Experimental study on radiative opacity of radiatively heated carbon plasma at SGIII prototype laser facility

ZHAO Yang; QING Bo; XIONG Gang; ZHANG Zhiyu; SUN Ao; YANG Guohong; ZHAO Yan; ZHANG Yuxue; HUANG Chengwu; ZHU Tuo; SONG Tianming; LI Liling; LI Jin; CHE Xingsen; ZHAN Xiayu; ZHANG Jiyan; DONG Yunsong; YANG Jiamin

doi:10.7498/aps.74.20250600

Abstract

Experimental opacity data are used to evaluate the opacity models and their accuracy of the calculated results. In order to study the opacity of carbon material in the shell of the inertial confinement fusion ignition target, the experimental study of the spectrally-resolved opacity of radiatively heated carbon plasma is carried out on the Shenguang III prototype laser facility. Eight nanosecond lasers are injected into a conical-cylindrical gold hohlraum and converted into intense X-ray radiation, the high-temperature plasma is obtained by radiatively heating the CH film in the center of the hohlraum. Temporal evolutions of temperature and density of carbon plasma are simulated with the Multi-1D code. By using a spatially-resolved flat-field grating spectrometer combined with the ninth beam smoothing surface backlight technology, the absorption spectra of CH sample and the backlighter spectra are measured in one shot. Finally, the experimental transmission spectra of carbon plasma (with a temperature of 65 eV and density of 0.003 g/cm³) in a range of 300–500 eV are obtained and compared with the calculated results of a DCA/UTA opacity code. The datasets presented in this paper are openly available at https://doi.org/10.57760/sciencedb.j00213.00153.

Keywords:

Authors and contacts

National Key Laboratory of Plasma Physics, Research Center of Laser Fusion, China Academy of Engineering Physics, Mianyang 621900, China

Corresponding author: ZHANG Jiyan, zhangjiyanzjy@163.com

Funds: Project supported by the Science Challenge Project (Grant Nos. TZ2018005, TZ2018001) and the National Natural Science Foundation of China (Grant Nos. 12374261, 12335015, 12375238, U2430206).

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References

[1]	Rogers F J, Iglesias C A, 1994 Science 263 50 Google Scholar
[2]	Perry T S, Davidson S J, Serduke F J D, Bach D R, Smith C C, Foster J M, Doyas R J, Ward R A, Iglesias C A, Rogers F J, Abdallah J, Stewart R E, Kilkenny J D, Lee R W 1991 Phys. Rev. Lett. 67 3784 Google Scholar
[3]	Springer P T, Fields D J, Wilson B G, Nash J K, Goldstein W H, Iglesias C A, Rogers F J, Swenson J K, Chen M H, Bar-Shalom A, Stewart R E 1992 Phys. Rev. Lett. 69 3735 Google Scholar
[4]	Bailey J E, Nagayama T, Loisel G P, Rochau G A, Blancard C, Colgan J, Cosse P, Faussurier G, Fontes C J, Gilleron F, Golovkin I, Hansen S B, Iglesias C A, Kilcrease D P, MacFarlane J J, Mancini R C, Nahar S N, Orban C, Pain J C, Pradhan A K, Sherrill M, Wilson B G 2015 Nature 517 56 Google Scholar
[5]	Nagayama T, Bailey J E, Loisel G P, Dunham G S, Rochau G A, Blancard C, Colgan J, Cosse P, Faussurier G, Fontes C J, Gilleron F, Hansen S B, Iglesias C A, Golovkin I E, Kilcrease D P, MacFarlane J J, Mancini R C, More R M, Orban C, Pain J C, Sherrill M E, Wilson B G 2019 Phys. Rev. Lett. 122 235001 Google Scholar
[6]	高城, 刘彦鹏, 严冠鹏, 闫杰, 陈小棋, 侯永, 靳奉涛, 吴建华, 曾交龙, 袁建民 2023 物理学报 72 183101 Google Scholar Gao C, Liu Y P, Yan G P, Yan J, Chen X Q, Hou Y, Jin F T, Wu J H, Zeng J L, Yuan J M 2023 Acta Phys. Sin. 72 183101 Google Scholar
[7]	MacKinnon A J, Meezan N B, Ross J S, Pape S L, Hopkins L B, Divol L, Ho D, Milovich J, Pak A, Ralph J, Döppner T, Patel P K, Thomas C, Tommasini R, Haan S, MacPhee A G, McNaney J, Caggiano J, Hatarik R, Bionta R, Ma T, Spears B, Rygg J R, Benedetti L R, Town R P J, Bradley D K, Dewald E L, Fittinghoff D, Jones O S, Robey H R, Moody J D, Khan S, Callahan D A, Hamza A, Biener J, Celliers P M, Braun D G, Erskine D J, Prisbrey S T, Wallace R J, Kozioziemski B, Dylla-Spears R, Sater J, Collins G, Storm E, Hsing W, Landen O, Atherton J L, Lindl J D, Edwards M J, Frenje J A, Gatu-Johnson M, Li C K, Petrasso R, Rinderknecht H, Rosenberg M, Séguin F H, Zylstra A, Knauer J P, Grim G, Guler N, Merrill F, Olson R, Kyrala G A, Kilkenny J D, Nikroo A, Moreno K, Hoover D E, Wild C, Werner E 2014 Phys. Plasmas 21 056318 Google Scholar
[8]	Zylstra A B, Kritcher A L, Hurricane O A, Callahan D A, Baker K, Braun T, Casey D T, Clark D, Clark K, Doppner T, Divol L, Hinkel D E, Hohenberger M, Kong C, Landen O L, Nikroo A, Pak A, Patel P, Ralph J E, Rice N, Tommasini R, Schoff M, Stadermann M, Strozzi D, Weber C, Young C, Wild C, Town R P J, Edward M J 2021 Phys. Rev. Lett. 126 025001 Google Scholar
[9]	Olson R E, Rochau G A, Landen O L, Leeper R J 2011 Phys. Plasmas 18 032706 Google Scholar
[10]	Zhao Y, Wei M X, Deng B, Zhu T, Hu Z M, Xiong G, Shang W L, Kuang L Y, Yang G H, Zhang J Y, Yang J M 2011 Chin. Phys. Lett. 28 060701 Google Scholar
[11]	Zhao Y, Zhang J Y, Liu J S, Yuan X, Jin F T 2009 Rev. Sci. Instrum. 80 043505.Google Scholar
[12]	Xiong G, Yang G H, Li H, Zhang J Y, Zhao Y, Hu Z M, Wei M X, Qing B, Yang J M, Liu S Y, Jiang S N 2014 Rev. Sci. Instrum. 85 43104 Google Scholar
[13]	Qing B, Wei M X, Yang G H, Zhang Z Y, Zhao Y, Xiong G, Lv M, Hu Z M, Zhang J Y, Liu S Y, Yang J M 2018 Rev. Sci. Instrum. 89 083108 Google Scholar
[14]	Zhang J Y, Yang J M, Xu Y, Yang G H, Ding Y N, Yan J, Yuan J M, Ding Y K, Zheng Z J, Zhao Y, Hu Z M 2009 Phys. Rev. E 79 016401 Google Scholar
[15]	Zhao Y, Shang W L, Xiong G, Jin F T, Hu Z M, Wei M X, Yang G H, Zhang J Y, Yang J M 2010 Chin. Phys. Lett. 27 113202 Google Scholar
[16]	Xiong G, Yang J M, Zhang J Y, Hu Z M, Zhao Y, Qing B, Yang G H, Wei M X, Yi R Q, Song T M, Li H, Yuan Z, Lv M, Meng X J, Xu Y, Wu Z Q, Yan J 2016 Astrophys. J. 816 36 Google Scholar
[17]	Qing B, Zhang Z Y, Wei M X, Yang Y M, Yang Z W, Yang G H, Zhao Y, Lv M, Xiong G, Hu Z M, Zhang J Y, Yang J M, Yan J 2018 Phys. Plasma 25 023301 Google Scholar
[18]	Xiong G, Qing B, Zhang Z Y, Jing L F, Zhao Y, Wei M X, Yang Y M, Hou L F, Huang C W, Zhu T, Song T M, Lv M, Zhao Y, Zhang Y X, Yang G H, Wu Z Q, Yan J, Zou Y M, Zhang J Y, Yang J M 2024 Matter Radiat. Extremes 9 047801 Google Scholar
[19]	Yang J M, Ding Y N, Yan J, Li J M, Zhang B H, Yang G H, Zhang W H, Wang Y M 2002 Phys. Plasmas 9 678 Google Scholar
[20]	Zhang J Y, Yang J M, Xiong G, Meng X J, Yang G H, Zhao Y, Qing B, Li H, Yuan Z, Yang Y M, Wu Z Q, Yan J, Liu S Y, Jiang S E, Ding Y K 2015 Science and Technology of High Energy Density 1 1
[21]	Zhao Y, Yang J M, Zhang J Y, Yang G H, Wei M X, Xiong G, Song T M, Zhang Z Y, Bao L H, Deng B, Li Y K, He X A, Li C G, Mei Y, Yu R Z, Jiang S E, Liu S Y, Ding Y K Zhang B H 2013 Phys. Rev. Lett. 111 155003 Google Scholar
[22]	Li Z C, Jiang X H, Liu S Y, Huang T X, Zheng J, Yang J M, Li S W, Guo L, Zhao X F, Du H B, Song T M, Yi R Q, Liu Y G, Jiang S E, Ding Y K 2010 Rev. Sci. Instrum. 81 073504 Google Scholar
[23]	Zhang Z Y, Zhao Y, Zhang J Y, Hu Z M, Jing L F, Qing B, Xiong G, Lv M, Du H B, Yang Y M, Zhan X Y, Yu R Z, Mei Y, Yang J M 2019 Phys. Plasmas 26 072704 Google Scholar
[24]	Ramis R, Schmalz R, Meyer-Ter-Vehn J 1988 Comput. Phys. Commun. 49 475 Google Scholar
[25]	Yan J, Qiu Y B 2001 Phys. Rev. E 64 056401 Google Scholar

Cited By

图 1 实验排布示意图

Figure 1. Schematic of the experimental setup.

DownLoad: Full-Size Img PowerPoint

图 2 CH样品的辐射流体力学模拟　(a)辐射温度时间演化; (b)温度和密度时间演化

Figure 2. Hydrodynamic simulation of the CH sample: (a) The temporal evolution of radiation temperature at the sample; (b) the temporal evolutions of temperature and density.

DownLoad: Full-Size Img PowerPoint

图 3 0.65 ns时刻CH样品的温度密度空间分布

Figure 3. Temperature and density profile of the CH sample at 0.65 ns.

DownLoad: Full-Size Img PowerPoint

图 4 空间分辨的X光吸收与背光源谱图像

Figure 4. Space-resolved X-ray absorption and backlighter spectra.

DownLoad: Full-Size Img PowerPoint

图 5 (a)实验背光源谱与吸收谱; (b)实验与理论透过率光谱的比较

Figure 5. (a) Experimental backlighter and absorption spectra; (b) the comparison of the measured transmission spectrum with the calculated result.

DownLoad: Full-Size Img PowerPoint

[1]	Rogers F J, Iglesias C A, 1994 Science 263 50 Google Scholar
[2]	Perry T S, Davidson S J, Serduke F J D, Bach D R, Smith C C, Foster J M, Doyas R J, Ward R A, Iglesias C A, Rogers F J, Abdallah J, Stewart R E, Kilkenny J D, Lee R W 1991 Phys. Rev. Lett. 67 3784 Google Scholar
[3]	Springer P T, Fields D J, Wilson B G, Nash J K, Goldstein W H, Iglesias C A, Rogers F J, Swenson J K, Chen M H, Bar-Shalom A, Stewart R E 1992 Phys. Rev. Lett. 69 3735 Google Scholar
[4]	Bailey J E, Nagayama T, Loisel G P, Rochau G A, Blancard C, Colgan J, Cosse P, Faussurier G, Fontes C J, Gilleron F, Golovkin I, Hansen S B, Iglesias C A, Kilcrease D P, MacFarlane J J, Mancini R C, Nahar S N, Orban C, Pain J C, Pradhan A K, Sherrill M, Wilson B G 2015 Nature 517 56 Google Scholar
[5]	Nagayama T, Bailey J E, Loisel G P, Dunham G S, Rochau G A, Blancard C, Colgan J, Cosse P, Faussurier G, Fontes C J, Gilleron F, Hansen S B, Iglesias C A, Golovkin I E, Kilcrease D P, MacFarlane J J, Mancini R C, More R M, Orban C, Pain J C, Sherrill M E, Wilson B G 2019 Phys. Rev. Lett. 122 235001 Google Scholar
[6]	高城, 刘彦鹏, 严冠鹏, 闫杰, 陈小棋, 侯永, 靳奉涛, 吴建华, 曾交龙, 袁建民 2023 物理学报 72 183101 Google Scholar Gao C, Liu Y P, Yan G P, Yan J, Chen X Q, Hou Y, Jin F T, Wu J H, Zeng J L, Yuan J M 2023 Acta Phys. Sin. 72 183101 Google Scholar
[7]	MacKinnon A J, Meezan N B, Ross J S, Pape S L, Hopkins L B, Divol L, Ho D, Milovich J, Pak A, Ralph J, Döppner T, Patel P K, Thomas C, Tommasini R, Haan S, MacPhee A G, McNaney J, Caggiano J, Hatarik R, Bionta R, Ma T, Spears B, Rygg J R, Benedetti L R, Town R P J, Bradley D K, Dewald E L, Fittinghoff D, Jones O S, Robey H R, Moody J D, Khan S, Callahan D A, Hamza A, Biener J, Celliers P M, Braun D G, Erskine D J, Prisbrey S T, Wallace R J, Kozioziemski B, Dylla-Spears R, Sater J, Collins G, Storm E, Hsing W, Landen O, Atherton J L, Lindl J D, Edwards M J, Frenje J A, Gatu-Johnson M, Li C K, Petrasso R, Rinderknecht H, Rosenberg M, Séguin F H, Zylstra A, Knauer J P, Grim G, Guler N, Merrill F, Olson R, Kyrala G A, Kilkenny J D, Nikroo A, Moreno K, Hoover D E, Wild C, Werner E 2014 Phys. Plasmas 21 056318 Google Scholar
[8]	Zylstra A B, Kritcher A L, Hurricane O A, Callahan D A, Baker K, Braun T, Casey D T, Clark D, Clark K, Doppner T, Divol L, Hinkel D E, Hohenberger M, Kong C, Landen O L, Nikroo A, Pak A, Patel P, Ralph J E, Rice N, Tommasini R, Schoff M, Stadermann M, Strozzi D, Weber C, Young C, Wild C, Town R P J, Edward M J 2021 Phys. Rev. Lett. 126 025001 Google Scholar
[9]	Olson R E, Rochau G A, Landen O L, Leeper R J 2011 Phys. Plasmas 18 032706 Google Scholar
[10]	Zhao Y, Wei M X, Deng B, Zhu T, Hu Z M, Xiong G, Shang W L, Kuang L Y, Yang G H, Zhang J Y, Yang J M 2011 Chin. Phys. Lett. 28 060701 Google Scholar
[11]	Zhao Y, Zhang J Y, Liu J S, Yuan X, Jin F T 2009 Rev. Sci. Instrum. 80 043505.Google Scholar
[12]	Xiong G, Yang G H, Li H, Zhang J Y, Zhao Y, Hu Z M, Wei M X, Qing B, Yang J M, Liu S Y, Jiang S N 2014 Rev. Sci. Instrum. 85 43104 Google Scholar
[13]	Qing B, Wei M X, Yang G H, Zhang Z Y, Zhao Y, Xiong G, Lv M, Hu Z M, Zhang J Y, Liu S Y, Yang J M 2018 Rev. Sci. Instrum. 89 083108 Google Scholar
[14]	Zhang J Y, Yang J M, Xu Y, Yang G H, Ding Y N, Yan J, Yuan J M, Ding Y K, Zheng Z J, Zhao Y, Hu Z M 2009 Phys. Rev. E 79 016401 Google Scholar
[15]	Zhao Y, Shang W L, Xiong G, Jin F T, Hu Z M, Wei M X, Yang G H, Zhang J Y, Yang J M 2010 Chin. Phys. Lett. 27 113202 Google Scholar
[16]	Xiong G, Yang J M, Zhang J Y, Hu Z M, Zhao Y, Qing B, Yang G H, Wei M X, Yi R Q, Song T M, Li H, Yuan Z, Lv M, Meng X J, Xu Y, Wu Z Q, Yan J 2016 Astrophys. J. 816 36 Google Scholar
[17]	Qing B, Zhang Z Y, Wei M X, Yang Y M, Yang Z W, Yang G H, Zhao Y, Lv M, Xiong G, Hu Z M, Zhang J Y, Yang J M, Yan J 2018 Phys. Plasma 25 023301 Google Scholar
[18]	Xiong G, Qing B, Zhang Z Y, Jing L F, Zhao Y, Wei M X, Yang Y M, Hou L F, Huang C W, Zhu T, Song T M, Lv M, Zhao Y, Zhang Y X, Yang G H, Wu Z Q, Yan J, Zou Y M, Zhang J Y, Yang J M 2024 Matter Radiat. Extremes 9 047801 Google Scholar
[19]	Yang J M, Ding Y N, Yan J, Li J M, Zhang B H, Yang G H, Zhang W H, Wang Y M 2002 Phys. Plasmas 9 678 Google Scholar
[20]	Zhang J Y, Yang J M, Xiong G, Meng X J, Yang G H, Zhao Y, Qing B, Li H, Yuan Z, Yang Y M, Wu Z Q, Yan J, Liu S Y, Jiang S E, Ding Y K 2015 Science and Technology of High Energy Density 1 1
[21]	Zhao Y, Yang J M, Zhang J Y, Yang G H, Wei M X, Xiong G, Song T M, Zhang Z Y, Bao L H, Deng B, Li Y K, He X A, Li C G, Mei Y, Yu R Z, Jiang S E, Liu S Y, Ding Y K Zhang B H 2013 Phys. Rev. Lett. 111 155003 Google Scholar
[22]	Li Z C, Jiang X H, Liu S Y, Huang T X, Zheng J, Yang J M, Li S W, Guo L, Zhao X F, Du H B, Song T M, Yi R Q, Liu Y G, Jiang S E, Ding Y K 2010 Rev. Sci. Instrum. 81 073504 Google Scholar
[23]	Zhang Z Y, Zhao Y, Zhang J Y, Hu Z M, Jing L F, Qing B, Xiong G, Lv M, Du H B, Yang Y M, Zhan X Y, Yu R Z, Mei Y, Yang J M 2019 Phys. Plasmas 26 072704 Google Scholar
[24]	Ramis R, Schmalz R, Meyer-Ter-Vehn J 1988 Comput. Phys. Commun. 49 475 Google Scholar
[25]	Yan J, Qiu Y B 2001 Phys. Rev. E 64 056401 Google Scholar

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