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Temporal and spatial resolved optical emission behaviors of a cold atmospheric pressure plasma jet

J. Appl. Phys. 106, 083302 (2009); doi:10.1063/1.3239512

Published 22 October 2009

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Q. Xiong, X. Lu, J. Liu, Y. Xian, Z. Xiong, F. Zou, C. Zou, W. Gong, J. Hu, K. Chen, X. Pei, Z. Jiang, and Y. Pan
College of Electrical and Electronic Engineering, HuaZhong University of Science and Technology, WuHan, Hubei 430074, People's Republic of China
The propagation behavior of cold atmospheric pressure plasma jets has recently attracted lots of attention. In this paper, a cold He plasma jet generated by a single plasma electrode jet device is studied. The spatial-temporal resolved optical emission spectroscopy measurements are presented. It is found that the emission intensity of the He 706.5 nm line of the plasma behaves similarly both inside the syringe and in the surrounding air (plasma plume). It decreases monotonously, which is different from the emission lines, such as N2 337.1 nm line, N2+ 391.4 nm line, and O 777.3 nm line. For the discharge inside the syringe, the emission intensity of the He 706.5 nm line decays more rapidly than that of the other three spectral lines mentioned above. The N2 337.1 nm line behaves a similar time evolution with the discharge current. For the N2+ 391.4 nm line and the atomic O 777.3 nm line, both of them decay slower than that of the He 706.5 nm and the N2 337.1 nm. When the plasma plume propagates further away from the nozzle, the temporal behaviors of the emission intensities of the four lines tend to be similar gradually. Besides, it is found that, when the size of the plasma bullet appears biggest, the propagation velocity of the bullet achieves its highest value while the emission intensity of the N2+ 391.4 nm line reaches its maximum. Detailed analysis shows that the Penning effect between the metastable state Hem and the air molecules may play a significant role in the propagation of the plasma bullet in the open air. ©2009 American Institute of Physics
History: Received 11 August 2009; accepted 4 September 2009; published 22 October 2009
Permalink: http://link.aip.org/link/?JAPIAU/106/083302/1
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KEYWORDS and PACS

Keywords
PACS
  • 52.25.Os
    Emission, absorption, and scattering of electromagnetic radiation from plasmas
  • 52.30.-q
    Plasma dynamics and flow
  • 52.70.Kz
    Optical (ultraviolet, visible, infrared) plasma diagnostic measurements
  • YEAR: 2009

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ISSN:
0021-8979 (print)   1089-7550 (online)
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REFERENCES (51)

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  1. M. Laroussi and T. Akan, Plasma Processes Polym. 4, 777 (2007).
  2. J. Walsh and M. Kong, Appl. Phys. Lett. 91, 221502 (2007).
  3. R. Dorai and M. Kushner, J. Phys. D 36, 666 (2003).
  4. G. Fridman, G. Friedman, A. Gutsol, A. Shekhter, V. Vasilets, and A. Fridman, Plasma Processes Polym. 5, 503 (2008).
  5. Q. Nie, C. Ren, D. Wang, and J. Zhang, Appl. Phys. Lett. 93, 011503 (2008).
  6. I. Kieft, D. Darios, A. Roks, and E. Stoffels, IEEE Trans. Plasma Sci. 33, 771 (2005).
  7. M. Laroussi and X. Lu, Appl. Phys. Lett. 87, 113902 (2005).
  8. X. Lu, Z. Jiang, Q. Xiong, Z. Tang, X. Hu, and Y. Pan, Appl. Phys. Lett. 92, 081502 (2008).
  9. S. Li, W. Huang, J. Zhang, and D. Wang, Phys. Plasmas 16, 073503 (2009).
  10. Z. Cao, J. Walsh, and M. Kong, Appl. Phys. Lett. 94, 021501 (2009).
  11. Q. Xiong, X. Lu, K. Ostrikov, Z. Xiong, Y. Xian, F. Zhou, C. Zou, J. Hu, W. Gong, and Z. Jiang, Phys. Plasmas 16, 043505 (2009).
  12. D. Mariotti, Appl. Phys. Lett. 92, 151505 (2008).
  13. A. Shashurin, M. Keidar, S. Bronnikov, R. Jurjus, and M. Strpp, Appl. Phys. Lett. 93, 181501 (2008).
  14. X. Lu, Z. Jiang, Q. Xiong, Z. Tang, and Y. Pan, Appl. Phys. Lett. 92, 151504 (2008).
  15. Y. Hong and H. Uhm, Phys. Plasmas 14, 053503 (2007).
  16. F. Iza, G. Kim, S. Lee, J. K. Lee, J. Walsh, Y. Zhang, and M. Kong, Plasma Processes Polym. 5, 322 (2008).
  17. G. Li, H. Li, L. Wang, S. Wang, H. Zhao, W. Sun, X. Xing, and C. Bao, Appl. Phys. Lett. 92, 221504 (2008).
  18. G. Fridman, A. Brooks, M. Galasubramanian, A. Fridman, A. Gutsol, V. Vasilets, H. Ayan, and G. Friedman, Plasma Processes Polym. 4, 370 (2007).
  19. J. Goree, B. Liu, and D. Drake, J. Phys. D 39, 3479 (2006).
  20. J. Lim, H. Uhm, and S. Li, Phys. Plasmas 14, 093504 (2007).
  21. Y. Hong and H. Uhm, Appl. Phys. Lett. 89, 221504 (2006).
  22. K. Becker, K. Schoenbach, and J. Eden, J. Phys. D 39, R55 (2006).
  23. X. Zhang, J. Huang, X. Liu, L. Peng, L. Guo, G. Lv, W. Chen, K. Feng, and S. Yang, J. Appl. Phys. 105, 063302 (2009).
  24. X. Lu, T. Ye, Y. Cao, Z. Sun, Q. Xiong, Z. Tang, Z. Xiong, J. Hu, Z. Jiang, and Y. Pan, J. Appl. Phys. 104, 053309 (2008).
  25. X. Lu, Y. Cao, P. Yang, Q. Xiong, Z. Xiong, Y. Xian, and Y. Pan, IEEE Trans. Plasma Sci. 37, 668 (2009).
  26. T. Ni, F. Ding, X. Zhu, X. Wen, and H. Zhou, Appl. Phys. Lett. 92, 241503 (2008).
  27. J. Kolb, A. Mohamed, R. Price, R. Swanson, A. Bowman, R. Chiavarini, M. Stacey, and K. Schoenbach, Appl. Phys. Lett. 92, 241501 (2008).
  28. E. Stoffels, I. Kieft, and R. Sladek, J. Phys. D 36, 2908 (2003).
  29. J. Walsh and M. Kong, Appl. Phys. Lett. 93, 111501 (2008).
  30. D. Kim, J. Rhee, B. Gweon, S. Moon, and W. Choe, Appl. Phys. Lett. 91, 151502 (2007).
  31. X. Lu and M. Laroussi, J. Appl. Phys. 100, 063302 (2006).
  32. A. Shashurin, M. Shneider, A. Dogariu, R. Miles, and M. Keidar, Appl. Phys. Lett. 94, 231504 (2009).
  33. M. Teschke, J. Kedzierski, E. Finantu-Dinu, K. Korzec, and J. Engemann, IEEE Trans. Plasma Sci. 33, 310 (2005).
  34. B. Sands, B. Ganguly, and K. Tachibana, Appl. Phys. Lett. 92, 151503 (2008).
  35. R. Ye and W. Zheng, Appl. Phys. Lett. 93, 071502 (2008).
  36. N. Mericam-Bourdet, M. Laroussi, A. Begum, and E. Karakas, J. Phys. D 42, 055207 (2009).
  37. X. Lu, Q. Xiong, Z. Xiong, J. Hu, F. Zhou, W. Gong, Y. Xian, C. Zhou, Z. Tang, Z. Jiang, and Y. Pan, J. Appl. Phys. 105, 043304 (2009).
  38. E. Stoffels, Y. Sakiyama, and D. Graves, IEEE Trans. Plasma Sci. 36, 1441 (2008).
  39. M. Laroussi, Plasma Processes Polym. 2, 391 (2005).
  40. G. Nersisyan and W. Graham, Plasma Sources Sci. Technol. 13, 582 (2004).
  41. F. Massines, P. Segur, N. Gherardi, C. Khamphan, and A. Ricard, Surf. Coat. Technol. 174–175, 8 (2003).
  42. A. Ricard, P. Decomps, and F. Massines, Surf. Coat. Technol. 112, 1 (1999).
  43. R. Deloche, P. Monchicourt, M. Cheret, and F. Lambert, Phys. Rev. A 13, 1140 (1976).
  44. N. Bibinov, A. Fateev, and K. Wiesemann, Plasma Sources Sci. Technol. 10, 579 (2001).
  45. G. Cartry, L. Magne, and G. Cernogora, J. Phys. D 32, 1894 (1999).
  46. E. Collart, J. Baggerman, and R. Visser, J. Appl. Phys. 70, 5278 (1991).
  47. X. Lu and M. Laroussi, Appl. Phys. Lett. 92, 051501 (2008).
  48. X. Yuan and L. Raja, IEEE Trans. Plasma Sci. 31, 495 (2003).
  49. T. Martens, A. Bogaerts, W. Brok, and J. Dijk, Appl. Phys. Lett. 92, 041504 (2008).
  50. P. Bruggeman, D. Schram, M. Gonzalez, R. Rego, M. Kong, and C. Leys, Plasma Sources Sci. Technol. 18, 025017 (2009).
  51. N. Bibinov, A. Fateev, and K. Wiesemnn, J. Phys. D 34, 1819 (2001).

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