L. Stagner
University of California, Irvine
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Featured researches published by L. Stagner.
Physical Review Letters | 2016
C. S. Collins; W.W. Heidbrink; M. E. Austin; G. J. Kramer; D. C. Pace; C. C. Petty; L. Stagner; M. A. Van Zeeland; R. B. White; Y. B. Zhu; Diii-D Team
Experiments in the DIII-D tokamak show that fast-ion transport suddenly becomes stiff above a critical threshold in the presence of many overlapping small-amplitude Alfvén eigenmodes (AEs). The threshold is phase-space dependent and occurs when particle orbits become stochastic due to resonances with AEs. Above threshold, equilibrium fast-ion density profiles are unchanged despite increased drive, and intermittent fast-ion losses are observed. Fast-ion Dα spectroscopy indicates radially localized transport of the copassing population at radii that correspond to the location of midcore AEs. The observation of stiff fast-ion transport suggests that reduced models can be used to effectively predict alpha profiles, beam ion profiles, and losses to aid in the design of optimized scenarios for future burning plasma devices.
Plasma Physics and Controlled Fusion | 2016
A. S. Jacobsen; L. Stagner; M. Salewski; B. Geiger; W.W. Heidbrink; S. B. Korsholm; F. Leipold; S. K. Nielsen; J. Juul Rasmussen; M. Stejner; H. Thomsen; M. Weiland
Author(s): Jacobsen, AS; Stagner, L; Salewski, M; Geiger, B; Heidbrink, WW; Korsholm, SB; Leipold, F; Nielsen, SK; Rasmussen, J; Stejner, M; Thomsen, H; Weiland, M | Abstract:
Plasma Physics and Controlled Fusion | 2015
M. Salewski; B. Geiger; W.W. Heidbrink; A. S. Jacobsen; Søren Bang Korsholm; F. Leipold; Jens Madsen; D. Moseev; S. K. Nielsen; J. Juul Rasmussen; L. Stagner; D Steeghs; M. Stejner; G. Tardini; M. Weiland
Doppler tomography is a well-known method in astrophysics to image the accretion flow, often in the shape of thin discs, in compact binary stars. As accretion discs rotate, all emitted line radiation is Doppler-shifted. In fast-ion D� (FIDA) spectroscopy measurements in magnetically confined plasma, the D�-photons are likewise Doppler-shifted ultimately due to gyration of the fast ions. In either case, spectra of Doppler-shifted line emission are sensitive to the velocity distribution of the emitters. Astrophysical Doppler tomography has lead to images of accretion discs of binaries revealing bright spots, spiral structures, and flow patterns. Fusion plasma Doppler tomography has lead to an image of the fast-ion velocity distribution function in the tokamak ASDEX Upgrade. This image matched numerical simulations very well. Here we discuss achievements of the Doppler tomography approach, its promise and limits, analogies and differences in astrophysical and fusion plasma Doppler tomography, and what can be learned by comparison of these applications.
Review of Scientific Instruments | 2016
S.R. Haskey; B.A. Grierson; K.H. Burrell; C. Chrystal; R. J. Groebner; D. H. Kaplan; N. Pablant; L. Stagner
Recent completion of a thirty two channel main-ion (deuterium) charge exchange recombination spectroscopy (CER) diagnostic on the DIII-D tokamak [J. L. Luxon, Nucl. Fusion 42, 614 (2002)] enables detailed comparisons between impurity and main-ion temperature, density, and toroidal rotation. In a H-mode DIII-D discharge, these new measurement capabilities are used to provide the deuterium density profile, demonstrate the importance of profile alignment between Thomson scattering and CER diagnostics, and aid in determining the electron temperature at the separatrix. Sixteen sightlines cover the core of the plasma and another sixteen are densely packed towards the plasma edge, providing high resolution measurements across the pedestal and steep gradient region in H-mode plasmas. Extracting useful physical quantities such as deuterium density is challenging due to multiple photoemission processes. These challenges are overcome using a detailed fitting model and by forward modeling the photoemission using the FIDASIM code, which implements a comprehensive collisional radiative model.
Nuclear Fusion | 2016
M. Salewski; B. Geiger; A. S. Jacobsen; Per Christian Hansen; W.W. Heidbrink; S. B. Korsholm; F. Leipold; Jens Madsen; D. Moseev; S. K. Nielsen; M. Nocente; T. Odstrcil; J. Juul Rasmussen; L. Stagner; M. Stejner; M. Weiland
Author(s): Salewski, M; Geiger, B; Jacobsen, AS; Hansen, PC; Heidbrink, WW; Korsholm, SB; Leipold, F; Madsen, J; Moseev, D; Nielsen, SK; Nocente, M; Odstrcil, T; Rasmussen, J; Stagner, L; Stejner, M; Weiland, M | Abstract:
Physics of Plasmas | 2017
W.W. Heidbrink; C. S. Collins; M. Podesta; G. J. Kramer; D. C. Pace; C. C. Petty; L. Stagner; M. A. Van Zeeland; R. B. White; Y. B. Zhu
Experiments on the DIII-D tokamak have identified how multiple simultaneous Alfven eigenmodes (AEs) lead to overlapping wave-particle resonances and stochastic fast-ion transport in fusion grade plasmas [C. S. Collins et al., Phys. Rev. Lett. 116, 095001 (2016)]. The behavior results in a sudden increase in fast-ion transport at a threshold that is well above the linear stability threshold for Alfven instability. A novel beam modulation technique [W. W. Heidbrink et al., Nucl. Fusion 56, 112011 (2016)], in conjunction with an array of fast-ion diagnostics, probes the transport by measuring the fast-ion flux in different phase-space volumes. Well above the threshold, simulations that utilize the measured mode amplitudes and structures predict a hollow fast-ion profile that resembles the profile measured by fast-ion Dα spectroscopy; the modelling also successfully reproduces the temporal response of neutral-particle signals to beam modulation. The use of different modulated sources probes the details of pha...
Physics of Plasmas | 2017
L. Stagner; W.W. Heidbrink
Due to the usually complicated and anisotropic nature of the fast-ion distribution function, diagnostic velocity-space weight functions, which indicate the sensitivity of a diagnostic to different fast-ion velocities, are used to facilitate the analysis of experimental data. Additionally, when velocity-space weight functions are discretized, a linear equation relating the fast-ion density and the expected diagnostic signal is formed. In a technique known as velocity-space tomography, many measurements can be combined to create an ill-conditioned system of linear equations that can be solved using various computational methods. However, when velocity-space weight functions (which by definition ignore spatial dependencies) are used, velocity-space tomography is restricted, both by the accuracy of its forward model and also by the availability of spatially overlapping diagnostic measurements. In this work, we extend velocity-space weight functions to a full 6D generalized coordinate system and then show how ...
Review of Scientific Instruments | 2018
S. R. Haskey; B.A. Grierson; L. Stagner; C. Chrystal; Arash Ashourvan; A. Bortolon; M. D. Boyer; K.H. Burrell; C. Collins; R. J. Groebner; D. H. Kaplan; N. Pablant
Main-ion charge exchange recombination spectroscopy (MICER) uses the neutral beam induced D α spectrum to measure the local deuterium ion (D+) temperature, rotation, and density, as well as parameters related to the neutral beams, fast ions, and magnetic field. An edge MICER system consisting of 16 densely packed chords was recently installed on DIII-D, extending the MICER technique from the core to the pedestal and steep gradient region of H-mode plasmas where the D+ and commonly measured impurity ion properties can differ significantly. A combination of iterative collisional radiative modeling techniques and greatly accelerated spectral fitting allowed the extension of this diagnostic technique to the plasma edge where the steep gradients introduce significant diagnostic challenges. The importance of including the fast ion D α emission in the fit to the spectrum for the edge system is investigated showing that it is typically not important except for cases which can have significant fast ion fractions near the plasma edge such as QH-mode. Example profiles from an Ohmic L-mode and a high power ITER baseline case show large differences in the toroidal rotation of the two species near the separatrix including a strong co-current D+ edge rotation. The measurements and analysis demonstrate the state of the art in active spectroscopy and integrated modeling for diagnosing fusion plasmas and the importance of direct main ion measurements.
Review of Scientific Instruments | 2018
G. Z. Hao; W.W. Heidbrink; D. Liu; L. Stagner; M. Podesta; A. Bortolon
Analysis of fast-ion D-alpha (FIDA) data on National Spherical Torus Experiment-Upgrade (NSTX-U) shows that the cold Dα line contaminates the FIDA baseline. The scattered light is comparable to the FIDA emission. A scattering correction is required to extract the FIDA signal. Two methods that relate the scattered light contamination to the intensity of the cold Dα line are employed. One method uses laboratory measurements with a calibration lamp; the other method uses data acquired during plasma operation and singular value decomposition analysis. After correction, both the FIDA spectra and spatial profile are in better agreement with theoretical predictions.
Plasma Physics and Controlled Fusion | 2014
W.W. Heidbrink; J.R. Ferron; C.T. Holcomb; M. A. Van Zeeland; Xi Chen; C. Collins; A. M. Garofalo; X.Z. Gong; B.A. Grierson; M. Podesta; L. Stagner; Y. B. Zhu