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author:

Wang, Songbai (Wang, Songbai.) [1] | Lei, Guangjiu (Lei, Guangjiu.) [2] | Liu, Dongping (Liu, Dongping.) [3] | Yang, Size (Yang, Size.) [4]

Indexed by:

EI CSCD

Abstract:

Hα (Balmer-alpha), Hβ (Balmer-beta) and Hγ (Balmer-gamma) spectral line intensities in atomic hydrogen plasma are investigated by using a high-power RF source. The intensities of the Hα, Hβ and Hγ spectral lines are detected by increasing the input power (0-6 kW) of ICPs (inductively coupled plasmas). With the increase of net input power, the intensity of H α improves rapidly (0-2 kW), and then reaches its dynamic equilibrium; the intensities of Hβ can be divided into three processes: obvious increase (0-2 kW), rapid increase (2-4 kW), almost constant (4-6 kW); while the intensities of Hγ increase very slowly. The energy levels of the excited hydrogen atoms and the splitting energy levels produced by an obvious Stark effect play an important role in the results.

Keyword:

Atoms Boltzmann equation Electromagnetic induction Inductively coupled plasma Spectroscopy Stark effect Voltage dividers Water vapor

Community:

  • [ 1 ] [Wang, Songbai]College of Physics and Information Engineering, Fuzhou University, Fuzhou 350108, China
  • [ 2 ] [Wang, Songbai]School of Physics and Mechanical and Electrical Engineering, Xiamen University, Xiamen 361005, China
  • [ 3 ] [Lei, Guangjiu]Southwestern Institute of Physics, Chengdu 610041, China
  • [ 4 ] [Liu, Dongping]School of Physics and Mechanical and Electrical Engineering, Xiamen University, Xiamen 361005, China
  • [ 5 ] [Yang, Size]School of Physics and Mechanical and Electrical Engineering, Xiamen University, Xiamen 361005, China

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Source :

Plasma Science and Technology

ISSN: 1009-0630

Year: 2014

Issue: 3

Volume: 16

Page: 219-222

0 . 5 7 9

JCR@2014

1 . 6 0 0

JCR@2023

ESI HC Threshold:213

JCR Journal Grade:4

CAS Journal Grade:4

Cited Count:

WoS CC Cited Count:

SCOPUS Cited Count: 12

ESI Highly Cited Papers on the List: 0 Unfold All

WanFang Cited Count:

Chinese Cited Count:

30 Days PV: 0

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