Summary
A previous model which allows the calculation of the target gain consistently with the implosion phase is used to study how the ignition energy is determined by the parameters which control the implosion and the ignition. Location and height of the ignition cliff are found to be strongly dependent on the implosion velocity and on the cold fuel isentrope, in good agreement with recently reported simulations. Besides, gain and ignition energy depend on the constraints imposed by the symmetry and hydrostability criteria.
Similar content being viewed by others
References
E. M. Campbell:J. Fusion Energy,10, 277 (1991).
R. E. Kidder:Nucl. Fusion,16, 405 (1976).
S. E. Bodner:J. Fusion Energy,1, 221 (1981).
J. Meyer-Ter-Vehn:Nucl. Fusion,22, 561 (1982).
S. Atzeni andA. Caruso:Nuovo Cimento B,80, 71 (1984).
A. R. Piriz andJ. G. Wouchuk:Nucl. Fusion,32, 933 (1992).
G. S. Fraley, E. J. Linnebur, R. J. Mason andR. L. Morse:Phys. Fluids,17, 474 (1974).
A. R. Piriz andJ. G. Wouchuk:Phys. Fluids B,3, 2889 (1991).
J. D. Lindl:Inertial Confinement Fusion, edited byA. Caruso andE. Sindoni (Editrice Compositori, Bologna, 1989), p. 617.
F. J. Mayer, J. Larsen andJ. W. Steele:Phys. Fluids,26, 830 (1983).
J. D. Lindl, R. L. McCrory andE. M. Campbell:Phys. Today, Sept. 1992, p. 32.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Piriz, A.R., Wouchuk, J.G. Energy gain of spherical shell targets ablatively imploded by thermal radiation. Nuov Cim A 106, 1901–1907 (1993). https://doi.org/10.1007/BF02780593
Received:
Revised:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1007/BF02780593