Zobrazeno 1 - 10
of 16
pro vyhledávání: '"D. C. Marion"'
Autor:
C. C. Kuranz, H.-S. Park, C. M. Huntington, A. R. Miles, B. A. Remington, T. Plewa, M. R. Trantham, H. F. Robey, D. Shvarts, A. Shimony, K. Raman, S. MacLaren, W. C. Wan, F. W. Doss, J. Kline, K. A. Flippo, G. Malamud, T. A. Handy, S. Prisbrey, C. M. Krauland, S. R. Klein, E. C. Harding, R. Wallace, M. J. Grosskopf, D. C. Marion, D. Kalantar, E. Giraldez, R. P. Drake
Publikováno v:
Nature Communications, Vol 9, Iss 1, Pp 1-6 (2018)
Radiation and conduction are generally considered as the main energy transport mechanisms for the evolution of early supernova remnants. Here the authors experimentally show the role of electron heat transfer on the growth of Rayleigh–Taylor instab
Externí odkaz:
https://doaj.org/article/f153b9b02a5a45d6934610dc34ba9b57
Autor:
Kirk Flippo, W. C. Wan, Channing Huntington, A. Shimony, R. P. Drake, Forrest Doss, H.-S. Park, Kumar Raman, Sallee Klein, Timothy Handy, Steve MacLaren, C.C. Kuranz, A. R. Miles, Bruce Remington, Daniel H. Kalantar, Dov Shvarts, E. M. Giraldez, Tomasz Plewa, D. C. Marion, C. M. Krauland, Shon Prisbrey, Michael Grosskopf, R. J. Wallace, Guy Malamud, Eric Harding, John Kline, Matthew Trantham, Harry Robey
Publikováno v:
Nature Communications, Vol 9, Iss 1, Pp 1-6 (2018)
Nature Communications
Nature Communications
Energy-transport effects can alter the structure that develops as a supernova evolves into a supernova remnant. The Rayleigh–Taylor instability is thought to produce structure at the interface between the stellar ejecta and the circumstellar matter
Autor:
C.C. Kuranz, H.-S. Park, Omar Hurricane, Bruce Remington, Christine Krauland, Dov Shvarts, David Martinez, J. F. Hansen, D. C. Marion, Y. Elbaz, R. J. Wallace, G. Langstaff, Harry Robey, Oleg Schilling, R. P. Drake, C. A. Di Stefano, A. Shimony, V. A. Smalyuk, Kumar Raman
Publikováno v:
High Energy Density Physics. 9:47-51
Kelvin–Helmholtz (KH) turbulent mixing measurements were performed in experiments on the OMEGA Laser Facility [T.R. Boehly et al., Opt. Commun. 133 (1997) 495]. In these experiments, laser-driven shock waves propagated through low-density plastic f
Publikováno v:
High Energy Density Physics. 8:360-365
Laser-driven blast waves are frequently used to explore hydrodynamic instability at high energy density. Experiments are designed such that the instability physics occurs in isolation, but secondary processes will eventually develop within the experi
Autor:
Erica M. Rutter, R. P. Drake, Quentin F. Stout, Ryan G. McClarren, Vijay Nair, Marvin L. Adams, C. M. Huntington, Bani K. Mallick, Lawrence Rauchwerger, Michael Grosskopf, A. J. Visco, Jim E. Morel, Krzysztof J. Fidkowski, Kenneth G. Powell, Nancy M. Amato, Carolyn Kuranz, B. van Leer, Philip L. Roe, C.A. Di-Stefano, E.S. Myra, Edward W. Larsen, Igor V. Sokolov, Gabor Toth, Bruce Fryxell, F. W. Doss, James Paul Holloway, Chuan-Chih Chou, William R. Martin, Tamas I. Gombosi, Ben Torralva, Katsuyo Thornton, Smadar Karni, B. van der Holst, D. C. Marion, Derek Bingham, Christine Krauland
Publikováno v:
High Energy Density Physics. 7:130-140
Using modern high-energy-density facilities it is straightforward to produce radiative shock waves in which the transfer of energy by radiation controls the hydrodynamic structure of the system. Some of these experiments use shock tubes. This paper d
Autor:
George A. Kyrala, Tomasz Plewa, H. S. Park, Abbas Nikroo, W. D. Arnett, C.C. Kuranz, D. C. Marion, John Kline, John C Wheeler, B. K. F. Young, R. P. Drake, A. R. Miles, Christine Krauland, Bruce Remington, E. M. Giraldez, F. W. Doss, Harry Robey, J. D. Kilkenny, E. C. Harding, Brian Maddox, E.S. Myra, Christopher J. Keane, Daniel H. Kalantar, Michael Grosskopf, R. J. Wallace, C. M. Huntington
Publikováno v:
Astrophysics and Space Science. 336:207-211
The National Ignition Facility (NIF) is capable of creating new and novel high-energy-density (HED) systems relevant to astrophysics. Specifically, a system could be created that studies the effects of a radiative shock on a hydrodynamically unstable
Autor:
A. J. Visco, Carolyn Kuranz, E. C. Harding, C. M. Huntington, R. P. Drake, Michael Grosskopf, C. A. Di Stefano, D. C. Marion, F. W. Doss, Christine Krauland
Publikováno v:
Fusion Science and Technology. 59:250-256
At the University of Michigan (U-M), we have successfully fabricated and characterized targets for our experimental campaigns since 2003. Because of the unique production environment, we iterate many models in the course of a single-shot plan and hav
Autor:
B. E. Blue, J. P. Knauer, D.J. Kremer, N. Hearn, J. F. Hansen, Harry Robey, Carolyn Kuranz, Michael Grosskopf, Christine Krauland, T. L. Donajowski, K. K. Dannenberg, D. C. Marion, R. P. Drake, Bruce Remington, Tomasz Plewa
Publikováno v:
Astrophysics and Space Science. 307:115-119
We present data from recent high-energy-density laboratory experiments designed to explore the Rayleigh-Taylor instability under conditions relevant to supernovae. The Omega laser is used to create a blast wave structure that is similar to that of th
Autor:
Carolyn Kuranz, G. Langstaff, J. F. Hansen, J. A. Greenough, Bruce Remington, D. C. Marion, C. A. Di Stefano, R. J. Wallace, H.-S. Park, Christine Krauland, Omar Hurricane, Harry Robey, David Martinez, Oleg Schilling, R. P. Drake, V. A. Smalyuk, Kumar Raman
Publikováno v:
Physical review letters. 109(15)
Following the successful demonstration of an OMEGA laser-driven platform for generating and studying nearly two-dimensional unstable plasma shear layers [Hurricane et al., Phys. Plasmas 16, 056305 (2009); Harding et al., Phys. Rev. Lett. 103, 045005
Autor:
M.R. Taylor, D. R. Leibrandt, R. P. Drake, David Arnett, C.C. Kuranz, Casey Meakin, A. R. Miles, Tomasz Plewa, D. C. Marion, Harry Robey, A. J. Visco, Christine Krauland, M. J. Edwards, J. P. Knauer, D.J. Kremer, N. Hearn, Michael Grosskopf, E. C. Harding, B. E. Blue, K.K. Killibrew, J. F. Hansen
Publikováno v:
The 33rd IEEE International Conference on Plasma Science, 2006. ICOPS 2006. IEEE Conference Record - Abstracts..
Summary form only given. Our goal is to experimentally confirm or disprove the hypothesis that the Rayleigh-Taylor instability could be responsible for the observed transport of heavy elements from the core of SN1897A, a core-collapse supernova, into