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58149376419
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To calculate the projected climate for 2090, we first added the observed temperature departures (in blue) to the change in the summer temperature, taken to be the mean summer temperature for 2080-2100 minus that for 1980-2000, simulated by each of the 23 climate models from the IPCC AR4 forced by the middle of the road emission scenario, A1B. We then combined the 23 x 107 projections to create the probability distribution function for summer temperature in 2090 (see SOM).
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To calculate the projected climate for 2090, we first added the observed temperature departures (in blue) to the change in the summer temperature, taken to be the mean summer temperature for 2080-2100 minus that for 1980-2000, simulated by each of the 23 climate models from the IPCC AR4 forced by the "middle of the road" emission scenario, A1B. We then combined the 23 x 107 projections to create the probability distribution function for summer temperature in 2090 (see SOM).
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58149374516
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The probability distribution of future summer temperature is calculated as described in (21). Here, summer is defined north of the equator as the average temperature from June through August and south of the equator as December through February. In the immediate vicinity of the equator, values in Fig. 3 are qualitatively insensitive to the choice of months that define the season.
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The probability distribution of future summer temperature is calculated as described in (21). Here, summer is defined north of the equator as the average temperature from June through August and south of the equator as December through February. In the immediate vicinity of the equator, values in Fig. 3 are qualitatively insensitive to the choice of months that define the season.
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23
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58149382537
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This work was made possible by grants from the NSF (grant SES 0433679) and the Tamaki Foundation. We thank M. Baker, M. Burke, W. Falcon, D. Kennedy, S.-H. Kim, D. Lobell, R. Nicholas, K. Niemer Johnson, K. Rennert, and D. Vimont for comments and/or assistance on the draft
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This work was made possible by grants from the NSF (grant SES 0433679) and the Tamaki Foundation. We thank M. Baker, M. Burke, W. Falcon, D. Kennedy, S.-H. Kim, D. Lobell, R. Nicholas, K. Niemer Johnson, K. Rennert, and D. Vimont for comments and/or assistance on the draft.
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