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Leo J. Donner, Bruce L. Wyman, Richard S. Hemler, Larry W. Horowitz, Yi Ming, Ming Zhao, Jean-Christophe Golaz, Paul Ginoux, S.-J. Lin, M. Daniel Schwarzkopf, John Austin, Ghassan Alaka, William F. Cooke, Thomas L. Delworth, Stuart M. Freidenreich, C. T. Gordon, Stephen M. Griffies, Isaac M. Held, William J. Hurlin, Stephen A. Klein, Thomas R. Knutson, Amy R. Langenhorst, Hyun-Chul Lee, Yanluan Lin, Brian I. Magi, Sergey L. Malyshev, P. C. D. Milly, Vaishali Naik, Mary J. Nath, Robert Pincus, Jeffrey J. Ploshay, V. Ramaswamy, Charles J. Seman, Elena Shevliakova, Joseph J. Sirutis, William F. Stern, Ronald J. Stouffer, R. John Wilson, Michael Winton, Andrew T. Wittenberg, and Fanrong Zeng

the GPCP analysis ( Huffman et al. 1997 ), broad features of the observed pattern are simulated ( Fig. 18 ). The magnitude of the anomalies is largest in AM3 and smallest in CM3, with GPCP being intermediate. The maxima in AM3 are clustered more closely together than in CM3. GPCP does not exhibit multiple maxima. Fig . 18. DJF product of the standard deviation of the Niño-3 index and regression coefficient between precipitation and Niño-3 index (mm day −1 ) for (a) AM3, (b) CM3, and (c) GPCP. The

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