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Negative Turbulent Magnetic Diffusivity ๐œท\beta effect in a Magnetically Forced System

Kiwan Park,11footnotetext: Corresponding author. โ€ƒโ€ƒ Myung-Ki Cheoun
Abstract


We have studied the large scale dynamo process forced with helical magnetic energy (magnetic helicity). The magnetically driven dynamo is not so well studied as kinetically forced dynamo. It has been thought to represent the amplification of magnetic field in the stellar corona, accretion disk, or plasma lab. However, the interaction between the helical magnetic field and plasma is a more fundamental phenomenon that can be extended to the early Universe. The scale-invariant helical magnetic field not only explains the currently observed large scale astrophysical magnetic fields but also has information on the horizon scale in the early Universe.

The interaction between magnetic field and plasma is inherently non-linear, making its mechanism difficult to understand. But, if the plasma system is driven with helical field, the process can be linearized with ฮฑ\alpha&ฮฒ\beta and large scale magnetic field ๐ยฏ{\overline{\bf B}}. Conventionally, ฮฑ\alpha effect is thought to transfer magnetic field to the large scale regime, and ฮฒ\beta effect diffuses magnetic field. However, these conclusions are based on the incompletely derived ฮฑ\alpha&ฮฒ\beta. In this paper, to get the exact profiles of evolving ฮฑ\alpha&ฮฒ\beta, we solved a coupled semi-analytic equation set and applied the result to simulation data for the large scale magnetic helicity HยฏM\overline{H}_{M} and magnetic energy EยฏM\overline{E}_{M}.

Our result shows that the averaged ฮฑ\alpha effect decreases before making a significant contribution to the amplification of ๐ยฏ{\overline{\bf B}} field. Rather, ฮฒ\beta effect, which keeps negative, de facto plays a key role in the amplification of Bยฏ\overline{B} field with Laplacian (โˆ‡2โ†’โˆ’k2\nabla^{2}\rightarrow-k^{2}). And, this negative diffusivity accounts for the attenuation of plasma kinetic energy EยฏV\overline{E}_{V}. Helical plasma velocity field UU plays a more complex role in dynamo. In addition to the conventional diffusion effect, poloidal field ๐”pโ€‹oโ€‹l{\bf U}_{pol} and toroidal field ๐”tโ€‹oโ€‹r{\bf U}_{tor} interact with ๐โ‹…โˆ‡๐”{\bf B}\cdot\nabla{\bf U} and โˆ’๐”โ‹…โˆ‡๐-{\bf U}\cdot\nabla{\bf B} to produce ฮฑ\alpha effect and negative ฮฒ\beta effect. We discussed this process using the theoretical method and the intuitive field structure model.

1 Introduction and method

Most celestial plasma systems are constrained by magnetic field BB. BB field takes energy from the turbulent plasma (dynamo), and the amplified field back reacts to the system (magnetic back reaction). Through this mutual interaction, BB field controls the rate of formation of a star and accretion disk [1, 2]. Also, the balanced pressure between the magnetic field and plasma can decide the stability of the system (see sausage, kink, or Kruskal-Schwarzschild instability, see [3]). However, their detailed internal mechanisms related to the interaction between plasma and magnetic field are not yet clearly understood.

The amplification of BB field in plasma usually requires seed magnetic field. However, the origin of seed field (primordial magnetic field, PMF) is still under debate. At present, its cosmological origins are divided into the era of inflationary genesis and post-inflationary magneto-genesis.

The first inflationary scenario generates the very large scale PMF, but it needs the breaking of conformal symmetry by the interaction of the electromagnetic field and the gravitational field. The breaking of the conformal symmetry is to consider the Electro-Magnetic (EM) coupling to scalar field [4, 5], coupling to the modified general relativity f(R) theory, coupling to pseudo scalar field and so on. The PMF strength could be generated by quantum fluctuations and has been estimated as 10โˆ’5โ€‹nโ€‹Gโˆ’1โ€‹nโ€‹G10^{-5}nG-1nG[6].

The second scenario is based on the cosmological Quantum Chromo Dynamics (QCD) phase transition (โˆผ\sim250MeV) [7, 8] and the electroweak phase transition (โˆผ\sim100MeV). The PMF could be generated by collision and percolation of some bubbles from the first order transition and estimated as 10โˆ’710^{-7}nG by the quark-hadron and 10โˆ’1410^{-14}nG - 10โˆ’810^{-8}nG order by the electroweak transition.

The third scenario can occur during or after the epoch of photon last scattering. The PMF can be produced by non-vanishing vorticity, which arises from the non-zero electron and proton fluid angular velocities by the different masses of proton and electron in the gravitational field (Harrisonโ€™s mechanism, [9]). The PMF is thought to be about 10โˆ’9โ€‹nโ€‹G10^{-9}nG

The second and third scenarios are thought to occur on a correlation scale smaller than the Hubble radius, by which we expect a suitable field generated by another dynamical effect, for instance, Biermann battery mechanism [10]. When the hot ionized particles (plasma) collide mutually, the fluctuating electron density โˆ‡ne\nabla n_{e} and pressure โˆ‡pe\nabla p_{e} (or temperature โˆ‡Te\nabla T_{e}) can be misaligned. This instability โˆ’โˆ‡pe/neโ€‹e-\nabla p_{e}/n_{e}e can drive currents to generate magnetic fields. Also, the neutrino interaction with charged leptons at the early epoch is thought to have generated primordial magnetic helicity, the measure of twist and linkage of magnetic fields (HM=โŸจ๐€โ‹…๐โŸฉH_{M}=\langle{\bf A}\cdot{\bf B}\rangle, ๐=โˆ‡ร—๐€{\bf B}=\nabla\times{\bf A}) [11]. But, since the neutrino interaction exists not only in the early universe epoch but also are abundant in the present Universe including the Sun, lepton-neutrino interaction in primordial plasma can be one of the promising candidates of (origin) magnetic field generation.

The PMF may have scalar, vector and tensor fluctuations, which may affect CMB observables such as the CMA anisotropies and the matter power spectrum. Also the helical PMF may produce parity-odd cross correlations which results in the non-Gaussian CMB. The PMF effect on the BBN has been shown to be not large enough to explain the Li7 problem [12]. But a recent paper [13] assumed inhomogeneous PMF, which causes inhomogeneous temperature and non-Maxwell Boltzmann (MB) velocity distributions of baryons, and affect the relevant nuclear reaction on the BBN epoch.

These quantum fluctuating effects on magnetic field generation were followed by that of the collective plasma particles, i.e., fluid. The statistical feature of charged particles constraining one another became more important. Their aggregative motion formed a flow, which interacted with the seed magnetic fields, led to the amplification (dynamo) of BB field or its decay according to the various conditions. The evolution of magnetic field is now explained with Faraday equation โˆ‚๐/โˆ‚t=โˆ’โˆ‡ร—๐„{\partial\bf B}/\partial t=-\nabla\times{\bf E} combined with Ohmโ€™s law ฮทโ€‹๐‰=(๐„+๐”ร—๐)\eta{\bf J}=({\bf E}+{\bf U}\times{\bf B}) in the level of magnetohydrodynamics (MHD).222๐‰,ฮท,๐„,๐”{\bf J},\,\eta,\,{\bf E},\,{\bf U} are current density, magnetic diffusivity, electric field, and plasma velocity. This combined equation, i.e., magnetic induction equation implies that any electromagnetic instability such as Biermannโ€™s battery effect or lepton-neutrino interaction can be merged into electromotive force (EMF, โˆผ๐”ร—๐\sim{\bf U}\times{\bf B} omitting โˆซ๐‘‘ฯ„\int d\tau) in the equation: โˆ‚๐/โˆ‚t=โˆ‡ร—(๐”ร—๐โˆ’ฮทโ€‹๐‰+๐Ÿmโ€‹aโ€‹g){\partial\bf B}/\partial t=\nabla\times({\bf U}\times{\bf B}-\eta{\bf J}+{\bf f}_{mag}). Then, the provided magnetic energy grows and propagates in the plasma system. This type of process is called magnetic forcing dynamo (MFD).

In comparison with kinetic forcing dynamo (KFD), MFD has its own characteristic features. For example, seed magnetic field is not necessary, and magnetic helicity is not conserved. The most unusual thing is that plasma kinetic energy (EV=U2/2E_{V}=U^{2}/2) is not converted into magnetic energy (EM=B2/2E_{M}=B^{2}/2). Rather, partial magnetic energy is converted into kinetic energy through Lorentz force. The converted velocity field forms EMF, which transfers magnetic energy. This energy convert process minimizes the thermal dissipation in plasma so that the amplification of magnetic field in MFD is more efficient than that of KFD. In our case, we used only 20% of forcing strength compared to KFD, but the saturated magnetic energy is larger. MFD itself is one of the prominent processes that connect the cosmological magnetic field and the seed magnetic field for KFD.

Basically, dynamo is a nonlinear phenomenon. However, when the field is helical (โˆ‡ร—๐…=ฮปโ€‹๐…\nabla\times{\bf F}=\lambda{\bf F}), the dynamo process, i.e., EMF can be linearized with ฮฑ\alpha & ฮฒ\beta and large scale magnetic field ๐ยฏ\overline{\bf B}. At present, the exact analytic forms of ฮฑ\alpha & ฮฒ\beta are unknown. Only, their sketchy representations can be derived with closure theory and function reiterative method, e.g., mean field theory (MFT, [14]), eddy damped quasi normal markovianized approximation (EDQNM, [15]), direct interactive approximation (DIA, [16]). Physically, ฮฑ\alpha effect is thought to arise with Coriolis force and buoyancy (kinetic helicity โ€˜โˆ’โŸจ๐ฎโ‹…โˆ‡ร—๐ฎโŸฉ-\langle{\bf u}\cdot\nabla\times{\bf u}\rangle) and gradually becomes quenched by current helicity โ€˜โŸจ๐›โ‹…โˆ‡ร—๐›โŸฉ(=k2โŸจ๐šโ‹…โˆ‡ร—๐›โŸฉ\langle{\bf b}\cdot\nabla\times{\bf b}\rangle\,(=k^{2}\langle{\bf a}\cdot\nabla\times{\bf b}\rangle, k: wavenumber in Fourier space)โ€™ generated by the growing magnetic back reaction333The over bar in the variable Xยฏ\overline{X} means the large scale quantity, and the small letter xx means the quantity in the small (turbulent) scale regime. And, the angle bracket indicates its spatial average over the large scale regime: (1/2โ€‹L)3โ€‹โˆซโˆ’LLXโ€‹๐‘‘๐ซ(1/2L)^{3}\int^{L}_{-L}{X}d{\bf r}. We assume โŸจXยฏโŸฉโˆผXยฏ\langle\overline{X}\rangle\sim\overline{X}. Adding these two effects qualitatively explains how the large scale magnetic field grows and finally becomes saturated. However, for some systems like Solar(stellar) corona or a jet structure above the accretion disk, it is hard to expect that such helical kinetic motion exists and triggers the dynamo process. Rather, the transferred helical magnetic field (โˆ‡ร—๐=ฮป๐(\nabla\times{\bf B}=\lambda{\bf B}) from the structures is more likely to play a key role in dynamo.

Theoretically, ฮฑ\alpha effect is derived from the differentiation of EMF over time: โˆ‚โŸจ๐ฎร—๐›โŸฉ/โˆ‚t\partial\langle{\bf u}\times{\bf b}\rangle/\partial t. โˆ‚๐ฎ/โˆ‚t\partial{\bf u}/\partial t and โˆ‚๐›/โˆ‚t\partial{\bf b}/\partial t are replaced by MHD equations leading to ฮฑโˆผโˆซ๐‘‘tโ€‹(โˆ’โŸจ๐ฎโ‹…โˆ‡ร—๐ฎโŸฉ+โŸจ๐›โ‹…โˆ‡ร—๐›โŸฉ)\alpha\sim\int dt(-\langle{\bf u}\cdot\nabla\times{\bf u}\rangle+\langle{\bf b}\cdot\nabla\times{\bf b}\rangle). During this analytic calculation, there is no constraint on the derivation of โˆ’โŸจ๐ฎโ‹…โˆ‡ร—๐ฎโŸฉ-\langle{\bf u}\cdot\nabla\times{\bf u}\rangle and โŸจ๐›โ‹…โˆ‡ร—๐›โŸฉ\langle{\bf b}\cdot\nabla\times{\bf b}\rangle. The calculation is done only with tensor identity and the assumption of isotropy. This implies that we can drive the system either kinetic energy or magnetic energy. Current density ๐‰\bf J is the source of magnetic field as Biot-Savart law and Maxwell theory indicate. Moreover, to produce magnetic helicity in a lab., ๐‰\bf J is transmitted along magnetic field. These theoretical and experimental examples show that helical magnetic forcing dynamo (HMFD) is not forbidden but a feasible process in nature.

However, there are a couple of things to be made clear in HMFD. The growth rate (ฮฑ\alpha) should be larger than the dissipation rate to arise magnetic field. If current helicity is a unique component in ฮฑ\alpha effect, magnetic field grows without stop. To prevent this catastrophic amplification, there should be sort of a constraining effect such as kinetic helicity. However, since helical magnetic field โˆ‡ร—๐โˆผ๐\nabla\times{\bf B}\sim{\bf B} nullifies Lorentz force ๐‰ร—๐{\bf J}\times{\bf B}, the generation of helical velocity field by ๐{\bf B} looks contradictory. Moreover, even if the generation of ๐”\bf U is explained, there remain tricky issues in the conservation and chirality of helicity. For example, if the system is forced by right handed(++) helical kinetic energy, left handed(โˆ’-) magnetic helicity is generated and inversely cascaded. And, this (โˆ’-) magnetic helicity in the large scale produces (++) magnetic helicity in the small-scale regime to conserve magnetic helicity in the system. However, in HMFD, if (++) helical magnetic energy drives the system, (++) magnetic helicity is generated in the whole scale.

Besides, the scale invariant helical magnetic field, i.e., magnetic helicity provides us with information on the horizon during inflation. The correlation length of PMF is constrained by hubble horizon, beyond which the correlation vanishes with sudden cut-off. Therefore, within the subhorizon with the condition of ๐โ‹…๐ง^=0{\bf B}\cdot{\bf\hat{n}}=0, magnetic helicity becomes gauge free. However, the correlation length scale will be smaller than the typical galaxy scale. Even if the scale had been expanded through MHD process, the strength of magnetic field would have become too weak. An efficient dynamo process by helicity leading to both inverse cascade of magnetic energy and scale expansion is required.

In the present paper, to explain the inconsistent features depending on the forcing method, we apply the analytic method and field structure model used in helical kinetic forcing dynamo [17] to helical magnetic forcing dynamo. Followed by this introductory section, numerical method and related MHD equations for simulation are introduced in chapter 2. In chapter 3, we show numerical results for the evolving B{B} field and its inverse cascade to the large scale regime. And then, we show the evolving profile of ฮฑ\alpha & ฮฒ\beta along with the growth of BB field and investigate their physical features and mutual relations. In chapter 4, we discuss the parameterisations of EMF: โŸจ๐ฎร—๐›โŸฉโˆผโˆซdฯ„(ฮฑ๐ยฏโˆ’ฮฒโˆ‡ร—๐ยฏ\langle{\bf u}\times{\bf b}\rangle\sim\int d\tau(\alpha\overline{\bf B}-\beta\nabla\times\overline{\bf B}) and compare them using numerical data and analytic approach. Using field structure model, we explain the intuitive meaning of ฮฑ\alpha effect and how ฮฒ\beta becomes negative. Then, to supplement them, we derive ฮฒ\beta coefficient again when the field is helical. ฮฒ\beta effect also explains how the plasma velocity field is suppressed when the system is forced by helical magnetic field. This work focuses on the physical mechanism of helical forcing dynamo which occurs in the fundamental level of astro-plasma system. In chapter 5, we summarize our work.

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Figureย 1: Plot (a) & (c) show the logarithmic evolution of energy and helicity of the system forced with right handed helical magnetic field (fh=+1f_{h}=+1). Plot (b) & (d) are the same as (a) & (c), but the system was forced with left handed helical magnetic field (fh=โˆ’1f_{h}=-1). In (c), (d), k=5k=5 indicates the forcing scale eddy, and k=8k=8 indicates one of the small scale ones. The red dashed line means magnetic energy โŸจb2โŸฉ\langle b^{2}\rangle, and the red dotted one means its helical contribution kโ€‹โŸจ๐šโ‹…๐›โŸฉk\langle{\bf a}\cdot{\bf b}\rangle. Here, small character u,bu,\,b represent the turbulent scale regime. The symbol (B), (U) are to indicate they are for magnetic field and velocity field. In forcing scale (k=5), magnetic energy and its helical part are practically the same so that the corresponding lines are overlapped. On the other hand, the black solid line indicates kinetic energy โŸจu2โŸฉ\langle u^{2}\rangle, and the black dotted line indicates its helical part โŸจ๐ฎโ‹…โˆ‡ร—๐ฎโŸฉ/k\langle{\bf u}\cdot\nabla\times{\bf u}\rangle/k. In (a) & (c) kinetic and magnetic helicity clearly show up, but those in (b) & (d) are not shown except some part of large scale kinetic helicity. This indicates that the polarization of helicity in HMFD, except the large scale velocity, is consistently decided by forcing magnetic field.
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Figureย 2: The evolution of helicity ratio: kโ€‹โŸจ๐€โ‹…๐โŸฉ/โŸจB2โŸฉk\langle{\bf A}\cdot{\bf B}\rangle/\langle B^{2}\rangle for magnetic energy and helicity, โŸจ๐”โ‹…โˆ‡ร—๐”โŸฉ/kโ€‹โŸจU2โŸฉ\langle{\bf U}\cdot\nabla\times{\bf U}\rangle/k\langle U^{2}\rangle for kinetic energy and helicity (k=1, 5, 8). (a) It should be noted that fhf_{h} of large scale magnetic field (red thick line) is not 1 from the first. Rather, it begins from a low value and converges to 1 as the system becomes saturated. (b) fhf_{h} of large scale magnetic field converges to -1. The constantly saturated magnetic helicity ratio that kk for the large scale field is clearly 1, not 2\sqrt{2}. Moreover, the wavenumber does not depend on time with the normalized code data.

2 Numerical method

The basic MHD equations are composed of continuity, momentum, and magnetic induction equation as follows:

โˆ‚ฯโˆ‚t\displaystyle\frac{\partial\rho}{\partial t} =\displaystyle= โˆ’๐”โ‹…โˆ‡ฯโˆ’ฯโ€‹โˆ‡โ‹…๐”,\displaystyle-{\bf U}\cdot{\bf\nabla}\rho-\rho{\bf\nabla}\cdot{\bf U}, (2.1)
โˆ‚๐”โˆ‚t\displaystyle\frac{\partial{\bf U}}{\partial t} =\displaystyle= โˆ’๐”โ‹…โˆ‡๐”โˆ’โˆ‡lnโ€‹ฯ+1ฯโ€‹๐‰ร—๐\displaystyle-{\bf U}\cdot{\bf\nabla}\mathbf{U}-{\bf\nabla}\mathrm{ln}\,\rho+\frac{1}{\rho}{\bf J}\times{\bf B} (2.2)
+ฮฝโ€‹(โˆ‡2๐”+13โ€‹โˆ‡โˆ‡โ‹…๐”)+fkโ€‹iโ€‹n,\displaystyle+\nu\big{(}{\bf\nabla}^{2}{\bf U}+\frac{1}{3}{\bf\nabla}{\bf\nabla}\cdot{\bf U}\big{)}+\textbf{f}_{kin},
โˆ‚๐€โˆ‚t\displaystyle\frac{\partial\mathbf{A}}{\partial t} =\displaystyle= ๐”ร—๐โˆ’ฮทโ€‹โˆ‡ร—๐+fmโ€‹aโ€‹g.\displaystyle\mathbf{U}\times\mathbf{B}-\eta\nabla\times\mathbf{B}+\textbf{f}_{mag}. (2.3)
(โ‡’โˆ‚๐โˆ‚t\displaystyle\bigg{(}\Rightarrow\frac{\partial\mathbf{B}}{\partial t} =\displaystyle= โˆ‡ร—(๐”ร—๐)+ฮทโˆ‡2๐+โˆ‡ร—fmโ€‹aโ€‹g),\displaystyle\nabla\times(\mathbf{U}\times\mathbf{B})+\eta\nabla^{2}\mathbf{B}+\nabla\times\textbf{f}_{mag}\bigg{)}, (2.4)

Here, the symbols ฯ\rho, ฮฝ\nu, and ฮท\eta indicate density, kinematic viscosity, and magnetic diffusivity. โ€˜Uโ€™ is in the units of sound speed csc_{s}, and โ€˜Bโ€™ is normalized by (ฯ0โ€‹ฮผ0)1/2โ€‹cs(\rho_{0}\,\mu_{0})^{1/2}c_{s} (ฮผ0:\mu_{0}: magnetic permeability in vacuum. The variables in these equations are unitless.)

The fields ๐”\bf U, ๐\bf B can be separated into the large scale fields ๐”ยฏ\overline{\bf U}, ๐ยฏ\overline{\bf B} and turbulent small scale ones ๐ฎ\bf u, ๐›\bf b. Analytically, the evolution of ๐ยฏ\overline{\mathbf{B}} can be represented as follows:

โˆ‚๐ยฏโˆ‚t\displaystyle\frac{\partial\overline{\mathbf{B}}}{\partial t} โˆผ\displaystyle\sim โˆ‡ร—โŸจ๐ฎร—๐›โŸฉ+ฮทโ€‹โˆ‡2๐ยฏ,\displaystyle\nabla\times\langle\mathbf{u}\times\mathbf{b}\rangle+\eta\nabla^{2}\overline{\mathbf{B}}, (2.5)
โˆผ\displaystyle\sim โˆ‡ร—(ฮฑโ€‹๐ยฏ)+(ฮฒ+ฮท)โ€‹โˆ‡2๐ยฏ\displaystyle\nabla\times(\alpha\overline{\mathbf{B}})+(\beta+\eta)\nabla^{2}\overline{\mathbf{B}} (2.6)

Since ฮฑ\alpha&ฮฒ\beta are turbulent quantities, their curl effect over the large scale is negligible. Then, with some rearrangement, we can derive Eq.ย (2.6). And, this diffusion equation can be analytically solved with some appropriate closure theory. However, since Eq.ย (2.1)-(2.3) should be numerically solved, we used Pencil-Code [18](see the manual http://pencil-code.nordita.org). Pencil-code is a 6th order finite-difference code for compressible fluid dynamics (CFD) with magnetic field. The code solves vector potential โ€˜๐€\bf Aโ€™ in Eq.ย (2.3) instead of magnetic field โ€˜๐{\bf B}โ€™ Eq.ย (2.4). Solving โ€˜๐€\bf Aโ€™, the condition of divergence free magnetic field (โˆ‡โ‹…๐=0\nabla\cdot{\bf B}=0) is met without any numerical manipulation. Moreover, magnetic helicity HM(=โŸจ๐€โ‹…๐โŸฉ)H_{M}(=\langle{\bf A}\cdot{\bf B}\rangle) as well as magnetic energy EM(=โŸจB2/2โŸฉ)E_{M}(=\langle B^{2}/2\rangle) can be calculated free from the gauge issue with the assumption of the simply connected volume bounded by a magnetic surface (๐โ‹…n^=0{\bf B}\cdot\hat{n}=0.)

We initially gave a random seed magnetic field B0โˆผ10โˆ’4B_{0}\sim 10^{-4} (no unit) to a cube simulation box (8ฯ€3(8\pi^{3}) with a periodic boundary condition. But, what determines the evolution of the system is the forcing method. We used a forcing function as follows:

๐Ÿโ€‹(k,t)=iโ€‹๐คโ€‹(t)ร—(๐คโ€‹(t)ร—๐ž^)โˆ’ฮปโ€‹|๐คโ€‹(t)|โ€‹(๐คโ€‹(t)ร—๐ž^)kโ€‹(t)2โ€‹1+ฮป2โ€‹1โˆ’(๐คโ€‹(t)โ‹…๐ž)2/kโ€‹(t)2.\displaystyle{\bf f}(k,\,t)=\frac{i\mathbf{k}(t)\times(\mathbf{k}(t)\times\mathbf{\hat{e}})-\lambda|{\bf k}(t)|(\mathbf{k}(t)\times\mathbf{\hat{e}})}{k(t)^{2}\sqrt{1+\lambda^{2}}\sqrt{1-(\mathbf{k}(t)\cdot\mathbf{e})^{2}/k(t)^{2}}}. (2.7)

This is the Fourier transformed function represented by a wavenumber โ€˜kkโ€™, helicity ratio controller ฮป\lambda, and arbitrary unit vector โ€˜๐ž^\mathbf{\hat{e}}โ€™. โ€˜kkโ€™ is inversely proportional to the eddy scale lโˆผ1/kl\sim 1/k. For instance, k=1k=1 indicates the large scale regime, and k>2k>2 indicates the small (turbulent) scale regime. We gave helical magnetic field (energy) at the randomly chosen wavenumber kk, which is constrained by โŸจkโŸฉaโ€‹vโ€‹eโ‰กkfโˆผ5\langle k\rangle_{ave}\equiv k_{f}\sim 5. This forcing function can be located at Eq.ย (2.2) (KFD), or Eq.ย (2.3) (MFD). And, if ฮป\lambda is +(โˆ’)โ€‹1+(-)1, the forcing energy is fully right (left) handed helical field iโ€‹๐คร—๐Ÿ=ยฑkโ€‹๐Ÿi\mathbf{k}\times\mathbf{f}=\pm k\mathbf{f}. But, ฮป=0\lambda=0 yields a nonhelical forcing source.

Of course, the forcing source in nature is different from Eq.(2.7). In Appendix, we introduced two examples of magnetic forcing dynamo fmโ€‹aโ€‹gf_{mag}: Biermann battery effect and neutrino-lepton interaction. One of the most essential differences between them is magnetic helicity that decides the direction of magnetic energy transfer. Biermann effect does not have helicity so that the magnetic energy cascades toward the smaller scale regimes (small scale dynamo). In contrast, neutrino-lepton interaction yields magnetic helicity, i.e., ฮฑ\alpha effect, which can play an important role in large scale dynamo.

We prepared for the two systems with a unit magnetic Prandtl number Pโ€‹rM=ฮท/ฮฝ=1Pr_{M}=\eta/\nu=1. ฮท=ฮฝ=6ร—10โˆ’3\eta=\nu=6\times 10^{-3}, and numerical resolution is 4003400^{3}. They were forced by Eq.ย (2.7) with fully helical magnetic field (ฮป=+1\lambda=+1 or โˆ’1-1 at k=5k=5). We used basic data set such as kinetic energy EV(=โŸจU2โŸฉ/2)E_{V}(=\langle U^{2}\rangle/2), magnetic energy EM(=โŸจB2โŸฉ/2)E_{M}(=\langle B^{2}\rangle/2), kinetic helicity โŸจ๐”โ‹…โˆ‡ร—๐”โŸฉ\langle{\bf U}\cdot\nabla\times{\bf U}\rangle, and magnetic helicity โŸจ๐€โ‹…๐โŸฉ\langle{\bf A}\cdot{\bf B}\rangle. The stability of code and data have been verified.

3 Numerical Result

The system in Fig.ย 1(a), 1(c) is forced by the fully positive (right-handed) helical magnetic field (red dashed line, helicity ratio of forcing energy: fhโ‰กkfโ€‹โŸจ๐šโ‹…๐›โŸฉ/โŸจb2โŸฉ=1,kf=5f_{h}\equiv k_{f}\langle{\bf a}\cdot{\bf b}\rangle/\langle b^{2}\rangle=1,\,k_{f}=5 forcing wavenumber). In contrast, the system in the right panel Fig.ย 1(b), 1(d) is forced by the fully negative (left-handed) magnetic helicity (fh=โˆ’1f_{h}=-1). Peak speed UU is โˆผ2ร—10โˆ’3\sim 2\times 10^{-3}, and magnetic Reynolds number is defined as Rโ€‹eMโ‰กUโ€‹L/ฮทโˆผ2โ€‹ฯ€/3Re_{M}\equiv UL/\eta\sim 2\pi/3, where LL, ฮท\eta are 2โ€‹ฯ€2\pi and 6ร—10โˆ’36\times 10^{-3}, respectively. In HMFD, the least amount of magnetic energy is transferred to plasma.

In Fig.ย 1(a), large scale magnetic energy โŸจBยฏ2โŸฉ\langle{\overline{B}}^{2}\rangle (=2โ€‹EยฏM2\overline{E}_{M}, k=1k=1, solid line) grows to be saturated at tโˆผ100t\sim 100. Along with โŸจBยฏ2โŸฉ\langle{\overline{B}}^{2}\rangle, the large scale magnetic helicity โŸจ๐€ยฏโ‹…๐ยฏโŸฉ\langle{\overline{\bf A}}\cdot{\overline{\bf B}}\rangle(dashed line) evolves keeping the relation of โŸจBยฏ2โŸฉโ‰ฅkโ€‹โŸจ๐€ยฏโ‹…๐ยฏโŸฉ\langle{\overline{B}}^{2}\rangle\geq k\langle{\overline{\bf A}}\cdot{\overline{\bf B}}\rangle(k=1k=1). Also, kinetic energy โŸจUยฏ2โŸฉ\langle{\overline{U}}^{2}\rangle in the large scale grows keeping โŸจUยฏ2โŸฉโ‰ฅโŸจ๐”ยฏโ‹…โˆ‡ร—๐”ยฏโŸฉ/k\langle{\overline{U}}^{2}\rangle\geq\langle{\overline{\bf U}}\cdot\nabla\times{\overline{\bf U}}\rangle/k. But the direction of kinetic helicity fluctuates from positive to negative as the discontinuous cusp line implies in this log-scaled plot. Similarly, Fig.ย 1(c) shows that evolving small scale magnetic energy โŸจb2โŸฉ\langle b^{2}\rangle and kinetic energy โŸจu2โŸฉ\langle u^{2}\rangle with their helical part โŸจ๐ฎโ‹…โˆ‡ร—๐ฎโŸฉ/k\langle{{\bf u}}\cdot\nabla\times{{\bf u}}\rangle/k and kโ€‹โŸจ๐šโ‹…๐›โŸฉk\langle{{\bf a}}\cdot{{\bf b}}\rangle (kโ‰ฅ2k\geq 2). The fields grow and get saturated like the large scale field, but the saturation occurs earlier than that of the large scale field because of their smaller eddy turnover time.

Fig.ย 1(b), 1(d) show the growth of kinetic and magnetic energy in the system forced by the fully left-handed magnetic energy. Basically, they evolve consistently in comparison with Fig.ย 1(a), 1(c). But, the kinetic helicity and magnetic helicity are invisible in this logarithmic plot indicating their left-handed (negative) chirality. The direction of helicity in the magnetically forced system tends to be consistent with that of forcing energy. This is the opposite tendency of HKFD (helical kinetic forcing dynamo). Nonetheless, the practically same growth of energy shows that the chirality of the forcing energy is not a determinant to the evolution of the plasma system.

Fig.ย 2 shows the evolving magnetic helicity ratio fhโ‰กkโ€‹โŸจ๐šโ‹…๐›โŸฉ/โŸจb2โŸฉf_{h}\equiv k\langle{\bf a}\cdot{\bf b}\rangle/\langle b^{2}\rangle and kinetic helicity ratio โŸจ๐ฎโ‹…โˆ‡ร—๐ฎโŸฉ/kโ€‹โŸจu2โŸฉ\langle{\bf u}\cdot\nabla\times{\bf u}\rangle/k\langle u^{2}\rangle for kk=1, 5, 8. Left and right panel are for the right handed case (fh=1f_{h}=1) and left handed one (fh=โˆ’1f_{h}=-1), respectively. The helicity ratio of large scale Bยฏ{\overline{B}} is eventually saturated at fh=+1f_{h}=+1 (โˆ’1-1), and that of the small scale u & b reaches to the value less (larger) than โ€˜11 (โˆ’1-1)โ€™. However, the helicity ratio of Uยฏ{\overline{U}} is as low as โˆผ0.25\sim 0.25 (โˆ’0.25-0.25). The magnetic helicity ratio less than โ€˜1โ€™ in the small scale regime shows that the small scale magnetic field substantially accelerates the large scale plasma motion. Plasma in the large scale regime is driven by Lorentz force ๐‰โ€‹(p)ร—๐โ€‹(q){\bf J}(p)\times{\bf B}(q), where the wave numbers are constrained by p+q=1p+q=1. This implies that the eddies associated with pp, qq are very close to each other in the small scale regime and nearly out of phase. Their helicity ratios smaller than 11 implies Lorentz force forcing the large scale eddy meaningfully grows. But, the effect of the large-scale magnetic field on the plasma is limited: ๐‰ยฏร—๐ยฏโˆผ0\overline{\bf J}\times\overline{\bf B}\sim 0. The saturated helicity ratio โ€˜fh=f_{h}=1โ€™ for the large scale field indicates that kk for ๐ยฏ\overline{\bf B} is definitely โ€˜1โ€™. Also, the initial largest energy level with โ€˜k=5k=5โ€™ implies that the scale with this wavenumber is forced by an external energy source, which is consistent with our code setting.

Fig.ย 3 includes the temporally evolving ฮฑ\alpha & ฮฒ\beta effect and the large scale magnetic energy 2โ€‹EยฏM2\overline{E}_{M}. Left (right) panel shows the evolution of EME_{M}, ฮฑ\alpha and ฮฒ\beta effect for fh=1f_{h}=1 (fh=โˆ’1f_{h}=-1). ฮฑ\alpha effect for fh=1f_{h}=1 positively oscillates and decreases significantly as EME_{M} gets saturated. In contrast, ฮฑ\alpha effect for fh=โˆ’1f_{h}=-1 negatively oscillates before it disappears. ฮฑ\alpha effect is quenched much earlier than the slowly evolving EME_{M}. The decreasing oscillation in both cases implies that ฮฑ\alpha effect does not play a decisive role in the growth of the large scale magnetic field. Conversely, ฮฒ\beta retains the negative value in both cases and has a much larger size than that of ฮฑ\alpha. This negative ฮฒ\beta, combined with the negative Laplacian โˆ‡2โ†’โˆ’k2\nabla^{2}\rightarrow-k^{2} in Fourier space, can be considered as the actual source of the large scale magnetic field. This is contradictory to the current dynamo theory concluding that ฮฒ\beta is always positive to diffuse magnetic energy. We will show that this conventional inference is valid only for the ideally isotropic system with reflection symmetry. When the symmetry is broken, โ€˜๐ฎ\bf uโ€™ in the small scale regime can yield the anti-diffusing effect of magnetic field.

In Fig.ย 4, we compared โˆ‡ร—โŸจ๐ฎร—๐›โŸฉ\nabla\times\langle{\bf u}\times{\bf b}\rangle (black solid line) with โˆ‡ร—(ฮฑโ€‹๐ยฏโˆ’ฮฒโ€‹โˆ‡ร—๐ยฏ)\nabla\times(\alpha\overline{\bf B}-\beta\nabla\times\overline{\bf B}) (red dashed line) to verify Eq.ย (2.6) and Eq.ย (4.15), (LABEL:betaSolution3). The former uses only the simulation data for the large scale magnetic energy EยฏM\overline{E}_{M}, but the latter requires the data of large scale magnetic helicity HยฏM\overline{H}_{M} in addition to EยฏM\overline{E}_{M}. Although they use different types of data and formulas, they are coincident in the transient mode (t<โˆผ100t<\sim 100 and in the range of 10โˆ’8โˆ’10โˆ’210^{-8}-10^{-2}). Note that Eq.ย (4.15), (LABEL:betaSolution3) are valid until the system gets saturated where HยฏMโˆผ2โ€‹EยฏM\overline{H}_{M}\sim 2\overline{E}_{M}. As Fig.ย 1, 2 show, HยฏM\overline{H}_{M} is different from 2โ€‹EยฏM2\overline{E}_{M} in the transient state. As the field becomes saturated, EยฏM\overline{E}_{M} and HยฏM\overline{H}_{M} are so close that the logarithmic function diverges. For fh=โˆ’1f_{h}=-1, we used absolute values for a clear comparison.

Fig.ย 5, 6 show field structure models. They are introduced to explain the dynamo process in an intuitive way. We will discuss the mechanism in detail soon.

Fig.ย 7 is for the typical kinetic small scale dynamo. Nonhelical random velocity field was driven at k=5k=5. The plot includes large scale kinetic energy EVE_{V} and magnetic energy EME_{M}. Rโ€‹eMRe_{M} is approximately 8080. In comparison with LSD, EME_{M} grows a little bit, and EVE_{V} is not quenched. Most magnetic energy is transferred to the small scale regime, and its peak is located at kโˆผ10k\sim 10. These plots are to compare Fig.ย 1(a), 1(b).

Fig.ย 8, 8 in appendix include the simulations of solar magnetic field using Eq.ย (4.9) and (4.10). The horizontal axis means โ€˜scaled timeโ€™ (0.01โ€‹sโ†’15.530.01s\rightarrow 15.53 years), and the vertical line indicates the โ€˜latitudeโ€™ (0โˆ’ฯ€/20-\pi/2: northern hemisphere, ฯ€/2โˆ’ฯ€\pi/2-\pi: southern hemisphere). The color indicates the phase of a net magnetic field (toroidal ๐tโ€‹oโ€‹r{\bf B}_{tor} + poloidal ๐pโ€‹oโ€‹l{\bf B}_{pol}). The simulation in the left panel is the reproduction of [19] without Babcock effect. It shows the period of 16.31 years for the one complete cycle of solar magnetic field: amplification-annihilation-reverse. On the contrary, in right panel, the tidal effect of planets on the Solar tachocline is added to ฮฑ\alpha. The period elevates up to 21.74 years without manipulating the numerical variables. These plots show the practical applicability of Eq.ย (2.4).

Fig.ย 9 in appendix shows the time evolving 1/3โ€‹โŸจu2โŸฉ1/3\langle u^{2}\rangle and 1/6โ€‹โŸจ๐ฎโ‹…โˆ‡ร—๐ฎโŸฉ1/6\langle{\bf u}\cdot\nabla\times{\bf u}\rangle. This plot is to make sure the overall ฮฒ\beta effect in HMFD is negative. We will also briefly introduce Kraichnanโ€™s result [20]. He expanded ฮฑ\alpha with the unknown time constant ฯ„2\tau_{2} and correlation factor Aโ€‹(xโˆ’xโ€ฒ)A(x-x^{\prime}), and they work as a negative magnetic diffusivity.

Fig.ย 9 in appendix shows the effect of helical velocity field in magnetic diffusivity. Fully helical kinetic forcing is turned off at tโˆผ200t\sim 200 followed by nonhelical kinetic forcing where โŸจ๐ฎโ‹…โˆ‡ร—๐ฎโŸฉ=0\langle{\bf u}\cdot{\nabla\times\bf u}\rangle=0. After tโˆผ200t\sim 200, turbulent magnetic diffusivity becomes positive, which diffuses magnetic field in the system. The growth of large scale magnetic field is suppressed.

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Figureย 3: ฮฑโ€‹(t)\alpha(t), ฮฒโ€‹(t)\beta(t), and โŸจBยฏ2โŸฉ\langle{\overline{B}}^{2}\rangle for fh=1f_{h}=1 and โˆ’1-1. The small and early quenching ฮฑ\alpha effect shows its limited effect on the growth of 2EยฏM{\overline{E}}_{M}.
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Figureย 4: Comparison of EMF and ฮฑ\alpha & ฮฒ\beta approximation. These plots are to verify the separation of ฮฑ\alpha&ฮฒ\beta from Eโ€‹Mโ€‹FEMF. They are from different physical quantities and formulas but yield quite coincident results. โˆ‚๐ยฏ/โˆ‚tโˆ’ฮทโ€‹โˆ‡2๐ยฏ\partial{\overline{\bf B}}/\partial t-\eta\nabla^{2}{\overline{\bf B}} for โˆ‡ร—โŸจ๐ฎร—๐›โŸฉ\nabla\times\langle{\bf u}\times{\bf b}\rangle is the explicit function of EยฏM\overline{E}_{M}, ฮท\eta, and tt. But, ฮฑ\alpha&ฮฒ\beta are functions of EยฏM\overline{E}_{M} and HยฏM\overline{H}_{M} and ฮท\eta. Average is taken for the clear comparison.
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(a) Helical Magnetic forcing
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(b) Induced helical kinetic forcing
Figureย 5: ๐ฃ1,uโ€‹p{\bf j}_{1,\,up} and ๐ฃ1,dโ€‹oโ€‹wโ€‹n{\bf j}_{1,\,down} are represented as ๐ฃ1{\bf j}_{1} for simplicity. (a) Right handed(+)(+) magnetic helicity yields +|๐ฃ2โ‹…๐›iโ€‹nโ€‹d|+|{\bf j}_{2}\cdot{\bf b}_{ind}|, โˆ’|๐ฃ3โ‹…๐›pโ€‹oโ€‹l|-|{\bf j}_{3}\cdot{\bf b}_{pol}|, and right handed kinetic helicity. (b) Induced kinetic helicity also generates โˆ’|๐ฃ2โ€ฒโ‹…๐›|-|{\bf j}^{\prime}_{2}\cdot{\bf b}|, +|๐ฃ3โ€ฒโ‹…๐›iโ€‹nโ€‹dโ€ฒ|+|{\bf j}^{\prime}_{3}\cdot{\bf b}^{\prime}_{ind}| with ๐›\bf b.
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Figureย 6: More detailed field structure based on Eโ€‹Mโ€‹FEMF: โˆ‡ร—(๐”ร—๐)=โˆ’๐”โ‹…โˆ‡๐+๐โ‹…โˆ‡๐”\nabla\times({\bf U}\times{\bf B})=-{\bf U}\cdot\nabla{{\bf B}}+{\bf B}\cdot\nabla{{\bf U}}. These structures correspond to Fig.ย 5(b). The left field structure is for the early time regime while Bยฏ<b{\overline{B}}<b. Right structure is for the magnetic back reaction with Bยฏโ‰ณb{\overline{B}}\gtrsim b at later time regime, which is negligible in the magnetically forced system. The symbol โ€˜โจ‚\bigotimesโ€™ means the direction (โˆ’z^-\hat{z}) of induced current density ๐‰โˆผ๐”ร—๐{\bf J}\sim{\bf U}\times{\bf B}, and its size indicates the relative strength. In the figure, ๐ฎ\bf u and ๐›\bf b indicate turbulent velocity and magnetic field. We use ๐ยฏ\bf\overline{\bf B} for the large scale magnetic field through the paper. But, in this plot, it is used for the relatively larger scale magnetic field compared to ๐›\bf b. Also, the subindex โ€˜pโ€‹oโ€‹lpolโ€™ is added to ๐ยฏ\overline{\bf B} to discriminate ๐ยฏtโ€‹oโ€‹r\overline{\bf B}_{tor}.

4 Discussions on Theoretical analysis

We have shown that magnetic energy can be inversely cascaded in the system forced by the helical magnetic field (โˆ‡ร—๐=ฮปโ€‹๐\nabla\times{\bf B}=\lambda{\bf B}). HMFD has some unique features compared to HKFD. Helical magnetic field, which makes Lorentz force zโ€‹eโ€‹rโ€‹ozero, exerts a force on the system leading to the generation of helical velocity field with the same chirality. Moreover, the conservation of magnetic helicity is not valid anymore. We study the internal interaction of ๐”\bf U & ๐\bf B using field structure model and analytic method beyond conventional theory and phenomenological rope dynamo model. Although MHD theory is based on hydrodynamics, the generation and transport of BB field are innately electromagnetic phenomena constrained by the plasma motion. Note that plasma kinetic energy is converted into magnetic energy only through EMF ๐”ร—๐โˆผฮทโ€‹๐‰โˆผ๐„{\bf U}\times{\bf B}\sim\eta{\bf J}\sim\bf E, which is different from mechanical force. This electromagnetic force drives the charged plasma particles to produce current density which is the source of magnetic field.

4.1 Field structure model

4.1.1 ฮฑ\alpha effect

The right handed magnetic structure in Fig.ย 5(a) is composed of the toroidal magnetic component ๐›tโ€‹oโ€‹r{\bf b}_{tor} and poloidal part ๐›pโ€‹oโ€‹l{\bf b}_{pol}. Statistically, ๐›tโ€‹oโ€‹r{\bf b}_{tor} and ๐›pโ€‹oโ€‹l{\bf b}_{pol} are not distinguished in the homogeneous and isotropic system. But, if we remove reflection symmetry from the system, ๐›tโ€‹oโ€‹r{\bf b}_{tor} and ๐›pโ€‹oโ€‹l{\bf b}_{pol} become independent components playing different roles with ๐ฎ{\bf u}.

The interaction between ๐ฎ\bf u and ๐›tโ€‹oโ€‹r{\bf b}_{tor} yields current density, i.e., ๐ฎร—๐›tโ€‹oโ€‹rโˆผ๐ฃ1,dโ€‹oโ€‹wโ€‹n{\bf u}\times{\bf b}_{tor}\sim{\bf j}_{1,\,down} and ๐ฃ1,uโ€‹p{\bf j}_{1,\,up} in the front and back. These two components induce a new magnetic field ๐›iโ€‹nโ€‹d{\bf b}_{ind}. At the same time, ๐ฎร—๐›pโ€‹oโ€‹l{\bf u}\times{\bf b}_{pol} generates ๐ฃ2{\bf j}_{2}. This current density forms the right handed magnetic helicity with ๐›iโ€‹nโ€‹d{\bf b}_{ind}: โŸจ๐ฃ2โ‹…๐›iโ€‹nโ€‹dโŸฉโ†’k22โ€‹โŸจ๐š2โ‹…๐›iโ€‹nโ€‹dโŸฉ\langle{\bf j}_{2}\cdot{\bf b}_{ind}\rangle\rightarrow k_{2}^{2}\langle{\bf a}_{2}\cdot{\bf b}_{ind}\rangle, which is a (pseudo) scalar to be added to the system. There is also a possibility that ๐ฎ\bf u and ๐›iโ€‹nโ€‹d{\bf b}_{ind} induce ๐ฃ3{\bf j}_{3} yielding the left handed magnetic helicity โŸจ๐ฃ3โ‹…๐›pโ€‹oโ€‹lโŸฉ\langle{\bf j}_{3}\cdot{\bf b}_{pol}\rangle. However, the induced magnetic field from ๐ฃ3{\bf j}_{3} is weakened by the externally provided ๐›tโ€‹oโ€‹r{\bf b}_{tor}.

On the other hand, ๐ฃ1ร—๐›tโ€‹oโ€‹r{\bf j}_{1}\times{\bf b}_{tor} and ๐ฃ2ร—๐›pโ€‹oโ€‹l{\bf j}_{2}\times{\bf b}_{pol} generate Lorentz force toward โˆ’๐ฎ-\bf u, which may look just suppressing plasma motion. However, ๐ฃ2ร—๐›tโ€‹oโ€‹r{\bf j}_{2}\times{\bf b}_{tor} at the right and left end yields an rotation effect, which is toward โ€˜โˆ’๐ฎ-\bf uโ€™. This rotation with those two interactions generates the right handed kinetic helicity โŸจ๐ฎโ‹…โˆ‡ร—๐ฎโŸฉ\langle{\bf u}\cdot\nabla\times{\bf u}\rangle. The interaction between the current density and magnetic field makes two effects. Magnetic pressure effect โˆ’โˆ‡B2/2-\nabla B^{2}/2 from ๐ฃ1ร—๐›tโ€‹oโ€‹r{\bf j}_{1}\times{\bf b}_{tor} and ๐ฃ2ร—๐›pโ€‹oโ€‹l{\bf j}_{2}\times{\bf b}_{pol} suppresses the plasma motion with thermal pressure โˆ’โˆ‡P-\nabla P. And, ๐ฃ2ร—๐›tโ€‹oโ€‹r{\bf j}_{2}\times{\bf b}_{tor} creates a rotational force to form kinetic helicity with the two suppressing effects. As Fourier transformed Lorentz force ๐ฃโ€‹(๐ฉ)ร—๐›โ€‹(๐ช)โˆผโˆ‚๐ฎโ€‹(๐ค)/โˆ‚t{\bf j}({\bf p})\times{\bf b}({\bf q})\sim\partial{\bf u}({\bf k})/\partial t shows, the wavenumbers โ€˜๐ฉ{\bf p}โ€™ and โ€˜๐ช{\bf q}โ€™ are constrained by the relation of ๐ฉ+๐ช=๐ค{\bf p}+{\bf q}={\bf k}.

The induced right handed kinetic helicity in Fig.ย 5(b) again generates ๐ฃโ€ฒ1{\bf j^{\prime}}_{1} in the front and back. The spatially inhomogeneous current density from ๐ฃโ€ฒ1,uโ€‹p{\bf j^{\prime}}_{1,\,up} and ๐ฃโ€ฒ1,dโ€‹oโ€‹wโ€‹n{\bf j^{\prime}}_{1,\,down} induces ๐›iโ€‹nโ€‹dโ€ฒ{\bf b}^{\prime}_{ind} leading to ๐ฃ2โ€ฒ{\bf j}^{\prime}_{2} with ๐ฎpโ€‹oโ€‹l{\bf u}_{pol}, i.e., ๐ฃ2โ€ฒโˆผ๐ฎpโ€‹oโ€‹lร—๐›bโ€‹iโ€‹nโ€‹dโ€ฒ{{\bf j}^{\prime}_{2}\sim{\bf u}_{pol}\times{\bf b}^{\prime}_{bind}}. Then, ๐ฃ2โ€ฒ{\bf j}^{\prime}_{2} forms the left handed magnetic helicity with ๐›{\bf b}. Also, ๐ฎpโ€‹oโ€‹lร—๐›{\bf u}_{pol}\times{\bf b} yields ๐ฃ3โ€ฒ{\bf j}^{\prime}_{3} leading to right handed magnetic helicity. If all interactions are summed up, magnetic helicity in the system is +|โŸจ๐ฃ2โ‹…๐›iโ€‹nโ€‹dโŸฉ|+|\langle{\bf j}_{2}\cdot{\bf b}_{ind}\rangle|โˆ’|โŸจ๐ฃ3โ‹…๐›pโ€‹oโ€‹lโŸฉ|-|\langle{\bf j}_{3}\cdot{\bf b}_{pol}\rangle|โˆ’|โŸจ๐ฃ2โ€ฒโ‹…๐›โŸฉ|-|\langle{\bf j}^{\prime}_{2}\cdot{\bf b}\rangle|+|โŸจ๐ฃ3โ€ฒโ‹…๐›iโ€‹nโ€‹dโ€ฒโŸฉ|+|\langle{\bf j}^{\prime}_{3}\cdot{\bf b}^{\prime}_{ind}\rangle| qualitatively. Comparing this result with ฮฑ\alpha quenching in Fig.ย 3, we may question what indeed amplifies magnetic field and determines the net magnetic helicity. There is one more term to be considered, ฮฒ\beta effect.

4.1.2 ฮฒ\beta effect

Fig.ย 6 is the more detailed right handed helical kinetic structure of Fig.ย 5(b). It is based on the geometrical meaning of โ€˜โˆ‡ร—(๐ฎร—๐ยฏ)โˆผ๐ยฏโ‹…โˆ‡๐ฎโˆ’๐ฎโ‹…โˆ‡๐ยฏ\nabla\times({\bf u}\times{\overline{\bf B}})\sim{\overline{\bf B}}\cdot\nabla{\bf u}-{\bf u}\cdot\nabla{\overline{\bf B}}โ€™. Here, we name โ€˜โˆ’๐ฎโ‹…โˆ‡๐ยฏ-{\bf u}\cdot\nabla{\overline{\bf B}}โ€™ as โ€˜local transfer (advective) termโ€™, and we call โ€˜๐ยฏโ‹…โˆ‡๐ฎ{\overline{\bf B}}\cdot\nabla{\bf u}โ€™ โ€˜nonlocal transfer termโ€™. The symbol โ€˜โŠ—\otimesโ€™ means the direction of current density โ€˜๐‰i{\bf J}_{i}โ€™ heading for โˆ’๐ณ^-\hat{\bf z}. It is from ๐ฎtโ€‹oโ€‹r,iร—๐›โ€‹(oโ€‹rโ€‹๐ยฏ){\bf u}_{tor,\,i}\times{\bf b}(or\,\overline{\bf B}). And, the size of โŠ—\otimes implies its relative strength. Its distribution is spatially inhomogeneous so that the nontrivial curl effect generates the magnetic fields toward ๐ฑ^{\bf\hat{x}} (locally transferred โˆซ๐‘‘ฯ„โ€‹(โˆ’๐ฎโ‹…โˆ‡๐ยฏ)\int d\tau(-{\bf u}\cdot\nabla{\overline{\bf B}})) and ๐ฒ^\bf{\hat{y}} (nonlocally transferred โˆซ๐‘‘ฯ„โ€‹(๐ยฏโ‹…โˆ‡๐ฎ)\int d\tau({\overline{\bf B}}\cdot\nabla{\bf u})). Their net magnetic field ๐›nโ€‹eโ€‹t{\bf b}_{net} becomes a new seed field for the next dynamo process. As the net magnetic field grows, it approaches to the velocity field โ€˜๐ฎ\bf uโ€™ so that โ€˜๐ฎร—๐›nโ€‹eโ€‹t{\bf u}\times{{\bf b}_{net}}โ€™ itself decreases. The field gets saturated eventually if there is no additional reason e.g., frozen field or helicity.

๐ฎpโ€‹oโ€‹l{\bf u}_{pol} interacts with โˆซ๐‘‘ฯ„โ€‹๐ยฏโ‹…โˆ‡๐ฎ\int d\tau{\overline{\bf B}}\cdot\nabla{\bf u} to induce ๐ฃ2โ€ฒ{\bf j}^{\prime}_{2}, which yields the left handed helicity with ๐ยฏpโ€‹oโ€‹l{\overline{\bf B}}_{pol}. 444We add a subindex โ€˜pโ€‹oโ€‹lpolโ€™ to ๐ยฏ{\overline{\bf B}} to discriminate it from ๐ยฏtโ€‹oโ€‹r{\overline{\bf B}}_{tor}. ๐ฎpโ€‹oโ€‹l{\bf u}_{pol} also interacts with ๐ยฏpโ€‹oโ€‹l\overline{\bf B}_{pol} (or ๐›{\bf b}) and โˆซ๐‘‘ฯ„โ€‹(โˆ’๐ฎโ‹…โˆ‡๐ยฏ)\int\,d\tau(-{\bf u}\cdot\nabla{\overline{\bf B}}) yielding ๐ฃ3โ€ฒ{\bf j}^{\prime}_{3} and ๐ฃ4โ€ฒ{\bf j}^{\prime}_{4}, respectively. The polarization of โŸจ๐ฃ3โ€ฒโ‹…โˆซ๐‘‘ฯ„โ€‹๐ยฏโ‹…โˆ‡๐ฎโŸฉ\langle{\bf j}^{\prime}_{3}\cdot\int d\tau\overline{\bf B}\cdot\nabla{\bf u}\rangle is opposite (+)(+) to that of โŸจ๐ฃ2โ€ฒโ‹…๐ยฏpโ€‹oโ€‹lโŸฉโ€‹(โˆ’)\langle{\bf j}^{\prime}_{2}\cdot\overline{\bf B}_{pol}\rangle\,(-), but that of โŸจ๐ฃ4โ€ฒโ‹…โˆซ๐‘‘ฯ„โ€‹๐ยฏโ‹…โˆ‡๐ฎโŸฉ\langle{\bf j}^{\prime}_{4}\cdot\int d\tau\overline{\bf B}\cdot\nabla{\bf u}\rangle depends on the relative value of โˆ’๐ฎโ‹…โˆ‡๐ยฏ-{\bf u}\cdot\nabla{\overline{\bf B}}. When this locally transferred field is weak, ๐ฃโ€ฒ4{\bf j^{\prime}}_{4} is parallel to โˆซ๐‘‘ฯ„โ€‹(๐ยฏโ‹…โˆ‡๐ฎ)\int d\tau({\overline{\bf B}}\cdot\nabla{\bf u}) producing the oppositely polarized (++) magnetic helicity with reference to โŸจ๐ฃ2โ€ฒโ‹…๐ยฏpโ€‹oโ€‹lโŸฉโ€‹(โˆ’)\langle{\bf j}^{\prime}_{2}\cdot\overline{\bf B}_{pol}\rangle\,(-). However, as the strength of ๐ยฏ{\overline{\bf B}} grows to surpass โ€˜|๐›||{\bf b}|โ€™, โ€˜โˆ’๐ฎโ‹…โˆ‡๐ยฏ-{\bf u}\cdot\nabla{\overline{\bf B}}โ€™ turns over so that the direction of ๐ฃ4โ€ฒ{\bf j}^{\prime}_{4} is opposite to โˆซ๐ยฏโ‹…โˆ‡๐ฎโ€‹dโ€‹ฯ„\int{\overline{\bf B}}\cdot\nabla{\bf u}\,d\tau yielding the left handed (โˆ’)(-) magnetic helicity. This is the result of magnetic back reaction. However, this effect is negligible in HMFD where the helical magnetic field is continuously provided by the external source. The net magnetic helicity is โ€˜+|โŸจ๐ฃ2โ‹…๐›iโ€‹nโ€‹dโŸฉ|โˆ’|โŸจ๐ฃ3โ‹…๐›pโ€‹oโ€‹lโŸฉ|โˆ’|โŸจ๐ฃ2โ€ฒโ‹…๐ยฏpโ€‹oโ€‹lโŸฉ|+|โŸจ๐ฃ3โ€ฒโ‹…โˆซ๐‘‘ฯ„โ€‹๐ยฏโ‹…โˆ‡๐ฎโŸฉ|ยฑ|โŸจ๐ฃ4โ€ฒโ‹…โˆซ๐‘‘ฯ„โ€‹๐ยฏโ‹…โˆ‡๐ฎโŸฉ|+|\langle{\bf j}_{2}\cdot{\bf b}_{ind}\rangle|-|\langle{\bf j}_{3}\cdot{\bf b}_{pol}\rangle|-|\langle{\bf j}^{\prime}_{2}\cdot{\overline{\bf B}}_{pol}\rangle|+|\langle{\bf j}^{\prime}_{3}\cdot\int d\tau\overline{\bf B}\cdot\nabla{\bf u}\rangle|\pm|\langle{\bf j}^{\prime}_{4}\cdot\int d\tau\overline{\bf B}\cdot\nabla{\bf u}\rangle|โ€™. The first four terms correspond to ฮฑ\alpha effect, and the last term representing ฮฒ\beta effect substantially amplifies the large scale magnetic field when ฮฑ\alpha effect becomes negligible (Fig.ย 3, 3).

4.2 Analytical derivation of ฮฑ\alpha&ฮฒ\beta

In the helical dynamo, the basis of Eq.ย (2.6) from Eq.ย (2.5) is the replacement of small scale EMF โŸจ๐ฎร—๐›โŸฉ\langle\mathbf{u}\times\mathbf{b}\rangle with ฮฑโ€‹๐ยฏโˆ’ฮฒโ€‹โˆ‡ร—๐ยฏ\alpha\overline{\mathbf{B}}-\beta\nabla\times\overline{\mathbf{B}}. This relation can be approximately derived using sort of a function iterative method with some appropriate closure theories such as MFT[21], EDQNM[15], DIA[16]. All theories show qualitatively the same results; but, they have their own limitations, too. For example, for MFT, the variable XX is divided into the mean (large) scale quantity ๐—ยฏ\overline{\bf X} and small (turbulent) one ๐ฑ\bf x. Then, they are taken average over the large scale โŸจโ‹…โŸฉ\langle\cdot\rangle, and calculated with Reynolds rule and tensor identity.

ฮฑ\displaystyle\alpha =\displaystyle= 13โ€‹โˆซt(โŸจ๐ฃโ‹…๐›โŸฉโˆ’โŸจ๐ฎโ‹…โˆ‡ร—๐ฎโŸฉ)โ€‹๐‘‘ฯ„,\displaystyle\frac{1}{3}\int^{t}\big{(}\langle{\bf j}\cdot{\bf b}\rangle-\langle{\bf u}\cdot\nabla\times{\bf u}\rangle\big{)}\,d\tau, (4.1)
ฮฒ\displaystyle\beta =\displaystyle= 13โ€‹โˆซtโŸจu2โŸฉโ€‹๐‘‘ฯ„.\displaystyle\frac{1}{3}\int^{t}\langle u^{2}\rangle\,d\tau. (4.2)

During the analytic calculation, some turbulent variables with the triple correlation or higher order terms are derived. They are dropped with Reynolds rule or simply ignored with the assumption of being small. This may cause the increasing discrepancy between the real system and MFT as Rโ€‹eMRe_{M} grows. Also, the exact range of small scale regime and the eddy turnover time โ€˜ttโ€™ with integration are not yet known. If the whole turbulent scale regime is included, the large scale magnetic field with these ฮฑ\alpha&ฮฒ\beta exceeds the actual quantity. The small scale range for ฮฑ\alpha&ฮฒ\beta seems to be limited near to forcing scale [22]. However, at present, there is no general way to calculate them except some simple dimensional analysis or experimental approach.

Another issue is the existence of large scale plasma motion ๐”ยฏ\overline{\bf U}. If ๐”ร—๐{\bf U}\times{\bf B} is averaged over large scale and applied with Reynolds rule, two terms remain: ฮพโˆผ๐”ยฏร—๐ยฏ+โŸจ๐ฎร—๐›โŸฉ\xi\sim{\overline{\bf U}}\times{\overline{\bf B}}+\langle{\bf u}\times{\bf b}\rangle. In principle, they should be replaced by ฮฑโ€‹๐ยฏโˆ’ฮฒโ€‹โˆ‡ร—๐ยฏ\alpha{\overline{\bf B}-\beta\nabla\times{\overline{\bf B}}}. But, ๐”ยฏร—๐ยฏ{\overline{\bf U}}\times{\overline{\bf B}} is usually excluded with Galilean transformation. However, ๐”ยฏ{\overline{\bf U}} in simulation and observation does not disappear, rather its effect can grow with the increasing ๐ยฏ{\overline{\bf B}}. Eq.ย (4.1), (4.2) are over simplified results.

In DIA, those issues are included in formal Greenโ€™s function GG with statistical second order relation.

โŸจXiโ€‹(k)โ€‹Xjโ€‹(โˆ’k)โŸฉ=(ฮดiโ€‹jโˆ’kiโ€‹kjk2)โ€‹EXโ€‹(k)+i2โ€‹klk2โ€‹ฯตiโ€‹jโ€‹lโ€‹HXโ€‹(k)\displaystyle\langle X_{i}({k})X_{j}({-k})\rangle=(\delta_{ij}-\frac{k_{i}k_{j}}{k^{2}})E_{X}(k)+\frac{i}{2}\frac{k_{l}}{k^{2}}\epsilon_{ijl}H_{X}(k) (4.3)
(โŸจX2โŸฉ=2โ€‹โˆซEXโ€‹(k)โ€‹๐‘‘k,โŸจ๐—โ‹…โˆ‡ร—๐—โŸฉ=โˆซHXโ€‹(k)โ€‹๐‘‘k)\displaystyle\bigg{(}\langle X^{2}\rangle=2\int E_{X}(k)d{k},\,\,\langle{\bf X}\cdot\nabla\times{\bf X}\rangle=\int H_{X}(k)d{k}\bigg{)}

And, ฮฑ\alpha&ฮฒ\beta in DIA are

ฮฑ\displaystyle\alpha =\displaystyle= 13โ€‹โˆซ๐‘‘๐คโ€‹โˆซt(GMโ€‹โŸจ๐ฃโ‹…๐›โŸฉโˆ’GKโ€‹โŸจ๐ฎโ‹…โˆ‡ร—๐ฎโŸฉ)โ€‹๐‘‘ฯ„,\displaystyle\frac{1}{3}\int d{\bf k}\int^{t}(G_{M}\langle{\bf j}\cdot{\bf b}\rangle-G_{K}\langle{\bf u}\cdot\nabla\times{\bf u}\rangle)d\tau, (4.4)
ฮฒ\displaystyle\beta =\displaystyle= 13โ€‹โˆซt(GKโ€‹โŸจu2โŸฉ+GMโ€‹โŸจb2โŸฉ)โ€‹๐‘‘ฯ„.\displaystyle\frac{1}{3}\int^{t}(G_{K}\langle u^{2}\rangle+G_{M}\langle b^{2}\rangle)d\tau. (4.5)

They are quite similar to those of MFT except GKG_{K}&GMG_{M} and turbulent magnetic energy โŸจb2โŸฉ\langle b^{2}\rangle in ฮฒ\beta. ฮฑ\alpha coefficient implies its quenching as GMโ€‹โŸจ๐ฃโ‹…๐›โŸฉโ†’GKโ€‹โŸจ๐ฎโ‹…โˆ‡ร—๐ฎโŸฉG_{M}\langle{\bf j}\cdot{\bf b}\rangle\rightarrow G_{K}\langle{\bf u}\cdot\nabla\times{\bf u}\rangle. Also, the ฮฒ\beta effect depends on the turbulent energy including b2b^{2}. Since DIA calculates kinetic approach and counter kinetic (magnetic) one separately, Eq.ย (4.3) yields โŸจu2โŸฉ\langle u^{2}\rangle and โŸจb2โŸฉ\langle b^{2}\rangle in ฮฒ\beta (๐ฑ=๐ฎ,๐›{\bf x}={\bf u},\,{\bf b}).

ฮฑ\alpha&ฮฒ\beta calculated with EDQNM approximation show more or less similar physical properties such as quenching ฮฑ\alpha and energy dependent positive ฮฒ\beta [15].

ฮฑ\displaystyle\alpha =\displaystyle= 23โ€‹โˆซโˆžฮ˜kโ€‹pโ€‹qโ€‹(t)โ€‹(โŸจ๐ฃโ‹…๐›โŸฉโˆ’โŸจ๐ฎโ‹…โˆ‡ร—๐ฎโŸฉ)โ€‹๐‘‘q,\displaystyle\frac{2}{3}\int^{\infty}\Theta_{kpq}(t)\big{(}\langle{\bf j}\cdot{\bf b}\rangle-\langle{\bf u}\cdot\nabla\times{\bf u}\rangle\big{)}\,dq, (4.6)
ฮฒ\displaystyle\beta =\displaystyle= 23โ€‹โˆซโˆžฮ˜kโ€‹pโ€‹qโ€‹(t)โ€‹โŸจu2โŸฉโ€‹๐‘‘q,\displaystyle\frac{2}{3}\int^{\infty}\Theta_{kpq}(t)\langle u^{2}\rangle\,dq, (4.7)

where triad relaxation time ฮ˜kโ€‹pโ€‹q=(1โˆ’eโ€‹xโ€‹pโ€‹(โˆ’ฮผkโ€‹pโ€‹qโ€‹t))/ฮผkโ€‹pโ€‹q\Theta_{kpq}=(1-exp(-\mu_{kpq}t))/\mu_{kpq} and eddy damping operator ฮผkโ€‹pโ€‹q\mu_{kpq} are used. Note that ฮ˜โˆผฮผkโ€‹pโ€‹qโˆ’1\Theta\sim\mu^{-1}_{kpq}, ฮผkโ€‹pโ€‹q=cโ€‹oโ€‹nโ€‹sโ€‹t.\mu_{kpq}=const. as tโ†’โˆžt\rightarrow\infty (see [15] and references therein). Formally, DIA or EDQNM is free from the nonlinear effects neglected in MFT. However, still there are unknown Green function, triad relaxation time, and eddy damping rate including eddy turnover time.

Furthermore, the small scale EMF โŸจ๐ฎร—๐›โŸฉ\langle\mathbf{u}\times\mathbf{b}\rangle used in two scale MFT and DIA is not well defined quantity. It is inferred from ๐—โˆ’๐—ยฏ{\bf X}-\overline{\bf X} which is supposed to be in the range of kโ‰ฅ2k\geq 2 in Fourier space. However, the range participating in the amplification of large scale field is very narrow. Our previous work to find ฮฑ\alpha&ฮฒ\beta with the conventional MFT shows that ๐ฎ\bf u&๐›\bf b (or ฮฑ\alpha&ฮฒ\beta) exist only around the forcing scale. The whole turbulent range yields much larger growth of ๐ยฏ\overline{\bf B} than actual value (Fig.ย 1, [23], Fig.ย 1b, [24]). Kolmogorovโ€™s inertia range seems to separate the range of ๐ฎ\bf u&๐›\bf b for ฮฑ\alpha&ฮฒ\beta from other dissipation scale. However, it is not clear whether the latter just dissipates or plays some other roles in dynamo. At least, they do not amplify ๐ยฏ\overline{\bf B} directly. But, since the exact range cannot be found with theory, we may question if ฮฑ\alpha&ฮฒ\beta (or ๐ฎ\bf u&๐›\bf b) are just conceptual quantities. Statistically, however, it makes sense to substitute ฮฑ\alpha&ฮฒ\beta and ๐ยฏ\overline{\bf B} for EMF. And, the result is associated with the statistical correlation Eq.ย (4.3). If we apply [14]โ€™s assumption Eโ€‹Mโ€‹Fiโˆผฮฑiโ€‹jโ€‹๐ยฏj+ฮฒiโ€‹jโ€‹kโ€‹โˆ‡k๐ยฏjEMF_{i}\sim\alpha_{ij}\overline{\mathbf{B}}_{j}+\beta_{ijk}\nabla_{k}\overline{\mathbf{B}}_{j}555ฮณ\gamma is neglected for simplicity to magnetic induction equation, we get

โˆ‚๐ยฏโˆ‚tโˆผโˆ‡ร—(ฮฑโ€‹๐ยฏโˆ’(ฮฒ+ฮท)โ€‹โˆ‡ร—๐ยฏ).\displaystyle\frac{\partial\overline{\mathbf{B}}}{\partial t}\sim\nabla\times(\alpha\overline{\mathbf{B}}-(\beta+\eta)\nabla\times\overline{\mathbf{B}}). (4.8)

This shows that the growth rate of ๐ยฏ\overline{\mathbf{B}} is represented by its curl effect. And, if the divergenceless magnetic field โˆ‡โ‹…๐ยฏ=0\nabla\cdot\overline{\mathbf{B}}=0 is added, this equation is led to Helmholtz theory. This means that magnetic induction equation with ฮฑ\alpha, ฮฒ\beta, and diffusion is statistically self consistent. The properly found ฮฑ\alpha & ฮฒ\beta can describe the evolution of large scale magnetic field.

This formal equation can be applied to the practical dynamo phenomenon such as Solar dynamo. If the equation is divided into the poloidal component and toroidal one, two coupled equations from magnetic induction equation are derived [25]:

โˆ‚Aยฏโˆ‚t=(ฮท+ฮฒ)โ€‹(โˆ‡2โˆ’1ฯ–2)โ€‹Aยฏโˆ’๐ฎpฯ–โ‹…โˆ‡(ฯ–โ€‹Aยฏ)+ฮฑโ€‹Bยฏtโ€‹oโ€‹r,\displaystyle\frac{\partial\overline{A}}{\partial t}=(\eta+\beta)\bigg{(}\nabla^{2}-\frac{1}{\varpi^{2}}\bigg{)}\overline{A}-\frac{{\bf u}_{p}}{\varpi}\cdot\nabla(\varpi\overline{A})+\alpha\overline{B}_{tor}, (4.9)
โˆ‚Bยฏtโ€‹oโ€‹rโˆ‚t=(ฮท+ฮฒ)โ€‹(โˆ‡2โˆ’1ฯ–2)โ€‹Bยฏtโ€‹oโ€‹r+1ฯ–โ€‹โˆ‚(ฯ–โ€‹Bยฏtโ€‹oโ€‹r)โˆ‚rโ€‹โˆ‚(ฮท+ฮฒ)โˆ‚r\displaystyle\frac{\partial\overline{B}_{tor}}{\partial t}=(\eta+\beta)\bigg{(}\nabla^{2}-\frac{1}{\varpi^{2}}\bigg{)}\overline{B}_{tor}+\frac{1}{\varpi}\frac{\partial(\varpi\overline{B}_{tor})}{\partial r}\frac{\partial(\eta+\beta)}{\partial r} (4.10)
โˆ’ฯ–โ€‹๐ฎpโ‹…โˆ‡(Bยฏtโ€‹oโ€‹rฯ–)โˆ’Bยฏtโ€‹oโ€‹rโ€‹โˆ‡โ‹…๐ฎp+ฯ–โ€‹(โˆ‡ร—(Aยฏโ€‹e^ฯ•))โ‹…โˆ‡๐›€\displaystyle-\varpi{\bf u}_{p}\cdot\nabla\bigg{(}\frac{\overline{B}_{tor}}{\varpi}\bigg{)}-\overline{B}_{tor}\nabla\cdot{\bf u}_{p}+\varpi(\nabla\times(\overline{A}\hat{e}_{\phi}))\cdot\nabla{\bf\Omega}
+โˆ‡ร—(ฮฑโ€‹โˆ‡ร—(Aยฏโ€‹e^ฯ•)),\displaystyle+\nabla\times(\alpha\nabla\times(\overline{A}\hat{e}_{\phi})),

where ๐ยฏpโ€‹oโ€‹l=โˆ‡ร—๐€ยฏ\overline{\bf B}_{pol}=\nabla\times\overline{\bf A}, ฯ–=rโ€‹sโ€‹iโ€‹nโ€‹ฮธ\varpi=r\,sin\theta, and ฮฉ\Omega is the angular velocity from convetive motion ๐”ยฏ=๐ซร—๐›€{\overline{\bf U}={\bf r}\times{\bf\Omega}}. This equation set reproduces the periodic solar magnetic field: amplification-annihilation-reverse. In Appendix, we show Solar dynamo simulation. Fig.ย 8 in appendix includes the reproduction of [19]โ€™s work. ฮฑ\alpha&ฮฒ\beta were chosen for the critical dynamo yielding 16.3 year period. Stefani et al.[26] added the effect of synchronized helicity oscillation from planets to ฮฑ\alpha effect and solved the 1D equation to get โˆผ22\sim 22 year oscillation period. We solved it in 2D (r,ฮธr,\,\theta) simulation in spherical coordinates. Fig.ย  8 in appendix shows that the modified ฮฑ\alpha reproduces the period of 21.7 without tuning any code variable. If additional physical effect exists, it can be applied to ฮฑ\alpha&ฮฒ\beta rather than EMF. It is also possible to infer ฮฑ\alpha&ฮฒ\beta from EMโ€‹(t)E_{M}(t) and HMโ€‹(t)H_{M}(t).

Refer to caption
Refer to caption
Figureย 7: Nonhelical kinetic forcing small scale dynamo. Nonhelical velocity field was given to k=5. ฮท=ฮฝ=0.001\eta=\nu=0.001, and magnetic Reynolds number Rโ€‹eMRe_{M} is โˆผ80\sim 80. Left panel shows the temporal evolution of EVE_{V} and EME_{M}. Rght panel shows their spectra at t=100t=100, 240240, 16001600. The peak of EME_{M} is located between the forcing scale and dissipation scale.

4.3 Half Analytic and Half Numerical Method

We can find ฮฑ\alpha & ฮฒ\beta using the data of magnetic helicity and magnetic energy. We pointed out that Eq.ย (4.8) is formally consistent with the statistical relation. Then, from Eq.ย (2.6) we get

๐ยฏโ‹…โˆ‚๐ยฏโˆ‚t\displaystyle\overline{\mathbf{B}}\cdot\frac{\partial\overline{\mathbf{B}}}{\partial t} =\displaystyle= ฮฑโ€‹๐ยฏโ‹…โˆ‡ร—๐ยฏ+(ฮฒ+ฮท)โ€‹๐ยฏโ‹…โˆ‡2๐ยฏ\displaystyle\alpha\overline{\mathbf{B}}\cdot\nabla\times\overline{\mathbf{B}}+(\beta+\eta)\overline{\mathbf{B}}\cdot\nabla^{2}\overline{\mathbf{B}}
=\displaystyle= ฮฑโ€‹๐‰ยฏโ‹…๐ยฏโˆ’(ฮฒ+ฮท)โ€‹๐ยฏโ‹…๐ยฏโ€‹(k=1)\displaystyle\alpha\overline{\mathbf{J}}\cdot\overline{\mathbf{B}}-(\beta+\eta)\,\overline{\mathbf{B}}\cdot\overline{\mathbf{B}}\,(k=1)
โ†’โˆ‚โˆ‚tโ€‹EยฏM\displaystyle\rightarrow\frac{\partial}{\partial t}\overline{E}_{M} =\displaystyle= โˆ’2โ€‹(ฮฒ+ฮท)โ€‹EยฏM+ฮฑโ€‹HยฏM.\displaystyle-2(\beta+\eta){\overline{E}}_{M}+\alpha{\overline{H}}_{M}. (4.11)

We can also derive the evolving magnetic helicity as follows.

โ†’ddโ€‹tโ€‹HยฏM\displaystyle\rightarrow\frac{d}{dt}\overline{H}_{M} =\displaystyle= 4โ€‹ฮฑโ€‹EยฏMโˆ’2โ€‹(ฮฒ+ฮท)โ€‹HยฏM.\displaystyle 4\alpha\overline{E}_{M}-2(\beta+\eta)\overline{H}_{M}. (4.12)

These two equations are functions of actual data EยฏM\overline{E}_{M} and HยฏM\overline{H}_{M} resulting from all internal and external effects. One of a simple method to solve this coupled equation set is to diagonalize the matrix using a coefficient matrix PP,which satisfies [HยฏM,EยฏM]โ‰กPโ€‹[X,Y][{\overline{H}}_{M},\,{\overline{E}}_{M}]\equiv P\,[X,\,Y]. Then, we get
[โˆ‚X/โˆ‚tโˆ‚Y/โˆ‚t]=Pโˆ’1โ€‹[โˆ’2โ€‹(ฮฒ+ฮท)4โ€‹ฮฑฮฑโˆ’2โ€‹(ฮฒ+ฮท)]โ€‹Pโ€‹[XY]=[ฮป100ฮป2]โ€‹[XY].\left[\begin{array}[]{c}\partial X/\partial t\\ \partial Y/\partial t\end{array}\right]=P^{-1}\left[\begin{array}[]{cc}-2(\beta+\eta)&4\alpha\\ \alpha&-2(\beta+\eta)\end{array}\right]P\left[\begin{array}[]{c}X\\ Y\end{array}\right]=\left[\begin{array}[]{cc}\lambda_{1}&0\\ 0&\lambda_{2}\end{array}\right]\left[\begin{array}[]{c}X\\ Y\end{array}\right].

[HยฏM,EยฏM][{\overline{H}}_{M},\,{\overline{E}}_{M}] can be found from Pโˆ’1โ€‹[X,Y]P^{-1}[X,\,Y], where the column vector of PP forms the basis of eigenvectors. The result is,

2โ€‹HยฏMโ€‹(tn)\displaystyle 2\overline{H}_{M}(t_{n}) =\displaystyle= (2โ€‹EยฏMโ€‹(tnโˆ’1)+HยฏMโ€‹(tnโˆ’1))โ€‹e2โ€‹โˆซ0tn(ฮฑโˆ’ฮฒโˆ’ฮท)โ€‹๐‘‘ฯ„\displaystyle(2\overline{E}_{M}(t_{n-1})+\overline{H}_{M}(t_{n-1}))e^{2\int^{t_{n}}_{0}(\alpha-\beta-\eta)d\tau} (4.13)
โˆ’(2โ€‹EยฏMโ€‹(tnโˆ’1)โˆ’HยฏMโ€‹(tnโˆ’1))โ€‹e2โ€‹โˆซ0tn(โˆ’ฮฑโˆ’ฮฒโˆ’ฮท)โ€‹๐‘‘ฯ„,\displaystyle-(2\overline{E}_{M}(t_{n-1})-\overline{H}_{M}(t_{n-1}))e^{2\int^{t_{n}}_{0}(-\alpha-\beta-\eta)d\tau},
4โ€‹EยฏMโ€‹(tn)\displaystyle 4\overline{E}_{M}(t_{n}) =\displaystyle= (2โ€‹EยฏMโ€‹(tnโˆ’1)+HยฏMโ€‹(tnโˆ’1))โ€‹e2โ€‹โˆซ0tn(ฮฑโˆ’ฮฒโˆ’ฮท)โ€‹๐‘‘ฯ„\displaystyle(2\overline{E}_{M}(t_{n-1})+\overline{H}_{M}(t_{n-1}))e^{2\int^{t_{n}}_{0}(\alpha-\beta-\eta)d\tau} (4.14)
+(2โ€‹EยฏMโ€‹(tnโˆ’1)โˆ’HยฏMโ€‹(tnโˆ’1))โ€‹e2โ€‹โˆซ0tn(โˆ’ฮฑโˆ’ฮฒโˆ’ฮท)โ€‹๐‘‘ฯ„.\displaystyle+(2\overline{E}_{M}(t_{n-1})-\overline{H}_{M}(t_{n-1}))e^{2\int^{t_{n}}_{0}(-\alpha-\beta-\eta)d\tau}.

HยฏM\overline{H}_{M} is always smaller than 2โ€‹EยฏM2\overline{E}_{M}, which satisfies realizability condition. But, HยฏMโ†’2โ€‹EยฏM\overline{H}_{M}\rightarrow 2\overline{E}_{M} as the system is getting saturated. In case of right handed HMFD, clearly ฮฑ>0\alpha>0 so that the first term in Eq.ย (4.13), (4.14) are dominant. This means HยฏMโ€‹(tn)\overline{H}_{M}(t_{n}) as well as EยฏMโ€‹(tn)\overline{E}_{M}(t_{n}) is positive. But in case of left handed HMFD, the second term is dominant. This indicates that HยฏMโ€‹(tn)\overline{H}_{M}(t_{n}) is negative, but EยฏMโ€‹(tn)\overline{E}_{M}(t_{n}) is positive. On the contrary, in case of positively forced HKFD, ฮฑ\alpha is negative so that the second term in each equation is dominant leading to negative HยฏM\overline{H}_{M}. Still, EยฏM\overline{E}_{M} is not influenced by the chirality of forcing. These inferences are well consistent with the simulation result of HKFD or HMFD.

ฮฑ\alpha & ฮฒ\beta from above results are [17]

ฮฑโ€‹(t)\displaystyle\alpha(t) =\displaystyle= 14โ€‹ddโ€‹tโ€‹lโ€‹oโ€‹geโ€‹|2โ€‹EยฏMโ€‹(t)+HยฏMโ€‹(t)2โ€‹EยฏMโ€‹(t)โˆ’HยฏMโ€‹(t)|,\displaystyle\frac{1}{4}\frac{d}{dt}log_{e}\bigg{|}\frac{2\overline{E}_{M}(t)+\overline{H}_{M}(t)}{2\overline{E}_{M}(t)-\overline{H}_{M}(t)}\bigg{|}, (4.15)
ฮฒโ€‹(t)\displaystyle\beta(t) =\displaystyle= โˆ’14โ€‹ddโ€‹tโ€‹lโ€‹oโ€‹geโ€‹|(2โ€‹EยฏMโ€‹(t)โˆ’HยฏMโ€‹(t))โ€‹(2โ€‹EยฏMโ€‹(t)+HยฏMโ€‹(t))|โˆ’ฮท.\displaystyle-\frac{1}{4}\frac{d}{dt}log_{e}\big{|}\big{(}2\overline{E}_{M}(t)-\overline{H}_{M}(t)\big{)}\big{(}2\overline{E}_{M}(t)+\overline{H}_{M}(t)\big{)}\big{|}-\eta.

To get the ฮฑ\alpha&ฮฒ\beta, we need the simulation or observation data of EยฏMโ€‹(t)\overline{E}_{M}(t) and HยฏMโ€‹(t)\overline{H}_{M}(t) in each time โ€˜tnt_{n}โ€™. For example, dโ€‹EยฏM/dโ€‹td\overline{E}_{M}/dt is approximately โˆผ(EยฏMโ€‹(tn)โˆ’EยฏMโ€‹(tnโˆ’1))/(tnโˆ’tnโˆ’1)\sim(\overline{E}_{M}(t_{n})-\overline{E}_{M}(t_{n-1}))/(t_{n}-t_{n-1}). We compared โˆ‡ร—โŸจ๐ฎร—๐›โŸฉ\nabla\times\langle{\bf u}\times{\bf b}\rangle with โˆ‡ร—(ฮฑโ€‹๐ยฏโˆ’ฮฒโ€‹โˆ‡ร—๐ยฏ)\nabla\times(\alpha{\overline{\bf B}}-\beta\nabla\times{\overline{\bf B}}) in Fig.ย 4, 4. In the early time regime, they are quite close to each other. But, oscillation increases as the field becomes saturated (2โ€‹EยฏMโˆผHยฏM2\overline{E}_{M}\sim\overline{H}_{M}). Also, note that we used k=1k=1 for the large scale field in the analytic and numerical calculation. And, for the anisotropic system, we need data for EยฏโŠฅ,Mโ€‹(t)\overline{E}_{\bot,\,M}(t) & HยฏโŠฅ,Mโ€‹(t)\overline{H}_{\bot,\,M}(t), Eยฏ||,Mโ€‹(t)\overline{E}_{||,\,M}(t) & Hยฏ||,Mโ€‹(t)\overline{H}_{||,\,M}(t), and the anisotropic solution of Eq.ย (4.15), (LABEL:betaSolution3). When these theoretical results are applied to the real data, some appropriate filtering, simplifying, or normalizing data may be required according the quality of data.

4.4 Derivation of ฮฒ\beta

Now, we check the possibility of negative ฮฒ\beta using analytic method.

โŸจ๐ฎร—(โˆ’๐ฎโ‹…โˆ‡๐ยฏ)โŸฉโ†’โŸจโˆ’ฯตiโ€‹jโ€‹kโ€‹ujโ€‹(r,t)โ€‹umโ€‹(r+l,ฯ„)โ€‹โˆ‚Bยฏkโˆ‚rยฏmโŸฉ\displaystyle\langle{\bf u}\times(-{\bf u}\cdot\nabla\overline{\bf B})\rangle\rightarrow\big{\langle}-\epsilon_{ijk}u_{j}(r,\,t)u_{m}(r+l,\,\tau)\frac{\partial\overline{B}_{k}}{\partial\overline{r}_{m}}\big{\rangle} (4.17)
โˆผ\displaystyle\sim โˆ’ฯตiโ€‹jโ€‹kโ€‹โŸจujโ€‹(t)โ€‹umโ€‹(ฯ„)โŸฉโ€‹โˆ‚Bยฏkโˆ‚rยฏmโˆ’โŸจujโ€‹(t)โ€‹lnโ€‹โˆ‚numโ€‹(ฯ„)โŸฉโ€‹ฯตiโ€‹jโ€‹kโ€‹โˆ‚Bยฏkโˆ‚rยฏm\displaystyle-\epsilon_{ijk}\langle u_{j}(t)u_{m}(\tau)\rangle\frac{\partial\overline{B}_{k}}{\partial\overline{r}_{m}}-\langle u_{j}(t)\,l_{n}\partial_{n}u_{m}(\tau)\rangle\epsilon_{ijk}\frac{\partial\overline{B}_{k}}{\partial\overline{r}_{m}} (4.18)
โˆผ\displaystyle\sim โˆ’13โ€‹โŸจu2โŸฉโ€‹ฯตiโ€‹jโ€‹kโ€‹โˆ‚Bยฏkโˆ‚rยฏmโ€‹ฮดjโ€‹mโŸ1โ€‹โˆ’โŸจl6โ€‹|HV|โŸฉโ€‹ฯตiโ€‹jโ€‹kโ€‹โˆ‚Bยฏkโˆ‚rยฏmโ€‹ฮดnโ€‹kโ€‹ฮดmโ€‹iโŸ2,\displaystyle\underbrace{-\frac{1}{3}\langle u^{2}\rangle\epsilon_{ijk}\frac{\partial\overline{B}_{k}}{\partial\overline{r}_{m}}\delta_{jm}}_{1}\,\underbrace{-\big{\langle}\frac{l}{6}|H_{V}|\big{\rangle}\epsilon_{ijk}\frac{\partial\overline{B}_{k}}{\partial\overline{r}_{m}}\delta_{nk}\delta_{mi}}_{2}, (4.19)

In Eq.ย (4.17) we used the approximation of (uโ€‹(r+l,ฯ„)โˆ’uโ€‹(r,ฯ„))/lโ‰กฮ”โ€‹u/ฮ”โ€‹rโˆผโˆ‚uโ€‹(rโ€ฒ,ฯ„)/โˆ‚r(u(r+l,\,\tau)-u(r,\,\tau))/l\equiv\Delta u/\Delta r\sim\partial u(r^{\prime},\,\tau)/\partial r with the spatially small increment โ€˜llโ€™. We assumed that the sufficiently many eddies make the plasma system statistically continuous. Then, there should be at least one point โ€˜rโ€ฒr^{\prime}โ€™ between โ€˜r+lr+lโ€™ and โ€˜rrโ€™, whose tangential line is parallel to the slope between them. Moreover, it is not difficult to find โˆ‚u/โˆ‚r>uโ€‹(r+l)\partial u/\partial r>u(r+l), especially when uโ€‹(r+l)โ€‹uโ€‹(r)<0u(r+l)u(r)<0.

For the nonhelical field, the result will be (โŸจu2/3โŸฉ+lโ‹…โˆ‡โŸจu2/2โŸฉ)โ€‹(โˆ’โˆ‡ร—๐ยฏ)(\langle u^{2}/3\rangle+l\cdot\nabla\langle u^{2}/2\rangle)(-\nabla\times\overline{\bf{B}}), which is the conventional positive ฮฒ\beta. For the helical fields of uj{u}_{j}, the first term can be still calculated as the energy density โ€˜mโ†’jm\rightarrow jโ€™. However, in the second term, uju_{j}, umu_{m}, and Bยฏk\overline{B}_{k} are mutually perpendicular. Without loss of generality, โ€˜uj{u}_{j}โ€™ can be considered as โ€˜upโ€‹oโ€‹l{u}_{pol}โ€™. Then, โ€˜um{u}_{m}โ€™ should be โ€˜utโ€‹oโ€‹r{u}_{tor}โ€™ (โ€˜mmโ€™โ†’\rightarrowโ€˜iiโ€™), and โ€˜nnโ€™ should be โ€˜kkโ€™.666Kronecker delta is used to indicate the index for a specific direction. It is not from Levi-Civita relation. Also, note that โˆ‚Bยฏk/โˆ‚rยฏm\partial\overline{B}_{k}/\partial\overline{r}_{m} is taken out of the bracket which is for the average over large scale. Since the turbulent velocity part is saturated earlier than the large scale eddy, it can be calculated separately: l/6โ€‹โŸจ๐ฎโ‹…โˆ‡ร—๐ฎโŸฉ(โ‰กl/6โ€‹HV)l/6\langle{\bf u}\cdot\nabla\times{\bf u}\rangle(\equiv l/6H_{V}). As mentioned, โ€˜lnl_{n}โ€™ or โ€˜l(=|ln|)l(=|l_{n}|)โ€™ is the increment of โ€˜rrโ€™. But it can be also considered as correlation length. Since the helical velocity field ๐ฎtโ€‹oโ€‹r{\bf u}_{tor} can be converted into ๐ฎpโ€‹oโ€‹l{\bf u}_{pol} through curl operator, โ€˜lnl_{n}โ€™ indicates lateral correlation length. For the left handed helical structure, we first place a virtual mirror on the right side of ๐ฎtโ€‹oโ€‹r,โ€‰2{\bf u}_{tor,\,2}. Then, the toroidal velocity eddies will be reflected on the other side, and the correlation length โ€˜lnl_{n}โ€™ is toward โ€˜โˆ’l^-\hat{l}โ€™. The reflection makes โˆ‡num\nabla_{n}{u}_{m} negative, but ๐ฎpโ€‹oโ€‹l{\bf u}_{pol} does not change. That is, โ€˜lnl_{n}โ€™ should be sort of a pseudo-scalar (refer to the difference between โŸจu2โŸฉ\langle u^{2}\rangle and โŸจ๐ฎโ‹…ฯ‰โŸฉ\langle{\bf u}\cdot{\bf\omega}\rangle). Considering the statistical meaning of each component, we can make a more general form as follows:

โˆผโˆ’13โ€‹โŸจu2โŸฉโ€‹โˆ‡ร—๐ยฏ+l6โ€‹|HV|โ€‹โˆ‡ร—๐ยฏโ†’โˆ’ฮฒโ€‹โˆ‡ร—๐ยฏ.\displaystyle\sim-\frac{1}{3}\langle u^{2}\rangle\nabla\times\overline{\bf B}+\frac{l}{6}|H_{V}|\nabla\times\overline{\bf B}\rightarrow-\beta\nabla\times\overline{\bf B}. (4.20)

The total diffusion effect becomes (ฮฒ+ฮท)โ€‹โˆ‡2๐ยฏ(\beta+\eta)\nabla^{2}{\overline{\bf B}}, whose Fourier transformed expression is โˆ’(ฮฒ+ฮท)โ€‹k2โ€‹๐ยฏ-(\beta+\eta)k^{2}{\overline{\bf B}} regardless of chirality.

With these analytical analysis, โ€˜llโ€™ is not yet clearly defined. If we consider the correlation length between two eddies (helical field), we can derive with the parallel correlation gโ€‹(r)g(r)

โŸจuโ€‹(r)โ€‹uโ€‹(r+l)โŸฉโ‰กโŸจu2โ€‹(r)โŸฉโ€‹gโ€‹(r)โˆผ13โ€‹โŸจu2โŸฉโˆ’l6โ€‹โŸจ๐ฎโ‹…โˆ‡ร—๐ฎโŸฉโˆผ(2โˆ’lโ€‹k)6โ€‹โŸจu2โŸฉ.\displaystyle\langle u(r)u(r+l)\rangle\equiv\langle u^{2}(r)\rangle g(r)\sim\frac{1}{3}\langle u^{2}\rangle-\frac{l}{6}\langle{\bf u}\cdot\nabla\times{\bf u}\rangle\sim\frac{\big{(}2-lk\big{)}}{6}\langle u^{2}\rangle. (4.21)

The condition for 2โˆ’lโ€‹k<02-lk<0 is actually the correlation position that makes gโ€‹(r)<0g(r)<0, which is the typical property of parallel correlation length[27]. We can get the condition l>2/kl>2/k. Since kk for small scale is larger than 2, the condition of negative ฮฒ\beta is not the hard one. At present, we leave lโ€‹HV/6lH_{V}/6 to be an independent quantity. But it should be noted that this term cannot be considered as ฮฑ\alpha effect because โˆ‡ร—(โˆ’โŸจu2โŸฉ/3+l/|6โ€‹HV|)โ€‹โˆ‡ร—๐ยฏโ†’(โŸจu2โŸฉ/3โˆ’l/6โ€‹|HV|)โ€‹โˆ‡2๐ยฏ\nabla\times(-\langle u^{2}\rangle/3+l/|6H_{V}|)\nabla\times\overline{\bf B}\rightarrow(\langle u^{2}\rangle/3-l/6|H_{V}|)\nabla^{2}\overline{\bf B}. This is a typical diffusion term.

Fig.ย 9 in appendix includes how 1/3โ€‹โŸจu2โŸฉ1/3\langle u^{2}\rangle and 1/6โ€‹โŸจ๐ฎโ‹…โˆ‡ร—๐ฎโŸฉ1/6\langle{\bf u}\cdot\nabla\times{\bf u}\rangle evolve. It is easy to check โŸจ๐ฎโ‹…โˆ‡ร—๐ฎโŸฉโˆผkโ€‹โŸจu2โŸฉ\langle{\bf u}\cdot\nabla\times{\bf u}\rangle\sim k\langle u^{2}\rangle with k=k=2, 3, 4, โ€ฆ is larger than โŸจu2โŸฉ\langle u^{2}\rangle both in Fourier and real space. This negative magnetic diffusivity plays and opposite role in plasma motion (see Eq.ย (4.23), (4.24)).

On the other hand, Kraichnan derived the negative magnetic diffusion effect in Lagrangian formation with the assumption of strong helical field([20], see also [28]):

โˆ‚๐ยฏโˆ‚t=ฮฒ0โ€‹โˆ‡2๐ยฏ+ฯ„2โ€‹โˆ‡ร—โŸจฮฑโ€‹โˆ‡ร—ฮฑโŸฉโ€‹๐ยฏโ†’(ฮฒ0โˆ’ฯ„2โ€‹A)โ€‹โˆ‡2๐ยฏ.\displaystyle\frac{\partial\overline{\mathbf{B}}}{\partial t}=\beta_{0}\nabla^{2}\overline{\mathbf{B}}+\tau_{2}\nabla\times\langle\alpha\nabla\times\alpha\rangle\,\overline{\mathbf{B}}\rightarrow(\beta_{0}-\tau_{2}A)\nabla^{2}\overline{\mathbf{B}}. (4.22)

(Here, ฮฒ0=โˆซฯ„1u02โ€‹๐‘‘tโˆผฯ„1โ€‹u02,ฮฑโ€‹(๐ฑ,t)=(โˆ’)โ€‹1/3โ€‹โŸจ๐ฎโ‹…ฯ‰โŸฉโ€‹ฯ„1\beta_{0}=\int^{\tau_{1}}u^{2}_{0}dt\sim\tau_{1}u^{2}_{0},\,\alpha(\mathbf{x},\,t)=(-)1/3\langle\mathbf{u}\cdot\omega\rangle\tau_{1}, โŸจฮฑโ€‹(๐ฑ,t)โ€‹ฮฑโ€‹(๐ฑโ€ฒ,tโ€ฒ)โŸฉ\langle\alpha(\mathbf{x},\,t)\alpha(\mathbf{x}^{\prime},\,t^{\prime})\rangle=Aโ€‹(xโˆ’xโ€ฒ)โ€‹D2โ€‹(tโˆ’tโ€ฒ),ฯ„2=โˆซโˆžD2โ€‹(t)โ€‹๐‘‘tA(x-x^{\prime})D_{2}(t-t^{\prime}),\,\tau_{2}=\int^{\infty}D_{2}(t)\,dt.)
ฮฒ0\beta_{0} is the conventional positive magnetic diffusion effect. But, โˆ’ฯ„2โ€‹A-\tau_{2}A, which is from the correlation of โŸจฮฑโ€‹ฮฑโŸฉ\langle\alpha\alpha\rangle, actually plays the role of the negative magnetic diffusion ฮฒ\beta effect. The detailed derivation of Eq.ย (4.22) is not the same as Eq.ย (4.17)-(4.19). However, they both are from the turbulent velocity ๐ฎ\bf u and shows its helical feature produces the negative magnetic diffusion. Besides, there are some theoretical and experimental works associated with negative magnetic diffusivity ([20, 29], references therein). They are based on ฮฑโˆ’ฮฑ\alpha-\alpha correlation in the strong helical system and do not explain the coupling of HยฏM{\overline{H}}_{M} and EยฏM{\overline{E}}_{M}. These approaches are different from ours. However, it should be noted that the ฮฑโˆ’ฮฑ\alpha-\alpha correlation from ฮฑ\alpha effect eventually plays a role of negative magnetic diffusivity as the equation indicates.

So far, we have argued that the main reason of negative magnetic diffusivity is helical component in โ€˜uuโ€™(see Eq.ย (4.20), (4.22)). We can refer to the numerically supporting result in Fig.ย 9 in appendix [17]. When the helical kinetic forcing is turned off at tโˆผ200t\sim 200 and nonhelical forcing is on, negative ฮฒ\beta becomes positive. This negative magnetic diffusivity suppresses the growth of large scale magnetic field. It should be noted that ฮฒ\beta is the function of turbulent kinetic energy and kinetic helicity, not the forcing method itself.

The negative magnetic diffusivity is observed in liquid sodium experiment[30]. Simon et al. found that the small scale turbulent fluctuations (โˆผu\sim u) contribute to the negative magnetic diffusivity in the interior region. ฮฑ\alpha effect practically disappears for the lower Rโ€‹eMRe_{M} value. Instead, ฮฒ\beta effect increases strongly, which can promote the dynamo action.

4.5 Plasma quenching

As Fig.ย 1(a), 1(b) show, we briefly discuss how the helical magnetic field constrains plasma with the negative ฮฒ\beta effect [17]. As Eq.ย (2.2), (2.4) imply, plasma and magnetic field are coupled through Lorentz force and EMF. If we take the scalar product of ๐\bf B or ๐”\bf U on the curl of EMF or momentum equation respectively, we get ๐โ‹…โˆ‡ร—(๐”ร—๐){\bf B}\cdot\nabla\times({\bf U}\times{\bf B}) or ๐”โ‹…(๐‰ร—๐){\bf U}\cdot({\bf J}\times{\bf B}). And they are practically the same except the opposite sign. To make it clear, the field scales can be divided into ๐”ยฏ\overline{\bf U}, ๐ยฏ\overline{\bf B} and turbulent ๐ฎ\bf u, ๐›\bf b. Taking the average and applying Reynolds rule, we get

๐”โ‹…๐‰ร—๐\displaystyle{{\bf U}}\cdot{\bf J}\times{\bf B} =\displaystyle= โˆ’๐ยฏโ‹…โˆ‡ร—(๐”ยฏร—๐ยฏ)โˆ’๐ยฏโ‹…โˆ‡ร—โŸจ๐ฎร—๐›โŸฉ\displaystyle-{\overline{\bf B}}\cdot\nabla\times(\overline{\bf U}\times\overline{\bf B})-\overline{\bf B}\cdot\nabla\times\langle{\bf u}\times{\bf b}\rangle (4.23)
โˆ’โŸจ๐›โ‹…โˆ‡ร—(๐”ยฏร—๐›)โŸฉโˆ’โŸจ๐›โ‹…โˆ‡ร—๐ฎร—๐ยฏโŸฉ\displaystyle-\langle{\bf b}\cdot\nabla\times(\overline{\bf U}\times{\bf b})\rangle-\langle{\bf b}\cdot\nabla\times{\bf u}\times\overline{\bf B}\rangle

Considering Fig.ย 2, we see the first term is negligible. The third term is not so significant because of the high helicity ratio in the small scale regime. And the fourth term can be dropped replacing ๐ฃ{\bf j} with ฯโ€‹๐ฎ\rho\,{\bf u}. The second term can be rewritten like

โˆ’๐ยฏโ‹…โˆ‡ร—โŸจ๐ฎร—๐›โŸฉ\displaystyle-\overline{\bf B}\cdot\nabla\times\langle{\bf u}\times{\bf b}\rangle =\displaystyle= โˆ’๐ยฏโ‹…โˆ‡ร—(ฮฑโ€‹๐ยฏโˆ’ฮฒโ€‹โˆ‡ร—๐ยฏ)\displaystyle-\overline{\bf B}\cdot\nabla\times(\alpha\overline{\bf B}-\beta\nabla\times\overline{\bf B}) (4.24)
=\displaystyle= โˆ’ฮฑโ€‹๐ยฏโ‹…โˆ‡ร—๐ยฏโˆ’ฮฒโ€‹๐ยฏโ‹…โˆ‡2๐ยฏ.\displaystyle-\alpha\overline{\bf B}\cdot\nabla\times\overline{\bf B}-\beta\overline{\bf B}\cdot\nabla^{2}\overline{\bf B}.

The first term becomes negligible, but the second term is โˆ’ฮฒโ€‹๐ยฏโ‹…โˆ‡2๐ยฏโ†’ฮฒโ€‹k2โ€‹Bยฏ2-\beta\overline{\bf B}\cdot\nabla^{2}\overline{\bf B}\rightarrow\beta k^{2}\overline{B}^{2}. Then, the negative ฮฒ\beta suppresses the plasma motion ๐”ยฏ\overline{\bf U} while it amplifies ๐ยฏ\overline{\bf B} (see Fig.ย 1(a), (b)).

In comparison with helical large scale dynamo in Fig.ย 1, nonhelical small scale dynamo in Fig.ย 7 shows the supplementary role of ฮฒ\beta in the large scale plasma motion ๐”ยฏ\overline{\bf U}. Although small scale kinetic energy (โˆผโŸจu2โŸฉ\sim\langle u^{2}\rangle) is much larger than that of HMFD, there is no significant decrease in EV(โˆผUยฏ2E_{V}(\sim{\overline{U}^{2}}). This indicates that the positive ฮฒ\beta provides magnetic energy to the large scale plasma motion.

5 Summary

In this paper, we have pointed out the possibility of helical magnetic forcing dynamo (HMFD). HMFD has several features distinguished from helical kinetic forcing dynamo (HKFD). Externally given EME_{M} is converted into EVE_{V} through Lorentz force, which activates the plasma motion and EMF. This nontrivial EMF transports EME_{M} into the large and small scale region. EVE_{V} in HMFD is subsidiary to the migration of EME_{M} so that magnetic Reynolds number Rโ€‹eM(=Uโ€‹L/ฮท)Re_{M}(=UL/\eta) is negligibly small. Large scale magnetic energy EยฏM{\overline{E}}_{M} is amplified and saturated more efficiently than that of HKFD. Compared to our previous HKFD experiment, only 20% of provided magnetic energy produced the higher magnetic energy level. This may be able to explain the big gap between the cosmological seed magnetic field (โˆผ10โˆ’19โ€‹G\sim 10^{-19}G) and the galactic magnetic field (โˆผ10โˆ’6โ€‹G\sim 10^{-6}G).

The nonlinear interaction of helical field and plasma can be explained with ฮฑ\alpha and ฮฒ\beta effect which linearlize the nonlinear dynamo process. Since the exact definitions of ฮฑ\alpha&ฮฒ\beta are not yet known, we calculated them using Eq.ย (4.15), (LABEL:betaSolution3). Compared to the conventional theory, ฮฑ\alpha becomes negligible much earlier than the saturation of ๐ยฏ{\overline{\bf B}}. In contrast, ฮฒ\beta keeps negative and gets saturated along with EยฏM{\overline{E}}_{M}. Clearly, the effect of ฮฑ\alpha as a generator of EยฏM{\overline{E}}_{M} is not much. Rather, the negative ฮฒ\beta effect plays the substantial role of amplifying EยฏM{\overline{E}}_{M} with Laplacian โˆ‡2โ†’โˆ’k2\nabla^{2}\rightarrow-k^{2}(k=1). And we have discussed the wavenumber for the normalized large scale field should be constantly 1. In Fig.ย  2, 4, we used k=1 leading to the consistent result.

The main dynamo processes in the system are as follows: โˆซโˆ‚๐ฎ/โˆ‚tโ€‹dโ€‹ฯ„ร—๐›โˆผโˆซ๐ยฏโ‹…โˆ‡๐›โ€‹dโ€‹ฯ„ร—๐›โˆผโˆซ(๐›โ‹…โˆ‡ร—๐›)โ€‹๐‘‘ฯ„โ€‹๐ยฏ\int\partial{\bf u}/\partial t\,d\tau\times{\bf b}\sim\int{\overline{\bf B}}\cdot\nabla{\bf b}\,d\tau\times{\bf b}\sim\int({\bf b}\cdot\nabla\times{\bf b})\,d\tau\,\,{\overline{\bf B}} (positive magnetic helicity), ๐ฎร—โˆซโˆ‚๐›/โˆ‚tโ€‹dโ€‹ฯ„โˆผ๐ฎร—โˆซ๐ยฏโ‹…โˆ‡๐ฎโ€‹dโ€‹ฯ„โˆผโˆ’โˆซ(๐ฎโ‹…โˆ‡ร—๐ฎ)โ€‹๐‘‘ฯ„โ€‹๐ยฏ{\bf u}\times\int\partial{\bf b}/\partial t\,d\tau\sim{\bf u}\times\int{\overline{\bf B}}\cdot\nabla{\bf u}\,d\tau\sim-\int({\bf u}\cdot\nabla\times{\bf u})\,d\tau\,{\overline{\bf B}} (negative magnetic helicity), ๐ฎร—โˆซโˆ’๐ฎโ‹…โˆ‡๐ยฏโ€‹dโ€‹ฯ„ร—๐›โˆผฮฒโ€‹โˆ‡2๐ยฏ{\bf u}\times\int-{\bf u}\cdot\nabla{\overline{\bf B}}d\tau\times{\bf b}\sim\beta\nabla^{2}{\overline{\bf B}} (positive magnetic helicity). The first two interactions correspond to ฮฑ\alpha quenching, and the last one is associated to the negative ฮฒ\beta effect. These ฮฑ\alpha and negative ฮฒ\beta effect are commonly originated from the helical component in velocity field. In addition to the helical effect in conventional ฮฑ\alpha effect, we newly showed that the role of helical velocity field in the advection term โˆ’๐ฎโ‹…โˆ‡๐ยฏ-{\bf u}\cdot\nabla\overline{\bf B} leads to the negative ฮฒ\beta effect. And its prerequisite is turbulent kinetic helicity is larger than kinetic energy. We prepared for a supporting plot in Fig.ย 9 in appendix.

We showed the evolution of ฮฑ\alpha, ฮฒ\beta in Fig.ย 3 and verified their consistency in Fig.ย 4. The importance of this approach is the separation of ฮฑ\alpha&ฮฒ\beta from EMF without ambiguity. Numerically and analytically verified ฮฑ\alpha&ฮฒ\beta give us some clues to solve the nonlinear effects neglected in their analytic derivations as well as their experimental application. As long as EMF is represented as ฮฑโ€‹๐ยฏโˆ’ฮฒโ€‹โˆ‡ร—๐ยฏ\alpha\overline{\bf B}-\beta\nabla\times\overline{\bf B}, negative ฮฒ\beta replacing the quenching ฮฑ\alpha effect is a necessary condition for the amplification of large scale field. Moreover, the negative ฮฒ\beta effect suppresses the large scale plasma motion in the helical system.

The physical feature and effect of helical magnetic field in plasma are useful to investigate the origin of PMF as well as the current astrophysical phenomena. Biermann battery effect shows how the seed magnetic field in the early universe could be generated. And, neutrino-lepton interaction is a promising candidate of magnetic helicity in the Universe. The inverse cascade of magnetic helicity gives us a clue to the expansion of PMF scale constrained by the small horizon during inflation and amplification of its strength. And macroscopically, magnetic helicity explains how the evolution of magnetic field in plasma is constrained, which leads to the evolution of astro-plasma system eventually. All these events are closely related to HMFD.

In this paper we considered only the case of Pโ€‹rM=1Pr_{M}=1 with fully helical field in HMFD. However, we need to study more general system with Pโ€‹rMโ‰ 1Pr_{M}\neq 1 and arbitrary helicity ratio. Especially, the generation of poloidal magnetic field from the toroidal field in the solar convection zone with such a low Pโ€‹rM(โˆผ10โˆ’2)Pr_{M}\,(\sim 10^{-2}) challenges the current dynamo theory.

Acknowledgements
The authors appreciate support from National Research Foundation of Korea: NRF-2021R1I1A1A01057517, NRF-2020R1A2C3006177, and NRF-2021R1A6A1A03043957. Also, K. Park appreciates Dr. Frank Stefani and Dr. Matthias Rheinhardt for their useful advice on the Solar dynamo simulation.

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Appendix A Appendix

For Eq.(2.7), Biermannโ€™s effect is represented as

๐Ÿmโ€‹aโ€‹g=โˆ‡(peneโ€‹e)=โˆ‡neร—โˆ‡pene2โ€‹e,\displaystyle{\bf f}_{mag}=\nabla\bigg{(}\frac{p_{e}}{n_{e}e}\bigg{)}=\frac{\nabla n_{e}\times\nabla p_{e}}{n_{e}^{2}e}, (A.1)

which is a typical example of nonhelical magnetic forcing dynamo (NHMFD). Also, lepton-neutrino interaction produces the electromagnetic instability like below:

๐Ÿmโ€‹aโ€‹g=โˆ’GF2โ€‹|e|โ€‹neโ€‹โˆ‘ฮฝacAaโ€‹[(n0โˆ’+n0+)โ€‹๐›^โ€‹โˆ‚ฮดโ€‹nฮฝaโˆ‚t+(N0โˆ’+N0+)โ€‹โˆ‡(๐›^โ‹…ฮดโ€‹๐ฃฮฝa)].\displaystyle{\bf f}_{mag}=-\frac{G_{F}}{\sqrt{2}|e|n_{e}}\sum_{\nu_{a}}c_{A}^{a}\bigg{[}(n_{0}^{-}+n_{0}^{+})\,{\hat{\bf b}}\frac{\partial\delta n_{\nu_{a}}}{\partial t}+(N_{0}^{-}+N_{0}^{+})\nabla(\hat{\bf{b}}\cdot{\delta{\bf j}_{\nu_{a}}})\bigg{]}. (A.2)

Its axial vector term is represented as ๐Ÿmโ€‹aโ€‹g=ฮฑโ€ฒโ€‹๐{\bf f}_{mag}=\alpha^{\prime}{\bf B}, where ฮฑโ€ฒ\alpha^{\prime} is [31, 11]777Fermi constant GF=10โˆ’5/mp2G_{F}=10^{-5}/m^{2}_{p}(mpm_{p}: proton mass); cAa=โˆ“0.5c_{A}^{a}=\mp 0.5 (axial weak coupling, a:a: electron, muon, tau; (โˆ’)(-): electron, (+)(+)โ€™: muon or tau); ฮดโ€‹nฮฝa\delta n_{\nu_{a}}: neutrino density asymmetry; ฮดโ€‹๐ฃฮฝa\delta{\bf j}_{\nu_{a}} (neutrino current asymmetry); n0ยฑโˆผ(|e|โ€‹B/2โ€‹ฯ€2)โ€‹Tโ€‹lโ€‹nโ€‹โ€‰2n_{0}^{\pm}\sim(|e|B/2\pi^{2})Tln\,2 is the lepton number density at Landau level. ฮปfโ€‹lโ€‹uโ€‹iโ€‹dฮฝโˆผt\lambda^{\nu}_{fluid}\sim t is a scale of neutrino fluid inhomogeneity.:

ฮฑโ€ฒโˆผlโ€‹nโ€‹โ€‰24โ€‹2โ€‹ฯ€2โ€‹(10โˆ’5โ€‹Tmp2โ€‹ฮปfโ€‹lโ€‹uโ€‹iโ€‹dฮฝ)โ€‹ฮดโ€‹nฮฝnฮฝ.\displaystyle\alpha^{\prime}\sim\frac{ln\,2}{4\sqrt{2}\pi^{2}}\bigg{(}\frac{10^{-5}T}{m_{p}^{2}\lambda^{\nu}_{fluid}}\bigg{)}\frac{\delta n_{\nu}}{n_{\nu}}. (A.3)

These functions are not the same as our forcing function nor used in our simulation. However, ฮฑโ€ฒ\alpha^{\prime} is the result of ๐›^โ‹…ฮดโ€‹๐ฃฮฝa\hat{\bf{b}}\cdot{\delta{\bf j}_{\nu_{a}}}, which can produce helical magnetic field (HMFD).

Biermannโ€™s battery effect and neutrino-lepton interaction are developed with the quantum electromagnetic process and neutrino interaction. Their temporally and spatially inhomogeneous electromagnetic instabilities can induce the magnetic field and magnetic helicity. This generated magnetic field is amplified and transferred in the plasma system according to the MHD process. Their amplification processes are qualitatively consistent with the (magnetic) forcing dynamo with the modified EMF (ฮพ=๐”ร—๐+๐Ÿโˆ’ฮทโ€‹๐‰{\bf\xi}={\bf U}\times{\bf B}+{\bf f}-\eta{\bf J}, [23], and references therein).

Refer to caption
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Figureย 8: (a) 2D(azimuthal angle ฯ•\phi independent) simulation of Solar Magnetic field with Eq.ย (4.9), (4.10). The simulation yields the period ฮป=16.31\lambda=16.31 years. (b) Tidal effect of solar planets is added to ฮฑ\alpha. As the tidal effect grows, the period increases from ฮป<22\lambda<22 up to ฮป=21.74\lambda=21.74 years(Park 2021, not published). But in 1D, the period approaches in the opposite way.
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Figureย 9: (a) This plot is to compare the conventional ฮฒ\beta effect from EVE_{V} and that from HVH_{V}. All data for kโ‰ฅ2k\geq 2 are summed. (b) Helical kinetic forcing (HVโ‰ 0H_{V}\neq 0) is turned off at tโˆผ200t\sim 200. And the system was continuously driven with nonhelical kinetic energy (HV=0)H_{V}=0) [17].