Autor: |
Lebedev, Sergey V., Kuranz, C. C., Drake, R. P., Donajkowski, T. L., Dannenberg, K. K., Grosskopf, M., Kremer, D. J., Krauland, C., Marion, D. C., Robey, H. F., Remington, B. A., Hansen, J. F., Blue, B. E., Knauer, J., Plewa, T., Hearn, N. |
Zdroj: |
High Energy Density Laboratory Astrophysics (9781402060540); 2007, p115-119, 5p |
Abstrakt: |
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 the explosion phase of a core-collapse supernova. An unstable interface is shocked and then decelerated by the planar blast wave, producing Rayleigh-Taylor growth. Recent experiments were performed using dual, side-on, x-ray radiography to observe a 3D "egg crate" mode and an imposed, longer-wavelength, sinusoidal mode as a seed perturbation. This paper explores the method of data analysis and accurately estimating the position of important features in the data. [ABSTRACT FROM AUTHOR] |
Databáze: |
Supplemental Index |
Externí odkaz: |
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