Zobrazeno 1 - 10
of 94
pro vyhledávání: '"Chikang Li"'
Autor:
Hong Sio, Chikang Li, Cody E. Parker, Brandon Lahmann, Ari Le, Stefano Atzeni, Richard D. Petrasso
Publikováno v:
Matter and Radiation at Extremes, Vol 4, Iss 5, Pp 055401-055401-5 (2019)
The impact of fuel-ion diffusion in inertial confinement fusion implosions is assessed using nuclear reaction yield ratios and reaction histories. In T3He-gas-filled (with trace D) shock-driven implosions, the observed TT/T3He yield ratio is ∼2× l
Externí odkaz:
https://doaj.org/article/c8d49704026746e69beb2db953aee440
Autor:
Shu Zhang, Abraham Chien, Lan Gao, Hantao Ji, Eric G. Blackman, Russ Follett, Dustin H. Froula, Joseph Katz, Chikang Li, Andrew Birkel, Richard Petrasso, John Moody, Hui Chen
Magnetic reconnection converts magnetic energy into thermal and kinetic energy in plasma. Among numerous candidate mechanisms, ion acoustic instabilities driven by the relative drift between ions and electrons, or equivalently electric current, have
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::106dec8dce1755d80ca01a14b5995d8e
Autor:
Joseph M. Levesque, Andy S. Liao, Patrick Hartigan, Rachel P. Young, Matthew Trantham, Sallee Klein, William Gray, Mario Manuel, Gennady Fiksel, Joseph Katz, Chikang Li, Andrew Birkel, Petros Tzeferacos, Edward C. Hansen, Benjamin Khiar, John M. Foster, Carolyn C. Kuranz
The magnetic field produced by planets with active dynamos, like the Earth, can exert sufficient pressure to oppose supersonic stellar wind plasmas, leading to the formation of a standing bow shock upstream of the magnetopause, or pressure-balance su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b75a62f05d0eabb00dd99a04108b5bca
Autor:
W. Garbett, Duncan Barlow, Chikang Li, Matthew Khan, T. Goffrey, A. G. Seaton, Luca Antonelli, Robbie Scott, Mingsheng Wei, Dimitri Batani, Alexis Casner, W. Theobald, Riccardo Betti, Kevin Glize, Nigel Woolsey, Keith Bennett, Christian Stoeckl, Tony Arber, Stefano Atzeni
We use a subignition scale laser, the 30 kJ Omega, and a novel shallow-cone target to study laser-plasma interactions at the ablation-plasma density scale lengths and laser intensities anticipated for direct drive shock-ignition implosions at Nationa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7131fa9737549691b2dd14a701e9b683
https://eprints.whiterose.ac.uk/177608/1/PhysRevLett.127.065001.pdf
https://eprints.whiterose.ac.uk/177608/1/PhysRevLett.127.065001.pdf
Autor:
C. Shuldberg, M. Schoff, Michael Rosenberg, Chikang Li, J. J. Sanchez, L. F. Berzak Hopkins, Jacob Eriksson, David Schlossberg, Christian Stoeckl, Chad Forrest, Patrick Adrian, Johan Frenje, Owen Mannion, R. Janezic, G. Kagan, S. Fess, M. Hoppe, C. E. Parker, Raspberry Simpson, V. Yu. Glebov, Stefano Atzeni, R. D. Petrasso, Brandon Lahmann, H. Sio, M. Gatu Johnson, R.W. Luo, C. B. Yeamans, K. D. Hahn, Arijit Bose, H. G. Rinderknecht, Graeme Sutcliffe, Neel Kabadi, Fredrick Seguin
Publikováno v:
Physical Review E. 104
A series of thin glass-shell shock-driven DT gas-filled capsule implosions was conducted at the OMEGA laser facility. These experiments generate conditions relevant to the central plasma during the shock-convergence phase of ablatively driven inertia
Autor:
Johan Frenje, H. Sio, C. Sorce, M. Gatu Johnson, Brett Scheiner, R. C. Shah, R. D. Petrasso, Sean Regan, Graeme Sutcliffe, Brandon Lahmann, Benjamin Bachmann, Mark J. Schmitt, B Aguirre, Neel Kabadi, William E. Martin, Fredrick Seguin, A. Birkel, Chikang Li, Owen Mannion, H. G. Rinderknecht, Patrick Adrian, Z. L. Mohamed
Publikováno v:
The Review of scientific instruments. 92(4)
Hot-spot shape and electron temperature (Te) are key performance metrics used to assess the efficiency of converting shell kinetic energy into hot-spot thermal energy in inertial confinement fusion implosions. X-ray penumbral imaging offers a means t
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Autor:
Jena Meinecke, Petros Tzeferacos, James S. Ross, Archie F. A. Bott, Scott Feister, Hye-Sook Park, Anthony R. Bell, Roger Blandford, Richard L. Berger, Robert Bingham, Alexis Casner, Laura E. Chen, John Foster, Dustin H. Froula, Clement Goyon, Daniel Kalantar, Michel Koenig, Brandon Lahmann, Chikang Li, Yingchao Lu, Charlotte A. J. Palmer, Richard D. Petrasso, Hannah Poole, Bruce Remington, Brian Reville, Adam Reyes, Alexandra Rigby, Dongsu Ryu, George Swadling, Alex Zylstra, Francesco Miniati, Subir Sarkar, Alexander A. Schekochihin, Donald Q. Lamb, Gianluca Gregori
Publikováno v:
Meinecke, J, Tzeferacos, P, Ross, J S, Bott, A F A, Feister, S, Park, H-S, Bell, A R, Blandford, R, Berger, R L, Bingham, R, Casner, A, Chen, L E, Foster, J, Froula, D H, Goyon, C, Kalantar, D, Koenig, M, Lahmann, B, Li, C, Lu, Y, Palmer, C A J, Petrasso, R D, Poole, H, Remington, B, Reville, B, Reyes, A, Rigby, A, Ryu, D, Swadling, G, Zylstra, A, Miniati, F, Sarkar, S, Schekochihin, A A, Lamb, D Q & Gregori, G 2022, ' Strong suppression of heat conduction in a laboratory replica of galaxy-cluster turbulent plasmas ', Science Advances, vol. 8, no. 10 . https://doi.org/10.1126/sciadv.abj6799
Sci.Adv.
Sci.Adv., 2022, 8 (10), pp.abj6799. ⟨10.1126/sciadv.abj6799⟩
Sci.Adv.
Sci.Adv., 2022, 8 (10), pp.abj6799. ⟨10.1126/sciadv.abj6799⟩
Galaxy clusters are filled with hot, diffuse X-ray emitting plasma, with a stochastically tangled magnetic field whose energy is close to equipartition with the energy of the turbulent motions \cite{zweibel1997, Vacca}. In the cluster cores, the temp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ff0c9fd379ef50b4a8b06c2f794e60f9
http://arxiv.org/abs/2105.08461
http://arxiv.org/abs/2105.08461
Autor:
Matthew Trantham, P. Tzeferacos, M. J.-E. Manuel, Patrick Hartigan, Carolyn Kuranz, Chikang Li, John Foster, Andy Liao, Gennady Fiksel, Rachel Young, A. Birkel, Benjamin Khiar, Edward Hansen, Joseph M. Levesque, William J. Gray, Joseph Katz, Sallee Klein
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::672bc71af6012232f7030c2040e41332
https://doi.org/10.2172/1711332
https://doi.org/10.2172/1711332
Autor:
J. Steven Ross, Charlotte Palmer, Francesco Miniati, Gianluca Gregori, Robert Bingham, Brian Reville, Fredrick Seguin, Chikang Li, Thomas G. White, D. Q. Lamb, Petros Tzeferacos, R. D. Petrasso, C. Graziani, Michel Koenig, A. Rigby, Anthony R. Bell, Laura Chen, A. Birkel, Joseph Katz, Jena Meinecke, Bruce Remington, Dmitri Ryutov, Dustin Froula, Matthew W. Kunz, A. F. A. Bott, Alexander Schekochihin, Dongsu Ryu, Hye-Sook Park
Publikováno v:
Proceedings of the National Academy of Sciences of the United States of America
Proc Natl Acad Sci U S A
Proc Natl Acad Sci U S A
Understanding magnetic-field generation and amplification in turbulent plasma is essential to account for observations of magnetic fields in the universe. A theoretical framework attributing the origin and sustainment of these fields to the so-called
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5da530063f5e551b9858def22338c341