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The 11-year magnetic Solar Cycle: Chaos control due to Jupiter

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The 11-year magnetic Solar Cycle:

Chaos control due to Jupiter

Johan Hansson

Division of Physics

Lule˚ a University of Technology SE-971 87 Lule˚ a, Sweden

Abstract

The observed magnetic field of the Sun is believed to originate from a “dynamo-effect” in its convective surface layer. However, there is no natural 11-year timescale in such models. We show that this major magnetic solar cycle naturally may arise through magnetic “chaos- control” of the inherently chaotic solar dynamo, mainly due to Jupiter.

The Sun exhibits an approximate 11-year solar cycle during which time its magnetic activity increases to a maximum with a complex surface magnetic field with a maximal number of sunspots and then declines to a minimum, essentially with no sunspots, with approximately a simple dipole field.

• In a canonical “dynamo-model” [1] of the solar cycle [2]1, [3] - and its highly complex, but yet very approximate and idealized modern numer- ical computer simulation variants, still far removed from the conditions in the real Sun - there exists no natural 11-year timescale. The dif- ferential rotation and convective motion of the Sun, thought to drive the observable magnetic field, instead having a timescale of ∼ days or

c.johan.hansson@ltu.se

1“The model described here is a freely running oscillator that lacks stabilization [...] it will be extremely sensitive to disturbing influences, random or otherwise, which may have a relatively large effect on the amplitude or phase of the magnetic cycle” [2].

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weeks. The observed major 11-year period may, more or less, be ac- commodated in order of magnitude, giving∼ (multi)decadal timescales with large spread between different numerical codes, ∼ 1 − 100 years, but only by fine-tuning, i.e. fitting, the free parameters of the dynamo- model. They are inaccessible to direct detection, under extreme condi- tions unattainable in the lab, inside the solar interior. It seems more plausible that the cause of the quite regular solar cycle lies external to the Sun itself. In the following, we suggest just such a simple natural origin of the cycle.

• There is ample evidence that the surface (observable) magnetic field, i.e. the turbulent nonlinear convective dynamo, of the Sun is inher- ently chaotic over timescales of weeks and months, see e.g. [4] - that is, very well described by nonlinear deterministic chaos, but not by stochasticity/randomness. Spacecraft observations of the heliospheric magnetic field reveal tell-tale fluctuations over all observable timescales corresponding with this view.

• It is also known that a tiny outside control (mathematically, arbitrar- ily small [5]) can serve as “chaos suppressor” for a chaotic system, in simple cases making one - out of the ∞-many, in the chaotic region [6]

- periodic/nearly periodic unstable limit cycle of the system stable [7], [8]. Phase-locking regions, “Arnold tongues”, correspond to rational ratios between a control frequency and the individual frequency of the unstable periodic orbit embedded in the chaotic attractor of the freely running system. It is the extreme sensitivity of chaotic systems - expo- nential growth of small disturbances - that allow even very small per- turbations to, after some time, produce large stabilizing changes to the phase-space orbit. In fact, the existence of nonlinear resonances with outside forces is a characteristic property of dynamical systems, and even a small external influence can lead to major dynamical changes.

• In the solar system, Jupiter carries about 60% of the total angular momentum, the Sun only less than 1%. In the standard solar-nebula model of the origin of the solar system, however, the Sun instead should carry the bulk, as it contains over 99% of the total mass. The general consensus is that the transfer of angular momentum has been due to some form of magnetic interaction [9],[10].

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• The magnetic fields in the solar system are not isolated, they are all interconnected in a complex interacting web and should consequently be considered as a whole, as they developed and evolved together.

• Jupiter has, by far, the strongest magnetic field of the planets in the solar system (∼ 1 mT, which, in turn, also explains its main contri- bution to the total angular momentum). As first approximation we may thus consider only the Sun-Jupiter interaction2. Though it has probably diminished since the earlier epochs of the solar system it still exists, and has been acting for billions of years, making a resonance likely.

• The magnetic field strength of the Sun at large distances does not fall off ∝ r−3 (na¨ıve dipole in a vacuum), but ∝ r−1 [11] due to the interplanetary medium being a plasma. At Jupiter (r ≃ 5.2 AU, θ ≃ π/2), there is an azimuthal dominance3of the field, Bϕ/Br ≃ rR−10 sinθ.

• Although continuum magnetohydrodynamic systems inherently con- tain an infinite number of degrees of freedom4 (partial differential equa- tions) in most problems they can be described by a finite number of modes - often only a small number of coupled ordinary differential equa- tions. In [4] the chaotic (not stochastic) character of sunspots over weeks, i.e. the underlying dynamo, is very well-described by Lorenz’

deterministic equations [12] - a model for the physics of a gravity- and pressure-confined viscous fluid heated from below and cooled at the surface (in this case the solar convection zone) - with canonical values of the parameters σ = 10, b = 8/3, r = 28, giving a strange/chaotic attractor in phase-space for X - proportional to the convection cur- rent, Y - proportional to the temperature difference between upward

2The other planets with appreciable magnetic fields will slightly modulate the precise astronomical “clock”-period of Jupiter, T = 11.86 years, affecting both the amplitude and the longer and shorter periodicities in the solar cycle. The same is true for deviations from the simple Parker model [11] for the real solar magnetic field in interplanetary space.

And for systems with (semi)infinite sets of characteristic times, like the turbulent solar dynamo, perfect phase locking cannot occur anyway. Although deterministic, the result is not regular.

3R0≃ 1 AU

4At the fundamental microscopic level, due to the finite collection of protons and elec- trons, the governing laws in the Sun are really in principle given by a finite, but very large,

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and downward moving fluid, Z - proportional to the departure from linearity of vertical temperature profile.

To study the regulating mechanism we only have to add a tiny, but cumulative, “chaos-control” p(t) due to the planets (in first approxi- mation dominated by Jupiter)

X = σ(Y˙ − X) + p(t) (1)

Y = rX˙ − XZ − Y (2)

Z = XY˙ − bZ (3)

• For simplicity, we approximate the magnetic field of Jupiter as a static dipole, m (by virtue of its solid core, high viscosity, and, most impor- tantly, observations), with inclination ∼ 10. Through F≃ ∇(m · B) the chaos-control for the Sun’s convective magnetic field, in first ap- proximation, becomes

p(t)≃ ϵ cos(ωt), (4)

where ω = 2π/T , with T = Jupiter’s orbital period and ϵ ≪ ⟨| ˙X|⟩, the time average of | ˙X|. The characteristic mean timescale of (turbulent) solar surface convection being τ ∼ weeks ∝ characteristic sunspot life- time driven by Sun’s differential rotation, in our model Ω = 2π/τ thus being the mean frequency of the unperturbed chaotic Lorenz equations.

However, for systems with a very broad distribution of intrinsic time scales, like the Lorenz system5 with the canonical parameter values, perfect phase synchronization cannot be reached [13], and the unstable periodic orbits have unbounded return times, i.e. can have arbitrarily low frequencies. (A feedback-loop not included in our simple model is that the more sunspots, the more active the Sun which then would slightly alter the magnetic coupling to the planets.)

5And the real Sun.

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Our main results and interpretation are given in Figs. 1 - 4. They suggest a simple, transparent explanation of the 11-year cycle. This is an advantage from the viewpoint of a physical understanding of the cycle, as the highly elaborate numerical magnetohydrodynamic-codes of the solar magnetic dy- namo more have the nature of a “black-box”, with a plethora of adjustable entities “hidden” inside the Sun, giving no real insight into why the 11-year cycle should appear at all. Furthermore, they are still, even using today’s most powerful computers, nowhere near implementing neither realistic pa- rameter ranges nor all effects believed to occur inside the real Sun. It seems more plausible that the origin of the actual cycle itself is due to some nat- urally occurring nearly-periodic external influence. The real turbulent solar dynamo may still well work roughly as envisioned, but there is no reason why an 11-year cycle, stably and predictably occurring under at least mil- lennia and probably much longer, should magically pop out without serious fine-tuning of unobservable entities - which also makes testing/falsification problematic.

In contrast, our hypothesis of magnetic-cycle chaos-control is, fortunately, potentially falsifiable. It may e.g. be tested in exoplanetary systems around solar-like stars when a statistically significant number of magnetic field cycles of the stars and orbital periods & magnetic fields of (dominant) exoplanets are reliably measured with sufficient accuracy, in systems in similar states of evolution as our solar system6.

6Presently, reliable, albeit indirect, detection of starspots through minute variations in the stars brightnesses, and hence presumably their cycles, are limited by the resolution

∼ 100 times larger than sunspots (which in the mean are comparable to the size of the

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Figure 1: X, proportional to the convection current in the Sun’s surface layer, as a function of time, for ϵ = 0 (i.e. without Jupiter) resulting in chaotic solar-cycle without periodicity.

Figure 2: X as in Fig. 1, but with ϵ ̸= 0 (i.e. with Jupiter) - a roughly periodic subharmonic 2:1 resonance of ∼ 11 years in the mean is seen, su- perposed on the intrinsic solar short-term chaotic fluctuations. Turbulent chaos in the solar dynamo is not removed, due to the weak coupling ϵ. The dynamo works as usual, but is modulated on long timescales giving cycles of sunspot maxima and minima with long-term magnetic reversals.

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Figure 3: As in Fig. 1, ϵ = 0 (i.e. without Jupiter), for X2 ∝ the dynamo power ∝ mean number of sunspots. Physically, this would result in a Sun that is permanently active with, on the average, many sunspots without 11-year cycle (white line same as in Fig. 4).

References

[1] E.N. Parker, Hydromagnetic dynamo models, Astrophys. J. 122, 293 (1955).

[2] H.W. Babcock, The Topology of the Sun’s Magnetic Field and the 22- Year Cycle, Astrophys. J. 133, 572 (1961).

[3] R.B. Leighton, A magneto-kinematical model of the solar cycle, Astro- phys. J. 156, 1 (1969).

[4] G.E. Morfill, H. Scheingraber, W. Voges & C.P. Sonett, Sunspot vari- ations: Stochastic or Chaotic, p. 30 in “The Sun in Time”, edited by C.P. Sonett, M.S. Giampapa & M.S. Matthews, The University of Ari- zona Press, Tucson (1991).

[5] D.K. Arrowsmith, Products of flows, Proc. Camb. Phil. Soc. 73, 301 (1973).

[6] D. Auerbach, P. Cvitanovi´c, J.-P. Eckmann, G. Gunaratne & I. Procac- cia, Exploring chaotic motion through periodic orbits, Phys. Rev. Lett.

58, 2387 (1987).

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Figure 4: As in Fig. 2, ϵ ̸= 0 (i.e. with Jupiter), for X2 ∝ the dynamo power ∝ mean number of sunspots. There is good correspondence to real sunspot data, despite the simplicity of our model: We see the fast increase - slower decline, cycles with double peaks, polarity reversal of sunspots at their minimum (Fig. 2), most orderly (i.e. strong) solar dipole field when dynamo power is at minimum (at sunspot minimum), roughly periodic cycle ∼ 11 years in the mean, erratic number of sunspots between cycles, etc. The ever- present background deterministic “noise” is due to the short term motion of the dynamo, which never stops - the Sun is never magnetically inactive.

However, below some threshold (white line, same as in Fig. 3) the magnetic field will not be sufficiently strong to locally disturb the visible surface of the Sun - producing few/no sunspots.

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[7] E. Ott, C. Grebogi & J.A. Yorke, Controlling chaos, Phys. Rev. Lett.

64, 1196 (1990).

[8] K. Pyragas, Continuous control of chaos by self-controlling feedback, Phys. Lett. A 170, 421 (1992).

[9] H. Alfv´en, On the Cosmogony of the Solar System, Stockholms Obser- vatoriums Annaler, Band 14, N:o 2 (1942).

[10] L. Mestel, Magnetic braking by a stellar wind - I, Mon. Not. R. Astron.

Soc. 138, 359 (1968).

[11] E.N. Parker, Dynamics of the interplanetary gas and magnetic fields, Astrophys. J. 128, 664 (1958).

[12] E.N. Lorenz, Deterministic Nonperiodic Flow, J. Atmos. Sci. 20, 130 (1963).

[13] M.A. Zaks, E.-H. Park, M.G. Rosenblum & J. Kurths, Alternating lock- ing ratios in imperfect phase synchronization, Phys. Rev. Lett. 82, 4228 (1999).

References

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