High Power Laser Science and Engineering, Volume. 6, Issue 3, 03000e39(2018)
Conceptual design of an experiment to study dust destruction by astrophysical shock waves
Fig. 1. (a) Exploded view of the target layers. (b) Experimental schematic with drive parameters. Laser ablation drives a shock in the low-density foam. (c) When the shock passes the dust,
Fig. 2. Summary of 1D HYADES results for a nominal case of
Fig. 3. Top and axial views of the experimental geometry illustrating the targets and primary diagnostics.
Fig. 4. (a) Imaging geometry for the PCI diagnostic on MEC with an initial beam diameter . A 500 square area in the detector plane of a simulated 8.2 keV phase-contrast image. The simulation implemented randomly distributed C grains, a finite source size (100 nm) and instrumental broadening. (b) Simulated diffraction patterns in X-ray intensity from carbon grains for this PCI setup normalized to the background X-ray intensity. (c) The value is the measured peak-to-valley intensity relative to the background intensity and is shown for the different carbon grain sizes in (b). Abbreviation: , signal to background.
Fig. 5. (a) Simulated Thomson spectra for the proposed geometry using an 8.2 keV beam with an FWHM of 20 eV and the plasma parameters indicated. (b) Photonics calculations, where , for the diffraction orders , 4 and 6 using the HAPG crystal with an initial photon count of and 10 eV energy bins at the detector. Abbreviation: HAPG, highly annealed pyrolytic graphite.
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M. J.-E. Manuel, T. Temim, E. Dwek, A. M. Angulo, P. X. Belancourt, R. P. Drake, C. C. Kuranz, M. J. MacDonald, B. A. Remington. Conceptual design of an experiment to study dust destruction by astrophysical shock waves[J]. High Power Laser Science and Engineering, 2018, 6(3): 03000e39
Special Issue: LABORATORY ASTROPHYSICS
Received: Nov. 20, 2017
Accepted: May. 9, 2018
Published Online: Aug. 28, 2018
The Author Email: M. J.-E. Manuel (manuelm@fusion.gat.com)