Spatial and temporal plasma evolutions of magnetic reconnection in laser produced plasmas

N. Khasanah; C. W. Peng; C. H. Chen; T. Y. Huang; N. Bolouki; T. Moritaka; Y. Hara; H. Shimogawara; T. Sano; Y. Sakawa; Y. Sato; K. Tomita; K. Uchino; S. Matsukiyo; Y. Shoji; S. Tomita; S. Tomiya; R. Yamazaki; M. Koenig; Y. Kuramitsu

doi:10.1016/j.hedp.2017.02.004

Spatial and temporal plasma evolutions of magnetic reconnection in laser produced plasmas

N. Khasanah
, C. W. Peng
, C. H. Chen
, T. Y. Huang
, N. Bolouki
, T. Moritaka
, Y. Hara
, H. Shimogawara
, T. Sano
, Y. Sakawa
, Y. Sato
, K. Tomita
, K. Uchino
, S. Matsukiyo
, Y. Shoji
, S. Tomita
, S. Tomiya
, R. Yamazaki
, M. Koenig
, Y. Kuramitsu

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

Résumé

Magnetic reconnection is experimentally investigated in laser produced plasmas. By irradiating a solid target with a high-power laser beam, a magnetic bubble is generated due to the Biermann effect. When two laser beams with finite focal spot displacements are utilized, two magnetic bubbles are generated, and the magnetic reconnection can take place. We measure the spatial and temporal plasma evolutions with optical diagnostics using framing camera. We observed the plasma jets, which are considered to be reconnection out flows. Spatial and temporal scales of the plasma jets are much larger than those of laser. The magnetic reconnection time has been estimated from the expansion velocity, which is consistent with the Sweet-Parker model.

langue originale	Anglais
Pages (de - à)	15-19
Nombre de pages	5
journal	High Energy Density Physics
Volume	23
Les DOIs	https://doi.org/10.1016/j.hedp.2017.02.004
état	Publié - 1 juin 2017
Modification externe	Oui

Accès au document

10.1016/j.hedp.2017.02.004

Autres fichiers et liens

Lien vers la publication dans Scopus

Contient cette citation

Khasanah, N., Peng, C. W., Chen, C. H., Huang, T. Y., Bolouki, N., Moritaka, T., Hara, Y., Shimogawara, H., Sano, T., Sakawa, Y., Sato, Y., Tomita, K., Uchino, K., Matsukiyo, S., Shoji, Y., Tomita, S., Tomiya, S., Yamazaki, R., Koenig, M., & Kuramitsu, Y. (2017). Spatial and temporal plasma evolutions of magnetic reconnection in laser produced plasmas. High Energy Density Physics, 23, 15-19. https://doi.org/10.1016/j.hedp.2017.02.004

@article{49c12bcf404b4260a60d304bbc83071f,

title = "Spatial and temporal plasma evolutions of magnetic reconnection in laser produced plasmas",

abstract = "Magnetic reconnection is experimentally investigated in laser produced plasmas. By irradiating a solid target with a high-power laser beam, a magnetic bubble is generated due to the Biermann effect. When two laser beams with finite focal spot displacements are utilized, two magnetic bubbles are generated, and the magnetic reconnection can take place. We measure the spatial and temporal plasma evolutions with optical diagnostics using framing camera. We observed the plasma jets, which are considered to be reconnection out flows. Spatial and temporal scales of the plasma jets are much larger than those of laser. The magnetic reconnection time has been estimated from the expansion velocity, which is consistent with the Sweet-Parker model.",

keywords = "Laboratory astrophysics, Laser, Magnetic reconnection, Plasma",

author = "N. Khasanah and Peng, \{C. W.\} and Chen, \{C. H.\} and Huang, \{T. Y.\} and N. Bolouki and T. Moritaka and Y. Hara and H. Shimogawara and T. Sano and Y. Sakawa and Y. Sato and K. Tomita and K. Uchino and S. Matsukiyo and Y. Shoji and S. Tomita and S. Tomiya and R. Yamazaki and M. Koenig and Y. Kuramitsu",

note = "Publisher Copyright: {\textcopyright} 2017 Elsevier B.V.",

year = "2017",

month = jun,

day = "1",

doi = "10.1016/j.hedp.2017.02.004",

language = "English",

volume = "23",

pages = "15--19",

journal = "High Energy Density Physics",

issn = "1574-1818",

}

Khasanah, N, Peng, CW, Chen, CH, Huang, TY, Bolouki, N, Moritaka, T, Hara, Y, Shimogawara, H, Sano, T, Sakawa, Y, Sato, Y, Tomita, K, Uchino, K, Matsukiyo, S, Shoji, Y, Tomita, S, Tomiya, S, Yamazaki, R, Koenig, M & Kuramitsu, Y 2017, 'Spatial and temporal plasma evolutions of magnetic reconnection in laser produced plasmas', High Energy Density Physics, VOL. 23, p. 15-19. https://doi.org/10.1016/j.hedp.2017.02.004

TY - JOUR

T1 - Spatial and temporal plasma evolutions of magnetic reconnection in laser produced plasmas

AU - Khasanah, N.

AU - Peng, C. W.

AU - Chen, C. H.

AU - Huang, T. Y.

AU - Bolouki, N.

AU - Moritaka, T.

AU - Hara, Y.

AU - Shimogawara, H.

AU - Sano, T.

AU - Sakawa, Y.

AU - Sato, Y.

AU - Tomita, K.

AU - Uchino, K.

AU - Matsukiyo, S.

AU - Shoji, Y.

AU - Tomita, S.

AU - Tomiya, S.

AU - Yamazaki, R.

AU - Koenig, M.

AU - Kuramitsu, Y.

PY - 2017/6/1

Y1 - 2017/6/1

N2 - Magnetic reconnection is experimentally investigated in laser produced plasmas. By irradiating a solid target with a high-power laser beam, a magnetic bubble is generated due to the Biermann effect. When two laser beams with finite focal spot displacements are utilized, two magnetic bubbles are generated, and the magnetic reconnection can take place. We measure the spatial and temporal plasma evolutions with optical diagnostics using framing camera. We observed the plasma jets, which are considered to be reconnection out flows. Spatial and temporal scales of the plasma jets are much larger than those of laser. The magnetic reconnection time has been estimated from the expansion velocity, which is consistent with the Sweet-Parker model.

AB - Magnetic reconnection is experimentally investigated in laser produced plasmas. By irradiating a solid target with a high-power laser beam, a magnetic bubble is generated due to the Biermann effect. When two laser beams with finite focal spot displacements are utilized, two magnetic bubbles are generated, and the magnetic reconnection can take place. We measure the spatial and temporal plasma evolutions with optical diagnostics using framing camera. We observed the plasma jets, which are considered to be reconnection out flows. Spatial and temporal scales of the plasma jets are much larger than those of laser. The magnetic reconnection time has been estimated from the expansion velocity, which is consistent with the Sweet-Parker model.

KW - Laboratory astrophysics

KW - Laser

KW - Magnetic reconnection

KW - Plasma

UR - https://www.scopus.com/pages/publications/85014466054

U2 - 10.1016/j.hedp.2017.02.004

DO - 10.1016/j.hedp.2017.02.004

M3 - Article

AN - SCOPUS:85014466054

SN - 1574-1818

VL - 23

SP - 15

EP - 19

JO - High Energy Density Physics

JF - High Energy Density Physics

ER -

Spatial and temporal plasma evolutions of magnetic reconnection in laser produced plasmas

Résumé

Accès au document

Autres fichiers et liens

Empreinte digitale

Contient cette citation