This paper presents the first observations of coherent beam ion losses due to plasma waves in the DIII-D tokamak. The actual measurement is the flux of beam ions that hit a probe located at the outer wall. That diagnostic, the Fast Ion Loss Detector (FILD), was built as part of a collaboration with the ASDEX Upgrade tokamak. The FILD system is a great addition to the diagnostic suite available at DIII-D because it measures the energy and pitch angle of large gyroradius ions that hit it. Identifying the types of plasma waves that kick ions out of the plasma is valuable for designing operational scenarios for larger fusion reactors such as ITER.
Physics aside, what I remember most about publishing this paper is that the referees demanded a lot of extra material! If you view the Version of Record (i.e., the journal’s official version), you will notice that this is a “Brief Communication” type of paper. A Brief Communication was meant to serve for papers that reported really neat results in a rapid manner. Those papers were usually short, because they mostly wanted to announce the result, and they went through the review process quickly. The journal appears to have replaced the Brief Communication with a similarly-focused paper type called “Notes.”
Our first submission reported on the measurement of beam ion losses due to the presence of a particular plasma wave (see the RSAE below) that had never previously been observed. Our thinking was that we had a neat result and it was new, so let’s report it and try to get more theorists interested in helping to explain what it means. That presentation did not fly with the referees. They at least liked the idea of the paper and thought it was of interest to the research community, but they wanted a lot more detail and even an explanation for how the wave was kicking ions out of the plasma. All of these requests (demands?) were reasonable, so we revised the paper appropriately and the final result is a Brief Communication that is 12 pages long and has 9 figures! You cannot change the paper type after beginning the review process, so to publish this as a regular article we would have had to withdraw the Brief Communication and submit it all over again as a regular article.
In the end, we have a “brief” article that is not so brief, but that allowed us to describe an important physics mechanism thanks to the addition of Figure 7.
The following article appears in Plasma Physics and Controlled Fusion as,
D.C. Pace, R.K. Fisher, M García-Muñoz, W.W. Heidbrink, and M A Van Zeeland, Plasma Phys. Control. Fusion 53, 062001 (2011).
You can download the Accepted Manuscript (PDF, 1.5 MB).
Convective beam ion losses due to Alfvén eigenmodes in DIII-D reversed-shear plasmas
Abstract
Coherent losses of neutral beam ions are observed at frequencies corresponding to toroidal and reversed-shear Alfvén eigenmodes (RSAEs) in DIII-D. Reversed-shear profiles are created by injecting beam power during the plasma current ramp. Beam ion losses stemming from Alfvén eigenmode activity contribute to flattening of the energetic ion density profile in such discharges. This is the first observation of convective beam ion losses due to RSAEs. The energies and pitch angles of lost ions are measured and found to exist within a well-defined region of phase space. Loss flux signals decrease in time as current penetrates and Alfvén eigenmode activity becomes more core localized. Preliminary Monte Carlo simulations of energetic ion interactions with measured mode structures show the dominant loss mechanism is a transition from a counter-passing orbit to a trapped orbit that is lost to the wall.
1. Introduction
Energetic ion transport is an active area of interest for magnetically confined fusion research with particular relevance to ITER [1]. Fusion produced alpha particles will excite a spectrum of Alfvén eigenmodes (AEs) [2] in ITER that may, in turn, affect alpha confinement on time scales shorter than a slowing-down time. The resulting increase in alpha transport may reduce the self-heating ability of reactors, which would also reduce net energy gain.
Energetic ions are capable of experiencing radial transport from interactions with toroidal Alfvén eigenmodes (TAEs) [3, 4] and reversed-shear Alfvén eigenmodes (RSAEs) [5, 6]. In experiments, energetic ion sources include neutral beam injection and ion cyclotron resonance heating (ICRH). The first TAE experiments inferred losses of beam ions from drops in neutron emission [7, 8]. Measurements of direct losses to the walls were obtained shortly thereafter [9, 10]. Losses of ICRH tail ions due to TAEs were first measured by a neutral-particle analyzer [11] and by a poloidal array of scintillators [12]; the latter work also studied beam ion losses. More recently, coherent oscillations of escaping ICRH tail ions at TAE frequencies have been observed [13]. For RSAEs, suppressed neutron rates during neutral beam injection correlate with mode activity [14, 15]. Coherent oscillations of escaping ICRH tail ions at RSAE frequencies have also been observed [16]. In plasmas that produced RSAEs using neutral beam injection only, however, no coherent beam ion losses at RSAE frequencies were observed [17]. That work found RSAEs contributed to beam ion redistribution in the core and likely increased the ability of TAEs to produce direct losses.
A series of experiments investigating AE-induced transport of neutral beam injected ions has been conducted on the DIII-D tokamak [18, 19]. The core energetic ion density profile is observed to flatten in the presence of AE activity [20, 21]. A new fast ion loss detector (FILD) [22] has since been commissioned to measure the energy and pitch angle of energetic ions lost to its position on the wall. In reversed-shear plasmas similar to those of the earlier experiments, FILD measurements demonstrate losses at TAE and RSAE frequencies. This result helps us to explain the previously observed energetic ion profile flattening. Furthermore, these results represent the first direct measurement of beam ion losses at RSAE frequencies.
The organization of this paper is as follows. In section 2 the experimental setup and diagnostics are presented. Focus is placed on the energy and pitch angle measurement of beam ions reaching a detector at the wall. Section 3 presents the observations of beam ion losses coherent with Alfvénic activity. Conclusions are presented in section 4, where implications for future energetic ion transport studies are discussed.
2. Diagnostics and plasma parameters
The energetic ion population in DIII-D (typical parameters of BT = 2.1 T, R = 1.66 m and a = 0.67 m) is produced by neutral beam injection from up to eight sources providing 2.5 MW injected power each. The geometry of these beams is shown in figure 1. The beams are located at four different toroidal positions (φ = 30◦, 150◦, 210◦ and 330◦), with each unit housing a tangential (tangency radius Rtan = 1.15 m) and a perpendicular (Rtan = 0.74 m) injection line. Injection paths corresponding to each source are labeled in the figure according to whether they are the left or right source in the housing. The firing pattern of these beams determines the instantaneous pitch angle range (χ = v∥/v) of the energetic ion distribution. Additional variability is available from the 210◦ beam that injects counter to the standard plasma current direction shown in figure 1 (χ < 0). The behavior and confinement of the beams is well understood experimentally [23] and is modeled by the NUBEAM [24, 25] module of TRANSP [26] to calculate heating and other parameters of interest.
A collection of diagnostics used in this research is also shown in figure 1. Radial profiles of energetic ion density and information concerning the distribution is measured by the vertical fast ion Dα (FIDA) [27] system that views the 330◦-L neutral beam. This diagnostic measures Doppler shifted light emitted by energetic ions that charge exchange with beam injected neutrals. A neutron detection system [28] located at φ = 105◦ just outside of the vacuum vessel measures 2.45 MeV neutrons produced by DD fusion. While the FIDA and neutron diagnostics measure parameters related to the core confinement of beam ions, the scintillator based FILD measures energetic ion fluxes reaching its position on the wall as a function of pitch angle and energy. The scintillator is covered by a graphite head with a collimating aperture. Ions passing through the aperture strike the scintillator at a position determined according to their energy (gyroradius) and pitch angle. Scintillator light passes through an optical train and out of the probe shaft where it is split between a slow charge-coupled device (CCD) camera sampled at 160 Hz and a fast photomultiplier tube (PMT) sampled at 1 MHz. Figure 2 demonstrates the important features of the FILD. Figure 2(a) displays the poloidal cross-section from shot 142111 (BT = 2.05 T, R = 1.71 m, a = 0.62 m, inner wall limited) at t = 570 ms. The FILD is located at a position approximately 45◦ below the outer midplane and the aperture is marked in figure 2 by the × at [R, z] = [2.2, −0.7] m. Full orbit paths for ions of pitch angle α = cos−1(χ) = 35◦, 55◦ and 75◦ are plotted. All three ion orbits are detectable by the FILD and feature energy E = 80 keV. In figure 2(b) a schematic of the FILD highlights important operational features. An example ion orbit is shown passing through the aperture and striking the scintillator surface. The wide opening in the figure is the cutout of the graphite shield, while the collimating aperture is an Inconel slit inside of this shield that is <1 mm wide in the direction that resolves the gyroradius. Figure 2(c) is a partially three-dimensional view of a narrow region near the probe head. The FILD graphite head is labeled and the orbits from figure 2(a) intersect at the position of the aperture (which is drawn oversize for clarity). The FILD features a linear translator that allows adjustment of its radial position. The edge of the graphite head is typically placed more than 10 cm away from the last closed flux surface to minimize heat load that may lead to carbon impurity contributions.
In the results presented here, AEs are excited by neutral beam injection during the plasma current ramp [29]. Figure 3 displays the evolution of plasma parameters in shot 142111. A total of 7.1 MW of neutral beam power is injected during the current ramp as shown in figure 3(a). Electron density is plotted in figure 3(b), where it is observed to rise quickly when neutral beam injection begins. Indicators of energetic ion confinement are shown in figure 3(c). The FIDA density points are proportional to the energetic ion density [30] along the viewing chord at R = 1.80 m. The neutron rate is dominated by the beam-plasma production term and therefore represents beam ion confinement. In figure 3(c) these data are normalized to the classically expected values from TRANSP as developed in [20]. Both parameters are observed at values well below the expectation from classical transport alone, indicating the presence of an additional energetic ion transport mechanism.
3. Observed beam ion losses
A false color FILD camera frame from shot 142111 at t = 525 ms is shown in figure 4 labeling two regions of measured losses. Energetic ion losses measured by the FILD during this experiment include contributions from the convectively driven flux due to Alfvén eigenmodes and also from neutral beam prompt losses. Beam prompt losses occur when an injected neutral ionizes such that its first complete poloidal transit intersects the wall. Figure 4 shows prompt losses over the pitch angle range . The uncertainty in pitch angle is a combination of the intrinsic resolution of the diagnostic as calculated by the Monte Carlo strike map code EfipDesign [31], and an additional contribution due to vibration of the initially installed optics platform. The three individual ‘spots’ of loss within this pitch angle range are centered on and cm and correspond to the full, one-half and one-third energy injection of the 210◦-L source beam, respectively. Prompt losses are used to validate FILD operation and are modeled considering the three-dimensional geometry between the beams and the diagnostic [32].
By adjusting the zoom lens that focuses scintillator light onto the PMT-connected fiber optic it is possible to focus the PMT view onto a narrower region of the scintillator. During shot 142111 the PMT view is focused onto a region dominated by light from . The wings of this view do incorporate some light from the region where α > 60◦. Figure 5(a) displays neutral beam power reaching the limiters, , which is a measure of prompt losses as calculated by TRANSP. The prompt loss flux is reduced as the plasma current rises and banana orbit widths decrease. The firing patterns of the counter-injected neutral beams that produce FILD-observed prompt losses are indicated by rectangles below the trace. The 210◦-L beam is on continuously from ms (solid rectangle) while the 210◦-R beam fires in 10 ms wide pulses represented by the slender rectangles. The FILD PMT signal during this time is shown in figure 5(b). Over this wide time range only large scale changes due to prompt losses are discernible. The 210◦-L produces a slowly varying loss (signal level ≈1 V in figure 5(b)). Orbit modeling shows that the prompt loss contribution from the 210◦-R beam reaches the FILD in the 40◦–50◦ pitch angle range at low plasma current and moves closer to the midplane (where it is no longer detectable by the FILD) as the current increases. For early times, modulation of the PMT signal is dominated by pulses of the 210◦-R beam. This behavior confirms the expected viewing range set by the PMT zoom lens. The vertical dashed line of figures 5(a) and (b) marks the camera exposure of figure 4 showing that the 210◦-R beam is off and prompt losses do not contribute to the loss region.
The region of losses shown in figure 4 occurring over is identified as losses due to AEs. The raw PMT trace acquired over the exposure time of the camera frame is plotted in figure 5(c). Coherent oscillations with a period of T ≈ 12–17 μs (f ≈ 60–85 kHz) are observed (perhaps most clearly near t = 525.1 ms) and found to be consistent with AE frequencies. These losses occur at rL ≈ 3.5 cm, corresponding to ions of E ≈ 75 keV given the amplitude of the magnetic field at the FILD, T. The exposure time of the camera is 500 μs, which is short enough that a nearly constant set of AE frequencies is observed.
Power spectra demonstrating the presence of Alfvén eigenmodes and coherent energetic ion losses are shown in figure 6. Figure 6(a) displays the cross power between a line-integrated electron density measurement from a laser interferometer [33] and a -coil [34]. The activity occurring between approximately 50 and 100kHz is a collection of toroidal and RSAEs. Figure 6(b) is an autopower spectrogram from the FILD PMT demonstrating coherent losses in the RSAE and TAE frequency ranges. The dashed vertical arrow marks the time slice of the FILD camera frame in figure 4. The FILD spectrum shows that loss activity decreases steadily in time and is nearly zero by t = 800 ms. Figure 6(a) further shows that the core Alfvén eigenmode spectrum transitions from mostly TAEs at early times to nearly all RSAEs after 600 ms. The AE activity is becoming more core localized as plasma current increases, while particle loss boundaries are moving outward, thereby reducing the ability of AEs to place beam ions directly onto loss orbits (i.e. convective losses decrease [16]). Loss boundaries at t ≈ 525 ms and t ≈ 725 ms for ions of 80 keV energy in shot 142111 are shown in figures 7(a) and (b), respectively. These phase space contours describe orbits as a function of major radius position along the outer midplane. A dashed white line marks the innermost position for which loss orbits exist. During the earlier time shown in figure 7(a), the position of qmin (a proxy for AE location) is further out than the loss boundary and it is expected that convective AE-induced losses are more easily produced. For the later time shown in figure 7(b), qmin is inside of the loss boundary and convective losses are expected to decrease.
In addition to the Alfvén-induced loss activity above 60 kHz, the FILD spectrogram of figure 6(b) also displays coherent activity at lower frequencies. Prior to t = 400 ms there are losses at f ≈ 15 kHz, and a second and third harmonic, that are coherent with an observed energetic particle induced geodesic acoustic mode (EGAM) [35, 36]. The ion/EGAM interaction that leads to these losses is presently under investigation. Other apparent bursts of low frequency losses that extend down to zero frequency (e.g. appearing just before and after t = 400 ms) are artifacts due to the square-wave like prompt loss flux from individual pulses of the 210◦-R beam.
Spectrograms from a narrow time region, ms, when the RSAE losses are prominent, are shown in figure 8. The FILD spectrum of figure 8(a) displays the largest fluctuations due to RSAE losses in a 60–70 kHz band passing through 480 ms. The contour lines overlaid on this FILD spectrogram represent a single level from the interferometer phase spectrogram shown in figure 8(b). This interferometer data comes from a single chord passing through the plasma along the horizontal midplane. While there is little sign of TAEs in the interferometer spectra, these modes do still appear in the FILD spectra (e.g. the three nearly constant frequency features at 500 ms). A comparison between panels 8(a) and (b) shows that there are many instances in which an RSAE identified in the interferometer data does not produce FILD measured beam ion losses. It remains to be determined whether losses are being produced in another region of phase space for which there is no PMT view, or whether such losses may simply reach a different position on the outer wall of vessel. Future work adding more PMT views addresses the first point, while a new FILD installed just below the outer midplane will address the second.
A preliminary investigation of the interaction between beam ions and the excited AEs is conducted by way of simulation. The plasma equilibrium and Alfvén wave fields are provided as input to the Hamiltonian guiding center code ORBIT [37], which then calculates the resulting path of beam ions due to these modes. The full poloidal structure of the wave fields is calculated by NOVA-K [38] using the radial eigenmode profile from temperature fluctuations measured by an electron cyclotron emission diagnostic [39]. Resonance between the ions and the modes is achieved when [2, 40] ω = nωφ − (m + l)ωθ , where ω is the Alfvén eigenmode frequency, n (m) is the toroidal (poloidal) mode number, l is a quantum number and ωφ (ωθ) is the ion’s toroidal (poloidal) precession frequency. The simulation employs a Monte Carlo method in which a number of beam injected particles are tracked. Each ion’s initial properties (e.g. deposition position, energy, and pitch angle) are determined from NUBEAM modeling. The coordinate system in ORBIT is defined by flux surfaces and does not extend beyond the separatrix, meaning that simulated ions are defined to be lost when they reach the separatrix. This class of particles does not necessarily represent ions that are lost to the wall. To extend the applicability of ORBIT simulations to losses, a gyrocenter orbit code that works in real space has been incorporated. The implementation takes the properties of ORBIT ions at the position where they intersect the separatrix and uses that information to compute a gyrocenter orbit across a full poloidal transit. If this ion trajectory intersects the wall, then the ion is recorded as lost.
Figure 9 presents an example of the simulation result. The solid line is an ORBIT calculated gyrocenter trajectory of an ion with E = 75 keV and χ = 0.66 (pitch at the FILD, though the ion begins on a counter-current passing orbit) as simulated by ORBIT in the presence of a spectrum of AEs. The total time elapsed along this trajectory is t < 400 μs, demonstrating that the transport process may be studied in a fixed equilibrium. Interaction between the ion and the AEs results primarily in the reduction in the ion’s toroidal canonical momentum (δPφ /Pφ ≈ 14%). Ion energy changes much less (δE/E ≈ 2%), which is expected since the observed losses occur at energies corresponding to the full neutral beam energy. The dashed line connecting to the ORBIT evolved path represents the separately calculated wall-strike path using the properties of the ion at its intersection with the separatrix. This part of the trajectory intersects a small rectangle encompassing the FILD aperture (×). The rectangle defines the simulated FILD region: any ion that passes through this region is considered a FILD-detectable ion. The properties of this simulated ion are consistent with FILD measurements. Details of this work and the comparison between measured and simulated losses are given in [41].
4. Conclusion
In summary, convective losses of beam ions due to Alfvén eigenmode activity have been measured with a scintillator detector in reversed-shear DIII-D plasmas. These observations indicate the AE-induced losses likely contributed to the previously observed flattening of the energetic ion density profile [20, 21]. The first observations of beam ion losses coherent with RSAEs are also presented. Other experiments have shown that ICRH tail ions can be directly expelled by RSAEs [16], and that energetic ion losses increase in situations where RSAE existence regions overlap with TAE regions [14, 16]. The present results demonstrate that the energetic ion distribution produced in ICRH plasmas is not a requirement to satisfy the relevant resonance condition for convective RSAE losses. One suggestion to reduce RSAE-influenced losses is to operate with equilibria that place qmin outside the range in which RSAEs are able to transition to TAEs [14]. The results presented here suggest that a general emphasis should be placed on keeping qmin and AE radial extent inside of the energetic ion loss boundary. Simulation of beam ion interactions with a spectrum of AEs illustrates a possible trajectory evolution from a confined passing ion to a FILD-detectable loss on a large banana orbit. Future work should perform simulations using a larger number of Monte Carlo particles with the aim of providing adequate statistics in the perturbation field of a single RSAE. Given that RSAEs can be excited due to the equilibrium perturbation of sawtooth crashes [42], it is important to consider that they may be capable of contributing to the energetic ion transport observed in sawtoothing plasmas [43, 44]. Ongoing investigations of sawtooth-induced transport [45, 46] will be able to incorporate energetic ion loss measurements and core transport measurements simultaneously.
Acknowledgments
This work is supported by the US Department of Energy under DE-AC05-06ER23100, SC-G903402 and DE-FC02-04ER54698. The authors gratefully acknowledge helpful discussions with Y B Zhu, D S Darrow and C M Muscatello. In addition, the authors would like to thank the DIII-D team for their expertise in commissioning the FILD and their support of these experiments.
References
[1] Fasoli A et al 2007 Nucl. Fusion 47 S264
[2] Heidbrink W W 2008 Phys. Plasmas 15 055501
[3] Cheng C Z and Chance M S 1986 Phys. Fluids 29 3695
[4] Cheng C Z, Chen L and Chance M S 1985 Ann. Phys. 161 21
[5] Berk H L et al 2001 Phys. Rev. Lett. 87 185002
[6] Sharapov S E et al 2002 Phys. Plasmas 9 2027
[7] Wong K L et al 1991 Phys. Rev. Lett. 66 1874
[8] Heidbrink W W et al 1991 Nucl. Fusion 31 1635
[9] Duong H H et al 1993 Nucl. Fusion 33 749
[10] Darrow D S et al., 1992 Proc. 19th European Conf. on Plasma Physics and Controlled Fusion (Innsbruck, Austria)
[11] Ali-Arshad S and Campbell D J 1995 Plasma Phys. Control. Fusion 37 715
[12] Darrow D S et al 1997 Nucl. Fusion 37 939
[13] Garcia-Munoz M et al 2008 Phys. Rev. Lett. 100 055005
[14] Takechi M et al 2005 Phys. Plasmas 12 082509
[15] Van Zeeland M A et al 2008 Plasma Phys. Control. Fusion 50 035009
[16] Garcia-Munoz M et al 2010 Phys. Rev. Lett. 104 185002
[17] Garcia-Munoz M et al 2010 Proc. 23rd IAEA Fusion Energy Conference (Daejon, Korea) EXW/P7-07
[18] Luxon JL 2002 Nucl. Fusion 42 614
[19] Strait EJ 2009 Nucl. Fusion 49 104008
[20] Heidbrink WW et al 2007 Phys. Rev. Lett. 99 245002
[21] Heidbrink WW et al 2008 Nucl. Fusion 48 084001
[22] Fisher RK et al 2010 Rev. Sci. Instrum. 81 10D307
[23] Heidbrink WW et al 2009 Plasma Phys. Control. Fusion 51 125001
[24] Goldston RJ et al 1981 J. Comput. Phys. 43 61
[25] Pankin A et al 2004 Comput. Phys. Commun. 159 157
[26] See http://w3.pppl.gov/transp, the official homepage of TRANSP, for information concerning the models and methods employed, in addition to usage documentation
[27] Luo Y et al 2007 Rev. Sci. Instrum. 78 033505
[28] Heidbrink WW, Taylor PL and Phillips JA 1997 Rev. Sci. Instrum. 68 536
[29] Van Zeeland M A et al 2006 Phys. Rev. Lett. 97 135001
[30] Heidbrink WW et al 2004 Plasma Phys. Control. Fusion 46 1855
[31] Werner A et al 2001 Rev. Sci. Instrum. 72 780
[32] Pace DC et al 2010 Rev. Sci. Instrum. 81 10D305
[33] Van Zeeland M A et al 2006 Rev. Sci. Instrum. 77 10F325
[34] Strait EJ 2006 Rev. Sci. Instrum. 77 023502
[35] Nazikian R et al 2008 Phys. Rev. Lett. 101 185001
[36] Fu GY 2008 Phys. Rev. Lett. 101 185002
[37] White R B and Chance M S 1984 Phys. Fluids 27 2455
[38] Cheng CZ 1992 Phys. Rep. 211 1
[39] Austin M E and Lohr J 2003 Rev. Sci. Instrum. 74 1457
[40] Todo Y and Sato T 1998 Phys. Plasmas 5 1321
[41] Van Zeeland M A et al 2011 Measurements and modeling of Alfvén eigenmode induced fast ion transport and loss in DIII-D and ASDEX Upgrade Phys. Plasmas at press
[42] Edlund EM et al 2009 Phys. Rev. Lett. 102 165003
[43] Sadler GJ et al 1990 Fusion Technol.18 556
[44] Fisher RK et al 1995 Phys. Rev. Lett. 75 846
[45] Nielsen SK et al 2010 Plasma Phys. Control. Fusion 52 092001
[46] Van Zeeland M A et al 2010 Nucl. Fusion 50 084002
Leave a Reply