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CHAPTER 2 • Climate Archives, Data, and Models  33


                                                                        FIGURE 2-19 3-D GCMs General circulation
                              Back                      Incoming
           3-D Grid box     radiation                 solar radiation   models (GCMs) are full 3-D representations of
         (CO , dust, H O )                                              Earth’s surface and atmosphere, represented
            2       2  v
                                                                        by individual grid boxes. Representations of
                                                                        Earth’s surface within each grid box are entirely
                                                                        land, ocean, or ice. (Adapted from W. F.
                                                                        Ruddiman and J. E. Kutzbach, “Plateau Uplift
                                                                        and Climate Change,” Scientific American 264
                                                                        [1991]: 66–75.)







                   Mountains
                                Land
                                           Ocean























           The operation of A-GCMs incorporates the physi-  compared with regional instrumental measurements of
        cal laws and equations that govern the circulation of  temperature, precipitation, pressure, and winds in the
        Earth’s atmosphere: the fluid motion of air; conserva-  present climate system averaged over the last several
        tion of mass, energy, and other properties; and gas laws  decades (for example, Figure 2–21). Areas of major dis-
        covering the expansion and contraction of air. The indi-  agreement between the model output and instrumental
        vidual grid boxes in A-GCMs interact with their imme-  observations often become the focus of additional
        diate neighbors.                                    improvements in the model.
           Model runs begin with the atmosphere in a state of  As noted earlier, A-GCM experiments on past cli-
        rest. After solar heating causes air to begin to move, the  mates require scientists to specify major changes in
        model is run long enough for the atmosphere to reach a  boundary conditions on the basis of geological evidence
        state of equilibrium (Figure 2–20). Equilibrium occurs  from Earth’s history. In one approach, called a sensitivity
        when the long-term drift in the simulated climate data  test, just one boundary condition is altered in relation to
        disappears. The oscillations that remain are analogous  the present-day configuration. When the output of such
        to short-term changes in weather over days and weeks.  an experiment is compared with the output from the
           Running climate experiments on current-genera-   modern control case, the differences in climate between
        tion A-GCMs requires a simulation of at least 20 years  the two runs isolate and reveal the unique impact caused
        of climate. The first 15 years of the simulation are the  by the change in that one boundary condition.
        “spin-up” interval, used to let the model attain a state of  In contrast, a climate reconstruction requires chang-
        equilibrium. The last 5 years of the simulation produce  ing all known boundary conditions at the same time to
        the climate data that form the actual output of the  try to simulate the full state of the climate system at
        model. For the control-case simulation of modern    some time in the past. This approach is more demanding
        climate, the climate-data output from the GCM are   than a sensitivity test, because all the potentially critical
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