138 research outputs found
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Neutron-induced noise in NIF-class diagnostic instruments
Neutron yields form DT-filled ICF targets have reached 10{sup 14}. Above 10{sup 13}, a significant neutron-induced background appears in images recorded with nearby streak cameras. Since cameras components (streak tube, image-intensifier tube, and CCD array) are similar to components that will be used in many NIF instruments, streak camera images provide information about neutron-induced backgrounds that will be encountered in the NIF environment. At a fluence of 10{sup 7} neutrons/cm{sup 2}, the background consists of two distinct components: a uniform component equal to nearly 20% of the camera`s linear range and sharp, intense peaks each localized to just a couple of image pixels. About 80% of the uniform background is caused by interactions with the streak tube and image-intensifier tube. Nearly all of the sharp spikes are caused by interactions with pixels of the CCD array. The spikes make the most significant contribution to image noise
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Neutron time-of-flight spectrometer for laser-fusion experiments
The basic concept of a time-of-flight spectrometer is illustrated. The spectrometer described can measure 14.1-MeV neutrons coming directly from the D-T plasma and also neutrons scattered by the air or ground or other structures within the vicinity of the flight path. (MOW
Numerical studies on the structure of the cosmic ray electron halo in starburst galaxies
The structure of the cosmic ray electron halo of a starburst galaxy depends
strongly on the nature of galactic wind and the configuration of the magnetic
field. We have investigated these dependencies by solving numerically the
propagation of electrons originating in starburst galaxies, most likely in
supernova remnants. The calculations are made for several models for the
galactic winds and for the configuration of the magnetic fields for comparison
with observations. Our simulation of a quasi-radio halo reproduces both the
extended structure of ~ 9 kpc and the subtle hollow structure near the polar
region of the radio halo that are observed in the starburst galaxy NGC 253.
These findings suggest the existence of strong galactic wind in NGC 253.Comment: 4 pages, 6 figures, to appear in Proceeding of the conference "The
multi messenger approach to high energy gamma ray sources", Barcelona, July
200
Simulation of ITER ICWC scenarios in JET
Encouraging results recently obtained with alternative ion cyclotron wall conditioning (ICWC) in the present-day tokamaks and stellarators have elevated ICWC to the status of one of the most promising techniques available to ITER for routine interpulse conditioning in the presence of the permanent high toroidal magnetic field. The paper presents a study of ICWC discharge performance and optimization of the conditioning output in the largest tokamak JET using the standard ICRF heating antenna A2 in a scenario envisaged at ITER full field, BT=5.3 T: on-axis location of the fundamental ICR for deuterium, ω=ωcD+. The perspective of application of the alternative technique in ITER is analyzed using the 3-D MWS electromagnetic code, 1-D RF full wave and 0-D plasma codes.Обнадёживающие результаты по альтернативной ионно-циклотронной (ИЦ) чистке поверхностей вакуумной камеры, полученные недавно на современных токамаках и стеллараторах, выдвинули этот метод в число наиболее вероятных технологий, планирующихся использовать в ITERe между импульсами в присутствии постоянного сильного тороидального магнитно поля. В настоящей работе представлены результаты исследований ВЧ-разряда и его оптимизаци по усилению эффекта чистки в крупнейшем из ныне действующих токамаке JET с использованием стандартных ИЦ A2 антенн. Эксперименты по ВЧ-чистке на JETе были осуществлены в режиме, моделирующем сценарий ИЦ-разряда в токамаке-реакторе ITER, при работе на полном магнитном поле BT=5.3 T и при расположении фундаментального ИЦ-резонанса для дейтерия ω=ωcD+ в центре вакуумной камеры. Перспективы применения альтернативной ВЧ-чистки в ITERе анализируются с помощью численных кодов: 3-D MWS- электромагнитного кода, 1-D ВЧ-кода и 0-D плазменного кода.Обнадійливі результати з альтернативної іонної циклотронної (ІЦ) чистки поверхонь вакуумної камери, отримані останнім часом в сучасних токамаках і стелараторах, висунули цей метод до числа найбільш вірогідних технологій, які планується використовувати в ІТЕРі між імпульсами в присутності постійного сильного тороїдального магнітного поля. В роботі представленo результати дослідження ВЧ-розряду та його оптимізації щодо підсилення ефекту чистки в найбільшому з нині діючих токамаці JET з використанням стандартних ІЦ А2 антен. Експерименти по ВЧ-чищенню на JETі були здійснені в режимі, що моделює сценарій ІЦ-розряду в токамаці-реакторі ITER, при роботі на повному магнітному полі BT=5.3 T та при розміщенні фундаментального ІЦ-резонансу для дейтерію ω=ωcD+ в центрі вакуумної камери. Перспективи застосування альтернативної ВЧ-чистки в ITERі аналізуються за допомогою числових кодів: 3-D MWS- електромагнітного коду, 1-D ВЧ-коду і 0-D плазмового коду
Velocity-space sensitivity of the time-of-flight neutron spectrometer at JET
The velocity-space sensitivities of fast-ion diagnostics are often described by so-called weight functions. Recently, we formulated weight functions showing the velocity-space sensitivity of the often dominant beam-target part of neutron energy spectra. These weight functions for neutron emission spectrometry (NES) are independent of the particular NES diagnostic. Here we apply these NES weight functions to the time-of-flight spectrometer TOFOR at JET. By taking the instrumental response function of TOFOR into account, we calculate time-of-flight NES weight functions that enable us to directly determine the velocity-space sensitivity of a given part of a measured time-of-flight spectrum from TOFOR
On the mechanisms governing gas penetration into a tokamak plasma during a massive gas injection
A new 1D radial fluid code, IMAGINE, is used to simulate the penetration of gas into a tokamak plasma during a massive gas injection (MGI). The main result is that the gas is in general strongly braked as it reaches the plasma, due to mechanisms related to charge exchange and (to a smaller extent) recombination. As a result, only a fraction of the gas penetrates into the plasma. Also, a shock wave is created in the gas which propagates away from the plasma, braking and compressing the incoming gas. Simulation results are quantitatively consistent, at least in terms of orders of magnitude, with experimental data for a D 2 MGI into a JET Ohmic plasma. Simulations of MGI into the background plasma surrounding a runaway electron beam show that if the background electron density is too high, the gas may not penetrate, suggesting a possible explanation for the recent results of Reux et al in JET (2015 Nucl. Fusion 55 093013)
Relationship of edge localized mode burst times with divertor flux loop signal phase in JET
A phase relationship is identified between sequential edge localized modes (ELMs) occurrence times in a set of H-mode tokamak plasmas to the voltage measured in full flux azimuthal loops in the divertor region. We focus on plasmas in the Joint European Torus where a steady H-mode is sustained over several seconds, during which ELMs are observed in the Be II emission at the divertor. The ELMs analysed arise from intrinsic ELMing, in that there is no deliberate intent to control the ELMing process by external means. We use ELM timings derived from the Be II signal to perform direct time domain analysis of the full flux loop VLD2 and VLD3 signals, which provide a high cadence global measurement proportional to the voltage induced by changes in poloidal magnetic flux. Specifically, we examine how the time interval between pairs of successive ELMs is linked to the time-evolving phase of the full flux loop signals. Each ELM produces a clear early pulse in the full flux loop signals, whose peak time is used to condition our analysis. The arrival time of the following ELM, relative to this pulse, is found to fall into one of two categories: (i) prompt ELMs, which are directly paced by the initial response seen in the flux loop signals; and (ii) all other ELMs, which occur after the initial response of the full flux loop signals has decayed in amplitude. The times at which ELMs in category (ii) occur, relative to the first ELM of the pair, are clustered at times when the instantaneous phase of the full flux loop signal is close to its value at the time of the first ELM
Operating procedures: Fusion Experiments Analysis Facility
The Fusion Experiments Analysis Facility (FEAF) is a computer facility based on a DEC VAX 11/780 computer. It became operational in late 1982. At that time two manuals were written to aid users and staff in their interactions with the facility. This manual is designed as a reference to assist the FEAF staff in carrying out their responsibilities. It is meant to supplement equipment and software manuals supplied by the vendors. Also this manual provides the FEAF staff with a set of consistent, written guidelines for the daily operation of the facility
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Resolution limitations and optimization of the LLNL streak camera focus
The RCA C73435 image tube is biased at voltages far from its original design in the LLNL ultrafast (10 ps) streak camera. Its output resolution at streak camera operating potentials has been measured as a function of input slit width, incident-light wavelength, and focus-grid voltage. The temporal resolution is insensitive to focus-grid voltage for a narrow (100 ..mu..m) input slit, but is very sensitive to focus-grid voltage for a wide (2 mm) input slit. At the optimum wide-slit focus voltage, temporal resolution is insensitive to slit width. Spatial resolution is nearly independent of focus-grid voltage for values that give good temporal resolution. Both temporal and spatial resolution depend on the incident-light wavelength. Data for 1.06-..mu..m light show significantly better focusing than for 0.53-..mu..m light. Streak camera operation is simulated with a computer program that calculates photoelectron trajectories. Electron ray tracing describes all of the observed effects of slit width, incident-light wavelength, and focus-grid voltage on output resolution. 7 refs
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