Laboratory Simulations of Supernova Shockwave Progagation and ISM Interaction
Conference
·
OSTI ID:15005168
High Mach number shockwaves were launched in laboratory plasmas to simulate supernova shockwave propagation. The experiments were carried out at inertial fusion facilities using large lasers. Spherical shocks were created by focusing laser pulses onto the tip of a solid pin surrounded by ambient gas. Ablated material from the pin would rapidly expand and launch a shock through the surrounding gas. Planar shocks were created by ablating material from one end of a cylindrical shocktube. Laser pulses were typically 1 ns in duration with ablative energies ranging from <1 J to >4 kJ. Shocks were propagated through various plasmas, and observed at spatial scales of up to 5 cm using optical and x-ray cameras. Interferometry techniques were used to deduce densities, and emission spectroscopy data were obtained to infer electron temperatures. Experimental results confirm that spherical shocks are Taylor-Sedov, and that radiative shocks stall sooner than non-radiative shocks. Unexpected results include the birth of a second shock ahead of the original, stalling shock, at the edge of the radiatively preheated region. We have begun experiments to simulate the interaction between shocks and interstellar material (ISM), and the subsequent turbulent mixing. Comparisons between experimental data and numerical simulations of shock evolution, stall, second shock birth, and interstellar material (ISM) interaction will be presented.
- Research Organization:
- Lawrence Livermore National Lab., CA (US)
- Sponsoring Organization:
- US Department of Energy (US)
- DOE Contract Number:
- W-7405-ENG-48
- OSTI ID:
- 15005168
- Report Number(s):
- UCRL-JC-152369
- Country of Publication:
- United States
- Language:
- English
Similar Records
Laboratory simulations of supernova shockwaves: Formation of a second shock ahead of a radiative shock
Laboratory simulations of supernova shockwaves: Formation of a second shock ahead of a radiative shock
Dynamics of plasma expansion and shockwave formation in femtosecond laser-ablated aluminum plumes in argon gas at atmospheric pressures
Conference
·
Thu Jan 27 23:00:00 EST 2005
·
OSTI ID:895436
Laboratory simulations of supernova shockwaves: Formation of a second shock ahead of a radiative shock
Journal Article
·
Wed Sep 28 00:00:00 EDT 2005
· AIP Conference Proceedings
·
OSTI ID:20719385
Dynamics of plasma expansion and shockwave formation in femtosecond laser-ablated aluminum plumes in argon gas at atmospheric pressures
Journal Article
·
Tue Apr 15 00:00:00 EDT 2014
· Physics of Plasmas
·
OSTI ID:22252994