Plasma stability

A ball at rest in a valley (right) will return to the bottom if moved slightly, or perturbed, and is thus dynamically stable. One on the top of a hill (left) will accelerate away from its rest point if perturbed, and is thus dynamically unstable. Plasmas have many mechanisms that make them fall into the second group under certain conditions.

In plasma physics, plasma stability concerns the stability properties of a plasma in equilibrium and its behavior under small perturbations. The stability of the system determines if the perturbations will grow, oscillate, or be damped out. It is an important consideration in topics such as nuclear fusion and astrophysical plasma.

In many cases, a plasma can be treated as a fluid and analyzed with the theory of magnetohydrodynamics (MHD). MHD stability is necessary for stable operation of magnetic confinement fusion devices and places certain operational limits. The beta limit, for example, sets the maximum achievable plasma beta in tokamaks.

On the other hand, small-scale plasma instabilities (typically described by kinetic theory), such as the drift wave instability, are believed to be the driving mechanism of turbulent transport in tokamaks, which leads to high rate of particle and energy transport across the confining magnetic fields. Plasma instabilities described by kinetic theory can contain aspects such as finite Larmor radius (FLR) effects and resonant wave-particle interactions, which is not captured in fluid models such as MHD.

Plasma instabilities

Plasma instabilities can be divided into two general groups:

1. hydrodynamic instabilities
2. kinetic instabilities.

Plasma instabilities are also categorised into different modes (e.g. with reference to a particle beam): ^{[1] [2]}

Mode (azimuthal wave number)	Note	Description	Radial modes	Description
m=0		Sausage instability: displays harmonic variations of beam radius with distance along the beam axis	n=0	Axial hollowing
			n=1	Standard sausaging
			n=2	Axial bunching
m=1		Sinuous, kink or hose instability: represents transverse displacements of the beam cross-section without change in the form or in a beam characteristics other than the position of its center of mass
m=2	Filamentation modes: growth leads towards the breakup of the beam into separate filaments.	Gives an elliptic cross-section
m=3		Gives a pyriform (pear-shaped) cross-section
m=4		Consists of four intertwined helices

List of plasma instabilities

• Buneman instability, ^[3]
  • Farley–Buneman instability, ^{[4] [5]}
  • Jeans–Buneman instability, ^{[6] [7]}
  • Relativistic Buneman instability, ^[8]
• Cherenkov instability, ^[9]
• Coalescence instability, ^[10]
  • Non-linear coalescence instability
• Chute instability,
• Collapse instability,
• Cyclotron instabilities, including:
  • Alfven cyclotron instability
  • Cyclotron maser instability, ^[11]
  • Electron cyclotron instability
  • Electrostatic ion cyclotron Instability
  • Ion cyclotron instability
  • Magnetoacoustic cyclotron instability
  • Proton cyclotron instability
  • Non-resonant beam-type cyclotron instability
  • Relativistic ion cyclotron instability
  • Whistler cyclotron instability
• Diocotron instability, ^[12] (similar to the Kelvin-Helmholtz fluid instability).
• Disruptive instability (in tokamaks) ^[13]
• Double emission instability,
  • Edge-localized modes, ^{[14] [15]}
  • Explosive instability (or Ballooning instability), ^[16]
• Double plasma resonance instability, ^[17]
• Drift instability ^[18] (a.k.a. drift-wave instability, ^[19] or universal instability ^[20] )
  • Lower hybrid (drift) instability (in the Critical ionization velocity mechanism)
  • Magnetic drift instability, ^[21]
  • Slow Drift Instability
• Electrothermal instability
• Fan instability, ^[22]
• Firehose instability (a.k.a. hose instability), not to be confused with the similarly named Firehose instability in galactic dynamics
• Fish instability,
• Free electron maser instability,
• Gyrotron instability,
• Helical (Helix) instability,
• Jeans instability, ^{[23] [24]}
• Magnetic buoyancy instability
  • Interchange instability (a.k.a. flute instability), ^[25]
  • Parker instability ^[26] (a.k.a. undular instability or magnetic Rayleigh–Taylor instability)
  • Mixed instability (a.k.a. quasi-interchange instability)
• Magnetorotational instability (in accretion disks)
• Magnetothermal instability (Laser-plasmas), ^[27]
• Modulational instability
• Non-Abelian instability,
• Pair instability (in supernovae)
• Peratt instability (stacked toroids)
• Pinch instability (a.k.a. Bennett pinch instability), ^{[28] [29]}
  • Sausage instability (m=0)
  • Kink instability (m=1)
    • Helical kink instability (a.k.a. helical instability)
• Rayleigh–Taylor instability (RTI, a.k.a. gravitational instability)
• Rotating instability, ^[30]
• Tearing mode instability (or resistive tearing instability ^[31] )
• Two-stream instability (a.k.a. beam-plasma instability, counter-streaming instability)
  • Beam acoustic instability
  • Bump-on-tail instability
  • Ion beam instability
  • Weak beam instability
• Weibel instability
  • Chromo–Weibel instability (i.e. non-abelian instability)
  • Filamentation instability (a.k.a. beam-Weibel instability), ^[32]

MHD Instabilities

Beta is a ratio of the plasma pressure over the magnetic field strength. ^[33] $${\displaystyle \beta ={\frac {p}{p_{\text{mag}}}}={\frac {nk_{B}T}{(B^{2}/2\mu _{0})}}}$$

MHD stability at high beta is crucial for a compact, cost-effective magnetic fusion reactor. Fusion power density varies roughly as ${\displaystyle \beta ^{2}}$ at constant magnetic field, or as ${\displaystyle \beta _{N}^{4}}$ at constant bootstrap fraction in configurations with externally driven plasma current. (Here ${\displaystyle \beta _{N}=\beta /(I/aB)}$ is the normalized beta.) In many cases MHD stability represents the primary limitation on beta and thus on fusion power density. MHD stability is also closely tied to issues of creation and sustainment of certain magnetic configurations, energy confinement, and steady-state operation. Critical issues include understanding and extending the stability limits through the use of a variety of plasma configurations, and developing active means for reliable operation near those limits. Accurate predictive capabilities are needed, which will require the addition of new physics to existing MHD models. Although a wide range of magnetic configurations exist, the underlying MHD physics is common to all. Understanding of MHD stability gained in one configuration can benefit others, by verifying analytic theories, providing benchmarks for predictive MHD stability codes, and advancing the development of active control techniques.

The most fundamental and critical stability issue for magnetic fusion is simply that MHD instabilities often limit performance at high beta. In most cases the important instabilities are long wavelength, global modes, because of their ability to cause severe degradation of energy confinement or termination of the plasma. Some important examples that are common to many magnetic configurations are ideal kink modes, resistive wall modes, and neoclassical tearing modes. A possible consequence of violating stability boundaries is a disruption, a sudden loss of thermal energy often followed by termination of the discharge. The key issue thus includes understanding the nature of the beta limit in the various configurations, including the associated thermal and magnetic stresses, and finding ways to avoid the limits or mitigate the consequences. A wide range of approaches to preventing such instabilities is under investigation, including optimization of the configuration of the plasma and its confinement device, control of the internal structure of the plasma, and active control of the MHD instabilities.

Ideal Instabilities

Ideal MHD instabilities driven by current or pressure gradients represent the ultimate operational limit for most configurations. The long-wavelength kink mode and short-wavelength ballooning mode limits are generally well understood and can in principle be avoided.

Intermediate-wavelength modes (n ~ 5–10 modes encountered in tokamak edge plasmas, for example) are less well understood due to the computationally intensive nature of the stability calculations. The extensive beta limit database for tokamaks is consistent with ideal MHD stability limits, yielding agreement to within about 10% in beta for cases where the internal profiles of the plasma are accurately measured. This good agreement provides confidence in ideal stability calculations for other configurations and in the design of prototype fusion reactors.

Resistive Wall Modes

Resistive wall modes (RWM) develop in plasmas that require the presence of a perfectly conducting wall for stability. RWM stability is a key issue for many magnetic configurations. Moderate beta values are possible without a nearby wall in the tokamak, stellarator, and other configurations, but a nearby conducting wall can significantly improve ideal kink mode stability in most configurations, including the tokamak, ST, reversed field pinch (RFP), spheromak, and possibly the FRC. In the advanced tokamak and ST, wall stabilization is critical for operation with a large bootstrap fraction. The spheromak requires wall stabilization to avoid the low-m, n tilt and shift modes, and possibly bending modes. However, in the presence of a non-ideal wall, the slowly growing RWM is unstable. The resistive wall mode has been a long-standing issue for the RFP, and has more recently been observed in tokamak experiments. Progress in understanding the physics of the RWM and developing the means to stabilize it could be directly applicable to all magnetic configurations. A closely related issue is to understand plasma rotation, its sources and sinks, and its role in stabilizing the RWM.

Resistive instabilities

Resistive instabilities are an issue for all magnetic configurations, since the onset can occur at beta values well below the ideal limit. The stability of neoclassical tearing modes (NTM) is a key issue for magnetic configurations with a strong bootstrap current. The NTM is a metastable mode; in certain plasma configurations, a sufficiently large deformation of the bootstrap current produced by a “seed island” can contribute to the growth of the island. The NTM is already an important performance-limiting factor in many tokamak experiments, leading to degraded confinement or disruption. Although the basic mechanism is well established, the capability to predict the onset in present and future devices requires better understanding of the damping mechanisms which determine the threshold island size, and of the mode coupling by which other instabilities (such as sawteeth in tokamaks) can generate seed islands. Resistive Ballooning Mode, similar to ideal ballooning, but with finite resistivity taken into consideration, provides another example of a resistive instability.

Opportunities for Improving MHD Stability

Configuration

The configuration of the plasma and its confinement device represent an opportunity to improve MHD stability in a robust way. The benefits of discharge shaping and low aspect ratio for ideal MHD stability have been clearly demonstrated in tokamaks and STs, and will continue to be investigated in experiments such as DIII-D, Alcator C-Mod, NSTX, and MAST. New stellarator experiments such as NCSX (proposed) will test the prediction that addition of appropriately designed helical coils can stabilize ideal kink modes at high beta, and lower-beta tests of ballooning stability are possible in HSX. The new ST experiments provide an opportunity to test predictions that a low aspect ratio yields improved stability to tearing modes, including neoclassical, through a large stabilizing “Glasser effect” term associated with a large Pfirsch-Schlüter current. Neoclassical tearing modes can be avoided by minimizing the bootstrap current in quasi-helical and quasi-omnigenous stellarator configurations. Neoclassical tearing modes are also stabilized with the appropriate relative signs of the bootstrap current and the magnetic shear; this prediction is supported by the absence of NTMs in central negative shear regions of tokamaks. Stellarator configurations such as the proposed NCSX, a quasi-axisymmetric stellarator design, can be created with negative magnetic shear and positive bootstrap current to achieve stability to the NTM. Kink mode stabilization by a resistive wall has been demonstrated in RFPs and tokamaks, and will be investigated in other configurations including STs (NSTX) and spheromaks (SSPX). A new proposal to stabilize resistive wall modes by a flowing liquid lithium wall needs further evaluation.

Internal Structure

Control of the internal structure of the plasma allows more active avoidance of MHD instabilities. Maintaining the proper current density profile, for example, can help to maintain stability to tearing modes. Open-loop optimization of the pressure and current density profiles with external heating and current drive sources is routinely used in many devices. Improved diagnostic measurements along with localized heating and current drive sources, now becoming available, will allow active feedback control of the internal profiles in the near future. Such work is beginning or planned in most of the large tokamaks (JET, JT–60U, DIII–D, C–Mod, and ASDEX–U) using RF heating and current drive. Real-time analysis of profile data such as MSE current profile measurements and real-time identification of stability boundaries are essential components of profile control. Strong plasma rotation can stabilize resistive wall modes, as demonstrated in tokamak experiments, and rotational shear is also predicted to stabilize resistive modes. Opportunities to test these predictions are provided by configurations such as the ST, spheromak, and FRC, which have a large natural diamagnetic rotation, as well as tokamaks with rotation driven by neutral beam injection. The Electric Tokamak experiment is intended to have a very large driven rotation, approaching Alfvénic regimes where ideal stability may also be influenced. Maintaining sufficient plasma rotation, and the possible role of the RWM in damping the rotation, are important issues that can be investigated in these experiments.

Feedback Control

Active feedback control of MHD instabilities should allow operation beyond the “passive” stability limits. Localized RF current drive at the rational surface is predicted to reduce or eliminate neoclassical tearing mode islands. Experiments have begun in ASDEX–U and COMPASS-D with promising results, and are planned for next year ^{[ clarification needed ]} in DIII–D. Routine use of such a technique in generalized plasma conditions will require real-time identification of the unstable mode and its radial location. If the plasma rotation needed to stabilize the resistive wall mode cannot be maintained, feedback stabilization with external coils will be required. Feedback experiments have begun in DIII–D and HBT-EP, and feedback control should be explored for the RFP and other configurations. Physics understanding of these active control techniques will be directly applicable between configurations.

Disruption Mitigation

The techniques discussed above for improving MHD stability are the principal means of avoiding disruptions. However, in the event that these techniques do not prevent an instability, the effects of a disruption can be mitigated by various techniques. Experiments in JT–60U have demonstrated reduction of electromagnetic stresses through operation at a neutral point for vertical stability. Pre-emptive removal of the plasma energy by injection of a large gas puff or an impurity pellet has been demonstrated in tokamak experiments, and ongoing experiments in C–Mod, JT–60U, ASDEX–U, and DIII–D will improve the understanding and predictive capability. Cryogenic liquid jets of helium are another proposed technique, which may be required for larger devices. Mitigation techniques developed for tokamaks will be directly applicable to other configurations.

See also

• List of hydrodynamic instabilities named after people

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