoclimatic research when observed cloud forcing is so large? Because they have left no geological record, and even the instrumental record is unreliable. Because we do not understand cloud processes well enough to calculate cloud properties in different atmospheres. Indeed, we know that the parameterization of clouds is the largest identifiable source of error (disagreement) in global climate models [ Cess et al., 1989]. These reasons, although compelling, do not justify the neglect of what may be a dominant influence on climate evolution. In what follows I shall suggest how clouds may help to resolve three important paleoclimatic problems: the irregular increase of global average temperature during the industrial revolution, the amplification of ice age climate fluctuations, and the progressive cooling of high latitudes during the Cenozoic. My suggestions are no more than speculations. It is hard to see how we can be sure of the role of clouds in climate change until our simulations include much more convincing representations of cloud-climate interactions or some clever person discovers a paleocloud record. I offer these suggestions to stimulate thinking along these lines.



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Next: Industrial Revolution Up: There is more to Previous: Global Energy Balance



U.S. National Report to IUGG, 1991-1994
Rev. Geophys. Vol. 33 Suppl., © 1995 American Geophysical Union