Zobrazeno 1 - 10
of 174
pro vyhledávání: '"Lamb, Donald Q."'
Autor:
Bott, Archie F. A., Tzeferacos, Petros, Chen, Laura, Palmer, Charlotte A. J., Rigby, Alexandra, Bell, Anthony R., Bingham, Robert, Birkel, Andrew, Graziani, Carlo, Froula, Dustin H., Katz, Joseph, Koenig, Michel, Kunz, Matthew W., Li, Chikang, Meinecke, Jena, Miniati, Francesco, Petrasso, Richard, Park, Hye-Sook, Remington, Bruce A., Reville, Brian, Ross, J. Steven, Ryu, Dongsu, Ryutov, Dmitri, Séguin, Fredrick H., White, Thomas G., Schekochihin, Alexander A., Lamb, Donald Q., Gregoria, Gianluca
Publikováno v:
Proceedings of the National Academy of Sciences of the United States of America, 2021 Mar . 118(11), 1-12.
Externí odkaz:
https://www.jstor.org/stable/27027585
Proton radiography is an important diagnostic method for laser plasma experiments, and is particularly important in the analysis of magnetized plasmas. The theory of radiographic image analysis has heretofore only permitted somewhat limited analysis
Externí odkaz:
http://arxiv.org/abs/1603.08617
We propose a new way of generating magnetized supersonic jets using a ring laser to irradiate a flat surface target. Using 2D FLASH code simulations which include the Biermann Battery term, we demonstrate that strong toroidal fields can be generated
Externí odkaz:
http://arxiv.org/abs/1409.4273
Autor:
Graziani, Carlo, Tzeferacos, Petros, Lee, Dongwook, Lamb, Donald Q., Weide, Klaus, Fatenejad, Milad, Miller, Joshua
The Biermann Battery effect is frequently invoked in cosmic magnetogenesis and studied in High-Energy Density laboratory physics experiments. Generation of magnetic fields by the Biermann effect due to mis-aligned density and temperature gradients in
Externí odkaz:
http://arxiv.org/abs/1408.4161
Autor:
Wollaeger, Ryan T., van Rossum, Daniel R., Graziani, Carlo, Couch, Sean M., Jordan IV, George C., Lamb, Donald Q., Moses, Gregory A.
We explore Implicit Monte Carlo (IMC) and Discrete Diffusion Monte Carlo (DDMC) for radiation transport in high-velocity outflows with structured opacity. The IMC method is a stochastic computational technique for nonlinear radiation transport. IMC i
Externí odkaz:
http://arxiv.org/abs/1306.5700
The potential for laser-produced plasmas to yield fundamental insights into high energy density physics (HEDP) and deliver other useful applications can sometimes be frustrated by uncertainties in modeling the properties and expansion of these plasma
Externí odkaz:
http://arxiv.org/abs/1306.1584
Autor:
Diemer, Benedikt, Kessler, Richard, Graziani, Carlo, Jordan IV, George C., Lamb, Donald Q., Long, Min, van Rossum, Daniel R.
Publikováno v:
2013 ApJ 773 119
We propose a robust, quantitative method to compare the synthetic light curves of a Type Ia Supernova (SNIa) explosion model with a large set of observed SNeIa, and derive a figure of merit for the explosion model's agreement with observations. The s
Externí odkaz:
http://arxiv.org/abs/1303.1168
Autor:
Fu, Wen, Liang, Edison P., Fatenejad, Milad, Lamb, Donald Q., Grosskopf, Michael, Park, Hye-Sook, Remington, Bruce, Spitkovsky, Anatoly
Publikováno v:
High Energy Density Physics, 2013, 9, 336
Supersonic plasma outflows driven by multi-beam, high-energy lasers, such as Omega and NIF, have been and will be used as platforms for a variety of laboratory astrophysics experiments. Here we propose a new way of launching high density and high vel
Externí odkaz:
http://arxiv.org/abs/1209.2150
Autor:
Shirasaki, Yuji, Yoshida, Atsumasa, Kawai, Nobuyuki, Tamagawa, Toru, Sakamoto, Takanori, Suzuki, Motoko, Nakagawam, Yujin, Kobayashi, Akina, Sugita, Satoshi, Takahashi, Ichiro, Arimoto, Makoto, Shimokawabe, Takashi, Pazmino, Nicolas Vasquez, Ishimura, Takuto, Sato, Rie, Matsuoka, Masaru, Fenimore, Edward E., Galassi, Mark, Lamb, Donald Q., Graziani, Carlo, Donaghy, Timothy Q., Atteia, Jean-Luc, Pelangeon, Alexandre, Vanderspek, Roland, Crew, Geoffrey B., Doty, John P., Villasenor, Joel, Prigozhin, Gregory, Butler, Nat, Ricker, George R., Hurley, Kevin, Woosley, Stanford E., Pizzichini, Graziella
Publikováno v:
Publ.Astron.Soc.Jap.60:919,2008
GRB 041006 was detected by HETE-2 at 12:18:08 UT on 06 October 2004. This GRB displays a soft X-ray emission, a precursor before the onset of the main event, and also a soft X-ray tail after the end of the main peak. The light curves in four differen
Externí odkaz:
http://arxiv.org/abs/0802.1649
Autor:
Arimoto, Makoto, Kawai, Nobuyuki, Yoshida, Atsumasa, Tamagawa, Toru, Shirasaki, Yuji, Suzuki, Motoko, Matsuoka, Masaru, Kotoku, Jun'ichi, Sato, Rie, Shimokawabe, Takashi, Pazmino, Nicolas Vasquez, Ishimura, Takuto, Nakagawa, Yujin, Ishikawa, Nobuyuki, Kobayashi, Akina, Sugita, Satoshi, Takahashi, Ichiro, Kuwahara, Makoto, Yamauchi, Makoto, Takagishi, Kunio, Hatsukade, Isamu, Atteia, Jean-Luc, Pelangeon, Alexandre, Vanderspek, Roland, Graziani, Carlo, Prigozhin, Gregory, Villasenor, Joel, Jernigan, J. Garrett, Crew, Geoffrey B., Hurley, Kevin, Sakamoto, Takanori, Ricker, George R., Woosley, Stanford E., Butler, Nat, Levine, Al, Doty, John P., Donaghy, Timothy Q., Lamb, Donald Q., Fenimore, Edward E., Galassi, Mark, Boer, Michel, Dezalay, Jean-Pascal, Olive, Jean-Francios, Braga, Joao, Manchanda, Ravi, Pizzichini, Graziella
A long X-ray flash was detected and localized by the instruments aboard the High Energy Transient Explorer II (HETE-2) at 00:03:30 UT on 2004 September 16. The position was reported to the GRB Coordinates Network (GCN) approximately 2 hours after the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0703045