Zobrazeno 1 - 10
of 727
pro vyhledávání: '"Nagi, N."'
We present a 3-dimensional (3D) numerical solver of the linearized compressible Euler equations (GALE -- Global Acoustic Linearized Euler), used to model acoustic oscillations throughout the solar interior. The governing equations are solved in conse
Externí odkaz:
http://arxiv.org/abs/2011.03131
Autor:
Meurisse, Jeremie B.E., Chatzigeorgis, Georgios Bellas, Diaz, Patricia Ventura, Bessire, Brody K., Panerai, Francesco, Mansour, Nagi N.
Publikováno v:
In International Journal of Heat and Mass Transfer February 2023 201 Part 1
Publikováno v:
In Polymer Degradation and Stability January 2023 207
Autor:
Kitiashvili, Irina N., Kosovichev, Alexander G., Mansour, Nagi N., Wray, Alan A., Sandstrom, Timothy A.
It is generally accepted that solar acoustic (p) modes are excited by near-surface turbulent motions, in particular, by downdrafts and interacting vortices in intergranular lanes. Recent analysis of Solar Dynamics Observatory data by (Zhao et al., 20
Externí odkaz:
http://arxiv.org/abs/1810.06133
Publikováno v:
In Aerospace Science and Technology April 2022 123
Autor:
Swaminathan Gopalan, Krishnan, Borner, Arnaud, Ferguson, Joseph C., Panerai, Francesco, Mansour, Nagi N., Stephani, Kelly A.
Publikováno v:
In Computational Materials Science 1 April 2022 205
Publikováno v:
In Computational Materials Science 15 February 2022 203
Autor:
Panerai, Francesco, White, Jason D., Cochell, Thomas J., Schroeder, Olivia M., Mansour, Nagi N., Wright, Michael J., Martin, Alexandre
Publikováno v:
International Journal of Heat and Mass Transfer, vol. 101, Oct. 2016, pp. 267-273
A series of experiments was performed to obtain permeability data on FiberForm(R), a commercial carbon preform used for manufacturing thermal protection systems. A porous sample was placed in a quartz flow-tube heated by an isothermal furnace. The se
Externí odkaz:
http://arxiv.org/abs/1603.04844
Publikováno v:
In Computational Materials Science January 2021 186
Continued progress in observational stellar astrophysics requires a deep understanding of the underlying convection dynamics. We present results of realistic 3D radiative hydrodynamic simulations of the outer layers of a moderate mass star (1.47 Msun
Externí odkaz:
http://arxiv.org/abs/1512.07298