Langmuir probe study of an inductively coupled magnetic-pole-enhanced helium plasma
- Authors: Younus M.1, Rehman N.U.2, Shafiq M.1, Naeem M.1, Zaka-ul-Islam M.3, Zakaullah M.1
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Affiliations:
- Department of Physics
- Plasma Physics Laboratory
- Department of Physics, Faculty of Science
- Issue: Vol 43, No 5 (2017)
- Pages: 588-593
- Section: Low-Temperature Plasma
- URL: https://journals.rcsi.science/1063-780X/article/view/186507
- DOI: https://doi.org/10.1134/S1063780X17050105
- ID: 186507
Cite item
Abstract
This study reports the effects of RF power and filling gas pressure variation on the plasma parameters, including the electron number density ne, electron temperature Te, plasma potential Vp, skin depth δ, and electron energy probability functions (EEPFs) in a low-pressure inductively coupled helium plasma source with magnetic pole enhancement. An RF compensated Langmuir probe is used to measure these plasma parameters. It is observed that the electron number density increases with both the RF power and the filling gas pressure. Conversely, the electron temperature decreases with increasing RF power and gas pressure. It is also noted that, at low RF powers and gas pressures, the EEPFs are non-Maxwellian, while at RF powers of ≥50 W, they evolve into a Maxwellian distribution. The dependences of the skin depth and plasma potential on the RF power are also studied and show a decreasing trend.
About the authors
Maria Younus
Department of Physics
Email: najeeb-ur-rehman@comsats.edu.pk
Pakistan, Islamabad
N. U. Rehman
Plasma Physics Laboratory
Author for correspondence.
Email: najeeb-ur-rehman@comsats.edu.pk
Pakistan, Islamabad
M. Shafiq
Department of Physics
Email: najeeb-ur-rehman@comsats.edu.pk
Pakistan, Islamabad
M. Naeem
Department of Physics
Email: najeeb-ur-rehman@comsats.edu.pk
Pakistan, Islamabad
M. Zaka-ul-Islam
Department of Physics, Faculty of Science
Email: najeeb-ur-rehman@comsats.edu.pk
Saudi Arabia, Jazan
M. Zakaullah
Department of Physics
Email: najeeb-ur-rehman@comsats.edu.pk
Pakistan, Islamabad
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