Abstract
A new tangential two-dimensional soft x-ray imaging system (SXRIS) is being designed to examine the edge island structure in the lower X-point region of DIII-D. Plasma shielding and/or amplification of the calculated vacuum islands may play a role in the suppression of edge-localized modes via resonant magnetic perturbations (RMPs). The SXRIS is intended to improve the understanding of three-dimensional (3D) phenomena associated with RMPs. This system utilizes a tangential view with a pinhole imaging system and spectral filtering with beryllium foils. SXR emission is chosen to avoid line radiation and allows suitable signal at the top of a H-mode pedestal where Te ∼1-2 keV. A synthetic diagnostic calculation based on 3D SXR emissivity estimates is used to help assess signal levels and resolution of the design. A signal-to-noise ratio of 10 at 1 cm resolution is expected for the perturbed signals, which are sufficient to resolve most of the predicted vacuum island sizes.
| Original language | English |
|---|---|
| Article number | 10E534 |
| Journal | Review of Scientific Instruments |
| Volume | 81 |
| Issue number | 10 |
| DOIs | |
| State | Published - Oct 2010 |
Funding
This work was supported in part by the U.S. Department of Energy under Grant Nos. DE-AC05-00OR22725 and DE-FC02-04ER54698.
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