Radiative effects in radiative shocks in shock tubes

R. P. Drake; F. W. Doss; R. G. McClarren; M. L. Adams; N. Amato; D. Bingham; C. C. Chou; C. DiStefano; K. Fidkowski; B. Fryxell; T. I. Gombosi; M. J. Grosskopf; J. P. Holloway; B. van der Holst; C. M. Huntington; S. Karni; C. M. Krauland; C. C. Kuranz; E. Larsen; B. van Leer; B. Mallick; D. Marion; W. Martin; J. E. Morel; E. S. Myra; V. Nair; K. G. Powell; L. Rauchwerger; P. Roe; E. Rutter; I. V. Sokolov; Q. Stout; B. R. Torralva; G. Toth; K. Thornton; A. J. Visco

doi:10.1016/j.hedp.2011.03.005

Radiative effects in radiative shocks in shock tubes

R. P. Drake, F. W. Doss, R. G. McClarren, M. L. Adams, N. Amato, D. Bingham, C. C. Chou, C. DiStefano, K. Fidkowski, B. Fryxell, T. I. Gombosi, M. J. Grosskopf, J. P. Holloway, B. van der Holst, C. M. Huntington, S. Karni, C. M. Krauland, C. C. Kuranz, E. Larsen, B. van LeerB. Mallick, D. Marion, W. Martin, J. E. Morel, E. S. Myra, V. Nair, K. G. Powell, L. Rauchwerger, P. Roe, E. Rutter, I. V. Sokolov, Q. Stout, B. R. Torralva, G. Toth, K. Thornton, A. J. Visco

Research output: Contribution to journal › Review article › peer-review

Abstract

Using modern high-energy-density facilities it is straightforward to produce radiative shock waves in which the transfer of energy by radiation controls the hydrodynamic structure of the system. Some of these experiments use shock tubes. This paper discusses such experiments, with an emphasis on the simple physical relations that determine the primary features of such shocks and on the details and impact of radiative energy transfer in such systems. Notable aspects include the creation of high-density shocked layers, the flow of radiative energy toward regions of higher energy density, and the creation of secondary shocks by ablation of the tube walls ahead of the primary shock front. Simulations of one such experimental system are also shown.

Original language	English (US)
Pages (from-to)	130-140
Number of pages	11
Journal	High Energy Density Physics
Volume	7
Issue number	3
DOIs	https://doi.org/10.1016/j.hedp.2011.03.005
State	Published - Sep 2011
Externally published	Yes

Keywords

Laboratory astrophysics
Radiation transfer
Radiative shocks
Shock waves

ASJC Scopus subject areas

Radiation
Nuclear and High Energy Physics

Online availability

10.1016/j.hedp.2011.03.005

Library availability

Discover UIUC Full Text

Cite this

Drake, R. P., Doss, F. W., McClarren, R. G., Adams, M. L., Amato, N., Bingham, D., Chou, C. C., DiStefano, C., Fidkowski, K., Fryxell, B., Gombosi, T. I., Grosskopf, M. J., Holloway, J. P., van der Holst, B., Huntington, C. M., Karni, S., Krauland, C. M., Kuranz, C. C., Larsen, E., ... Visco, A. J. (2011). Radiative effects in radiative shocks in shock tubes. High Energy Density Physics, 7(3), 130-140. https://doi.org/10.1016/j.hedp.2011.03.005

Drake, RP, Doss, FW, McClarren, RG, Adams, ML, Amato, N, Bingham, D, Chou, CC, DiStefano, C, Fidkowski, K, Fryxell, B, Gombosi, TI, Grosskopf, MJ, Holloway, JP, van der Holst, B, Huntington, CM, Karni, S, Krauland, CM, Kuranz, CC, Larsen, E, van Leer, B, Mallick, B, Marion, D, Martin, W, Morel, JE, Myra, ES, Nair, V, Powell, KG, Rauchwerger, L, Roe, P, Rutter, E, Sokolov, IV, Stout, Q, Torralva, BR, Toth, G, Thornton, K & Visco, AJ 2011, 'Radiative effects in radiative shocks in shock tubes', High Energy Density Physics, vol. 7, no. 3, pp. 130-140. https://doi.org/10.1016/j.hedp.2011.03.005

@article{8c05d078b9754e628a7d6f7db6ca0c72,

title = "Radiative effects in radiative shocks in shock tubes",

abstract = "Using modern high-energy-density facilities it is straightforward to produce radiative shock waves in which the transfer of energy by radiation controls the hydrodynamic structure of the system. Some of these experiments use shock tubes. This paper discusses such experiments, with an emphasis on the simple physical relations that determine the primary features of such shocks and on the details and impact of radiative energy transfer in such systems. Notable aspects include the creation of high-density shocked layers, the flow of radiative energy toward regions of higher energy density, and the creation of secondary shocks by ablation of the tube walls ahead of the primary shock front. Simulations of one such experimental system are also shown.",

keywords = "Laboratory astrophysics, Radiation transfer, Radiative shocks, Shock waves",

author = "Drake, {R. P.} and Doss, {F. W.} and McClarren, {R. G.} and Adams, {M. L.} and N. Amato and D. Bingham and Chou, {C. C.} and C. DiStefano and K. Fidkowski and B. Fryxell and Gombosi, {T. I.} and Grosskopf, {M. J.} and Holloway, {J. P.} and {van der Holst}, B. and Huntington, {C. M.} and S. Karni and Krauland, {C. M.} and Kuranz, {C. C.} and E. Larsen and {van Leer}, B. and B. Mallick and D. Marion and W. Martin and Morel, {J. E.} and Myra, {E. S.} and V. Nair and Powell, {K. G.} and L. Rauchwerger and P. Roe and E. Rutter and Sokolov, {I. V.} and Q. Stout and Torralva, {B. R.} and G. Toth and K. Thornton and Visco, {A. J.}",

note = "Funding Information: This work was funded by the Predictive Sciences Academic Alliances Program in DOE/NNSA-ASC via grant DEFC52-08NA28616 , by the DOE/NNSA-DS and DOE/SC-OFES Joint Program in High-Energy-Density Laboratory Plasmas, grant number DE-FG52-09NA29548 , by the National Laser User Facility Program , grant number DE-FG52-09NA29034 , by previous DOE grants and contracts, and by the University of Michigan . ",

year = "2011",

month = sep,

doi = "10.1016/j.hedp.2011.03.005",

language = "English (US)",

volume = "7",

pages = "130--140",

journal = "High Energy Density Physics",

issn = "1574-1818",

publisher = "Elsevier B.V.",

number = "3",

}

TY - JOUR

T1 - Radiative effects in radiative shocks in shock tubes

AU - Drake, R. P.

AU - Doss, F. W.

AU - McClarren, R. G.

AU - Adams, M. L.

AU - Amato, N.

AU - Bingham, D.

AU - Chou, C. C.

AU - DiStefano, C.

AU - Fidkowski, K.

AU - Fryxell, B.

AU - Gombosi, T. I.

AU - Grosskopf, M. J.

AU - Holloway, J. P.

AU - van der Holst, B.

AU - Huntington, C. M.

AU - Karni, S.

AU - Krauland, C. M.

AU - Kuranz, C. C.

AU - Larsen, E.

AU - van Leer, B.

AU - Mallick, B.

AU - Marion, D.

AU - Martin, W.

AU - Morel, J. E.

AU - Myra, E. S.

AU - Nair, V.

AU - Powell, K. G.

AU - Rauchwerger, L.

AU - Roe, P.

AU - Rutter, E.

AU - Sokolov, I. V.

AU - Stout, Q.

AU - Torralva, B. R.

AU - Toth, G.

AU - Thornton, K.

AU - Visco, A. J.

N1 - Funding Information: This work was funded by the Predictive Sciences Academic Alliances Program in DOE/NNSA-ASC via grant DEFC52-08NA28616 , by the DOE/NNSA-DS and DOE/SC-OFES Joint Program in High-Energy-Density Laboratory Plasmas, grant number DE-FG52-09NA29548 , by the National Laser User Facility Program , grant number DE-FG52-09NA29034 , by previous DOE grants and contracts, and by the University of Michigan .

PY - 2011/9

Y1 - 2011/9

N2 - Using modern high-energy-density facilities it is straightforward to produce radiative shock waves in which the transfer of energy by radiation controls the hydrodynamic structure of the system. Some of these experiments use shock tubes. This paper discusses such experiments, with an emphasis on the simple physical relations that determine the primary features of such shocks and on the details and impact of radiative energy transfer in such systems. Notable aspects include the creation of high-density shocked layers, the flow of radiative energy toward regions of higher energy density, and the creation of secondary shocks by ablation of the tube walls ahead of the primary shock front. Simulations of one such experimental system are also shown.

AB - Using modern high-energy-density facilities it is straightforward to produce radiative shock waves in which the transfer of energy by radiation controls the hydrodynamic structure of the system. Some of these experiments use shock tubes. This paper discusses such experiments, with an emphasis on the simple physical relations that determine the primary features of such shocks and on the details and impact of radiative energy transfer in such systems. Notable aspects include the creation of high-density shocked layers, the flow of radiative energy toward regions of higher energy density, and the creation of secondary shocks by ablation of the tube walls ahead of the primary shock front. Simulations of one such experimental system are also shown.

KW - Laboratory astrophysics

KW - Radiation transfer

KW - Radiative shocks

KW - Shock waves

UR - http://www.scopus.com/inward/record.url?scp=79955113649&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=79955113649&partnerID=8YFLogxK

U2 - 10.1016/j.hedp.2011.03.005

DO - 10.1016/j.hedp.2011.03.005

M3 - Review article

AN - SCOPUS:79955113649

SN - 1574-1818

VL - 7

SP - 130

EP - 140

JO - High Energy Density Physics

JF - High Energy Density Physics

IS - 3

ER -

Radiative effects in radiative shocks in shock tubes

Abstract

Keywords

ASJC Scopus subject areas

Online availability

Library availability

Related links

Fingerprint

Cite this