1. Field
The present teachings generally relate to the field of plasma containment and more particularly, to systems and methods for establishing a stable plasma in a relatively compact containment chamber.
2. Description of the Related Art
Nuclear fusion occurs when two relatively low mass nuclei fuse to yield a larger mass nucleus and reaction products. Because a substantial amount of energy is associated with the reaction products, controlled nuclear fusion research is an ongoing process with efficient power generation being one of the important goals. Secondary goals may include the production of neutrons or X rays, among other things. For fusion to occur, two nuclei need to interact at a nuclear level after overcoming the mutually repulsive Coulomb barrier. Different methods can be used to promote such an interaction.
One widely-used method of promoting the fusion process is to provide a volume of plasma having the fusable ions at sufficient density and temperature. Such a plasma needs to be contained sufficiently long enough to allow the fusion reaction to occur. Preferably, such a containment substantially isolates the plasma from the surrounding environment to reduce heat loss.
One way to contain the fusionable plasma is to use magnetic fields to “pinch” and restrict the plasma to certain volumes. One magnetic confinement design commonly referred to as a tokamak restricts the plasma in a donut shaped (toroid) volume. Because many conventional magnetically confined fusion devices are geared toward power production, confinement volumes are designed to be large. Consequently, such large devices and various supporting components can be prohibitively complex and/or expensive to operate in widespread applications.
The foregoing drawbacks can be overcome by a containment method that enhances stability. Such a plasma can be designed and operated by determining a stable energy state of the system without imposing a quasi-neutrality condition; a contained plasma that includes a substantial electrostatic field will contribute significantly to the stability of the plasma. Compact devices based on such contained plasmas can be used in different applications, such as a neutron generator, an X ray generator, and a power generator.
One aspect of the present teachings relates to a method for designing a plasma containment device, including generating a characterization of the energy of a plasma system having a distribution of electrons and a distribution of ions. The characterization includes an energy term associated with a bulk electrostatic field produced inside the plasma by dissimilarities between the distribution of electrons and the distribution of ions. The method further includes determining an equilibrium state associated with the characterization of the energy of the plasma system. The method further includes determining one or more plasma parameters associated with the equilibrium state.
In a further aspect, the present invention relates to a method of plasma containment, including providing a plasma system, comprising a plurality of charged first particles and a plurality of charged second particles, and creating a dissimilarity between the overall distributions of the first and second particles. In one embodiment, the method includes restricting the plasma to a first beta value, second beta value, and first particle skin depth, the first and second beta values depending on factors comprising average particle number density, average plasma temperature, and strength of a magnetic field established in the plasma. In one embodiment, the inverse of the first beta value is between approximately 0 and 30 and the inverse of the second beta value is between approximately 0 and 3, with a first particle skin depth of between 1 and 2 in a cylindrical configuration.
In a further aspect, the present invention relates to a method of plasma containment, including providing a plasma comprising a plurality of first particles and a plurality of second particles, confining the first particles substantially to a first volume, and confining the second particles substantially to a second volume, with the second volume being larger than and encompassing the first volume. In one embodiment, movement of the first particles creates an electric current, and confining the first particles substantially to the first volume comprises establishing a magnetic field in the plasma substantially perpendicular to the direction of the current. In a further embodiment, confining the second particles substantially to the second volume comprises separating the bulk distributions of the first particles and the second particles such that a bulk electrostatic field is created in the plasma between the first particles and the second particles.
In a further aspect, the present invention relates to a method of plasma containment, including providing a plasma comprising a plurality of charged first particles and a plurality of charged second particles, with the first particles establishing a current by acting as charge carriers in the plasma, and imposing a magnetic field on the plasma, the magnetic field being oriented substantially perpendicular to the current and acting on the first particles to create a dissimilarity in distributions between the first particles and the second particles within the plasma. In one embodiment, the first particles comprise electrons and the second particles comprise ions. In another embodiment, the first particles comprise ions and the second particles comprise electrons. In a further embodiment, the plasma is contained within a substantially cylindrical volume, the volume defining an axial direction and an azimuthal direction, which may constitute part of a toroid. The current may flow in a combined axial-azimuthal direction with the magnetic field oriented in a combined azimuthal-axial direction. The current flow and magnetic field may be oriented spirally.
In a further aspect, the present invention relates to a method of plasma containment, including providing a plasma comprising a plurality of charged first particles and a plurality of charged second particles, the first particles being charge carriers of a current in the plasma, establishing a magnetic field in the plasma that electromagnetically Co. influences the position of the first particles more than it influences the position of the second particles, confining the first particles substantially to a first volume under the influence of the magnetic field, and maintaining at least a portion of the second particles outside the first volume. The position of the first particles may be electromagnetically influenced through a screw pinch. A bulk electrostatic field may be established within the plasma, and confining the second particles to a second volume (the first volume being smaller than and contained within the second volume), under the influence of the bulk electrostatic field.
FIGS. 15A-C show various scales of plasma containment facilitated by electrostatic fields produced by separation of charges;
These and other aspects, advantages, and novel features of the present teachings will become apparent upon reading the following detailed description and upon reference to the accompanying drawings. In the drawings, similar elements have similar reference numerals.
The present teachings generally relate to systems and methods of plasma confinement at a relatively stable equilibrium. In one aspect, such a plasma includes a substantial internal electrostatic field that facilitates the stability and confinement of the plasma.
For the purpose of description, the plasma 100 can be characterized as a two-fluid system having an electron fluid (a fluid of a first particle species) and an ion fluid (a fluid of a second particle species). It will be understood that the ion fluid can involve one, two, or more species of ions based on the same or different elements and/or isotopes. It will also be understood that the collective fluid-equation of characterization of the plasma herein is simply one way of describing a plasma, and is in no way intended to limit the scope of the present teachings. A plasma can be characterized using other methods, such as a kinetic approach, as will be apparent to those skilled in the art in light of this disclosure.
As shown in
As further shown in
As described herein, formation of such electrostatic fields within the plasma 100 contributes to the energy of the plasma system. Determining a relatively-stable energy state of such a system yields plasma parameters, including selected ranges of a plasma dimension L, that are substantially different than that associated with conventional plasma systems. It is generally known that static electric fields in a plasma typically do not exist over a distance substantially greater than the Debye length. They are shielded out because of rearrangements of electrons and ions. This, however, is in the absence of external forces. In the present disclosure described herein, the plasma dimension L is generally greater than many Debye lengths; however this is permitted because of the presence of external forces due to, for example, presence of magnetic fields.
In the description below, various embodiments of plasma systems are described as cylindrical and toroidal systems. In the present disclosure a cylindrical geometry is used for a simplified description, and is not to be construed as limiting in any manner. Because at least some of the effects described herein depend on the scale of the contained plasma, many arbitrary shapes of a contained plasma can be used in connection with the present disclosure. As an example, the plasma 100 in
One aspect of the present teachings relates to a method for determining a plasma state that is relatively stable and wherein such stability is facilitated by formation of a relatively substantial internal electrostatic field.
One way to characterize the energy of the plasma system is to use a two-fluid approach without the quasi-neutrality assumption. In conventional approaches, quasi-neutrality is assumed such that electron and ion density distributions are substantially equal. In contrast, one aspect of the present teachings relates to characterizing the two-fluid system such that the electron and ion densities are allowed to vary independently substantially throughout the plasma. Such an approach allows the two fluids to be distributed differently, and thereby produce a bulk electrostatic field at an equilibrium state of the plasma.
For a plasma contained at least partially by a magnetic field, the energy U of the system can be expressed as an integral of a sum of an E-field energy term, a B-field energy term, kinetic energy terms of the two fluids, and energy terms associated with pressures of the two fluids. Thus,
where E represents the electric field strength, ε0 represents the permittivity of free space, B represents the magnetic field strength, μ0 represents the permeability of free space, the summation index and subscripts s denote the species electrons e or ions i, ms represents the mass of the corresponding species, ns represents the particle density of the corresponding species, us represents the velocity of the corresponding species, ps represents the pressure of the corresponding species fluid, and dV represents the differential volume element of the volume of plasma.
For the purpose of description herein, it will be understood that terms “particle density,” “number density,” and other similar terms generally refer to a distribution of particles. Terms such as “electron density” and “electron number density” generally refer to a distribution of electrons. Terms such as “ion density” and “ion number density” generally refer to a distribution of ion. Furthermore in the description herein, terms such as “average particle density” and “average number density” are used to generally denote an average value of the corresponding distribution.
One way to further characterize the two-fluid plasma of this example is to treat the system as being a substantially collisionless and substantially fully-ionized plasma in a steady-state equilibrium. Moreover, each species of the two fluids can be characterized as substantially obeying an adiabatic equation of state expressed as
ps=Csnsγ (2)
where the Cs represents a constant that can be substantially determined by a method described below, and γ represents the ratio of specific heats of the two species.
Temperatures associated with the two species can be determined through an ideal gas law relationship
ps=nskTs (3)
where k represents the Boltzmann's constant. Furthermore, both species are assumed to be substantially Maxwellian.
One way to further characterize the plasma is to express, for each species, a substantially collisionless, equilibrium force balance equation as
msns(us·∇)us=qsns(E+us×B)−∇ps (4)
where ms represents the particle mass of species s, qs represents the charge, us represents the fluid velocity, and where the anisotropic part of the stress tensor can be and is ignored for simplicity for the purpose of description.
One way to further characterize the plasma is to express, for the system, Maxwell's equations as
As is known, Equation (5) is one way of expressing Poisson's equation; Equation (6) is one way of expressing Ampere's law for substantially steady-state conditions; Equation (7) is one way of expressing the irrotational property of an electric field which follows from Faraday's Law for substantially steady-state conditions; and Equation (8) is one way of expressing the solenoidal property of a magnetic field.
As is also known, Maxwell's equations assume conservation of total charge of a system. Accordingly, one can introduce a dependent variable Q defined as
∇·Q=ne (9)
to substantially ensure electron conservation by adopting appropriate boundary conditions in a manner described below. The electron density ne can further be characterized as obeying a relationship ne≧0.
One way to determine a relatively stable confinement state of a plasma system is to determine an equilibrium state that arises from a first variation of the total energy of the plasma system as expressed in Equation (1) subject to various constraints as expressed in Equations (2)-(9). For the present invention, total energy may be defined as the combination of energy associated with pressure due to the temperature of the plasma particles, in this case ions and electrons, energy stored in the net electric field, energy stored in the net magnetic field, and kinetic energy associated with the movement of the plasma particles, in this case ions and electrons. In one such determination, the pressure term in Equations (1) and (4) can be eliminated by using Equation (2). The resulting constraints can be adjoined to the resulting energy expression U by using Lagrange multiplier functions. Such a variational procedure generally known in the art can result in a relatively complex general vector form of nonlinear differential equations.
One way to simplify the variational procedure without sacrificing interesting properties of the resulting solutions is to perform the procedure using cylindrical coordinates and symmetries associated therewith. The cylindrical symmetries can be used to reduce the independent variables of the system to one variable r. Accordingly, dependent variables of the system can be expressed as ni, ne, Er, Bz, Bθ, Q, uiz, uiθ, uez, and ueθ, where subscripts i and e respectively represent ion and electron species. The first six are state variables. Because derivatives of the last four (velocity components) do not appear in Equations (11A)-(11P) they can be treated as control variables in a manner described below.
Applying the cylindrical symmetries to the plasma system (where constraints ∇×E=0 and ∇·B=0 of Equations (7) and (8) are substantially satisfied identically), cylindrical coordinate expressions associated with Equations (4)-(6) and (9) can be adjoined to U of Equation (1) using Lagrange multiplier functions Mi, Me, ME, Mz, Mθ, and MQ. As the name implies, variations of the control variables may be considered as N 2 producing variations in the state variables as well as in the Lagrange multiplier functions.
The variation of U leads to first-order differential equations for the state variables and for the Lagrange multiplier functions, and to algebraic equations for the control variables. Such equations can conveniently be expressed as equations in dimensionless form using the following replacements: r→rΛe, us→usc, n→N0n, E→EeN0Λe/ε0, B→BeN0Λe/μ0c. Cs→Csmec2N01−γ, ps→psmeN0c2, Q→QΛe and T→Tsk/mc2, where c represents the speed of light, N0 represents the average particle density, e represents the magnitude of the electron charge, and Λe represents the electron skin depth expressed as
Λe=(me/μoN0e2)1/2. (10)
One system of equations that follows from the foregoing energy variation method can be expressed as
One set of boundary conditions (at r=0 and r=a, where a is defined as an outer boundary in
In one implementation of a method for determining a stable equilibrium of the foregoing cylindrical plasma system, input parameters (expressed in dimensional form) for solving the system of equations (Equations (11A-P)) include the cylindrical radius a, the average particle number density N0 substantially equal for both species, the axial magnetic field at the boundary a such that Bz(a)=B0, the net axial current I, and a temperature value T0 for both electrons and ions that is the temperature taken at that value of r at which ns=N0. Using these input parameters, one can determine that Bθ(a)=μ0I/(2πa).
Furthermore, the values of Cs can be determined by combining the adiabatic equation of state from Equation (2) and the ideal gas law from Equation (3) so as to yield Cs=ns1−γkT0. Thus, Cs=N01−γkT0 when evaluated at the value of r where ns=N0 and Ts=T0. The electron and ion average temperatures may be different, which would result in different values of Ci and Ce. For the examples of the present disclosure, they are taken to be substantially the same, i.e., T0. Such a simplification for the purpose of description should not be construed to limit the scope of the present teachings in any manner.
Another useful set of input parameters can be obtained by replacing B0 with a plasma beta value defined as β=N0kT0/(B02/2μ0) (in the geometry of
The foregoing energy variational method yields a description of the plasma system by twelve first-order coupled nonlinear ordinary differential equations, four algebraic equations, and one inequality condition (ne≧0), with sixteen unknowns. Numerical solutions to such a system of equations can be obtained in a number of ways. Solutions disclosed herein are obtained using a known differential equation solving routine such as BVPFD that is part of a known numerical analysis software IMSL.
The plasma 140 defines a first cylindrical volume 150 extending from the Z-axis to r=Y, and a second cylindrical volume 152 extending from the Z-axis to r=a. The first volume 150 generally corresponds to a region of the plasma 140 where the first species of the two fluids is distributed as n1(r). The second volume 152 generally corresponds to a region of the plasma 140 where the second species of the two fluids is distributed as n2(r).
In general, the first and second species are distributed such that
That is, the first region 150 has more of the first species than the second species, and the portion of the second region 152 outside of the first region has substantially none of the first species. As Equation (12C) shows, the total number of particles in the two species is substantially the same in one embodiment.
In some embodiments, substantially all of the first species is located within the first region 150 such that r=Y defines a boundary for the first species. Consequently, the region Y<r<a has substantially none of the first species, and is populated by the second species by an amount ΔN. Since the total numbers of the first and second species are substantially the same in one embodiment, the value of ΔN is also representative of the excess number of the first species relative to the second species in the first region 150.
In some embodiments, as described below in greater detail, the first species can be the electrons, and the second species the ions when a plasma is contained within one or more selected ranges of value for the boundary r=Y. In other embodiments, as also described below in greater detail, the first species can be the ions, and the second species the electrons when the plasma is contained in one or more other selected ranges of value for the boundary r=Y.
As shown in
As described below in greater detail, when the radial dimension of the plasma is selected in certain ranges, motion of one species relative to the other species can be enhanced and thereby be more subject to the magnetic pinching force. Thus, as shown in
As shown in
One can see that when the distance R is relatively large compared to a, such as in a high aspect ratio (R/a) toroid, a given segment of the toroid geometry can be approximated by the cylindrical geometry. Thus, one can obtain design parameters using a cylindrical geometry, and apply such a solution to designing of a toroidal device. As is known in the art, such a cylindrical approximation provides a good base for a toroidal design. One way to correct for the differences between the toroidal and cylindrical geometries is to provide a corrective external field, often referred to as a vertical field that inhibits the plasma toroid radius R from increasing due to magnetic hoop forces, to confine the plasma.
Thus as shown in
The foregoing analysis of the cylindrical plasma includes a one-dimensional (r) analysis using the energy variation method. As described above in reference to
One aspect of the present teachings relates to a scale of a contained plasma having a substantial electrostatic field therein. Various results of the foregoing energy variational procedure are described in the context of cylindrical symmetry. It will be appreciated, however, that such results can also be manifested in other shapes of contained plasma having a similar scale.
The foregoing input parameters result in a contained plasma where the electrons are pinched by magnetic forces thereby giving rise to electron-ion charge separation. Consequently, the electrons are distributed substantially within the inner region of the cylinder (first region 150 in
It will be appreciated that while the magnetic field provides an initial N f confinement mechanism for the plasma, the internally-produced electric field plays an important and substantial role in establishing a stable plasma equilibrium. The force profiles shown in
As shown in
As further shown in
One aspect of the present teachings relates to a plasma system having a bulk separation of charges, as shown by the electron and ion distributions 250 and 254, thereby causing formation of the radially directed electric field profile 252 that substantially overlaps with the plasma volume. Such a coverage of the produced electrostatic field can be achieved in contained plasma systems where the boundary Y for electrons has a dimension on the order of the electron scale length Λe.
For a system to lie within an energy well sufficiently deep to provide a robust confinement for one embodiment, the cylinder radius can lie within a range near the value of the electron scale length (skin depth) Λe. In the example embodiment described above in reference to
A relatively large radius configuration (e.g., Y=6Λe) can result in a substantial electric field being produced near the outer region of the plasma cylinder. An energy well associated with such a configuration can be relatively shallow when compared to the Y≈1.2Λe case. Also, a relatively small radius configuration (e.g., Y=0.3Λe) can result in confinement being lost.
Thus in one embodiment, a plasma confinement that is facilitated by the electrostatic field has a value of Y that is in a range of approximately 1 to 2 times the electron scale length Λe. In one embodiment, a value of Y around 1.2Λe appears to provide a near optimal confinement condition. For a plasma with N0=1019/m3 (as with the example plasma of
The plasma is contained such that energy and/or particle loss(es) from the plasma to a wall defining a containment volume is reduced. One way to achieve such energy/particle loss reduction is to reduce the number of plasma particles coming into contact with the wall. As shown in
As described above, for a plasma containment design where a 3Λe the outer radius a is approximately 5.1 mm for the Y=1.2Λe case. For such a system, a wall can be positioned at a location r>5.1 mm and still allow construction of a relatively small containment device. Moreover, the ion number density at r>5.1 mm (3Λe) is substantially lower than the 0.1% level described above. Thus, the number of ions coming into contact with the wall at r>5.1 mm and transferring energy thereto and/or interacting therewith is reduced even more.
The example plasma described above in reference to
The present disclosure reveals substantial electric fields due to excess electrons in the r<Y region and ions being substantially the only species in the r>Y region. As described above, numerical solutions can be obtained by solving Equations (11A)-(11P) for r<Y and substituting Y for a in the boundary conditions. One can solve the modified set (for ions) for r>Y and replacing 0 by Y in the boundary conditions and then matching the solutions of the two sets at r=Y. In one embodiment, the number density of the magnetically bound species becomes substantially zero at r=Y.
In one embodiment, accomplishing such a matching process can place an additional restriction on the input or control parameters that can be expressed in terms of 1/α and 1/β. For example, in the cylindrical coordinate treatment of the Z-pinch embodiment, 1/α, which can be obtained from N0, T0, and B0, is approximately 2 (for typical fusion plasma parameter values). A more precise value of 1/α can be expressed as a slowly varying function of T0 and n0. For the example cylindrical geometry, an approximate value can be obtained from an example contour plot of 1/α as a function of Y/Λe and temperature T, such as that of
The example plasma described above in reference to
For the theta-pinch example, an outer diameter a of approximately 3Λe is used. Furthermore, input parameters N0=1019/m3, T0=104 keV, 1/α=0, and 1/β=20.5 are used. The corresponding electron scale length Λe=(me/μoN0e2)1/2 is approximately 1.7 mm.
Based on the foregoing example inputs,
The foregoing example theta-pinch confinement results in the value of Y being approximately 2.04 mm. Thus, a theta-pinched plasma with a confinement dimension on the order of the electron scale length Λe can provide the various advantageous features described above in reference to the Z-pinched plasma system.
As previously described, a screw-pinch can be achieved by a combination of Z and theta pinches. Thus, an energy variational analysis similar to the foregoing can be performed with 1/α≠0 and 1/β≠0 to yield similar results where a substantial electrostatic field is produced by separation of charges. Furthermore, a screw-pinched plasma with a confinement dimension on the order of the electron scale length Λe can provide similar advantageous features described above in reference to Z and theta pinched plasma systems. Screw-pinch magnetically confined plasmas are generally regarded as more stable than simple Z- or theta-pinches. It is expected that screw-pinch embodiments of the present teachings will share the various features disclosed herein.
As also described, magnetically confining a plasma in a dimension on the order of the plasma's electron scale length results in separation of charges, thereby inducing a substantial electrostatic field over a substantial portion of the plasma volume. Such an electric field can be characterized so as to correspond to a depth of an energy well associated with a stable equilibrium. Moreover, the energy well depth is expected to be relatively deep when the electron fluid radius Y is in a range of approximately 1-2 Λe. Such relatively deep energy well of the equilibrium provides a relatively stable confined plasma. Such stability of a confined plasma at a value of Y of approximately 1-2 Λe, however, does not preclude a possibility that magnetic confinement at larger values of Y can have its stability facilitated significantly by the electrostatic field.
One aspect of the present teachings relates to a magnetically confined and relatively stable equilibriated plasma at different dimensional scales. FIGS. 15A-C show electron and ion distributions for different plasma sizes. While the larger sized plasma systems may not yield equilibria that are as stable as the case where Y=1-2 Λe, such equilibria may nevertheless have sufficient stabilities that are facilitated by the electric field.
In various plasma embodiments, the electric field coverage scales (304, 310, 316) are generally similar, and can be on the order of few electron scale lengths. Thus, one way to characterize a role of the electrostatic field in the stability of the plasma is to consider the electric field as a layer formed near the surface of the plasma volume. In systems where a plasma volume dimension (e.g., radius a in cylindrical systems) is on the order of the E-field layer “thickness” (such as the system of
In systems where a plasma volume dimension is substantially larger than the E-field layer “thickness” (such as the systems of
One aspect of the present teachings relates to a plasma having a substantially larger scale length (skin depth) than that of plasmas where the electrostatic field is on the order of an electron scale length (electron skin depth).
In such a role-reversed plasma, ions act as charge carriers, thereby being subject to magnetic confinement. The value of a for the ions-moving plasma would be many times that for the electrons-moving plasma because of the much larger ion skin depth Λion=(mion/μoN0e2)1/2. For plasmas having a similar average density value, the ratio of Λion/Λe=(mion/me)1/2. For deuterium, the ratio Λion/Λe is approximately 61. Thus, a plasma having moving ions would have a volume of approximately 612=3700 times that of the similar electrons-moving plasma, all else being substantially the same. The energy variational method described herein can be modified readily for analysis, and a resulting plasma system likely would be sufficiently large to allow power production.
As described above in connection with
As described above in connection with
As described above in connection with
Being a charge carrier in the plasma can be characterized in different ways. One way is to say that charge carriers cause a current in the plasma. Another way is to say that charge carriers undergo a bulk motion in the plasma. Yet another way is to say that charge carriers flow in the plasma.
In one embodiment, both the electrons and the ions can act as charge carriers. That is, both the electrons and the ions can contribute to the current, undergo bulk motions, and flow in the plasma. A difference in the degrees of a current-producing characteristic of the two species can give rise to one species being confined magnetically more than the other. Such a difference in the magnetic confinements of the two species can produce a charge separation that causes formation of an electrostatic field in the plasma.
As previously described, the Z- and theta-pinches can be combined to yield a screw-pinch. Thus, the Z and theta pinch devices of
As shown in
The plasma 372 contained in the foregoing manner can undergo a nuclear fusion reaction that can yield neutrons, x-rays, power, and/or other reaction products. Some of the possible reaction configurations and products for an example deuterium-tritium (DT) reaction at various example operating conditions are summarized in Tables 1-3.
Table 1 summarizes various dimensions associated with an electron-scaled high aspect ratio toroidal system at various particle densities. Quantities associated with Table 1 are defined as follows: n=average particle density; Λ=electron scale length; Y=electron fluid boundary radius=set to 1.5Λ; a=toroid's minor radius=ion fluid boundary radius=set to 2.5Y; R=toroid's major radius=set to 20a; V=toroid's volume=2π2Ra2.
Table 2 summarizes various neutron production rate estimates with the system of Table 1 at various temperatures. Quantities associated with Table 2 are defined as follows: T=plasma temperature; σν=reaction rate; neutron rate=n2(σν)V/4. These reaction rate and neutron rate expressions are well known in the art.
Table 3 summarizes various power production estimates with the system of Table 1 at various temperatures for a deuterium-tritium device. Quantities associated with Table 3 are defined as follows: T=plasma temperature; power associated with charged particles=(nDnTσν)(5.6×10−13) (Watts). The power expression is well known in the art.
As an example from Tables 1-3, not to be construed as limiting in any manner, consider a plasma system having a DT fuel confined in a high aspect ratio toroidal chamber. An average number density n of approximately 1020 m−3, which could arise in later stages of plasma compression (discussed below), corresponds to an electron scale length Λ of approximately 0.0532 cm. Setting Y=1.5Λe=0.080 cm, the minor radius a at 2.5 Λe=0.20 cm, the major radius R at 20a=4 cm results in a volume V of approximately 3.13 cm3.
Operating such a plasma at a temperature of approximately 5 keV (where the reaction rate is approximately 1.30×10−17) can yield approximately 1.02×1011 neutrons per second. Neutron fluxes of such an order in such a compact device are useful in many areas such as antiterrorist materials detection, well logging, underground water monitoring, radioactive isotope production, and other applications.
Operation of such a DT-fueled plasma can also yield high intensity soft x-rays having energies in a range of approximately 1-5 keV. Such x-rays from such compact device are useful in areas such as photolithography. In one embodiment, the soft x-rays are produced from the plasma even if fusion does not occur.
From Tables 1-3, one can see that the example operating parameters of 1020 m−3 average number density at temperature of 5 keV yields a power output of approximately 57 mW. Power output can be increased dramatically by varying different plasma parameters. As previously described, the example plasma solution in reference to
As a relatively conservative estimate for a possible power increase, a change in temperature by a factor of approximately 20 yields a plasma temperature of approximately 100 keV, where power output is approximately 3.72 W when n=1020 m−3. Additionally, as described above in connection with FIGS. 15A-C, electrostatic field facilitated stable plasmas can be formed with an increased volume. Thus, scaling both major and minor radii of the high aspect ratio toroid by a factor of 10 increases the volume by a factor of 103. Thus, because the power output is proportional to the volume of the plasma, the foregoing example 3.72 W output device can be scaled so as to produce several kilo-Watts of power. Such a device has a major radius of approximately 40 cm, which is still a relatively compact device for a power generator.
Various example plasma devices described herein can be operated by including one embodiment of an example start-up process that facilitates formation of a stable and confined plasma. The example start-up process is described in context of a plasma device having a toroidal geometry where both toroidal (axial) and poloidal (azimuthal) magnetic fields play a substantial role in confinement. A similar start-up process generally applies to the Z, theta and screw pinch concepts described herein.
In one embodiment, a vacuum toroidal magnetic field is established by current-carrying toroidal field coils wound in the poloidal direction (such as that shown in
The foregoing example start-up process can bring the plasma into a parameter regime of substantial densities and temperatures that characterize the plasma environment. Subsequently, the plasma proceeds toward a stable, confined equilibrium configuration via relaxation processes with the concomitant development of a substantial, radial electrostatic field that provides confinement for the ions. Additional heating mechanisms such as radio frequency heating can be used to further increase the plasma temperature and hence the probability of fusion events occurring in the plasma environment.
The schematic flow chart diagram that follows, as well as any preceding flow chart diagrams, are generally set forth as logical flow chart diagrams. As such, the depicted order and labeled steps are indicative of one embodiment of the presented method. Other steps and methods may be conceived that are equivalent in function, logic, or effect to one or more steps, or portions thereof, of the illustrated method. Additionally, the format and symbols employed are provided to explain the logical steps of the method and are understood not to limit the scope of the method. Although various arrow types and line types may be employed in the flow chart diagrams, they are understood not to limit the scope of the corresponding method. Some arrows or other connectors may be used to indicate only the logical flow of the method. For instance, an arrow may indicate a waiting or monitoring period of unspecified duration between enumerated steps of the depicted method. Additionally, the order in which a particular method occurs may or may not strictly adhere to the order of the corresponding steps shown. The steps themselves may occur rapidly or over a longer period of time, and may be referred to as time periods.
Referring now to
The principle of the minimum-energy equilibrium holds for many different geometries (e.g., toroidal, such as in a tokamak, linear, such as in a Z pinch, etc.) and the method for heating the plasma may vary from one embodiment to another. The method 500 described here is one embodiment of a method that may be used with the toroidal version.
As is known, all of the many toroidal plasma containment systems known in the art provide a method for raising the plasma temperature. Some of them (e.g., a reversed field pinch) are not initially in their final containment state, but relax to that state after a period of heating. For example, during the initial heating period the reversed field pinch develops magnetic instabilities that actually enhance the relaxation process by which the final containment state is achieved.
In the method 500, the method begins in block 502, the plasma is created from a gas and put into tokamak containment mode, block 503, and the plasma is heated while in the tokamak mode, block 504, tokamak-type plasma containment being well known in the art. After the heating period of block 504 the toroidal magnetic field is reduced, block 505, and there is a rapid transition to the final minimum-energy confinement state of the present invention, block 506, and the plasma is maintained in that state, block 508, with heating continuing. When a plasma makes the transition to the final containment state, we may refer to it as relaxing to the new state. The method 500 ends in block 510.
In order for Et to appear within the plasma itself rather than in the conducting wall of the chamber 400, insulating breaks 401 (in poloidal orientation) and 402 (in toroidal orientation) are provided. These separate the chamber into four conducting pieces so that there is no complete conducting path for either poloidal or toroidal current to flow within the wall of the chamber 400. Under some circumstances, if these breaks are not present, the external, transformer-type magnetic fields may only drive currents within the conducting chamber wall rather than in the plasma contained therein.
The poloidally oriented breaks 401 keep toroidal current from flowing in the wall of the chamber 400 whereas the toroidally oriented breaks 402 stop poloidal current in the wall.
A third embodiment is also possible and has sometimes been used in toroidal magnetic containment. As is known, in that case the containment chamber is conducting, but has no insulating breaks. Under some circumstances, induction of electric fields in this embodiment, though somewhat less efficient, is not reduced sufficiently to hamper the operation of the machine. An advantage of this embodiment is that a conducting wall with complete toroidal and poloidal current paths may tend to suppress certain instabilities.
Referencing step 503 of the method 500, to put the plasma into the tokamak-type containment state in the chamber 390 (a similar process is used with regard to the chamber 400), one or more vacuum ports 393 is provided on the chamber wall to which a vacuum pump 394 and gas supply 396 are connected via valves 395 and 397, respectively. With the valve 397 closed and the valve 395 open, the pump 394 is turned on. After the chamber reaches a sufficiently low pressure (less than approximately 10−7 torr) the valve 395 is closed. This action substantially eliminates impurity gases from the chamber. The valve 397 is then opened and the desired fill gas flows into the chamber until it reaches the desired pressure, after which the valve 397 is closed. The desired pressure is determined from the minor radius a of the actual plasma toroid and the gas fill density, as described below. Any gas that is currently used in tokamak confinement, examples of which are mentioned above, may be used.
For the plasma to ultimately enter the minimum-energy equilibrium of the present invention, the gas fill density must be such that the number of particles per unit length around a high-aspect-ratio toroidal chamber such as the chamber 400 has a value within a range given by
N/l≈mπη2/(μoe2) (13)
where N is the total number of particles per species in the chamber and l is the approximate major toroidal distance around the toroid, l=2πR, where R is the major radius of the chamber. The N/l range corresponds to the approximate range 1<η<2, which is required for robust confinement, and m is the mass of the individual charge OC) g carriers. For the electron mode of operation, m is the mass of the electron. For the ion mode of operation, where the fill gas results in a plasma consisting of an electron fluid and a single type of ion fluid, m is the mass of that ion. For fills involving more than one ion, the value of N/l lies between the extreme values for the individual ions and can be determined by solving the set of differential equations obtained by minimizing the total energy, as illustrated above with regard to a single ion. To illustrate a possible value for an electron mode of operation, using η=1.6, N/l has the value 2.3×1014/m. Typical values of N/l for other containment systems are much higher; for example, one small tokamak (STOR-1M) has N/l on the order of 1018/m, and larger tokamaks have N/l on the order of 1020/m or higher.
While the fill gas density of the described embodiment is small compared to standard tokamak containment systems, later compression during the minimum-energy confinement state of the present invention will cause the plasma number density to be considerably higher than the initial fill gas density.
The right side of Equation 13 applies to other geometries as well, such that the fill gas density is approximately mπη2/(μoe2) however that fill gas density is calculated, whether it be N/l for a high-aspect-ratio toroidal chamber or other combinations for other geometries.
Equation 13 is generated by conditions represented by the following equations:
a=ηΛ (14A)
Λ=(m/(μone2))1/2 (14B)
n=N/(πa2l) (14C)
Equation 14A was discovered computationally through the minimum-energy calculation described above, with η≈1.6. Equations 14B and 14C are definitions. The quantity n is the charge carrier density, μo is the permeability of free space, and e is the electronic charge.
Continuing with step 503, after filling the chamber to the appropriate density and pressure, a substantially toroidal magnetic field Bt (often called vacuum field) is generated within the chamber 390. In the case of the apparatus shown in
The gas is then ionized by one of several standard methods known in the art, and a short time later a toroidal electric field Et is induced into the plasma by, for example, the above-mentioned transformer action described in connection with
At the moment that Et is first applied, i.e., at t=0, the plasma cannot immediately reside in the minimum-energy quasi equilibrium because the driving electric field would have to be so large as to be mechanically unattainable. As a consequence, at t=0 the plasma must be confined by some means other than minimum-energy confinement. This alternate confinement continues until the plasma is heated to an intermediate temperature sufficiently high to enable it to relax into the minimum-energy state of the invention, with parameters that permit reasonable values of Et for further heating.
There are substantially three time periods to note, indicated by their beginning points t0 (=0), t1, and t2, the time periods corresponding to steps 504, 505/506, and 508 respectively, of the method 500.
At t0, the driving electric field Et is applied and the plasma begins to heat, with the plasma being confined by a tokamak-type containment, although, as previously noted, because of the N/l restriction in Equation 13 the plasma number density at this point will be considerably smaller than that normally used in tokamaks. The behavior during this period, i.e., step 504, is well known in the art. During the next time period t1<t<t2, steps 505 and 506, the plasma is caused to make a rapid transition from tokamak-type confinement to the minimum-energy confinement of the present invention. After t2 (the time period of step 508) the plasma continues to heat with the plasma in quasi minimum-energy confinement.
Control of the plasma during the three time periods is now described. During the time period t0<t<t1 of step 504, the heating is substantially ohmic; i.e., the plasma current, acting against plasma resistance, heats the plasma. By means of the large toroidal magnetic field Bt the minor radius of the plasma is held approximately constant without significant compression or pinching, quasi neutrality is maintained, the machine is operating substantially as a tokamak, and current flow and magnetic field are substantially parallel, as is well known in tokamak operation. The equations governing the plasma during this period are
Λ×B=μoj (15A)
and
j×B=Λp (15B)
where p is the scalar pressure and j is the net current.
The net magnetic field B has two components, Bt and Bp. In one embodiment, the primary contribution to the toroidal field Bt is made by the external coils 344 of
During the time period t0<t<t1 of step 504, the contributions to Bt from the external coils 344 is large. As the current jt increases because of the induced transformer-action electric field Et, the poloidal magnetic field Bp produced by the plasma current grows and the total field B begins to deviate from purely toroidal to helical. A measure of the relative contributions of these two field components is called the safety factor, as is known. As expressed by Equation 15B, the poloidal magnetic field produces a force on the toroidally-moving current carriers that is in the inward radial direction and maintains an equilibrium against the outward radial force due to the plasma pressure gradient.
In the tokamak operation of step 504, the large toroidal field Bt is important to confinement and stability. The plasma minor radius a does not change significantly, the electron and ion volumes are the same, quasi neutrality is sustained, the electron and ion charge distributions are substantially the same, and no significant radial electric field is built up. Ions are confined to substantially the same volume as the electrons as expressed in the notion of quasi neutrality.
The purpose for the tokamak-like manner of operation during the period t0<t<t1 of step 504 is to enable the plasma to remain confined while achieving a temperature level and concomitant conditions (e.g., magnetic fields, beta values) such that the plasma can be caused to relax into the minimum-energy state with heating continuing at a reasonable value of Et.
It is well known that large tokamaks operate well using ohmic heating up to temperatures of approximately 3 keV. Above such temperatures, auxiliary heating is necessary (a requirement that is alleviated by the present invention) and the technology required to further heat the plasma while maintaining confinement becomes complex and expensive. An example of this is the large, expensive machine ITER (International Thermonuclear Experimental Reactor).
Between t1 and t2, steps 505 and 506, the plasma crosses over from tokamak-type confinement to the minimum-energy quasi equilibrium state wherein the direction of the plasma bulk flow velocity v relative to B changes from substantially parallel to substantially perpendicular. At t1, the temperature T and the magnitude of the poloidal magnetic field Bp will have a value such that α (=nkT2μo/Bp2) satisfies the relationship necessary for minimum-energy confinement. In the toroidal geometry of a tokamak, α is a toroidal beta value.
One embodiment of carrying out step 505 in the tokamak configuration under consideration is to, at time t1, rapidly reduce or ramp down the external coil contribution to Bt by lowering the current 346 in the coil 344 of
The two beta values are equivalent to, and applications to the tokamak configuration of, the beta values described earlier, i.e., α=N0kT0/(Bθ(a)2/2μ0), and β=N0kT0/(B02/2μ0). The notation is somewhat different but expresses the same concepts, i.e., N0=n and T0=T. In the tokamak configuration, B0 is the toroidal magnetic field Bt, and B0(a) is the poloidal magnetic field Bp.
The relationship between α (toroidal beta) and β (poloidal beta) sufficient for the plasma to enter the minimum-energy state of the present invention is illustrated for a particular plasma (n=1×1019/m3, kT=100 eV, and Y=2.5 mm) in
As mentioned above,
With the particular values mentioned, 1/α and 1/β should fall on or near the curve in
The current jt and magnetic field Bp are already perpendicular at t1. As a result, when the external toroidal magnetic field Bt, which earlier substantially controlled the system, is reduced to very low values, the angle between the total magnetic field and the current approaches 90°. As a consequence, this condition for minimum-energy equilibrium should be easily satisfied.
In an electron mode (electrons carrying the current), as Bt becomes small, a pinch effect from Bp will cause the electron flow to develop a radially inward component, the electrons will pinch, the electron containment radius will reduce, and electron containment volume will diminish. The electrons and ions separate and an inwardly directed, radial electrical field builds up to contain the ions as described by the minimum-energy equilibrium conditions.
How fast the ramping down of Bt can occur is controlled in part by the plasma resistance—if the plasma were a perfect conductor (zero resistance) one could not ramp down the magnetic field; the time it would take would approach infinity. This is because the resulting change of magnetic flux induces an electric field within the plasma that drives a poloidal current in the plasma (Faraday's Law) directed in such a manner as to maintain the original magnetic field Bt unchanged (Lenz's Law). Resistance within the plasma causes this induced poloidal current to decay and, as a consequence, allows the magnitude of Bt to lower. The scale time for this to occur is approximately the well-known time constant L/Ω where L is the circuit inductance and K is the equivalent circuit resistance. An estimate of this time constant is
τ=[μoe2a2(kT)3/2ln(8R/a)]/(2mκ) (16)
where the variables have their usual meanings and κ is given in connection with Equation 21.
In one embodiment, step 505 is rapid in order to avoid instabilities that are destructive to confinement. The scale time that measures the growth rate of many rapid tokamak instabilities can be estimated by dividing the plasma minor radius a=ηΛ by the Alfven velocity νA=B/(μomionn)1/2. For typical values in the present illustration this is on the order of 30×10−6 s and is independent of number density. Using R=10a, a=2 cm, and kT=1 eV Eq. (o) gives τ=1.1×10−6s for the ramping-down time constant—an adequate number to avoid disruptive instabilities. Other embodiments may echo the reverse field pinch and use the instabilities to help relax to the minimum-energy state.
With regard to step 506, there is evidence, both observational (e.g., Venus flux ropes) and theoretical, that systems that are near the minimum-energy quasi equilibrium will relax to that state explosively. According to this, when Bp, Bt, T, α, β, n, and θ (the angle between the magnetic field and the flow velocity), near the values required for minimum-energy equilibrium, they will relax to the quasi equilibrium state very quickly through rapid internal adjustments of the plasma radius a, internal currents, and other parameters.
After properly ramping down Bt in step 505, the plasma will have the proper values of T, α, and β for the minimum-energy state. These quantities, however, represent only boundary conditions (coupled with input initial conditions) whereas the minimum-energy state specifies radial profiles of all variables. For example, T is the average temperature, α is determined by the average number density n0, average temperature T, and toroidal current I; β is determined by n0, T, and the boundary value of the toroidal magnetic field. None of these are actual radial profiles. Although these quantities may have the proper values for minimum-energy confinement, this, in itself, does not say that that the system is yet in the minimum-energy state, though it does indicate that it will go there in accordance with step 506. To be in the minimum-energy containment, in addition to those boundary conditions, one must have the correct profiles for all radius-dependent variables: T(r), Bt(r), Bp(r), ne(r), ni(r), ve(r), vi(r), and so on.
Again, even though a proper minimum-energy set of boundary conditions does not require minimum-energy profiles, it will lead to them. Device designers or operators can achieve a minimum-energy state by manipulating those quantities that are under their control in such a manner as to establish the minimum-energy-state boundary conditions. Then, through internal adjustments of internal plasma profiles, the plasma will relax to the minimum-energy state in a self-consistent manner.
As explained above, for the minimum-energy state, poloidal currents in windings 344 (
When the minimum-energy set of boundary conditions is reached for a pure Z-pinch plasma (or the Z-pinch component of a screw-pinch plasma state), internal plasma variable profiles will already be near the true minimum-energy profiles and little internal relaxation of the plasma will be needed to achieve the true minimum-energy profiles. However, for a pure θ-pinch plasma (or the θ-pinch component of a screw-pinch plasma state), internal plasma variable profiles would likely be further away from the final, minimum-energy profiles. Consequently, relaxation of plasma profiles of the θ-pinch components would likely take longer than relaxation of the Z-pinch components.
According to the present invention, establishing the appropriate boundary conditions at reasonably high temperatures will produce the minimum-energy profiles. It is well-known that physical systems that are in equilibrium states having higher energy than corresponding minimum-energy equilibrium states are often unstable to small perturbations that tend to lower the energy. These instabilities rapidly (often exponentially) move the system away from higher-energy equilibria toward the lower energy states. Changes of this nature are sometimes called relaxation processes. Sometimes internal plasma resistance aids the relaxation.
After step 506—the transition to the new equilibrium state—beginning at time t2 the driving electric field Et will continue to heat the plasma, although the heating is progressively less ohmic and more compressional. The plasma system will substantially remain in the minimum-energy equilibrium with parameter adjustments tracking the heating due to Et (step 508). Inasmuch as the equilibrium parameters themselves change as heating continues, the state is called quasi minimum-energy equilibrium.
As the plasma enters the minimum-energy quasi-equilibrium state the plasma increasingly will no longer be forced to maintain its minor radius a constant. Instead the plasma will compress or pinch. This compression will cause the temperature to increase, likely by many factors, over and above that produced by the ohmic heating. For temperatures exceeding a few keV, compression will be by far the primary source of heat. For the electron mode of operation, compression will heat ions even without equilibration.
We now estimate the time-dependent values of various plasma parameters including temperature T(t), number density n(t), and radius a(t) during both time periods t<t1 (step 504) and t>t2 (step 508). The calculations are simplified to eliminate radial dependence of the various quantities. Despite this simplification, the general behavior of the actual plasma is expected to approximately follow these results and, consequently, the calculations are adequate for device design. Small corrections to design parameters can be determined experimentally by those skilled in the art in light of this disclosure.
We assume the random velocity distributions that represent temperature are Maxwellian. Although gradients in n and T (and consequently in pressure) are necessary during both stages of heating, a reasonable estimate of the heat produced can be determined by assuming that n(r) and T(r) are constant (i.e., have no radial dependence). This assumption also negates the need to consider radial heat transport which, for our purposes, is reasonable.
For convenience we calculate the heating of the plasma in the Z pinch mode, although in actual operation stability will be enhanced through introduction of some θ pinch.
Based on the foregoing assumptions, calculations of the time-dependent behavior of plasma parameters as the plasma is being heated follow:
Consider a volume
V=πa2l (17)
where a is the minor radius of the plasma toroid, assumed for these purposes to be substantially the same for both electrons and ions and l is the length of the approximate cylindrical volume
l=2πR (18)
where R is the major radius of the toroid. Using σ to represent the conductivity of the plasma and j the current density, production of heat energy Q through resistance in volume V will be
dQ/dt=j2V/σ (19)
In a two-species plasma, the conductivity is obtained, in terms of the electron-ion collision frequency v, by
σ=ne2/(mν) (20)
An estimate of the collision frequency is
v=κn/(kT)3/2 (21)
where κ depends upon the slowly varying coulomb logarithm (taken to be 10) and other parameters. For purposes of this illustration we take K to be 2.9×10−11 eV3/2m3/s.
The Second Law of Thermodynamics is
dQ=dU+dW (22)
where U is the internal energy and W is the work done on the system by changes in volume. For t<t2 there is no change in volume, hence
dW=0 (23)
however for t>t2
dW=pdV (24)
where p is the pressure.
Internal energy is given by
U=(3/2)NkT (25)
where N is the total number of particles in the system.
Plasma pressure is, by the ideal gas law,
p=nkT (26)
The total number of particles (see Equation 14C) is
N=nV (27)
hence dV=−Ndn/n2.
The magnitude of the poloidal component of the magnetic field intensity Bp at r=a is, from Amperes Law,
Bp=μoI/(2πa) (28)
where μo is the permeability of free space, and the current I is given in terms of the current density, and the velocity of the charge carriers,
I=jπa2 (29)
and j is expressed in terms of the velocity of the charge carriers, v,
j=nev (30)
Acceleration of the charge carriers and consequent heating is caused by the toroidal electric field E(t) that is induced through the transformer action previously discussed. This acceleration of the charge carriers also does work to increase the magnetic field and is resisted by the ohmic resistance.
mdv/dt=eE−ej/σ+[L/(2πR)]dI/dt (31)
L is the inductance of the single loop of plasma. This we estimate through
L=Rμoln(8R/a) (32)
which neglects internal inductance.
It is convenient to indicate the radius in terms of the penetration depth or scale factor Λ. Using η to represent the proportionality factor, this gives
a=ηΛ (33)
where Λ is given as earlier in this document by
Λ=[m/(μone2)]1/2. (34)
As discussed earlier, we define a toroidal beta value for Z-pinch operation,
α=nkT(2μo)/Bp2 (35)
where Bp is the magnitude of the poloidal component of the magnetic field. Note that the actual plasma beta as conventionally defined requires the use of the total magnetic field rather than the poloidal component. The total magnetic field is 1/(1/α+1/β). Since these calculations are for a z-pinch configuration, β=0. See
All of the foregoing equations are evident from physical laws and definitions that follow from the assumptions made concerning this simple plasma system.
For t<t1 the plasma is in the tokamak-type mode where dW=0, a=constant, and n=constant. During this time period Equations (A) through (R) reduce to two nonlinear, first-order, ordinary differential equation for v(t) and T(t) as follows:
For t>t2 we assume that the plasma is in the minimum-energy state. In this mode the volume can change, so (G′) is used. Two restrictions on Equations (A) through (R) are required in order for the state to be minimum energy: First, as established earlier in Equations 13-14C, when the plasma is in the optimal minimum-energy state, η is a constant between 1 and 2. For convenience and to illustrate the heating characteristics, we take this constant to be 1.6. Second, as established earlier for a Z-pinch plasma in the minimum-energy quasi equilibrium, the toroidal beta value α is nearly constant (almost independent of all input and plasma parameters) at a value near ½. For convenience, and to illustrate the heating behavior, we take α=½ and β=0. These limitations effectively put this system into the quasi minimum-energy state. We assume, as noted above, that the minimum-energy equilibrium is maintained as other plasma parameters change and the plasma heats.
For the time period t>t2, Equations 17 through 35 reduce to two nonlinear, first-order, ordinary, differential equations in two unknowns. These are:
where a=η(m/μone2)1/2.
To give an explicit illustration of the solution of these equations we supply values for e, m, κ, and take R=0.44 m and a=0.010 m. In order for the minimum-energy state to be robust we use, for both time periods, N/l=2.3×1014. This, with the assumed value of a, determines n(0) through Equations 14C and 18. We use η=1.6 and the parameters that specify the minimum-energy state for a Z-pinch plasma, 1/α=2 and 1/β=0. At v(0) the equations are solved using Mathcad for n(t) and v(t).
Using various combinations of Equations 17-35, from solutions ν(t) and n(t) we obtain T(t), B(t), n(t), and a(t). For example we determine that
(U)T(t)=mν(t)2/(8k) (40)
This gives the heating and compression of the electron fluid. We have assumed that electrons and ions equilibrate immediately and that ion temperature is the same as electron temperature, although it is clear that the temperature of the ion fluid would lag that of the electrons even though its heating during t>t2 is primarily compressional.
Consideration of heat transport throughout the plasma is not necessary with this calculation, although in a better determination where we consider profiles n(r), v(r), etc., it would be necessary. Again, the development of the plasma should follow this calculation, more or less, and the general behavior would be as indicated.
To continue the illustration, during the tokamak period t0<t<t1 of step 504, we use kT0=0.03 eV (360 K), and n0=7.32×1017/m3. The value α=½ is achieved at to 9.4 μs. During both periods 504 and 508 we take E(t) as constant at 30 Volts/m.
The two columns of graphs in
In the time region t>t2, step 508, as shown in the second column of graphs in
Although the above-disclosed embodiments have shown, described, and pointed out the fundamental novel features of the invention as applied to the above-disclosed embodiments, it should be understood that various omissions, substitutions, and changes in the form of the detail of the devices, systems, and/or methods shown may be made by those skilled in the art without departing from the scope of the invention. Consequently, the scope of the invention should not be limited to the foregoing description, but should be defined by the appended claims.
This application is a continuation-in-part of U.S. patent application Ser. No. 10/804,520, filed 19 Mar. 2004, titled “Systems and Methods of Plasma Containment,” incorporated herein by reference. Application Ser. No. 10/804,520, in turn, claims priority benefit of U.S. provisional patent application No. 60/456,832, filed 21 Mar. 2003, titled “A Method of Obtaining Design Parameters for a Compact Thermonuclear Fusion Device,” incorporated herein by reference.
Number | Date | Country | |
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60456832 | Mar 2003 | US |
Number | Date | Country | |
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Parent | 10804520 | Mar 2004 | US |
Child | 11624672 | Jan 2007 | US |