메뉴 건너뛰기




Volumn 82, Issue 3, 2010, Pages

Optical emission and nanoparticle generation in Al plasmas using ultrashort laser pulses temporally optimized by real-time spectroscopic feedback

Author keywords

[No Author keywords available]

Indexed keywords


EID: 77956688883     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.82.035430     Document Type: Article
Times cited : (36)

References (97)
  • 3
    • 0038310286 scopus 로고    scopus 로고
    • 10.1103/PhysRevB.67.184102
    • D. Perez and L. J. Lewis, Phys. Rev. B 67, 184102 (2003). 10.1103/PhysRevB.67.184102
    • (2003) Phys. Rev. B , vol.67 , pp. 184102
    • Perez, D.1    Lewis, L.J.2
  • 30
  • 48
  • 54
    • 4944220525 scopus 로고
    • 10.1103/PhysRevLett.68.1500
    • R. S. Judson and H. Rabitz, Phys. Rev. Lett. 68, 1500 (1992). 10.1103/PhysRevLett.68.1500
    • (1992) Phys. Rev. Lett. , vol.68 , pp. 1500
    • Judson, R.S.1    Rabitz, H.2
  • 59
    • 33748485394 scopus 로고    scopus 로고
    • 10.1103/PhysRevLett.97.107601
    • H. Dachraoui and W. Husinsky, Phys. Rev. Lett. 97, 107601 (2006). 10.1103/PhysRevLett.97.107601
    • (2006) Phys. Rev. Lett. , vol.97 , pp. 107601
    • Dachraoui, H.1    Husinsky, W.2
  • 62
    • 84975633474 scopus 로고
    • 10.1364/OL.7.000196
    • J. M. Liu, Opt. Lett. 7, 196 (1982). 10.1364/OL.7.000196
    • (1982) Opt. Lett. , vol.7 , pp. 196
    • Liu, J.M.1
  • 66
    • 77956674564 scopus 로고    scopus 로고
    • The previous reported line of Al-II at 618.157 and 618.168 nm in Ref. is not considered anymore. This transition was previously associated with an Al-II line at 618.157 nm which was presenting an anomalous behavior. It is conceivable that we observe the Fe-I transitions at 618.02 or 618.799 nm.
    • The previous reported line of Al-II at 618.157 and 618.168 nm in Ref. is not considered anymore. This transition was previously associated with an Al-II line at 618.157 nm which was presenting an anomalous behavior. It is conceivable that we observe the Fe-I transitions at 618.02 or 618.799 nm.
  • 76
    • 33846807192 scopus 로고    scopus 로고
    • 10.1103/PhysRevE.75.026402
    • J. Daligault and D. Mozyrsky, Phys. Rev. E 75, 026402 (2007). 10.1103/PhysRevE.75.026402
    • (2007) Phys. Rev. e , vol.75 , pp. 026402
    • Daligault, J.1    Mozyrsky, D.2
  • 77
    • 77956682539 scopus 로고    scopus 로고
    • http://www.t4.lanl.gov/opacity/tops.html
  • 78
    • 0001872875 scopus 로고
    • Astronomical Society of the Pacific Conference Series Vol. edited by S. J. Adelman and W. L. Wiese (Astronomical Society of the Pacific, San Francisco
    • N. H. Magee, Jr., J. Abdallah, Jr., R. E. H. Clark, Astrophysical Applications of Powerful New Databases, Astronomical Society of the Pacific Conference Series Vol. 78, edited by, S. J. Adelman, and, W. L. Wiese, (Astronomical Society of the Pacific, San Francisco, 1995), p. 51.
    • (1995) Astrophysical Applications of Powerful New Databases , vol.78 , pp. 51
    • Magee, Jr.N.H.1    Abdallah, Jr.J.2    Clark, R.E.H.3
  • 79
    • 0942267622 scopus 로고    scopus 로고
    • 10.1103/PhysRevE.68.056410
    • D. K. Kim and I. Kim, Phys. Rev. E 68, 056410 (2003). 10.1103/PhysRevE.68.056410
    • (2003) Phys. Rev. e , vol.68 , pp. 056410
    • Kim, D.K.1    Kim, I.2
  • 82
  • 87
    • 34347355380 scopus 로고    scopus 로고
    • 10.1103/PhysRevB.75.214107
    • M. Kandyla, T. Shih, and E. Mazur, Phys. Rev. B 75, 214107 (2007). 10.1103/PhysRevB.75.214107
    • (2007) Phys. Rev. B , vol.75 , pp. 214107
    • Kandyla, M.1    Shih, T.2    Mazur, E.3
  • 90
  • 91
    • 0037837039 scopus 로고    scopus 로고
    • 10.1364/JOSAB.20.000125
    • T. E. Glover, J. Opt. Soc. Am. B 20, 125 (2003). 10.1364/JOSAB.20.000125
    • (2003) J. Opt. Soc. Am. B , vol.20 , pp. 125
    • Glover, T.E.1
  • 93
    • 66749163642 scopus 로고    scopus 로고
    • 10.1103/PhysRevB.79.184107
    • B. Chimier and V. T. Tikhonchuk, Phys. Rev. B 79, 184107 (2009). 10.1103/PhysRevB.79.184107
    • (2009) Phys. Rev. B , vol.79 , pp. 184107
    • Chimier, B.1    Tikhonchuk, V.T.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.