Metal-halide lamps in micro-gravity: experiment and model
The results from optical emission spectroscopy experiments of metal-halide lamps under the micro-gravity conditions on board the international space station are compared with the results of a numerical LTE model constructed with the platform Plasimo. At micro-gravity there is no convection which all...
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Published in | Journal of physics. D, Applied physics Vol. 41; no. 14; pp. 144024 - 144024 (9) |
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Main Authors | , , , , , , |
Format | Journal Article |
Language | English |
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IOP Publishing
21.07.2008
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Abstract | The results from optical emission spectroscopy experiments of metal-halide lamps under the micro-gravity conditions on board the international space station are compared with the results of a numerical LTE model constructed with the platform Plasimo. At micro-gravity there is no convection which allows for easier modelling and for a separate study of the diffusion-induced radial segregation effect, undisturbed by convection. The plasma parameters that were experimentally determined and compared with the model were the Dy atom and ion density, the Hg ion density and the temperature. |
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AbstractList | The results from optical emission spectroscopy experiments of metal-halide lamps under the micro-gravity conditions on board the international space station are compared with the results of a numerical LTE model constructed with the platform Plasimo. At micro-gravity there is no convection which allows for easier modelling and for a separate study of the diffusion-induced radial segregation effect, undisturbed by convection. The plasma parameters that were experimentally determined and compared with the model were the Dy atom and ion density, the Hg ion density and the temperature. |
Author | Nimalasuriya, T Kroesen, G M W Haverlag, M Beks, M L Stoffels, W W Flikweert, A J van der Mullen, J J A M |
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Cites_doi | 10.1088/0022-3727/40/9/025 10.1103/RevModPhys.76.541 10.1063/1.2175466 10.1088/0022-3727/39/20/017 10.1088/0022-3727/35/4/309 10.1088/0022-3727/40/9/026 10.1088/0022-3727/39/14/018 10.1007/978-1-349-09196-6 10.1103/PhysRev.128.2679 10.1088/0957-0233/17/11/N01 10.1016/0370-1573(90)90152-R 10.1103/PhysRevA.8.2348 10.1063/1.323033 10.1088/0022-3727/35/17/307 10.1071/PH910647 10.1063/1.2073970 10.1088/0022-3727/39/8/019 10.1016/S0022-4073(99)00173-9 |
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