Spherical shock in the presence of an external magnetic field

Y. Kuramitsu; S. Matsukiyo; S. Isayama; D. Harada; T. Oyama; R. Fujino; Y. Sakawa; T. Morita; Y. Yamaura; T. Ishikawa; T. Moritaka; T. Sano; K. Tomita; R. Shimoda; Y. Sato; K. Uchino; A. Pelka; R. Crowston; N. Woolsey; G. Gregori; M. Koenig; D. W. Yuan; C. L. Yin; Y. T. Li; K. Zhang; J. Y. Zhong; F. L. Wang; N. Ohnishi; K. Nagamine; H. Yoneda; H. Takabe

doi:10.1088/1742-6596/688/1/012056

Spherical shock in the presence of an external magnetic field

Y. Kuramitsu, S. Matsukiyo, S. Isayama, D. Harada, T. Oyama, R. Fujino, Y. Sakawa, T. Morita, Y. Yamaura, T. Ishikawa, T. Moritaka, T. Sano, K. Tomita, R. Shimoda, Y. Sato, K. Uchino, A. Pelka, R. Crowston, N. Woolsey, G. GregoriM. Koenig, D. W. Yuan, C. L. Yin, Y. T. Li, K. Zhang, J. Y. Zhong, F. L. Wang, N. Ohnishi, K. Nagamine, H. Yoneda, H. Takabe

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

2 Citations (Scopus)

Abstract

We investigate spherical collisionless shocks in the presence of an external magnetic field. Spherical collisionless shocks are common resultant of interactions between a expanding plasma and a surrounding plasma, such as the solar wind, stellar winds, and supernova remnants. Anisotropies often observed in shock propagations and their emissions, and it is widely believed a magnetic field plays a major role. Since the local observations of magnetic fields in astrophysical plasmas are not accessible, laboratory experiments provide unique capability to investigate such phenomena. We model the spherical shocks in the universe by irradiating a solid spherical target surrounded by a plasma in the presence of a magnetic field. We present preliminary results obtained by shadowgraphy.

Original language	English
Article number	012056
Journal	Journal of Physics: Conference Series
Volume	688
Issue number	1
DOIs	https://doi.org/10.1088/1742-6596/688/1/012056
Publication status	Published - Apr 1 2016
Event	8th International Conference on Inertial Fusion Sciences and Applications, IFSA 2013 - Nara, Japan Duration: Sept 8 2013 → Sept 13 2013

All Science Journal Classification (ASJC) codes

Physics and Astronomy(all)

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10.1088/1742-6596/688/1/012056

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Kuramitsu, Y., Matsukiyo, S., Isayama, S., Harada, D., Oyama, T., Fujino, R., Sakawa, Y., Morita, T., Yamaura, Y., Ishikawa, T., Moritaka, T., Sano, T., Tomita, K., Shimoda, R., Sato, Y., Uchino, K., Pelka, A., Crowston, R., Woolsey, N., ... Takabe, H. (2016). Spherical shock in the presence of an external magnetic field. Journal of Physics: Conference Series, 688(1), Article 012056. https://doi.org/10.1088/1742-6596/688/1/012056

Kuramitsu, Y, Matsukiyo, S , Isayama, S, Harada, D, Oyama, T, Fujino, R, Sakawa, Y, Morita, T, Yamaura, Y, Ishikawa, T, Moritaka, T, Sano, T, Tomita, K, Shimoda, R, Sato, Y, Uchino, K, Pelka, A, Crowston, R, Woolsey, N, Gregori, G, Koenig, M, Yuan, DW, Yin, CL, Li, YT, Zhang, K, Zhong, JY, Wang, FL, Ohnishi, N, Nagamine, K, Yoneda, H & Takabe, H 2016, 'Spherical shock in the presence of an external magnetic field', Journal of Physics: Conference Series, vol. 688, no. 1, 012056. https://doi.org/10.1088/1742-6596/688/1/012056

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title = "Spherical shock in the presence of an external magnetic field",

abstract = "We investigate spherical collisionless shocks in the presence of an external magnetic field. Spherical collisionless shocks are common resultant of interactions between a expanding plasma and a surrounding plasma, such as the solar wind, stellar winds, and supernova remnants. Anisotropies often observed in shock propagations and their emissions, and it is widely believed a magnetic field plays a major role. Since the local observations of magnetic fields in astrophysical plasmas are not accessible, laboratory experiments provide unique capability to investigate such phenomena. We model the spherical shocks in the universe by irradiating a solid spherical target surrounded by a plasma in the presence of a magnetic field. We present preliminary results obtained by shadowgraphy.",

author = "Y. Kuramitsu and S. Matsukiyo and S. Isayama and D. Harada and T. Oyama and R. Fujino and Y. Sakawa and T. Morita and Y. Yamaura and T. Ishikawa and T. Moritaka and T. Sano and K. Tomita and R. Shimoda and Y. Sato and K. Uchino and A. Pelka and R. Crowston and N. Woolsey and G. Gregori and M. Koenig and Yuan, {D. W.} and Yin, {C. L.} and Li, {Y. T.} and K. Zhang and Zhong, {J. Y.} and Wang, {F. L.} and N. Ohnishi and K. Nagamine and H. Yoneda and H. Takabe",

note = "Publisher Copyright: {\textcopyright} Published under licence by IOP Publishing Ltd.; 8th International Conference on Inertial Fusion Sciences and Applications, IFSA 2013 ; Conference date: 08-09-2013 Through 13-09-2013",

year = "2016",

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doi = "10.1088/1742-6596/688/1/012056",

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TY - JOUR

T1 - Spherical shock in the presence of an external magnetic field

AU - Kuramitsu, Y.

AU - Matsukiyo, S.

AU - Isayama, S.

AU - Harada, D.

AU - Oyama, T.

AU - Fujino, R.

AU - Sakawa, Y.

AU - Morita, T.

AU - Yamaura, Y.

AU - Ishikawa, T.

AU - Moritaka, T.

AU - Sano, T.

AU - Tomita, K.

AU - Shimoda, R.

AU - Sato, Y.

AU - Uchino, K.

AU - Pelka, A.

AU - Crowston, R.

AU - Woolsey, N.

AU - Gregori, G.

AU - Koenig, M.

AU - Yuan, D. W.

AU - Yin, C. L.

AU - Li, Y. T.

AU - Zhang, K.

AU - Zhong, J. Y.

AU - Wang, F. L.

AU - Ohnishi, N.

AU - Nagamine, K.

AU - Yoneda, H.

AU - Takabe, H.

PY - 2016/4/1

Y1 - 2016/4/1

N2 - We investigate spherical collisionless shocks in the presence of an external magnetic field. Spherical collisionless shocks are common resultant of interactions between a expanding plasma and a surrounding plasma, such as the solar wind, stellar winds, and supernova remnants. Anisotropies often observed in shock propagations and their emissions, and it is widely believed a magnetic field plays a major role. Since the local observations of magnetic fields in astrophysical plasmas are not accessible, laboratory experiments provide unique capability to investigate such phenomena. We model the spherical shocks in the universe by irradiating a solid spherical target surrounded by a plasma in the presence of a magnetic field. We present preliminary results obtained by shadowgraphy.

AB - We investigate spherical collisionless shocks in the presence of an external magnetic field. Spherical collisionless shocks are common resultant of interactions between a expanding plasma and a surrounding plasma, such as the solar wind, stellar winds, and supernova remnants. Anisotropies often observed in shock propagations and their emissions, and it is widely believed a magnetic field plays a major role. Since the local observations of magnetic fields in astrophysical plasmas are not accessible, laboratory experiments provide unique capability to investigate such phenomena. We model the spherical shocks in the universe by irradiating a solid spherical target surrounded by a plasma in the presence of a magnetic field. We present preliminary results obtained by shadowgraphy.

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U2 - 10.1088/1742-6596/688/1/012056

DO - 10.1088/1742-6596/688/1/012056

M3 - Conference article

AN - SCOPUS:84964832252

SN - 1742-6588

VL - 688

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

IS - 1

M1 - 012056

T2 - 8th International Conference on Inertial Fusion Sciences and Applications, IFSA 2013

Y2 - 8 September 2013 through 13 September 2013

ER -

Spherical shock in the presence of an external magnetic field

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