2006
DOI: 10.1088/0022-3727/39/14/018
|View full text |Cite
|
Sign up to set email alerts
|

Metal halide lamps in the international space station ISS

Abstract: Optical emission spectroscopy was performed on a metal-halide lamp under micro-gravity conditions of the international space station. Several transitions of atomic and ionic Dy and atomic Hg have been measured at different lateral positions from which we obtained atomic and ionic Dy and atomic Hg intensity profiles. After Abel inversion, the calibrated radial intensity profile of Hg was used to calculate a radial temperature profile. By combining the radial temperature profile with the calibrated radial intens… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
2

Citation Types

4
47
0

Year Published

2006
2006
2016
2016

Publication Types

Select...
7

Relationship

1
6

Authors

Journals

citations
Cited by 21 publications
(51 citation statements)
references
References 14 publications
4
47
0
Order By: Relevance
“…In case of the 579 nm line of Hg, the intensity is calibrated and then the absolute radial intensity profile is used to numerically determine the temperature profile. In case the atomic or ionic lines of Dy are measured, the temperature profile is combined with the calibrated radial intensity profile of the additive into an absolute radial system density profile using equation (2) [9].…”
Section: The Experimentsmentioning
confidence: 99%
See 1 more Smart Citation
“…In case of the 579 nm line of Hg, the intensity is calibrated and then the absolute radial intensity profile is used to numerically determine the temperature profile. In case the atomic or ionic lines of Dy are measured, the temperature profile is combined with the calibrated radial intensity profile of the additive into an absolute radial system density profile using equation (2) [9].…”
Section: The Experimentsmentioning
confidence: 99%
“…All measurements were done for different powers ranging from 70 to 150 W. The Hg ion distribution was also derived from the atomic Hg line using the Saha relation [12]. The results were reported in [9]. In order to cross-compare results of the various experiments done on metal-halide lamps and to compare the results from models to the experiments a reference lamp has been defined within the framework of the European project COST-529 [13].…”
Section: Introductionmentioning
confidence: 99%
“…Obviously, these variations have a strong impact on the lamp emission and its efficiency. More details on the various measurements both under normal and microgravity conditions can be found in the references [8,9].…”
Section: Microgravity Experimentsmentioning
confidence: 99%
“…Due to dominant radial segregation there is less emission from the central lamp region under micro-gravity conditions.The microgravity measurements are performed in the international space station where the lamp shows no axial segregation as seen in the picture.The normal gravity data are taken with the same lamp just before launching.The data are reconstructed from spectrally resolved side-on measurements, which is reliable until the shaded area. [8] number 6 volume 37 37 -W.…”
Section: Microgravity Experimentsmentioning
confidence: 99%
“…Single-walled carbon nanotubes were produced by arc discharge method in hypergravity [11] and also microgravity [12,13]. The flow phenomena in metal-halide arc discharge lamps were intensively investigated under varying gravity conditions [14][15][16]. Low pressure radio frequency plasmas with dust particles are currently researched in various gravity conditions, too [17][18][19].…”
Section: Introductionmentioning
confidence: 99%