September 2006 Monthly Report- ITER Visible/IRTV Optical Design Scoping Study

LLNL received a request from the US ITER organization to perform a scoping study of optical design for visible/IR camera systems for the 6 upper ports of ITER. A contract was put in place and the LLNL account number was opened July 19, 2006. A kickoff meeting was held at LLNL July 26. The principal work under the contract is being performed by Lynn Seppala (optical designer), Kevin Morris (mechanical designer), Max Fenstermacher (visible cameras), Mathias Groth (assisting with visible cameras), and Charles Lasnier (IR cameras and Principal Investigator), all LLNL employees. Kevin Morris has imported ITER CAD files and developed a simplified 3D view of the ITER tokamak with upper ports, which he used to determine the optimum viewing angle from an upper port to see the outer target. He also determined the minimum angular field of view needed to see the largest possible coverage of the outer target. We examined the CEA-Cadarache report on their optical design for ITER visible/IRTV equatorial ports. We found that the resolution was diffraction-limited by the 5-mm aperture through the tile. Lynn Seppala developed a similar front-end design for an upper port but with a larger 6-inch-diameter beam. This allows the beam to pass through the port plug and port interspace without further focusing optics until outside the bioshield. This simplifies the design as well as eliminating a requirement for complex relay lenses in the port interspace. The focusing optics are all mirrors, which allows the system to handle light from 0.4 {micro}m to 5 {micro}m wavelength without chromatic aberration. The window material chosen is sapphire, as in the CEA design. Sapphire has good transmission in the desired wavelengths up to 4.8 {micro}m, as well as good mechanical strength. We have verified that sapphire windows of the needed size are commercially available. The diffraction-limited resolution permitted by the 5 mm aperture falls short of the ITER specification value but is well-matched to the resolution of current detectors. A large increase in resolution would require a similar increase in the linear pixel count on a detector. However, we cannot increase the aperture much without affecting the image quality. Lynn Seppala is writing a memo detailing the resolution trade-offs. Charles Lasnier is calculating the radiated power, which will fall on the detector in order to estimate signal-to-noise ratio and maximum frame rate. The signal will be reduced by the fact that the outer target plates are tungsten, which radiates less than carbon at the same temperature. The tungsten will also reflect radiation from the carbon tiles private flux dome, which will radiate efficiently although at a lower temperature than the target plates. The analysis will include estimates of these effects. Max Fenstermacher is investigating the intensity of line emission that will be emitted in the visible band, in order to predict signal-to-noise ratio and maximum frame rate for the visible camera. Andre Kukushkin has modeling results that will give local emission of deuterium and carbon lines. Line integrals of the emission must be done to produce the emitted intensity. The model is not able to handle tungsten and beryllium so we will only be able to estimate deuterium and carbon emission. Total costs as of September 30, 2006 are $87,834.43. Manpower was 0.58 FTE's in August, 1.48 in August, and 1.56 in September

Modified Visible and Infrared Optical Design for the ITER Upper Ports

This document reports the results of a follow-on optical design study of visible-light and infrared optics for the ITER upper ports, performed by LLNL under contract for the US ITER Project Office. The major objectives of this work are to move the viewing aperture closer to the plasma so that the optical path does not cut through any adjacent blanket shield module other than the module designated for the port; move optics forward into the port tube to increase the aperture size and therefore improve the spatial resolution; assess the trade-off between spatial resolution and spatial coverage by reducing the field of view; and create a mechanical model with a neutron labyrinth. Here we show an optical design incorporating all these aspects. The new design fits into a 360 mm ID tube, as did the previous design. The entrance aperture is increased from 10 mm to 21 mm, with a corresponding increase in spatial resolution. The Airy disk diameter for 3.8 {micro}m wavelength IR light is 5.1 mm at the most distant target point in the field of view. The field of view is reduced from 60 toroidal degrees (full toroidal coverage with 6 cameras) to 50 toroidal degrees. The 10 degrees eliminated are those nearest the camera, which have the poorest view of the divertor plate and in fact saw little of the plate. The Cassegrain telescope that was outside the vacuum windows in the previous design is now in vacuum, along with lenses for visible light. The Cassegrain for visible light is eliminated. An additional set of optical relay lenses is added for the visible and for the IR

Characteristics of the Scrape-Off Layer in DIII-D High-Performance Negative Central Magnetic Shear Discharges

In this paper the authors present measurements of the global power and particle balance in the high-performance phase of negative central magnetic shear (NCS) discharges and compare with reference VH-mode discharges. The principal differences observed are that NCS has a much lower fraction of the total input power flowing into the boundary, less core radiation, and larger rate of stored energy increase as a fraction of total power. Scrape-off layer (SOL) temperature and divertor heat flux profiles, and radiation profiles at the midplane, are similar to VH-mode. Due to the good core particle confinement and efficient fueling by neutral beam injection (NBI), with little gas puffing, the gas load on the walls and the recycling are very low during the NCS discharges. This results in a rate of density rise relative to beam fueling at the L to H transition time which is 1/3 of the value for VH transitions, which is in turn 1/2 that for L-to-ELMing-H-mode transitions

Improved system for perpendicular electron-cyclotron emission measurements on TMX-Upgrade

Perpendicular electron-cyclotron emission (PECE) is used on TMX-U to diagnose thermal-barrier hot electrons (T/sub H/ approx. 100 to 400 keV); yielding the time history of the temperature of these relativistic electrons. We describe an improved quasi-optical viewing system for these measurements that uses high sensitivity superheterodyne receivers at fixed frequencies of 60, 98, 130, and 196 GHz. The improved viewing and transport system consists of an off-axis ellipsoidal mirror that images the plasma onto a V-band conical collection horn, an overmoded circular waveguide (7/8'' diam) that transports the radiation outside the vacuum vessel where the polarization is selected, and a high absorptivity Macor beam dump to prevent internal wall reflections from entering the viewing system. A relativistic code is used to calculate optically thin PECE signals from relativistic electrons for various energy and pitch angle distributions. 4 refs., 4 figs

Optically thin perpendicular electron-cyclotron emission from hot electrons in TMX-U

Perpendicular electron-cyclotron emission (PECE) from relativistic (T/sub H/ approx. 100 to 400 keV) hot electrons within the thermal-barrier region of TMX-U is detected at 35, 60, 94 and 98 GHz. For the operating regime of TMX-U these signals are optically thin (tau<<1) and thus proportional to the radial hot electron line density. A relativistic code is used to calculate the theoretical temperature dependence of the perpendicular emission coefficient, j perpendicular(..omega..,T/sub H/), for each of the detected frequencies. This dependence has been verified experimentally by x-ray measurements of the hot electron temperature, T/sub H/. The observed qualitative agreement demonstrates that optically thin PECE signals can be used to determine the temporal evolution of T/sub H/. An inability to absolutely calibrate the present PECE waveguide system has prevented quantitative agreement

Caveolin-1 expression and cavin stability regulate caveolae dynamics in adipocyte lipid store fluctuation

Adipocytes specialized in the storage of energy as fat are among the most caveolae-enriched cell types. Loss of caveolae produces lipodystrophic diabetes in humans, which cannot be reversed by endothelial rescue of caveolin expression in mice, indicating major importance of adipocyte caveolae. However, how caveolae participate in fat cell functions is poorly understood. We investigated dynamic conditions of lipid store fluctuations and demonstrate reciprocal regulation of caveolae density and fat cell lipid droplet storage. We identified caveolin-1 expression as a crucial step in adipose cell lines and in mice to raise the density of caveolae, to increase adipocyte ability to accommodate larger lipid droplets, and to promote cell expansion by increased glucose utilization. In human subjects enrolled in a trial of 8 weeks of overfeeding to promote fattening, adipocyte expansion response correlated with initial caveolin-1 expression. Conversely, lipid mobilization in cultured adipocytes to induce lipid droplet shrinkage led to biphasic response of cavin-1 with ultimate loss of expression of cavin-1 and -3 and EHD2 by protein degradation, coincident with caveolae disassembly. We have identified the key steps in cavin/caveolin interplay regulating adipocyte caveolae dynamics. Our data establish that caveolae participate in a unique cell response connected to lipid store fluctuation, suggesting lipid-induced mechanotension in adipocytes

The lipoatrophic caveolin-1 deficient mouse model reveals autophagy in mature adipocytes

Adipose tissue lipoatrophy caused by caveolin gene deletion in mice is not linked to defective adipocyte differentiation. We show that adipose tissue development cannot be rescued by endothelial specific caveolin-1 re-expression, indicating primordial role of caveolin in mature adipocytes. Partial or total caveolin deficiency in adipocytes induced broad protein expression defects, including but not limited to previously described downregulation of insulin receptor. Global alterations in protein turnover, and accelerated degradation of long-lived proteins were found in caveolin-deficient adipocytes. Lipidation of endogenous LC3 autophagy marker and distribution of GFP-LC3 into aggregates demonstrated activated autophagy in the absence of caveolin-1 in adipocytes. Furthermore, electron microscopy revealed autophagic vacuoles in caveolin-1 deficient but not control adipocytes. Surprisingly, significant levels of lipidated LC3-II were found around lipid droplets of normal adipocytes, maintained in nutrient-rich conditions or isolated from fed mice, which do not display autophagy. Altogether, these data indicate that caveolin deficiency induce autophagy in adipocytes, a feature that is not a physiological response to fasting in normal fat cells. This likely resulted from defective insulin and lipolytic responses that converge in chronic nutrient shortage in adipocytes lacking caveolin-1. This is the first report of a pathological situation with autophagy as an adaptative response to adipocyte failure