2. Canonical GC Hamiltonian

In a toroidal magnetic configuration consisting of nested magnetic-flux surfaces, the equilibrium magnetic field can be given in contravariant and covariant form using Boozer coordinates (Boozer Reference Boozer1981; White & Chance Reference White and Chance1984),

(2.1)\begin{equation} \left. \begin{gathered} \boldsymbol{B}=\boldsymbol{\nabla}\psi\times\boldsymbol{\nabla}\theta+\boldsymbol{\nabla}\zeta\times\boldsymbol{\nabla}\psi_p,\\ \boldsymbol{B}=g(\psi)\boldsymbol{\nabla}\zeta+I(\psi)\boldsymbol{\nabla}\theta+\delta(\psi,\theta)\boldsymbol{\nabla}\psi, \end{gathered} \right\} \end{equation}

where $\zeta$ and $\theta$ are the toroidal and poloidal angles, respectively, $\psi$ is the toroidal flux, $\psi _p$ is the poloidal flux, the functions $g(\psi )$, $I(\psi )$ are related to the poloidal and toroidal current, and $\delta (\psi,\theta )$ measures the non-orthogonality of the coordinate system. In such straight-field-line coordinates, the helicity of the field lines is given from the expression

(2.2)\begin{equation} \frac{{\rm d}\theta}{{\rm d}\zeta} =\frac{\boldsymbol{B}\boldsymbol{\cdot}\boldsymbol{\nabla}\theta}{\boldsymbol{B} \boldsymbol{\cdot}\boldsymbol{\nabla}\zeta}=\frac{1}{q(\psi)} \end{equation}

with $\textrm {d}\psi _p/\textrm {d}\psi =1/q(\psi )$ and $q(\psi )$ being the safety factor.

The GC Lagrangian of a charged particle in the presence of electromagnetic fields is given as $\mathcal {L}=(\boldsymbol {A}+\rho _\| \boldsymbol {B})\boldsymbol {\cdot }\boldsymbol {V}+\mu \dot {\xi }-\mathcal {H}$, where $\boldsymbol {A}$, $\boldsymbol {B}$ are the vector potential and the corresponding magnetic field, respectively, $\rho _\|$ is the velocity component parallel to the magnetic field, normalised to $B$, $\boldsymbol {V}$ is the velocity of the guiding centre, $\mu =v_\perp ^2/2B$ is the magnetic moment, conjugate to the gyro-phase $\xi$, and

(2.3)\begin{equation} \mathcal{H}=\rho_\|^2 B^2/2 + \mu B + \varPhi \end{equation}

is the Hamiltonian of the system, with the magnetic field being normalised to its value on magnetic axis $B_0$, and $\varPhi$ the electric potential (Littlejohn Reference Littlejohn1983). The GC motion is expressed in normalised units, namely, time is normalised to inverse cyclotron angular frequency $\omega _0^{-1}$, with $\omega _0=q_i B_0/m_i$ the on axis gyro-frequency, $q_i$ and $m_i$ the ion charge and mass, respectively, lengths are normalised to the major axis $R_0$, and consequently, energy is normalised to $m_i\omega _0^2R_0^2$.

The canonical momenta conjugate to angles $\zeta$ and $\theta$ are properly expressed in relation to the variables $\rho _\|$, $g(\psi )$ and $I(\psi )$ (White Reference White2014, p. 79), as

(2.4)\begin{gather} P_\zeta = g(\psi)\rho_\|-\psi_p(\psi), \end{gather}

(2.5)\begin{gather}P_\theta = \psi+\rho_\|I(\psi), \end{gather}

and consequently, the Hamiltonian in (2.3) is given in the form

(2.6)\begin{equation} \mathcal{H} = \frac{(P_\zeta+\psi_p(P_\zeta,P_\theta))^2}{2g^2(P_\zeta,P_\theta)} B^2(P_\zeta,P_\theta,\zeta, \theta) + \mu B(P_\zeta,P_\theta,\zeta,\theta) + \varPhi(P_\zeta,P_\theta,\zeta,\theta). \end{equation}

The absence of an explicit time dependence renders the Hamiltonian, and hence the energy $E$ of the system, a constant of the motion, whereas the absence of the gyro-phase $\xi$ results in the conservation of the magnetic moment $\mu$. In the case of an axisymmetric configuration where both the magnetic field and the electric potential are independent of the toroidal angle $\zeta$, the conjugate canonical momentum $P_\zeta$ is an additional invariant of the motion. The existence of three independent constants of the motion $(E,\mu,P_\zeta )$ renders the system integrable and along with the sign of $\rho _\|$, are uniquely defining, and hence labelling, the orbits of the particles in phase space.

In the following sections, our calculations are carried out under the consideration of a circular cross-section large aspect ratio (LAR) magnetic field equilibrium, with $\epsilon =r_0\ll 1$ being the inverse aspect ratio and $r_0$ the minor axis (normalised to major axis $R_0$). Under this approximation, it is easy to show that, to leading order, $I(\psi )\simeq 0$, $g(\psi )\simeq 1$, $\delta (\psi,\theta )=0$ (White & Chance Reference White and Chance1984; White Reference White2013b). Subsequently, from (2.5), we get $P_\theta =\psi =r^2/2$, while the magnetic field acquires the quite simple form $B=B_0(1-r\cos \theta )=B_0(1-\sqrt {2P_\theta }\cos \theta )$.

3. Radial electric field across the pedestal

We consider a strong, radially dependent and highly localised non-monotonic electric field, neglecting any dependence on the poloidal or toroidal angle, which is given from the expression

(3.1)\begin{equation} E_r(r)={-}E_a\exp\left[-\frac{(r-r_a)^2}{r_w^2}\right], \end{equation}

where $E_r(r)$ is the well-like profile of the electric field, $E_a$ is the amplitude (depth) of the well located at $r=r_a$ and $r_w$ is the waist of the radial profile. Adopting typical values for the electric field profile near the wall (Kurki-Suonio et al. Reference Kurki-Suonio, Lashkul and Heikkinen2002; Burrell et al. Reference Burrell, West, Doyle, Austin, deGrassie, Gohil, Greenfield, Groebner, Jayakumar and Kaplan2004; McDermott et al. Reference McDermott, Lipschultz, Hughes, Catto, Hubbard, Hutchinson, Granetz, Greenwald, Labombard and Marr2009; Viezzer et al. Reference Viezzer, Pütterich, Conway, Dux, Happel, Fuchs, McDermott, Ryter, Sieglin and Suttrop2013; Huang & Wang Reference Huang and Wang2020) and disregarding its shape close to the core, the respective well is placed at $r_a=0.98r_0$, having a waist $r_w=r_0/50$ and an amplitude $E_a\simeq 75\,\textrm {kV}\,\textrm {m}^{-1}$, deliberately selected to yield an electrostatic potential of approximately $\varPhi = 1.2\,\mathrm {kV}$ at the last closed flux surface (LCFS) denoted as $\psi _{\textrm {wall}}$.

The electric potential corresponding to (3.1) is straightforwardly calculated from the integral

(3.2)\begin{equation} \varPhi(r)={-}\int_0^r E_r(r')\,{\rm d}r', \end{equation}

which, in terms of the poloidal momentum $P_\theta =\psi =r^2/2$ (for a LAR magnetic field equilibrium), yields

(3.3)\begin{equation} \varPhi(P_\theta)=E_a\sqrt{\frac{{\rm \pi} P_{\theta w}}{2}}\left[\mathrm{erf}\left(\frac{\sqrt{P_\theta}-\sqrt{P_{\theta a}}}{\sqrt{P_{\theta w}}}\right) + \mathrm{erf}\left(\sqrt\frac{{P_{\theta a}}}{P_{\theta w}}\right)\right] \end{equation}

with $P_{\theta w}=r_w^2/2$ and $P_{\theta a}=r_a^2/2$ being the waist and the location of the well, respectively. Figures 1(a) and 1(b) show the radial profile of the radial electric field as well as the respective potential barrier, as functions of the toroidal flux $\psi$, coinciding with the canonical poloidal momentum $P_\theta$ for a LAR equilibrium.

Figure 1. Radial profiles of (a) the radial electric field $E_r(\psi )$ and of (b) the respective electric potential $\varPhi (\psi )$. For a LAR magnetic field equilibrium,$\psi =P_\theta$. The red vertical line marks the wall.

Under the aforementioned approximations of a LAR equilibrium magnetic field and a purely radial electric field, the GC Hamiltonian takes the form

(3.4)\begin{equation} \mathcal{H} = \frac{\left(P_\zeta+\psi_p(P_\theta)\right)^2}{2} (1-\sqrt{2P_\theta}\cos\theta)^2 + \mu(1-\sqrt{2P_\theta}\cos\theta) + \varPhi(P_\theta), \end{equation}

where the axisymmetry of the dynamical system is preserved due to the absence of the canonical angle $\zeta$. The corresponding equations of motion are derived from the expressions

(3.5)\begin{gather} \dot{P}_\zeta={-}\frac{\partial\mathcal{H}}{\partial\zeta} = 0, \end{gather}

(3.6)\begin{gather}\dot{P}_\theta={-}\frac{\partial\mathcal{H}}{\partial\theta} ={-}\,(P_\zeta+\psi_p(P_\theta))^2(1-\sqrt{2P_\theta}\cos\theta)\sqrt{2P_\theta}\sin\theta -\mu\sqrt{2P_\theta}\sin\theta, \end{gather}

(3.7)\begin{gather}\dot{\zeta}=\frac{\partial\mathcal{H}}{\partial P_\zeta} =(P_\zeta+\psi_p(P_\theta))(1-\sqrt{2P_\theta}\cos\theta)^2, \end{gather}

(3.8)\begin{gather}\dot{\theta}=\frac{\partial\mathcal{H}}{\partial P_\theta} ={-}\frac{(1-\sqrt{2P_\theta}\cos\theta)(P_\zeta+\psi_p(P_\theta))^2}{\sqrt{2P_\theta}} -\frac{\mu\cos\theta}{\sqrt{2P_\theta}}\nonumber\\+\,(1-\sqrt{2P_\theta}\cos\theta)^2(P_\zeta+\psi_p(P_\theta))\psi_p'(P_\theta) + \varPhi'(P_\theta), \end{gather}

where primes imply differentiation with respect to $P_\theta$. Equation (3.8) clearly shows that the radial electric field effects are introduced exclusively through the $\varPhi '(P_\theta )$ term of the poloidal angle time-derivative $\dot \theta$, appearing additively to the magnetic shear effects, as expressed by the term proportional to $\psi '_p(P_\theta )$, a fact that has a significant impact on the modification of GC orbits in terms of their shape and poloidal angular frequency, as will be shown in the following sections.

The magnetic shear is dictated by the $q$ factor profile, which in our analysis is considered according to the commonly used expression (White Reference White2014, p. 56)

(3.9)\begin{equation} q(P_\theta)=q_0\left[ 1+\left(\frac{P_\theta}{P_{\theta k}(q_{{\rm wall}})}\right)^n \right]^{1/n}, \end{equation}

where $q_0$ is the value of the safety factor on the magnetic axis, $P_{\theta k}$ is a function related to the location of the ‘knee’ of the profile and $n$ characterises the order of the equilibrium, with $n=1,2,4$ denoting a peaked, round or flat profile, respectively. In that respect, the poloidal flux can be analytically obtained by integrating the rotational transform $\textrm {i}(P_\theta )=1/q(P_\theta )$,

(3.10)\begin{equation} \psi_p(P_\theta)=\int {\rm i}(P_\theta) \,{\rm d}P_\theta, \end{equation}

which results in the hypergeometric function ${}_2F_1$ of the general form

(3.11)\begin{equation} \psi_p(P_\theta)=\frac{P_\theta}{q_0}\,{}_{2}F_1\left[\frac{1}{n},\frac{1}{n};1+\frac{1}{n},\left(1-\left(\frac{q_{{\rm wall}}}{q_0}\right)^n\right)\left(\frac{P_\theta}{P_{\theta\, {\rm wall}}} \right)^n\right], \end{equation}

where $q_{\textrm {wall}}$ and $P_{\theta \, \textrm {wall}}$ are the values of the safety factor and the poloidal momentum on the wall, respectively. In the following analysis, we select a $q$ profile with the moderate $n=2$ value, $q_0=1.1$ and $q_{\textrm {wall}}=3.5$.

The consideration of the LAR equilibrium, along with the corresponding simplification $\psi =P_\theta$ and the analytical expression (3.11) for $\psi _p(P_\theta )$, result in an explicit expression of the equations of motion. It is important to note that for a generic (non-LAR) equilibrium, the Hamiltonian cannot be explicitly expressed in canonical variables, instead, one should use the equations of motion in terms of $(\theta, \psi _p, \rho _\parallel, \zeta )$ (White Reference White2014) and afterwards calculate the canonical momenta $P_\theta$, $P_\zeta$, according to (2.4), (2.5). To solve the equations of motion (3.5)–(3.8), a fourth-order Runge–Kutta method is implemented, also used in well-known orbit following codes like ORBIT (White & Chance Reference White and Chance1984) or ASCOT (Hirvijoki et al. Reference Hirvijoki, Asunta, Koskela, Kurki-Suonio, Miettunen, Sipilä, Snicker and Äkäslompolo2014).

4. Change of the GC phase space topology and orbit shape due to $E_r$

The existence of a radial electric field that is localised near the LCFS of the tokamak affects the topology of the GC phase space by introducing additional fixed points and by modifying the shape of the GC orbits. As a result, the presence of the electric field can significantly modify the prompt particle losses by changing an otherwise confined orbit into a lost one, and vice versa (Hazeltine Reference Hazeltine1989; Chankin & McCracken Reference Chankin and McCracken1993; Krasheninnikov & Yushmanov Reference Krasheninnikov and Yushmanov1994).

For typical values of $E_r$ amplitude ($10\unicode{x2013} 60\,\textrm {kV}\,\textrm {m}^{-1}$) and waist ($1\unicode{x2013} 2\,\mathrm {cm}$, restricted in the range $0.85 r_0\unicode{x2013} 1.05 r_0$), the corresponding electric potential energy is of the order of a few hundreds of ${\textrm {eV}}$. Even though these values of the potential energy are not sufficient to essentially reshape the highly energetic particle trajectories, the impact to thermal and mildly energetic particles, located well inside the bulk of the distribution function profile, could considerably affect the confinement inside this region. Apparently, this impact depends strongly on the amplitude of the potential barrier and will increase as it becomes comparable to the kinetic energy of the particles, as well as on the effective time that a particle spends inside the well during its radial drift.

When no electric potential exists, the $\theta -P_\theta$ plane of the phase space of the LAR Hamiltonian demonstrates a single elliptical point along the outboard midplane $\theta =0$, with its location along $P_{\theta }$ depending on $\mu$ and $P_\zeta$. Evidently, the existence of a radial electric field can effectively modify this picture in two ways. First, the inclusion of the potential term $\varPhi (P_\theta )$ in the Hamiltonian may impose significant changes in the topology of the phase space, in the sense that either the location of the respective critical points may be rearranged or additional critical points may emerge due to bifurcations. In either case, the transformation of the phase space could significantly affect the respective orbits in terms of their characterisation as passing or trapped, and confined or lost. Second, when the elliptic point of the system lies in the neighbourhood of the pedestal, the lower-energy orbits residing relatively close to the elliptic point will undergo the strongest impact, as their energy will be comparable to the amplitude of the potential barrier. Moreover, due to their relatively small radial drift, these particles will remain well inside the vicinity of the strong potential barrier along their entire orbits, increasing the effective interaction time of the system. However, higher energy particles undergo a wider radial drift motion inside the torus, and therefore their trajectories spend a smaller fraction of their period inside the pedestal, decreasing the influence that $E_r$ has on the respective orbits.

These features are very clearly illustrated in figure 2, where in panels (a,c,e), we show the $\theta -P_\theta$ projection of the phase space of the Hamiltonian (3.4), for various values of the perpendicular kinetic energy $\mu B_0$ and the toroidal momentum $P_\zeta$, with the latter being properly selected for the elliptical point to be located in the vicinity of the potential barrier, where its effects are more acute. Coloured contour-plots correspond to the kinetic energy $E_k$ levels of (2.6), when $\varPhi (P_\theta )=0$, and red contour-lines correspond to energy levels with $\varPhi (P_\theta )$ being given from (3.3). Accordingly, in panels (b,d,f), the respective orbits are depicted in the configuration space of the LAR magnetic equilibrium. Greyed areas denote the wall (LCFS) of the equilibrium, and no re-entrance is allowed for particles beyond this point as they are considered to be lost. As it is clearly seen, the modification of the phase space trajectories is more vividly manifested for thermal and weakly energetic particles initialised along the potential gradient, whereas higher energy particles experience only minor modifications in their orbits, in the form of small variations from the original $E_r=0$ case.

Figure 2. (a,c,e) GC orbits depicted in phase space, with background coloured orbits corresponding to $E_r=0$ and red orbits corresponding to $E_r\neq 0$. (b,d,f) Characteristic GC orbits for $E_r\neq 0$, depicted in configuration space. Dots and crosses denote elliptic and hyperbolic critical points, respectively, and white dashed lines denote the trapped-passing boundaries (separatrices) when $E_r\neq 0$. (a,b) Thermal particles with $\mu B_0=0.5\,\mathrm {keV}$, $P_\zeta =-0.0272$. Here, $E_r$ causes the emergence of additional critical points near the wall, inducing additional trapped orbits along the $\theta ={\rm \pi}$ midplane and twice-reversed passing particles manifesting the abrupt changes of the perpendicular drift velocity. (c,d) Low-energy particles with $\mu B_0=2\,\mathrm {keV}$, $P_\zeta =-0.025$. Here, $E_r$ rearranges the orbits into the confined trapped domain. (e,f) Energetic particles with $\mu B_0=10\,\mathrm {keV}$, $P_\zeta =-0.0125$. As the kinetic energy increases, the contribution of the potential to the total energy decreases, leaving the phase space of such orbits practically undisturbed. The confined passing orbits retain their shapes, and only minor modifications near the wall witness the presence of $E_r$.

Focusing on the implications that the radial electric field imposes upon the particles’ orbits for various sets of parameters, in figure 2(a,b), we depict the orbits of thermal particles with $\mu B_0=0.5\,\mathrm {keV}$, $P_\zeta =-0.272$, for various values of the total energy $E$. In panel (a), it is shown that in the absence of $E_r$ (coloured orbits), the trapped/passing boundary is formed beyond the wall, hence, there exist low-energy counter-passing orbits being confined for small $P_\theta$ which become eventually lost as $P_\theta$ increases. In the presence of $E_r$ (red orbits), the picture changes significantly and confined trapped orbits populate the phase space near the wall, as a result of the emergence of an additional elliptical point inside of the wall, along outboard midplane $\theta =0$. Moreover, the appearance of a pair of critical points close to the wall, an elliptic along $\theta =\pm {\rm \pi}$ and a hyperbolic along $\theta =0$, respectively, is responsible for the appearance of a new family of orbits oscillating around the elliptic point at $\theta =\pm {\rm \pi}$, as well as for the unusual parallel velocity reversal points encountered by passing orbits, manifested also as turning points in the poloidal direction of the configuration phase (panel b).

The existence of turning points in the pedestal is associated with the contribution of $\boldsymbol {E}\times \boldsymbol {B}$ drift velocity to the total perpendicular velocity of the plasma particles and the conservation of the magnetic moment $\mu$. Normally, for a passing orbit in a torus, the initial velocity ratio $v_{\parallel 0}/v_{\perp 0}$ is sufficiently large to prevent the existence of a turning point; however, when a radial electric field is present, the sudden increase of the perpendicular drift velocity $V_{E\times B}$ inside the pedestal results in the decrease of the velocity ratio, allowing now the velocity reversal due to $\boldsymbol {\nabla } B$ drift along the orbit. As soon as the influence of the electric field starts to decline, the particle goes through its second turning point, carrying out a full rotation around the magnetic axis.

In figure 2(c,d), we depict low-energy particles with $\mu B_0=2\,\mathrm {keV}$ and $P_\zeta =-0.025$. In the absence of $E_r$ (coloured orbits), the dominant elliptic point roughly touches the wall, and consequently, the near-wall area is populated by either confined counter-passing or promptly lost trapped particles. In the presence of the radial electric field (red orbits), the existence of the elliptic point at $\theta =0$, $P_\theta \simeq 0.9 P_{\theta,\textrm {wall}}$, drastically changes the topology of the phase space, allowing for the banana orbit width squeezing (Hazeltine Reference Hazeltine1989; Chankin & McCracken Reference Chankin and McCracken1993; Krasheninnikov & Yushmanov Reference Krasheninnikov and Yushmanov1994) and the existence of confined trapped orbits, as well.

Finally, figure 2(e,f) depicts orbits of higher-energy particles with $\mu B_0=10\,\mathrm {keV}$ and $P_\zeta =-0.0125$. In this instance, the kinetic energy of the particles dominates over the potential barrier, and counter-passing orbits populate almost exclusively the outer area of the torus, regardless of the presence of the radial electric field. The relatively large radial drift undergone by the particles allows only a partial interaction with the potential gradient, which is constrained within the narrow pedestal region. This weak interaction is graphically witnessed in both the phase space (panel e) and the configuration space (panel f), by observing the minor deviations between the respective orbits in the absence (coloured orbits), and in the presence (red orbits) of $E_r$.

5. Orbital spectrum modification due to $E_r$

The electric potential term of the Hamiltonian does not affect the integrability property of the GC motion; however, as shown in (3.8), it directly affects the time evolution of the poloidal angle and modifies the poloidal period, as well as the periods of the other degrees of freedom that are coupled to the poloidal motion. Hence, apart from the shape variations that a trajectory undergoes due to the existence of the potential barrier, the frequency spectrum of the respective orbits may significantly deviate from that obtained in the absence of $E_r$, and consequently, rearrange dramatically the resonance condition of the particle orbits with non-axisymmetric perturbations. This aspect is of paramount importance as the resonant mode–particle interactions dictate momentum and particle transport phenomena in fusion plasmas (Heidbrink & White Reference Heidbrink and White2020; White & Bierwage Reference White and Bierwage2021).

In the following, we investigate the impact of the radial electric field on the orbital spectrum, namely the poloidal and the bounce/transit-averaged toroidal precession frequencies, of different orbits, characterised by a specific set of constants of the motion ($\mu, E, P_\zeta$), and therefore, the respective drift-mode resonant numbers corresponding to these orbits. To perform our calculations, we take advantage of the Hamiltonian framework by describing our system in the action-angle variables formalism which fully exploits the canonical structure of GC dynamics (Zestanakis et al. Reference Zestanakis, Kominis, Anastassiou and Hizanidis2016; Antonenas et al. Reference Antonenas, Anastassiou and Kominis2021).

The integrability of the GC Hamiltonian (3.4) allows for a canonical transformation from the original canonical variables to action-angle variables

(5.1)\begin{equation} \left. \begin{gathered} (\mu, \xi)\rightarrow(J_\xi, \hat{\xi}), \\ (P_\zeta, \zeta)\rightarrow(J_\zeta, \hat{\zeta}), \\ (P_\theta, \theta)\rightarrow(J_\theta, \hat{\theta}) , \end{gathered} \right\} \end{equation}

using the appropriate mixed-variable generating function (Lichtenberg & Lieberman Reference Lichtenberg and Lieberman1992; Goldstein, Poole & Safko Reference Goldstein, Poole and Safko2002)

(5.2)\begin{equation} F_2(J_\xi, J_\zeta, J_\theta, \xi, \zeta, \theta) = \xi J_\xi + \zeta J_\zeta + f_2(J_\xi, J_\zeta, J_\theta, \theta), \end{equation}

with

(5.3)\begin{equation} f_2(J_\xi, J_\zeta, J_\theta, \theta) = f_2(\boldsymbol{J},\boldsymbol{\theta})=\int^{\theta}P_\theta\left(J_\xi, J_\zeta, J_\theta(J_\xi, J_\zeta),\theta'\right)\,{\rm d}\theta'. \end{equation}

It is quite straightforward to show that in the first two sets of (5.1), the respective actions are equal to the old momenta, that is, $\mu =J_\xi$ and $P_\zeta =J_\zeta$, while the third action is defined as

(5.4)\begin{equation} J_\theta=\frac{1}{2{\rm \pi}}\oint P_\theta(E, J_\xi, J_\zeta,\theta)\,{\rm d}\theta, \end{equation}

where $E$ is the total energy of the dynamical system, and $J_\theta$ may correspond to either bounced (trapped) or transit (passing) motion. The new angles (canonical positions) corresponding to bounce-averaged gyro-angle, toroidal and poloidal angles, respectively, are given in relation to the old angles as (Kaufman Reference Kaufman1972; Zestanakis et al. Reference Zestanakis, Kominis, Anastassiou and Hizanidis2016)

(5.5a–c)\begin{equation} \hat{\xi}=\xi+\frac{\partial f_2(\boldsymbol{J,\theta})}{\partial J_\xi}, \quad \hat{\zeta}=\zeta+\frac{\partial f_2(\boldsymbol{J,\theta})}{\partial J_\zeta}, \quad \hat{\theta}=\frac{\partial f_2(\boldsymbol{J,\theta})}{\partial J_\theta}. \end{equation}

It is worth noting that the angles $(\xi, \zeta, \theta )$ do not exhibit a linear time dependence, and hence, the respective frequencies $(\dot {\xi }, \dot {\zeta }, \dot {\theta })$ do not represent any physical frequency of the Hamiltonian system. However, (5.5a–c) implies that $\hat {\theta }$ is a periodic function of $\theta$, and as such, both share the same periodicity, yielding

(5.6)\begin{equation} T_{\hat\theta}=T_\theta=2{\rm \pi}/\hat\omega_\theta, \end{equation}

a feature that does not apply to the rest of the angles $\hat {\xi }, \hat {\zeta }$.

Omitting the variables related to fast gyromotion for brevity, the orbital frequencies of the remaining degrees of freedom are acquired by virtue of implicit differentiation

(5.7)\begin{equation} \frac{\hat{\omega}_\zeta}{\hat{\omega}_\theta}=\frac{\partial\mathcal{H}\left(J_\xi,J_\zeta,J_\theta(J_\xi,J_\zeta)\right)/\partial J_\zeta}{\partial\mathcal{H}\left(J_\xi,J_\zeta,J_\theta(J_\xi,J_\zeta)\right)/\partial J_\theta} ={-}\frac{\partial J_\theta(J_\xi, J_\zeta)}{\partial J_\zeta} \end{equation}

revealing the fact that under the action-angle formalism, the poloidal action $(-J_\theta )$ can be considered as the new Hamiltonian of the system (White & Chance Reference White and Chance1984; Antonenas et al. Reference Antonenas, Anastassiou and Kominis2021), with the time being normalised to the inverse poloidal frequency $\hat \omega _\theta$. Substituting (5.4) into (5.7) yields

(5.8)\begin{equation} \left. \begin{aligned} \frac{\hat{\omega}_\zeta}{\hat{\omega}_\theta} & ={-}\frac{1}{2{\rm \pi}}\frac{\partial}{\partial J_\zeta}\oint P_\theta(E, \mu, P_\zeta, \theta)\,{\rm d}\theta ={-}\frac{1}{2{\rm \pi}}\oint \frac{\partial P_\theta(E, \mu, P_\zeta, \theta)}{\partial J_\zeta}\,{\rm d}\theta\\ & =\frac{1}{2{\rm \pi}}\oint\frac{1}{\dot{\theta}}\frac{\partial\mathcal{H}}{\partial P_\zeta}\,{\rm d}\theta=\frac{1}{2{\rm \pi}}\int_0^{T_\theta}\dot{\zeta}\,{\rm d}t = \frac{1}{2{\rm \pi}}\int_{\zeta_1(t=0)}^{\zeta_2(t=T_\theta)}\,{\rm d}\zeta,\\ \frac{\hat{\omega}_\zeta}{\hat{\omega}_\theta} & =\frac{(\Delta\zeta)_{T_{\theta}}}{2{\rm \pi}}. \end{aligned} \right\} \end{equation}

Considering also that

(5.9)\begin{equation} \langle\dot{\zeta}\rangle_{T_\theta} \doteq \frac{1}{T_\theta}\int_0^{T_\theta}\dot{\zeta}\,{\rm d}t = \frac{1}{T_\theta}\int_{\zeta_1(t=0)}^{\zeta_2(t=T_\theta)}\,{\rm d}\zeta =\frac{\hat\omega_\theta}{2{\rm \pi}}(\Delta\zeta)_{T_\theta}, \end{equation}

equations (5.8) and (5.9) lead us to the conclusion that

(5.10)\begin{equation} \hat\omega_\zeta=\dot{\hat\zeta}=\langle\dot\zeta\rangle_{T_\theta}, \end{equation}

suggesting that the frequency $\hat \omega _\zeta$ is directly associated with the bounce/transit averaged toroidal precession (White Reference White2015; Antonenas et al. Reference Antonenas, Anastassiou and Kominis2021).

The toroidal to poloidal frequency ratio calculated in (5.8) is associated with the kinetic resonance condition of the unperturbed GC particle motion with any non-axisymmetric perturbative mode of the form $F_{mn}(\psi )\exp [\textrm {i}(n\hat {\zeta }-m\hat {\theta })]$

(5.11)\begin{equation} \left. \begin{gathered} n\hat{\omega}_\zeta-m\hat{\omega}_\theta=0,\\ q_{{\rm kin}}\equiv\frac{\hat{\omega}_\zeta}{\hat{\omega}_\theta}=\frac{m}{n}, \end{gathered} \right\} \end{equation}

with $q_{\textrm {kin}}$ being the drift-frequency ratio, also known as the kinetic-$q$ factor, and $m,n$ being the (integer) poloidal and toroidal mode numbers, respectively. The concept of the kinetic-$q$ factor, first introduced by Gobbin et al. (Reference Gobbin, White, Marrelli and Martin2008), has a paramount role in resonant mode–particle interactions (White Reference White2014), and its significance was first reported when a discrepancy was detected between the location of the resonant orbits and the location of the resonant surfaces of the magnetic $q$ profile, in MST reversed field pinch (Fiksel et al. Reference Fiksel, Hudson, Den Hartog, Magee, O'Connell, Prager, Beklemishev, Davydenko, Ivanov and Tsidulko2005). The difference between kinetic and magnetic $q$ factors implies that kinetic and magnetic resonant islands, along with the accompanied chaoticity, may occur in different spatial positions, depending on the kinetic characteristic of each orbit, namely the energy, the magnetic moment, and the poloidal and toroidal momenta. In particular, higher energy particles experience significant radial drifts across the magnetic field lines, and their trajectory only partially resides in the vicinity of a magnetic island, suggesting that the chaoticity of the orbits cannot be directly derived from the chaoticity of the magnetic field lines. This is not the case for low-energy particles, whose radial drift is considerably smaller, and hence, particle trajectories follow the magnetic field lines, inheriting its chaoticity (Cambon et al. Reference Cambon, Leoncini, Vittot, Dumont and Garbet2014; He et al. Reference He, Wan, Sun, Jia, Shi, Wang and Zhang2019, Reference He, Sun, Wan, Gu and Jia2020; Moges et al. Reference Moges, Antonenas, Anastassiou, Skokos and Kominis2024).

To corroborate our arguments, regarding the expected changes of the orbital spectrum and the kinetic-$q$ factor, in this section, we present indicative cases, corresponding to those shown in figure 2. In figures 3–5, we present the orbital spectrum, that is, the poloidal and bounce/transit-averaged toroidal precession frequencies in panels (a), as well as the kinetic-$q$ factor $(q_{\textrm {kin}})$ in panels (b), in the absence of the radial electric field. Accordingly, panels (c,d) depict the same information when a radial electric field is present.

In particular, figure 3 depicts the orbital frequencies and the kinetic-$q$ factor for thermal particles corresponding to figure 2(a,b), with $\mu B_0=0.5\,\mathrm {keV}$ and $P_\zeta =-0.0272$, in the (a,b) absence and in the (c,d) presence of the radial electric field. The existence of a non-zero $E_r$ changes both quantitatively and qualitatively the orbital frequencies. The drastic qualitative changes, manifested by multiple branches, correspond to the introduction of additional orbit families due to the radial electric field. Kinetic-$q$ is modified accordingly, suggesting that the radial electric field drastically changes the conditions for resonant particle interaction with non-axisymmetric modes, since (5.11) can now be fulfilled for different mode numbers $(m,n)$ and particle energies. According to figure 3(d), the resonance condition can now be fulfilled for two different particle energies, for orbits belonging either in different families (upper branches) or in the same family (lower branch), where the latter presents a non-monotonic dependence on the energy. Moreover, the existence of a gap in the value range of $q_{\textrm {kin}}$ suggests that resonance conditions cannot be fulfilled for modes with an $m/n$ ratio residing within this gap. For example, a perturbative mode with $(m, n)=(10,-3)$ that can resonate with the particle motion when $E_r=0$ cannot resonate when $E_r\neq 0$. Such features evidently alter the resonant domain of the interaction upon the emergence of a radial electric field, cutting off or permitting specific modes to resonantly interact with the particles, indicating a major modification of stochastic particle transport in each case.

Figure 3. Effects of $E_r$ on the orbital spectrum and the kinetic-$q$ factor ($q_{\textrm {kin}}$) for thermal particles, with $\mu B_0=0.5\,\mathrm {keV}$, $P_\zeta =-0.0272$, corresponding to figure 2(a,b). (a,c) Poloidal frequency $\hat {\omega }_\theta$ (light blue points) and toroidal precession frequency $\hat {\omega }_\zeta$ (orange points), as functions of the energy $E$, for (a) $E_r=0$ and (c) $E_r \neq 0$. (b,d) Kinetic-$q$ factor $q_{\textrm {kin}}=m/n=\hat {\omega }_\zeta /\hat {\omega }_\theta$, as a function of the energy $E$, for (b) $E_r=0$ and (d) $E_r \neq 0$. Multiple branches correspond to different orbit families.

In figure 4, orbital frequencies and kinetic-$q$ factor are depicted for low-energy particles corresponding to figure 2(c,d), with $\mu B_0=2.0\,\mathrm {keV}$ and $P_\zeta =-0.025$. As already pointed out, the unconfined trapped orbits are transformed into confined trapped orbits due to the presence of $E_r$, but more importantly, the kinetic-$q$ curve is significantly changed. The orbital spectrum is modified due to the presence of the radial electric field in such a way that resonances with modes having negative $m/n$ can take place, whereas these modes are non-resonant when $E_r=0$.

Figure 4. Same as figure 3 for low energy particles with $\mu B_0=2\,\mathrm {keV}$, $P_\zeta =-0.025$, corresponding to figure 2(c,d). The presence of the radial electric field changes the sign and the monotonicity of the $q_{\textrm {kin}}(E)$ curve.

The case of mildly energetic counter-passing orbits corresponding to figure 2(e,f) is shown in figure 5. Although the modifications of the orbit shapes as well as of the orbital frequencies due to $E_r$ are not drastic, the respective effect on the kinetic-$q$ factor is quite important, as shown by comparing figure 5(b,d). In addition to the lack of resonances for $q_{\textrm {kin}}>2.62$ for $E_r \neq 0$, the non-monotonicity of the $q_{\textrm {kin}}(E)$ curve (also shown in the lower branch of figure 3d) introduces two qualitatively different features in comparison to the $E_r=0$ case. First, the non-monotonicity indicates the likeliness of particles with different energies (located at different flux surfaces) to resonantly interact with the same perturbative mode. For instance, a mode with $(m,n)=(5,2)$ could resonantly affect orbits with energy $E=14.7\,\mathrm {keV}$ when $E_r=0$, whereas all orbits with $E=\{14.7\,\mathrm {keV}, 16.8\,\mathrm {keV}, 18.4\,\mathrm {keV}\}$ will be susceptible to resonantly interact with the specific mode when a radial electric field is present. Second, the local extrema of the $q_{\textrm {kin}}(E)$ curve, where $q_{\textrm {kin}}'(E)=0$, indicate the existence of shearless points which have a great significance for stochastic transport, as they signify the onset of stochastic transport barriers (STBs), reducing the radial transport, even when chaotic orbits occur (Morrison Reference Morrison2000), as will also be discussed in the following section.

Figure 5. Same as figure 3 for mildly energetic particles with $\mu B_0=10\,\mathrm {keV}$, $P_\zeta =-0.0125$ corresponding to figure 2(e,f). The presence of the radial electric field renders the $q_{\textrm {kin}}(E)$ non-monotonic and introduces local extrema with important implications for stochastic transport related to stochastic transport barriers.

6. Resonant mode-particle interaction and stochastic transport in the presence of ${E_r}$

The calculations of the orbital spectrum and the kinetic-$q$ factor for the unperturbed GC motion in an axisymmetric LAR magnetic equilibrium in the presence of a radial electric field, allows for an a priori knowledge of important properties of stochastic transport under resonant mode–particle interaction with non-axisymmetric perturbative modes. More specifically, these calculations allow to pinpoint, with a remarkable accuracy, the regions of the six-dimensional phase space where significant particle and momentum transfer takes place, as well as the existence of dynamical barriers separating different regions of stochastic transport. This is of particular importance since the effects of resonant mode–particle interaction is strongly inhomogeneous in the phase space. It is worth emphasising that this information does not require time-consuming numerical particle tracing and provides physical intuition on the characteristics of complex particle dynamics and stochastic transport.

Time-independent perturbative magnetic modes can be given in the form

(6.1)\begin{equation} \delta \boldsymbol{B}=\boldsymbol{\nabla}\times \alpha\boldsymbol{B} \end{equation}

with $\alpha (\psi,\zeta,\theta )=\sum _{m,n}a_{mn}(\psi )\sin (n\zeta -m\theta )$, $a_{mn}(\psi )$ the amplitude profile of the perturbation, $m,n$ integers that correspond to poloidal and toroidal harmonics of the mode, and $\psi =P_\theta$ for the case of a LAR equilibrium (White Reference White2013b). This type of magnetic field perturbation is particularly useful under the GC approximation as it sufficiently describes the $\boldsymbol {\nabla }\psi$ component of any perturbation with practical interest, such as MHD activity of tearing or ideal modes, as well as resonant magnetic perturbations (RMPs) (White Reference White2013a,Reference Whiteb), whereas some possible limitations of that scheme are discussed by Ciaccio et al. (Reference Ciaccio, Veranda, Bonfiglio, Cappello, Spizzo, Chacón and White2013). The perturbation term is directly introduced as a modification in normalised parallel velocity, yielding the expression of the perturbed GC Hamiltonian (White Reference White1982; White & Chance Reference White and Chance1984)

(6.2)\begin{equation} \mathcal{H}=(\rho_\|-\alpha)^2 B^2/2 + \mu B + \varPhi. \end{equation}

Without loss of generality, in terms of the resonant character of mode–particle interactions and their effects on stochastic transport, in the following analysis, we consider perturbations with a constant mode amplitude, that is, $|a_{mn}|=\epsilon B_0$, with $\epsilon$ being designated as the ratio of the amplitude of the perturbative magnetic mode to the background magnetic field. It must be noted that, due to the nonlinear character of the canonical transformation to action-angle variables, a single mode in $(\zeta,\theta )$ results in a multi-mode Fourier expansion in terms of the $(\hat {\zeta },\hat {\theta })$ variables, according to (5.5a–c) (White Reference White2014, p. 109).

The axisymmetry-breaking perturbative modes render the GC Hamiltonian non- integrable, since the $\zeta$-dependence of the modes results in a no longer invariant toroidal momentum $P_\zeta$, whereas the time-independent character of the perturbations ensures the invariance of the total energy $E$. These features suggest that GC dynamics under time-independent, non-axisymmetric perturbations take place on constant energy surfaces of the phase space and facilitate their study in terms of Poincaré surfaces of section in the $(\zeta, P_\zeta )$ or $(\theta,P_\theta )$ planes, as well as the consideration of the kinetic-$q$ factor ($q_{\textrm {kin}}$) as a function of $P_\zeta$, for constant (invariant) values of the magnetic moment $\mu$ and the energy $E$.

In figure 6, we consider the case of thermal particles with $\mu B_0=0.5\,\mathrm {keV}$ and $E=1.5\,\mathrm {keV}$. Panel (a) depicts the projection of the unperturbed orbits in the absence and the presence of a radial electric field, for different values of the canonical toroidal momentum $P_\zeta$. The non-zero $E_r$ introduces unperturbed trapped orbits (red closed orbits), not existing for $E_r=0$ (coloured orbits). The kinetic-$q$ factor under the presence of the radial electric field, determining the position of the resonances with the perturbative mode, is depicted in panel (c) as a function of $P_\zeta$. The labelled red points indicate rational values of $q_{\textrm {kin}}$ corresponding to fractions of small integers, and therefore primary resonances with different Fourier components (in terms of the angle variables $\hat {\zeta }, \hat {\theta }$) of the perturbative mode with $(m,n)=(5,-3)$. Evidently, the exact locations of the resonant islands, as shown in a $(\zeta,P_\zeta )$ Poincaré surface of section in panel (d), are obtained with a remarkable accuracy from the curve $q_{\textrm {kin}}(P_\zeta )$. The number of resonant islands in $(\zeta,P_\zeta )$ Poincaré surface of section coincides with the denominator of the resonant fractions, while the numerator corresponds to the number of islands in a $(\theta,P_\theta )$ Poincaré surface of section, as shown in panel (b). It should be mentioned that the island width corresponding to different resonances in both Poincaré surfaces of section depends on the amplitude of each Fourier component of the perturbative mode, as expressed in angle variables, and determines the degree of the chaoticity of the phase space (Chirikov Reference Chirikov1979; Lichtenberg & Lieberman Reference Lichtenberg and Lieberman1992). In this specific case of thermal particles and perturbative mode, the phase space is mostly populated by regular orbits corresponding to well-defined KAM curves and island chains (Lichtenberg & Lieberman Reference Lichtenberg and Lieberman1992), and the perturbation does not lead to stochastic losses, since orbits are bounded by a surrounding KAM curve located inside the wall, as shown in panel (b). It is worth emphasising that the application of this specific perturbative mode $(m, n)=(5,-3)$ is non-resonant in this domain of the phase space when $E_r=0$, as can be seen in the range of $q_{\textrm {kin}}$ values shown in figure 3(b). The corresponding Poincaré surface of section in this case simply consists of plain KAM lines.

Figure 6. (a) Unperturbed phase space in $P_\zeta (\mu,E,P_\theta,\theta )$ representation for particles with $\mu B_0=0.5\,\mathrm {keV}$, $E=1.5\,\mathrm {keV}$. Coloured orbits are associated with the case $E_r=0$, while red orbits correspond to the $E_r\neq 0$ case. (b) Poincaré surface of sections at $\zeta =0$ for the perturbed Hamiltonian with $\epsilon =3\times 10^{-6}B_0$ and $(m,n)=(5,-3)$, in $\theta -P_\theta$ cross-section. (c) Demonstration of the semi-analytical profile of kinetic-$q$ (drift-resonance ratio) characterising constant energy orbits, for various values of $P_\zeta$, in the unperturbed system. (d) Poincaré surface of sections at $\theta =0$ when mode $(m,n)=(5,-3)$ is applied, in $\zeta -P_\zeta$ cross-section. Thick dashed red horizontal lines pinpoint the location of the excited resonant modes with respect to $P_\zeta$, exhibiting a perfect agreement between the numerically calculated values and the theoretically predicted values of the unperturbed system.

The case of low-energy particles with $\mu B_0=2\,\mathrm {keV}$ and $E=2.2\,\mathrm {keV}$ is shown in figure 7, where all unperturbed orbits are trapped for a non-zero $E_r$ (red orbits), as shown in panel (a). The location of resonance island chains, in the presence of a perturbative mode with $(m,n)=(3,-2)$, is accurately given by the rational values of $q_{\textrm {kin}}(P_\zeta )$, as shown in panels (c,d). Hence, the dominant mode $(m,n)=(3,-2)$ is identified by the two-island chain at $P_\zeta =-0.02597$ in panel (d) and by the three-island encircling chain in panel (c), having one of its elliptical points approximately at $\theta \simeq {\rm \pi}/10$, $P_\theta \simeq 0.825 P_{\theta \, \textrm {wall}}$. Accordingly, the secondary resonance $(m,n)=(5,-4)$ is identified by the four-island chain at $P_\zeta =-0.0268$ and a corresponding five-island encircling chain with one of each elliptical points approximately at $\theta \simeq 0$, $P_\theta \simeq 0.86 P_{\theta \, \textrm {wall}}$. In both Poincaré surfaces of section, we can observe the onset of stochastisation near the separatrix of the primary island with $(m,n)=(3,-2)$.

Figure 7. Same as figure 6, for particles with $\mu B_0=2\,\mathrm {keV}$, $E=2.2\,\mathrm {keV}$. Applied perturbations correspond to the fluctuating magnetic mode $(m,n)=(3,-2)$ with $\epsilon =2\times 10^{-6}B_0$.

For the case of higher-energy particles with $\mu B_0=10\,\mathrm {keV}$ and $E=18\,\mathrm {keV}$, depicted in figure 8, it is evident that the presence of a radial electric field does not significantly modify the unperturbed counter-passing orbits, as shown in panel (a). However, in accordance with figure 5, the kinetic-$q$ factor is drastically modified, as shown in panel (c). The non-monotonicity of the $q_{\textrm {kin}}(P_\zeta )$ curve results in the emergence of two local extrema, one local minimum at $(q_{\textrm {kin}},P_\zeta )_{\textrm {min}}=(2.47,-0.0123)$ and one local maximum at $(q_{\textrm {kin}},P_\zeta )_{\textrm {max}}=(2.61,-0.0111)$. The first consequence of this non-monotonic dependence concerns the multiplicity of specific resonances, in the sense that a particular resonant mode can interact with particles having different toroidal momentum $P_\zeta$, or equivalently, with particles that are located at different flux surfaces (different $P_\theta$). This feature is quite essential for particle and energy transport along the radial direction, as particles in different positions can undergo a resonant interaction with the same perturbative mode. Provided that the perturbation strength is sufficiently large, for the resonances to become overlapping, this mechanism describes how a particle can start from the plasma core and drift all the way to the wall and become lost, entirely through stochastic transport. Second, the local extrema $q_{\textrm {kin}}'(P_\zeta )=0$ indicate regions of zero kinetic shear which are responsible for the generation of stochastic transport barriers between two adjacent island-chains (Horton et al. Reference Horton, Park, Kwon, Strozzi, Morrison and Choi1998; Morrison Reference Morrison2000; Gobbin et al. Reference Gobbin, Bonfiglio, Escande, Fassina, Marrelli, Alfier, Martines, Momo and Terranova2011; Caldas et al. Reference Caldas, Viana, Abud, Fonseca, Guimarães Filho, Kroetz, Marcus, Schelin, Szezech and Toufen2012; Marcus et al. Reference Marcus, Roberto, Caldas, Rosalem and Elskens2019; Grime et al. Reference Grime, Roberto, Viana, Elskens and Caldas2023).

Figure 8. Same as figure 6, for trajectories with $\mu B_0=10\,\mathrm {keV}$, $E=18\,\mathrm {keV}$. Applied perturbations correspond to the synergetic effect of two resonant modes $(m_1,n_1)=(5,2)$ with $\epsilon _1=5\times 10^{-6}B_0$, and $(m_2,n_2)=(13,5)$ with $\epsilon _2=0.9\times 10^{-6}B_0$. Magenta and cyan lines indicate the existence of two STBs, due to $E_r$ shear, effectively separating neighbouring chaotic regions. The locations of the STBs are in perfect agreement with the analytically calculated locations of shearless points of $q_{\textrm {kin}}(P_\zeta )$ curve of panel (c).

Figure 8(b,d) illustrate the Poincaré surfaces of section corresponding to the unperturbed cases of panels (a) and (c), at $\zeta =0$ and $\theta =0$, respectively, in the presence of two perturbing modes with $(m,n)=(5,2)$ and $(m,n)=(13,5)$. It is clearly shown that the locations of the resonant island chains are very accurately predicted by the values of the kinetic-$q$ factor $q_{\textrm {kin}}(P_\zeta )$. Resonances with the $(m,n)=(5,2)$ mode appear for three different values of $P_\zeta$, whereas resonances with $(m,n)=(13,5)$ appear for two different values. In both cases, adjacent regions corresponding to resonances with the same mode, although highly chaotic, are well separated by persistent KAM curves forming stochastic transport barriers and bounding the complex particle motion, at $P_\zeta$ values corresponding to local extrema of the kinetic-$q$ factor. It is worth emphasising that non-axisymmetric perturbations induce magnetic field line chaoticity, with TBs bounding the chaotic regions of the magnetic field lines phase space, when non-monotonic $q$ profiles are considered. In such cases, STBs appear for low-energy, field-line following particles at shearless points corresponding to local extrema of the $q$ factor, where $q'(\psi )=0$. However, for a high-energy particle with large drifts across the magnetic field lines, the effective kinetic shear is properly described by the kinetic-$q$ factor (Gobbin et al. Reference Gobbin, White, Marrelli and Martin2008; White Reference White2014; Antonenas et al. Reference Antonenas, Anastassiou and Kominis2021), with its extrema pinpointing the location of the STB. Both cases are introduced on equal footing in the third and fourth term, respectively, of the equation of motion for $\dot {\theta }$, shown in (3.8). Experimental findings indicate that there is a strong correlation between the appearance of local extrema in $q_{\textrm {kin}}$ and the elimination of transport for high-energy particles, when an edge-localised radial electric field is present (Sanchis et al. Reference Sanchis, Garcia-Munoz, Snicker, Ryan, Zarzoso, Chen, Galdon-Quiroga, Nocente, Rivero-Rodriguez and Rodriguez-Ramos2019).

7. Summary and conclusions

The presence of a radial electric field in the pedestal area of a tokamak imposes significant modification in the orbit topology. Rearranged or bifurcated critical points of the phase space may dramatically change the type of the orbits residing in that area and significantly modify particle prompt losses, especially for thermal or low-energy particles. The radial electric field significantly alters the orbital spectrum of the particles in such a way that it can modify the location of the resonances in the particle phase space, and prevent or allow resonances with specific modes. The resonance conditions are determined by the kinetic-$q$ factor, which contains all the essential information for the shear of the background magnetic field, the $\boldsymbol {E}\times \boldsymbol {B}$ shear flow, as well as the neoclassical finite-orbit-width effects in a toroidal plasma configuration. Moreover, local extrema of the kinetic-$q$ factor correspond to locations where transport barriers are formed, preventing the extended stochastic particle transport. It is shown that the calculated kinetic-$q$ contains all the essential information of the macroscopic plasma configuration, allowing for the a priori knowledge of the exact locations of resonances and transport barriers that determine particle, energy and momentum transport, as confirmed by numerical particle tracing simulations.