G. Cristoforetti1、†, L. Antonelli2, D. Mancelli3、4, S. Atzeni5, F. Baffigi1, F. Barbato3, D. Batani3、6, G. Boutoux3、7, F. D’Amato1, J. Dostal8、9, R. Dudzak8、9, E. Filippov6、10, Y. J. Gu9、11, L. Juha8、9, O. Klimo12, M. Krus9, S. Malko13、14, A. S. Martynenko6、10, Ph. Nicolai3, V. Ospina13、14, S. Pikuz6、10, O. Renner8、11, J. Santos3, V. T. Tikhonchuk3、11, J. Trela3, S. Viciani1, L. Volpe13、14, S. Weber11, and L. A. Gizzi1
Author Affiliations
1National Institute of Optics, CNR, Pisa and Florence, Italy2York Plasma Physics Institute, University of York, Heslington, York, UK3Université de Bordeaux, CNRS, CEA, CELIA, Talence, France4Donostia International Physics Center (DIPC), Donostia/San Sebastian, Basque Country, Spain5Dipartimento SBAI, Università di Roma La Sapienza, Roma, Italy6National Research Nuclear University MEPhI, Moscow, Russia7CEA, DAM, DIF, Arpajon, France8Department of Radiation and Chemical Physics, Institute of Physics of the CAS, Prague, Czech Republic9Laser Plasma Department, Institute of Plasma Physics of the CAS, Prague, Czech Republic10Joint Institute for High Temperature RAS, Moscow, Russia11ELI-Beamlines, Institute of Physics of the CAS, Prague, Czech Republic12FNSPE, Czech Technical University in Prague, Prague, Czech Republic13Universidad de Salamanca, Ctr Laseres Pulsados, Salamanca, Spain14Centro de Laseres Pulsados (CLPU), Villamayor, Salamanca, Spainshow less
DOI: 10.1017/hpl.2019.37
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G. Cristoforetti, L. Antonelli, D. Mancelli, S. Atzeni, F. Baffigi, F. Barbato, D. Batani, G. Boutoux, F. D’Amato, J. Dostal, R. Dudzak, E. Filippov, Y. J. Gu, L. Juha, O. Klimo, M. Krus, S. Malko, A. S. Martynenko, Ph. Nicolai, V. Ospina, S. Pikuz, O. Renner, J. Santos, V. T. Tikhonchuk, J. Trela, S. Viciani, L. Volpe, S. Weber, L. A. Gizzi. Time evolution of stimulated Raman scattering and two-plasmon decay at laser intensities relevant for shock ignition in a hot plasma[J]. High Power Laser Science and Engineering, 2019, 7(3): 03000e51
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Fig. 1. Experimental setup used for the investigation of parametric instabilities.
Fig. 2. Instantaneous values of electron temperature $T_{e}$ (red squares) and density scalelength $L$ (blue stars) in the density range $0.05{-}0.25\,n_{c}$, as obtained by CHIC hydrosimulations in the experimental conditions of the interaction. The dashed line indicates the laser pulse profile.
Fig. 3. Typical time-integrated SRS spectra acquired at $\unicode[STIX]{x1D703}=20^{\circ }$ (BRS) and $\unicode[STIX]{x1D703}=50^{\circ }$ (SRSS).
Fig. 4. Scheme of regions of density where parametric instabilities are driven.
Fig. 5. Time-integrated half-integer harmonic spectra plotted versus the shift with respect to their nominal frequency. Dashed, red and green lines correspond to the peaks produced by Thomson scattering with EPWs driven by TPD, BRS and SRSS, respectively.
Fig. 6. Geometry of the Thomson up-scattering of $3\unicode[STIX]{x1D714}_{0}$ harmonic light with the EPW driven by SRSS at $n_{e}\approx 0.12\,n_{c}$. The dotted vectors refer to the up-scattering geometry involving the secondary EPW produced by LDI.
Fig. 7. Time-resolved $3/2\unicode[STIX]{x1D714}_{0}$ spectra. The time spanned across the vertical axis is 500 ps, with a time resolution of 25 ps. The laser pulse profile is indicated by the red curve and the peak time by the yellow dashed line. The spectra on the right are obtained by the lineout in windows a, b and c.
Fig. 8. Spectrum of backscattered light recorded in front of the target during the quasi-stationary stage of the interaction (5–9 ps). The frequency is normalized to the laser frequency $\unicode[STIX]{x1D714}_{0}$.
Fig. 9. Distribution of the Poynting flux in the laser propagation direction (in units $\text{W}\,\cdot \,\text{cm}^{-2}$) averaged temporally over 3 ps during the quasi-steady stage of interaction and spatially over one laser wavelength. Red and blue colours represent therefore incident and backscattered light, respectively. The incident laser beam is propagating from the left and the black vertical lines show the position of the quarter critical and critical density surfaces. The black dashed line is shown to guide the eye for the opening angle of backward propagating light.
| Coll. | SBS/laser | BRS | SRSS | HE |
---|
| Abs. | Back | All | | | |
---|
Experimental | – | 14%–20% | – | 0.6%–4% | * | 5.3% | PIC $\text{results}^{a}$ | – | 30% | $82\%^{b}$ | 3% | * | 10% | CHIC simul. | 9% | – | – | – | – | $3.4\%^{c}$ |
|
Table 1. Energy spent in different energy channels during the interaction. The * symbol indicates mechanisms which have been observed but not quantified