1887
banner image
No data available.
Please log in to see this content.
You have no subscription access to this content.
No metrics data to plot.
The attempt to load metrics for this article has failed.
The attempt to plot a graph for these metrics has failed.
Ab initio modeling of the motional Stark effect on MASTa)
a)Contributed paper, published as part of the Proceedings of the 17th Topical Conference on High-Temperature Plasma Diagnostics, Albuquerque, New Mexico, May 2008.
Rent:
Rent this article for
USD
10.1063/1.2966459
/content/aip/journal/rsi/79/10/10.1063/1.2966459
http://aip.metastore.ingenta.com/content/aip/journal/rsi/79/10/10.1063/1.2966459
View: Figures

Figures

Image of FIG. 1.
FIG. 1.

(a) Velocity distribution at point for three beamlets with a focus at point . (b) MAST velocity distribution for four spatial points around and on the beam axis at (probability: maximum of 0.5%, minimum of 0.1%, sum over all 262 beamlets: 100%).

Image of FIG. 2.
FIG. 2.

and as function of the intensity ratio of two polarized emission sources: one at and one at .

Image of FIG. 3.
FIG. 3.

Comparison between reduced and full modeling of the Stark spectrum. The spectra shown were calculated for a channel at .

Image of FIG. 4.
FIG. 4.

Spatial resolution, , and normalized ratio for a top viewing geometry and for a viewing geometry in the midplane.

Image of FIG. 5.
FIG. 5.

Overview of the multichord MSE setup at MAST.

Loading

Article metrics loading...

/content/aip/journal/rsi/79/10/10.1063/1.2966459
2008-10-31
2014-04-20
Loading

Full text loading...

This is a required field
Please enter a valid email address
752b84549af89a08dbdd7fdb8b9568b5 journal.articlezxybnytfddd
Scitation: Ab initio modeling of the motional Stark effect on MASTa)
http://aip.metastore.ingenta.com/content/aip/journal/rsi/79/10/10.1063/1.2966459
10.1063/1.2966459
SEARCH_EXPAND_ITEM