<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">JHEPGC</journal-id><journal-title-group><journal-title>Journal of High Energy Physics, Gravitation and Cosmology</journal-title></journal-title-group><issn pub-type="epub">2380-4327</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jhepgc.2019.51007</article-id><article-id pub-id-type="publisher-id">JHEPGC-89241</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Mitigation of ELMs by Electrostatic Field in Tokamaks
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Zhongtian</surname><given-names>Wang</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Xiaochang</surname><given-names>Chen</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Yifan</surname><given-names>Yan</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Huidong</surname><given-names>Li</given-names></name><xref ref-type="aff" rid="aff3"><sup>3</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Qian</surname><given-names>Liu</given-names></name><xref ref-type="aff" rid="aff4"><sup>4</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Maolin</surname><given-names>Mou</given-names></name><xref ref-type="aff" rid="aff5"><sup>5</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Na</surname><given-names>Wu</given-names></name><xref ref-type="aff" rid="aff5"><sup>5</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Zhanhui</surname><given-names>Wang</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Rui</surname><given-names>Ke</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Lin</surname><given-names>Nie</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Ming</surname><given-names>Xu</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Southwestern Institute of Physics, Chengdu, China</addr-line></aff><aff id="aff5"><addr-line>College of Physical Science and Technology, Sichuan University, Chengdu, China</addr-line></aff><aff id="aff4"><addr-line>Department of Engineering Physics, Tsinghua University, Beijing, China</addr-line></aff><aff id="aff1"><addr-line>School of Sciences, Nanchang University, Nanchang, China</addr-line></aff><aff id="aff3"><addr-line>School of Science, Xihua University, Chengdu, China</addr-line></aff><pub-date pub-type="epub"><day>15</day><month>11</month><year>2018</year></pub-date><volume>05</volume><issue>01</issue><fpage>149</fpage><lpage>155</lpage><history><date date-type="received"><day>25,</day>	<month>September</month>	<year>2018</year></date><date date-type="rev-recd"><day>17,</day>	<month>December</month>	<year>2018</year>	</date><date date-type="accepted"><day>20,</day>	<month>December</month>	<year>2018</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  Mitigation of ELMs by electrostatic field is studied. The perpendicular heating in cyclotron waves tends to pile up the resonant particles toward the low magnetic field side in which a electrostatic field may result [J. Y. Hsu, V. S. Chan, R. W. Harvey, R. Prater, and S. K. Wong, Phys. Rev. Lett. 53, 564 (1984)]. The electrostatic field can make circulating particles trapped or make trapped particles circulating depending on the field direction. The trapped- particle population and bootstrap current change accordantly. Modulating bootstrap current, mitigation of type-1 ELM by the electrostatic field is possible. The electrostatic potential needed for the mitigation is quantitatively estimated. Experiments by either ECRH or biasing are being prepared to verify the theory.
 
</p></abstract><kwd-group><kwd>Electrostatic Trapping</kwd><kwd> Bootstrap Current</kwd><kwd> Mitigation</kwd><kwd> Peeling-Ballooning Mode</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>In present tokamaks operating in high-confinement regimes (H-modes), the steep pressure gradients at edge are often observed to relax through frequent intermittent discharges of energy, known as ELMs. The physics of ELMs is a key issue for ITER operation. The onset of ELMs constrains the pressure at top of edge transport barrier (pedestal height). The ELMs events transport substantial heat and particle loads to plasma-facing materials. A predictive understanding of the onset of type-I ELMs has been gained via the development of peeling-ballooning modes [<xref ref-type="bibr" rid="scirp.89241-ref1">1</xref>] in which EL Ms are triggered by instabilities driven by the large pressure gradient and bootstrap current in the edge. High pressure is important for fusion efficiency. The bootstrap current can be changed.</p><p>The perpendicular heating in cyclotron waves tends to pile up the resonant particles toward the low magnetic field side. An electrostatic field may result [<xref ref-type="bibr" rid="scirp.89241-ref2">2</xref>] . Variations of the electrostatic potential at plasma edge are observed in HL -2A [<xref ref-type="bibr" rid="scirp.89241-ref3">3</xref>] . Full particle simulation is performed using the Boris algorithm [<xref ref-type="bibr" rid="scirp.89241-ref4">4</xref>] . The electrostatic field can make circulating particles trapped or make trapped particles circulating depending on the field direction. With the assumption neoclassical transport the population of the trapped particles and bootstrap current change accordantly. Modulating bootstrao current by changing the electrostatic field, mitigation of type-1 ELM is possible. The electrostatic potential needed for the mitigation is quantitatively calculated. Experiments by either ECRH or biasing [<xref ref-type="bibr" rid="scirp.89241-ref5">5</xref>] are being prepared to verify the theory.</p></sec><sec id="s2"><title>2. Full Particle Orbit Simulation in Tokamaks</title><p>In particle simulations of magnetized plasmas, the Boris algorithm [<xref ref-type="bibr" rid="scirp.89241-ref4">4</xref>] is the standard for advancing a charged particle in an electromagnetic field in accordance with the equation of motion associated with the Lorentz force,</p><disp-formula id="scirp.89241-formula5"><label>(1)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/7-2180325x2.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.89241-formula6"><label>(2)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/7-2180325x3.png"  xlink:type="simple"/></disp-formula><p>where the magnetic field and electric field are given respectively by</p><disp-formula id="scirp.89241-formula7"><label>(3)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/7-2180325x4.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.89241-formula8"><label>(4)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/7-2180325x5.png"  xlink:type="simple"/></disp-formula><p>where Ψ is the poloidal magnetic flux, Φ = E R 0 ( R 0 R − 1 ) is the electrostatic potential. We proceed from Solov’ev solution</p><disp-formula id="scirp.89241-formula9"><label>(5)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/7-2180325x8.png"  xlink:type="simple"/></disp-formula><p>where Ψ 0 = j φ μ 0 e 2 R 0 ( 1 + e 2 ) , e is elongation, Q is related to tri-angularity.</p><p>We use ITER’s parameters:<inline-formula><inline-graphic xlink:href="/html.scirp.org/file/7-2180325x10.png" xlink:type="simple"/></inline-formula>, e = 1.7 , Q = 0.33 , toroidal current I = 15   MA , aspect ratio A = 3.1 . So the tokamak magnetic field is well-determined. Full orbit simulations find electric trapping and de-trapping seen in <xref ref-type="fig" rid="fig1">Figure 1</xref> and <xref ref-type="fig" rid="fig2">Figure 2</xref> respectively.</p><p>Full particle orbit simulation is suitable to a multi-scale problem. The Boris algorithm [<xref ref-type="bibr" rid="scirp.89241-ref4">4</xref>] makes simulation in the long time simulation accurate.</p></sec><sec id="s3"><title>3. Bootstrap Current</title><p>The gyro-averaged Hamiltonian has been given in Ref. [<xref ref-type="bibr" rid="scirp.89241-ref6">6</xref>] ,</p><disp-formula id="scirp.89241-formula10"><label>(6)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/7-2180325x17.png"  xlink:type="simple"/></disp-formula><p>where the momenta</p><disp-formula id="scirp.89241-formula11"><label>(7)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/7-2180325x18.png"  xlink:type="simple"/></disp-formula><p>p φ = R v φ − e Ψ (8)</p><disp-formula id="scirp.89241-formula12"><label>(9)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/7-2180325x20.png"  xlink:type="simple"/></disp-formula><p>are conjugate to α , the gyrophase, φ, the toroidal angle, and x, expressed as</p><disp-formula id="scirp.89241-formula13"><label>(10)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/7-2180325x22.png"  xlink:type="simple"/></disp-formula><p>where R and Z are the coordinates of the guiding center in a cylindrical system, ρ is the Larmor radius, Ω is the toroidal gyro-frequency. The particle mass is taken to be unity for simplicity. The electrostatic potential is assumed in a form,</p><disp-formula id="scirp.89241-formula14"><label>(11)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/7-2180325x23.png"  xlink:type="simple"/></disp-formula><p>which is like the dipole potential produced by two close-point-charges, where ε is the inverse aspect ratio.</p><p>From Equation (6) we have</p><disp-formula id="scirp.89241-formula15"><label>(12)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/7-2180325x25.png"  xlink:type="simple"/></disp-formula><p>where H &#175; = H + e E R 0 , 1 2 v ⊥ 0 2 = ( Ω 0 P α + e E R 0 ) . For the large aspect-ratio approximation we have,</p><disp-formula id="scirp.89241-formula16"><label>(13)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/7-2180325x28.png"  xlink:type="simple"/></disp-formula><p>where k = 2 ε v ⊥ 0 2 v ϕ 0 2 . For the trapped particles v ϕ max 2 = 2 ε v ⊥ 0 2 and the bounce frequency is</p><disp-formula id="scirp.89241-formula17"><label>(14)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/7-2180325x31.png"  xlink:type="simple"/></disp-formula><p>The ions with v ϕ 0 2 2 ε ≤ e R 0 E are trapped, however, they are circulating without the electrostatic field. That is electrostatic trapping. For electrons the trapping condition is</p><disp-formula id="scirp.89241-formula18"><label>(15)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/7-2180325x33.png"  xlink:type="simple"/></disp-formula><p>There is minimum of ( Ω 0 P α ) min = v ϕ 0 2 2 + e E R 0 for trapping. If equilibrium distribution-function is Maxwellian it is easy to calculate trapped-electron population. The fraction of trapped electrons is Fraction = 2 ε e − e E R 0 T . Comparing with neoclassical transport [<xref ref-type="bibr" rid="scirp.89241-ref7">7</xref>] which increase by a factor e − e E R 0 T . And the bootstrap current changes accordantly [<xref ref-type="bibr" rid="scirp.89241-ref8">8</xref>] ,</p><disp-formula id="scirp.89241-formula19"><label>(16)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/7-2180325x37.png"  xlink:type="simple"/></disp-formula><p>where B p is the poloidal magnetic field, n is the density, T is plasma temperature, L n is the density scale length. The gradients in the electron profiles contribute to typically 70% - 90% of the total bootstrap current [<xref ref-type="bibr" rid="scirp.89241-ref9">9</xref>] .</p></sec><sec id="s4"><title>4. Peeling-Ballooning Modes</title><p>The criterion of peeling-ballooning modes can be expressed by the following formula [<xref ref-type="bibr" rid="scirp.89241-ref10">10</xref>] ,</p><disp-formula id="scirp.89241-formula20"><label>(17)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/7-2180325x40.png"  xlink:type="simple"/></disp-formula><p>where D m is the Mercier coefficient, D m &lt; 1 / 4 is the Mercier stability criterion, finite (positive) bootstrap current, j ∥ , is destabilizing and q ′ is the derivative of the safety factor with respect to the poloidal magnetic flux. At pedestal the temperature is low, therefore, from Equation (16) bootstrap current is sensitive to the electrostatic potential.</p><p>Now we use Equation (17) to calculate the criterion. For a large aspect ratio and low β ordering Equation (17) can be written [<xref ref-type="bibr" rid="scirp.89241-ref1">1</xref>]</p><p>D R &lt; − R q s ( j | | B ) e d g e (18)</p><p>where D R = 3 R s 2 B 2 d P d r e ( r R − 2 δ ) and e is the elongation [<xref ref-type="bibr" rid="scirp.89241-ref11">11</xref>] . We neglect triangularity, δ , then Equation (17) becomes</p><p>e E R 0 T &gt; ln ( ( s q 2 3 e 2 ε 3 ) (19)</p><p>If s = 0.2 , q = 2 , e = 2 , ε = 0.3 we have the criterion for stability</p><p>e E R 0 T &gt; 0.136 (20)</p><p>which can be produced in the practical experiments [<xref ref-type="bibr" rid="scirp.89241-ref5">5</xref>] .</p><p>Electrostatic field, hopefully, can realize ELM-control like that in Ref. [<xref ref-type="bibr" rid="scirp.89241-ref12">12</xref>] and show synchronization of the ELM cycle with added electrostatic field. Electrostatic field, hopefully, can realize ELM-ree discharge which appears in I-mode of Alcator C-mod [<xref ref-type="bibr" rid="scirp.89241-ref13">13</xref>] .</p></sec><sec id="s5"><title>5. Summary</title><p>Full particle simulation is suitable to a multi-scale problem. The Boris algorithm makes long-time simulation accurate. The perpendicular heating in cyclotron waves tends to pile up the resonant particles toward the low magnetic field side in which electrostatic field may result [<xref ref-type="bibr" rid="scirp.89241-ref2">2</xref>] . The electrostatic field can make circulating particles trapped or make trapped particles circulating depending on the field direction. The trapped-particle population and bootstrap current change accordingly in the process. Modulating bootstrap current, mitigation of type-1 ELM or ELM-free discharge is possible. Experiments by either ECRH or biasing [<xref ref-type="bibr" rid="scirp.89241-ref5">5</xref>] are being prepared to verify the theory in HL -2A Tokamak [<xref ref-type="bibr" rid="scirp.89241-ref14">14</xref>] .</p></sec><sec id="s6"><title>Acknowledgements</title><p>Helpful discussions with Prof. S. Q. Liu, Dr. Y. Liu and Dr. X. S, Yang are greatly appreciated. This work is supported by the National Natural Science Foundation for Young Scientists of China (Grant No. 11605143), Chinese National Science Foundation (Nos. 11261140327, 11005035, 11205053, 11575055). National Key R&amp;D Program of China under 2017YFE0300405.</p></sec><sec id="s7"><title>Conflicts of Interest</title><p>The authors declare no conflicts of interest regarding the publication of this paper.</p></sec><sec id="s8"><title>Cite this paper</title><p>Wang, Z.T., Chen, X.C., Yan, Y.F., Li, H.D., Liu, Q., Mou, M.L., Wu, N., Wang, Z.H., Ke, R., Nie, L. and Xu, M. (2019) Mitigation of ELMs by Electrostatic Field in Tokamaks. Journal of High Energy Physics, Gravitation and Cosmology, 5, 149-155. https://doi.org/10.4236/jhepgc.2019.51007</p></sec></body><back><ref-list><title>References</title><ref id="scirp.89241-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Connor, J.W., Hastie, R.J., Wilson, H.R. and Miller, R.L. (1998) Magnetohydrodynamic Stability of Tokamak Edge Plasmas. Physics of Plasmas, 5, 2687. https://doi.org/10.1063/1.872956</mixed-citation></ref><ref id="scirp.89241-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Hsu, J.Y., Chan, V.S., Harvey, R.W., Prater, R. and Wong, S.K. (1984) Resonance Localization and Poloidal Electric Field Due to Cyclotron Wave Heating in Tokamak Plasmas. 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