Electron energy probability function and L-p similarity in low pressure inductively coupled bounded plasma
被引:4
作者:
Chatterjee, Sanghamitro
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Indian Inst Technol, Dept Phys, Waves & Beams Lab, Grand Trunk Rd, Kanpur 208016, Uttar Pradesh, IndiaIndian Inst Technol, Dept Phys, Waves & Beams Lab, Grand Trunk Rd, Kanpur 208016, Uttar Pradesh, India
Chatterjee, Sanghamitro
[1
]
Bhattacharjee, Sudeep
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Indian Inst Technol, Dept Phys, Waves & Beams Lab, Grand Trunk Rd, Kanpur 208016, Uttar Pradesh, IndiaIndian Inst Technol, Dept Phys, Waves & Beams Lab, Grand Trunk Rd, Kanpur 208016, Uttar Pradesh, India
Bhattacharjee, Sudeep
[1
]
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Charles, Christine
[2
]
Boswell, Rod
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Australian Natl Univ, Res Sch Phys & Engn, Space Plasma Power & Prop Lab, Canberra, ACT, AustraliaIndian Inst Technol, Dept Phys, Waves & Beams Lab, Grand Trunk Rd, Kanpur 208016, Uttar Pradesh, India
Boswell, Rod
[2
]
机构:
[1] Indian Inst Technol, Dept Phys, Waves & Beams Lab, Grand Trunk Rd, Kanpur 208016, Uttar Pradesh, India
[2] Australian Natl Univ, Res Sch Phys & Engn, Space Plasma Power & Prop Lab, Canberra, ACT, Australia
来源:
FRONTIERS IN PHYSICS
|
2015年
/
3卷
关键词:
particle-in-cell (PIC) simulations;
electron energy probability function (EEPF);
inductively coupled plasma (ICP);
Maxwellian distribution;
particle balance;
L-p similarity;
D O I:
10.3389/fphy.2015.00007
中图分类号:
O4 [物理学];
学科分类号:
0702 ;
摘要:
Particle-In-Cell (PIC) simulations are carried out to investigate the effect of discharge length (L) and pressure (p) on Electron Energy Probability Function (EEPF) in a low pressure radio frequency (rf) inductively coupled plasma (ICP) at 13.56MHz. It is found that for both cases of varying L (0.1-0.5 m) and p (1-10 mTorr), the EEPF is a bi-Maxwellian with a step in the bounded direction (x) and non-Maxwellian with a hot tail in the symmetric unbounded directions (y, z). The plasma space potential decreases with increase in both L and p, the trapped electrons having energies in the range 0-20 eV. In a conventional discharge bounded in all directions, we infer that L and p are similarity parameters for low energy electrons trapped in the bulk plasma that have energies below the plasma space potential (eV(p)). The simulation results are consistent with a particle balance model.
机构:
Australian Natl Univ, Res Sch Phys & Engn, Space Plasma Power & Prop Grp, Canberra, ACT 0200, AustraliaAustralian Natl Univ, Res Sch Phys & Engn, Space Plasma Power & Prop Grp, Canberra, ACT 0200, Australia
Baalrud, S. D.
Lafleur, T.
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Australian Natl Univ, Res Sch Phys & Engn, Space Plasma Power & Prop Grp, Canberra, ACT 0200, AustraliaAustralian Natl Univ, Res Sch Phys & Engn, Space Plasma Power & Prop Grp, Canberra, ACT 0200, Australia
Lafleur, T.
Boswell, R. W.
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机构:
Australian Natl Univ, Res Sch Phys & Engn, Space Plasma Power & Prop Grp, Canberra, ACT 0200, AustraliaAustralian Natl Univ, Res Sch Phys & Engn, Space Plasma Power & Prop Grp, Canberra, ACT 0200, Australia
机构:
Australian Natl Univ, Res Sch Phys & Engn, Space Plasma Power & Prop Grp, Canberra, ACT 0200, AustraliaAustralian Natl Univ, Res Sch Phys & Engn, Space Plasma Power & Prop Grp, Canberra, ACT 0200, Australia
Baalrud, S. D.
Lafleur, T.
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h-index: 0
机构:
Australian Natl Univ, Res Sch Phys & Engn, Space Plasma Power & Prop Grp, Canberra, ACT 0200, AustraliaAustralian Natl Univ, Res Sch Phys & Engn, Space Plasma Power & Prop Grp, Canberra, ACT 0200, Australia
Lafleur, T.
Boswell, R. W.
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机构:
Australian Natl Univ, Res Sch Phys & Engn, Space Plasma Power & Prop Grp, Canberra, ACT 0200, AustraliaAustralian Natl Univ, Res Sch Phys & Engn, Space Plasma Power & Prop Grp, Canberra, ACT 0200, Australia