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Burning Plasma: Bringing a Star to Earth
Burning Plasma Assessment Committee
John Ahearne, Sigma Xi and Duke University and Raymond Fonck, University of Wisconsin at Madison, Co-chairs
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Burning Plasma: Bringing a Star to Earth
Significant advances have been made in fusion science, and a decision point has been reached about whether the United States is ready to begin a burning plasma experiment. A burning plasma—in which at least 50% of the energy to drive the fusion reaction is generated internally—is an essential step to reach the goal of fusion power generation. The Burning Plasma Assessment Committee was formed to provide advice on this decision.
The committee concluded that there is high confidence in the readiness to proceed with the burning plasma step. The International Thermonuclear Experimental Reactor (ITER), with the United States as a significant partner, was the best choice. Once a commitment to ITER is made, fulfilling it should become the highest priority of the U.S. fusion research program. A funding trajectory is required that both captures the benefits of joining ITER and retains a strong scientific focus on the long-range goal of the program. The addition of the ITER project will require the content, scope, and level of U.S. fusion activity be defined by program balancing through a priority-setting process initiated by the Office of Fusion Energy Science.
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Committee and Staff Rosters
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Committee Membership
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John F. Ahearne, Sigma Xi and Duke University, Co-chair
Raymond Fonck, University of Wisconsin at Madison, Co-chair
John N. Bahcall, Princeton University
Gordon A. Baym, University of Illinois at Urbana-Champaign
Ira B. Bernstein, Yale University
Steven C. Cowley, Imperial College London
Edward A. Frieman, SAIC
Walter Gekelman, University of California at Los Angeles
Joseph Hezir, EOP Group, Inc.
William M. Nevins, Lawrence Livermore National Laboratory
Ronald R. Parker, Massachusetts Institute of Technology
Claudio Pellegrini, University of California at Los Angeles
Burton Richter, Stanford Linear Accelerator Center
Clifford M. Surko, University of California at San Diego
Tony S. Taylor, General Atomics
Michael A. Ulrickson, Sandia National Laboratories
Michael C. Zarnstorff, Princeton Plasma Physics Laboratory
Ellen G. Zweibel, University of Wisconsin at Madison
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NRC Staff
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Donald C. Shapero, Board Director
Michael Moloney, Program Officer
Timothy I. Meyer, Program Officer
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Post Production Comments
The committee released its interim letter report on December 20, 2002. The unedited prepublication draft of its final report was released on September 26, 2003. The full report was published by the National Academies Press in April 2004.
The following communication was received from Dr. Bruno Coppi after production and release of the final report.
Call for community input
To assist BPAC in the execution of this study, the Committee invited the community to send brief statements or comments relevant to the committee’s charge. Comments were submitted by e-mail. Please note that all community input received was posted on this web site and is made available through the public access file for this committee as required by the Federal Advisory Committee Act. Community Input received
Related Links
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