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      The influence of internal variability on Earth's energy balance framework and implications for estimating climate sensitivity

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      Atmospheric Chemistry and Physics
      Copernicus GmbH

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          Abstract

          <p><strong>Abstract.</strong> Our climate is constrained by the balance between solar energy absorbed by the Earth and terrestrial energy radiated to space. This energy balance has been widely used to infer equilibrium climate sensitivity (ECS) from observations of 20th-century warming. Such estimates yield lower values than other methods, and these have been influential in pushing down the consensus ECS range in recent assessments. Here we test the method using a 100-member ensemble of the Max Planck Institute Earth System Model (MPI-ESM1.1) simulations of the period 1850–2005 with known forcing. We calculate ECS in each ensemble member using energy balance, yielding values ranging from 2.1 to 3.9<span class="thinspace"></span>K. The spread in the ensemble is related to the central assumption in the energy budget framework: that global average surface temperature anomalies are indicative of anomalies in outgoing energy (either of terrestrial origin or reflected solar energy). We find that this assumption is not well supported over the historical temperature record in the model ensemble or more recent satellite observations. We find that framing energy balance in terms of 500<span class="thinspace"></span>hPa tropical temperature better describes the planet's energy balance.</p>

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          Climate and carbon cycle changes from 1850 to 2100 in MPI-ESM simulations for the Coupled Model Intercomparison Project phase 5

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            Clouds and the Earth’s Radiant Energy System (CERES) Energy Balanced and Filled (EBAF) Top-of-Atmosphere (TOA) Edition-4.0 Data Product

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              Inference of Climate Sensitivity from Analysis of Earth's Energy Budget

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                Author and article information

                Journal
                Atmospheric Chemistry and Physics
                Atmos. Chem. Phys.
                Copernicus GmbH
                1680-7324
                2018
                April 17 2018
                : 18
                : 7
                : 5147-5155
                Article
                10.5194/acp-18-5147-2018
                aee78e4a-5c34-42fb-b614-3c027aabacca
                © 2018

                https://creativecommons.org/licenses/by/4.0/

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