This paper was converted on www.awesomepapers.org from LaTeX by an anonymous user.
Want to know more? Visit the Converter page.

Oscillation in the temperature profile of the large-scale circulation of turbulent convection induced by a cubic container

Dandan Ji Department of Physics, Yale University, New Haven, CT 06520    Eric Brown Department of Mechanical Engineering and Materials Science, Yale University, New Haven, CT 06520 [email protected]
Abstract

We present observations of oscillations in the shape of the temperature profile of the large-scale circulation (LSC) of turbulent Rayleigh-Bénard convection. Temperature measurements are broken down into Fourier moments as a function of θθ0\theta-\theta_{0}, where θ\theta is the azimuthal angle in a horizontal plane at mid-height, and θ0\theta_{0} is the LSC orientation. The oscillation structure is dominated by a 3rd order sine moment and 3rd order cosine moment in a cubic cell. In contrast, these moments are not found to oscillate in a cylindrical cell. This geometry-dependent behavior can be explained by a minimal model that assumes that the heat transported by the LSC is conducted from the thermal boundary layers, and is proportional to the pathlength of the LSC along boundary layers at the top and bottom plates. In a non-circular cross-section cell, oscillations of the LSC orientation θ0\theta_{0} result in an oscillation in the container shape in the reference frame of the LSC, resulting in an oscillation in the pathlength of the LSC at a given θθ0\theta-\theta_{0}. In a square-cross-section cell, this model predicts the dominant 3rd order sine moment and 3rd order cosine moment with magnitudes within 50% of measured values, when using the amplitude of the oscillation of θ0\theta_{0} as input. A cylindrical cell is special in that the pathlength is independent of θ0\theta_{0}, and so these oscillating moments are not induced. In a cylindrical cell, the model reproduces the sinusoidal mean temperature profile with a sloshing oscillation dominated by the 2nd order sine moment, consistent with previous observations in that geometry.

I Introduction

Turbulent flow often generates large-scale coherent structures, such as convection rolls in the atmosphere. Such structures can play important roles in directing heat and mass transport. The fact that these structures have typical shapes and are long-lived makes them more amenable to being approximately modeled by equations of motion, more so than the wide spectrum of small-scale turbulent fluctuations. A long-term goal is more complete modeling of such large-scale coherent flows in turbulence. We work toward this goal by presenting a model to explain a recently observed oscillation in the shape of the temperature profile of a large-scale coherent structure, described below.

We use Rayleigh-Bénard convection as a model laboratory system that generates large-scale coherent flow structures (for reviews, see Refs. Ahlers et al. (2009); Lohse and Xia (2010)). A fluid is heated from below and cooled from above to generate buoyancy-driven convection. This system exhibits robust large-scale coherent structures, i.e. they retain a particular organized flow structure over long times. For example, in containers of aspect ratio near 1, typically a large-scale circulation (LSC) forms. This LSC consists of temperature and velocity fluctuations which, when coarse-grain averaged, collectively form a single convection roll in a vertical plane that breaks the symmetry of the system, and exists nearly all of the time Krishnamurti and Howard (1981). Turbulent fluctuations drive the orientation θ0\theta_{0} of the LSC in the horizontal plane to meander spontaneously and erratically over time Cioni et al. (1996); Brown and Ahlers (2006); Xi et al. (2006).

The dynamics of the LSC includes a prominent oscillation mode that has long been observed in leveled cylindrical containers Heslot et al. (1987); Sano et al. (1989); Castaing et al. (1989); Ciliberto et al. (1996); Takeshita et al. (1996); Cioni et al. (1997); Qiu et al. (2000); Qiu and Tong (2001); Niemela et al. (2001); Qiu and Tong (2002); Qiu et al. (2004); Funfschilling and Ahlers (2004); Sun et al. (2005); Tsuji et al. (2005). The flow structure of these oscillations is a combination of twisting in θ0\theta_{0} Funfschilling and Ahlers (2004); Funfschilling et al. (2008) and sloshing Xi et al. (2009); Zhou et al. (2009); Brown and Ahlers (2009). This combination of flow structures can alternatively be described from a Lagrangian viewpoint as a single closed-loop advected oscillation mode, consisting of the hot and cold regions oscillating in the azimuthal coordinate while being advected around by the LSC with two oscillation periods per LSC rotation (referred to as the n=2n=2 advected mode) Brown and Ahlers (2009). This oscillation can be modeled with stochastic differential equations Brown and Ahlers (2009). The pressure from the sidewall creates a potential, with a corresponding restoring force against slosh displacements which pushes the LSC towards alignment with the center of the container Brown and Ahlers (2009). Turbulent fluctuations provide a broad-spectrum noise to drive oscillations at the resonant frequency of the potential.

In non-circular cross-section containers, the potential is further modified by the geometry of the cell, and the restoring force tends to push the LSC to align with the longest diagonals Zimin and Ketov (1978); Zocchi et al. (1990); Qiu and Xia (1998); Valencia et al. (2007); Ji and Brown (2020). This results in oscillations in θ0\theta_{0} around a potential minimum at a corner in rectangular cross-section containers Song et al. (2014); Vasiliev et al. (2016); Giannakis et al. (2018); Ji and Brown (2020). The addition of a restoring force acting directly on θ0\theta_{0} excites additional advected modes. In this case, the dominant structure has one oscillation per LSC rotation (referred to as the n=1n=1 advected oscillation mode), in which the oscillation in θ0\theta_{0} is in-phase at different heights, and the sloshing is out-of-phase at the top and bottom halves of the container Brown and Ahlers (2009); Ji and Brown (2020).

Several other oscillation modes are known to exist. The LSC orientation θ0\theta_{0} can oscillate between diagonals of a non-square rectangular cross-section in a wider potential well Song et al. (2014). In cylindrical cells tilted by several degrees relative to gravity, the LSC orientation can oscillate around the orientation of the tilt; the tilt produces an orientation-dependent forcing that provides a restoring force that can cause an oscillation around a potential minimum Brown and Ahlers (2008a). An oscillation in θ0\theta_{0} was found in a cubic cell where the preferred orientation aligns with grooves in the top and bottom plates Foroozani et al. (2019), which can also be described as an oscillation around a preferred orientation. An oscillation mode in which the rotational axis of of the LSC flexes and rotates around the center of the cell like a jump rope has been observed in aspect ratio 2 cells, although its cause is unknown Vogt et al. (2018).

In a previous manuscript, we reported observations of a new oscillation in the shape of the LSC Ji and Brown (2020). This was represented in terms of Fourier moments of the temperature profile in the azimuthal coordinate relative to the orientation θ0\theta_{0} of the LSC Ji and Brown (2020). Specifically, we found 3rd- and 4th-order sine moments in a cubic cell, which were not found in cylindrical cells Brown and Ahlers (2009), suggesting that this oscillation depends on cell geometry. The 3rd-order moment in the temperature profile does not have the antisymmetry of the temperature profile of the sloshing mode (where the hot and cold sides of the temperature profile move in opposite directions) Brown and Ahlers (2009), or the symmetry around the LSC plane of the jumprope oscillation Vogt et al. (2018), so is distinct from those known modes. As the goal of those measurements was to test the prediction of advected oscillation modes in a cubic container, which required measuring the sloshing oscillation but not the full temperature profile, an incomplete set of moments consisting of only sine terms was presented.

In this manuscript, we present a more complete set of Fourier moments of the temperature profile, and we present a minimal model to explain the oscillation in the shape of the temperature profile of the LSC in a non-circular cross-section container Ji and Brown (2020). Section II explains the experimental methods. Section III shows the observations of the temperature profile of the LSC in a cubic cell in terms of Fourier moments of the temperature profile, reporting a complete set of both sine and cosine moments. Section IV compares these to the same Fourier moments for a cylindrical cell to confirm that the new moments are not found in cylinders. Section V presents a model to explain the oscillation in the temperature profile.

II The experimental apparatus and methods

II.1 Experimental setup

Refer to caption
Figure 1: A schematic of the experimental setup. (a) Top view: the thick line represents the central circulation plane of the LSC, with θ0\theta_{0} defined as the orientation relative to a diagonal. Thermistor locations on the sidewall are indicated by solid circles. (b) Side view.

The design of the experimental setup is the same apparatus used in Ref. Bai et al. (2016), where it is described in more detail. We describe it briefly here. The flow chamber is nearly cubic, with height H=20.32H=20.32 cm, and horizontal dimensions of 20.0420.04 cm and 19.9919.99 cm, as shown in Fig. 1. The top and bottom surface are aluminum plates, with double-spiral water-cooling channels. To control the plates at a temperature difference of ΔT\Delta T, with the bottom plate hotter than the top plate, water is circulated through each plate by a temperature-controlled water bath. The sidewalls are made of plexiglas, and three out of four have a thickness of 0.55 cm. The fourth sidewall has thickness 0.900.90 cm, and is shared with another identical flow chamber to be used in future experiments, but the two chambers are designed to be thermally insulated from each other for the experiments reported here.

The working fluid is degassed and deionized water with mean temperature of 23.0C{}^{\circ}\mathrm{C}, for a Prandtl number Pr=ν/κ=6.4Pr=\nu/\kappa=6.4, where ν=9.4×107\nu=9.4\times 10^{-7} m2/s is the kinematic viscosity and κ\kappa is the thermal diffusivity. The Rayleigh number is given by Ra=gαΔTH3/κνRa=g\alpha\Delta TH^{3}/\kappa\nu where gg is the acceleration of gravity and α\alpha is the thermal expansion coefficient. We report measurements at ΔT=18.35\Delta T=18.35 C for Ra=2.62×109Ra=2.62\times 10^{9}.

The alignment of the LSC is partially locked along a diagonal to prevent corner-switching with a small tilt of the cell relative to gravity, as is commonly done Krishnamurti and Howard (1981). We report data for a tilt angle of β=(1.0±0.2)\beta=(1.0\pm 0.2)^{\circ}, at an orientation within 0.030.03 rad of the diagonal where we define θ0=0\theta_{0}=0.

To measure the LSC, thermistors were mounted in the sidewalls. There are 3 rows thermistors at heights H/4-H/4, 0, and H/4H/4 relative to the mid-height of the container, as shown in Fig. 1b. In each row there are 8 thermistors equally spaced in the azimuthal angle θ\theta measured in a horizontal plane, as shown in Fig. 1a. In this manuscript, we only report measurements from the middle row of thermistors, unless otherwise stated. Temperatures were recorded every 9.7 s at each thermistor.

II.2 Obtaining the LSC orientation θ0\theta_{0}

The LSC orientation was obtained using the same methods as Ref. Brown and Ahlers (2006). As the LSC pulls hot fluid from near the bottom plate up one side and cold fluid from near the top plate down the other side, a temperature difference is detected along a horizontal direction at the mid-height of the container. We fit the 8 thermistor temperatures at the middle row to the function

T=T0+δcos(θθ0)T=T_{0}+\delta cos(\theta-\theta_{0}) (1)

to get the orientation θ0\theta_{0} and strength δ\delta of the LSC at each time step.

II.3 Obtaining the Fourier moments of the temperature profile

We first fit Eq. 1 to T(θ)T(\theta) to obtain θ0\theta_{0} at each time step. This allows viewing of the temperature profile relative to the LSC orientation as T(θθ0)T(\theta-\theta_{0}) to separate out meandering and oscillations of the LSC orientation from changes in the temperature profile. We then express perturbations on the sinusoidal temperature profile as the Fourier series

T=T0+δcos(θθ0)+n=24Ansin(n(θθ0))+n=24Bncos(n(θθ0)),T=T_{0}+\delta\cos(\theta-\theta_{0})+\sum_{n=2}^{4}A_{n}\sin(n(\theta-\theta_{0}))\\ +\sum_{n=2}^{4}B_{n}\cos(n(\theta-\theta_{0}))\ , (2)

where the Fourier moments are calculated as

An=14i=18[TiT0δcos(θθ0)]sin[n(θθ0)]A_{n}=\frac{1}{4}\sum_{i=1}^{8}{[T_{i}-T_{0}-\delta\cos(\theta-\theta_{0})]\sin[n(\theta-\theta_{0})]} (3)

and

Bn=14i=18[TiT0δcos(θθ0)]cos[n(θθ0)].B_{n}=\frac{1}{4}\sum_{i=1}^{8}{[T_{i}-T_{0}-\delta\cos(\theta-\theta_{0})]\cos[n(\theta-\theta_{0})]}\ . (4)

Here the sum over ii corresponds to the sum over different thermistors. We can only calculate the first 4 moments due to the Nyquist limit with 8 measured temperatures. We don’t include B1B_{1} since that was already defined as δ\delta, and A1A_{1} is trivially zero since we first fit to Eq. 1.

III Fourier moments of the temperature profile of the LSC in a cubic cell

In this section, we identify oscillations in the temperature profile of the LSC in a cube in terms of Fourier moments of the temperature profile T(θθ0)T(\theta-\theta_{0}) as in Refs. Brown and Ahlers (2009); Vogt et al. (2018).

Refer to caption
Figure 2: Power spectrum of the Fourier moments AnA_{n}, as indicated in the legend. Thin lines show the linear background PbgP_{bg} subtracted off when integrating the peak power. Each moment oscillates, except for A2A_{2}.
Refer to caption
Figure 3: Power spectrum of the Fourier moments BnB_{n} and other terms of the temperature profile, as indicated in the legend. Each signal oscillates except for δδ\delta-\langle\delta\rangle.
Refer to caption
Figure 4: Power spectrum of θ0θ0\theta_{0}-\langle\theta_{0}\rangle. The oscillations of the Fourier moments have the same frequency as the oscillation of θ0\theta_{0}.

Fourier moments were calculated according to Sec. II.3, and the power spectrum of each Fourier moment was calculated as

P(ω)=1Nπ|x^(ω)|2dtP(\omega)=\frac{1}{N\pi}\sum\left|\hat{x}(\omega)\right|^{2}dt (5)

where NN is the number of data points, and x^(ω)=x(t)exp(iωt)\hat{x}(\omega)=\sum x(t)\exp(i\omega t) where xx can stand for any parameter of the temperature profile such as AnA_{n}, BnB_{n}, δδ\delta-\langle\delta\rangle, or T0T0T_{0}-\langle T_{0}\rangle. In each case we average P(ω)P(\omega) over a range of 9.88×1049.88\times 10^{-4} rad/s in ω\omega to smooth the data. The smoothed P(ω)P(\omega) are shown in Fig. 2 for AnA_{n} (AnA_{n} are reproduced from Ji and Brown (2020)) and in Fig. 3 for BnB_{n}, δδ\delta-\langle\delta\rangle, and T0T0T_{0}-\langle T_{0}\rangle. We also show the power spectrum of θ0θ0\theta_{0}-\langle\theta_{0}\rangle in Fig. 4 for comparison. Most of the power spectra have peaks (T0T0T_{0}-\langle T_{0}\rangle, B2B_{2}, B3B_{3}, B4B_{4}, A3A_{3}, and A4A_{4}), indicating oscillation, which is at the same frequency as the oscillation of θ0\theta_{0}. Only moments A2A_{2} and δδ\delta-\langle\delta\rangle do not have a resolvable peak in the power spectrum.

Refer to caption
Figure 5: Solid line: Illustration of a temperature profile with an A3A_{3} moment with amplitude of 0.15δ0.15\delta. Dotted line: cos(θθ0)\cos(\theta-\theta_{0}).

Some of the Fourier moments are already known as contributing to advected oscillation modes Brown and Ahlers (2009); Ji and Brown (2020). The oscillation in θ0\theta_{0} is part of the n=1n=1 advected oscillation mode which was predicted and observed to be dominant in cubic containers Ji and Brown (2020), in which the oscillation in θ0\theta_{0} has maximum amplitude at the mid-height of the container, and nodes at the center of the top and bottom plates Brown and Ahlers (2009); Ji and Brown (2020). The sloshing, typically represented by the moment A2A_{2}, is predicted to have nodes at the mid-height of the container, and maximum amplitude at the center of the top and bottom plates Brown and Ahlers (2009); Ji and Brown (2020). The lack of an A2A_{2} moment at the lowest frequency at mid-height in a cubic geometry is thus predicted by the advected oscillation model.

Other Fourier moments of the temperature profile can be related to oscillation structures as follows. In principal, any even-order AnA_{n} (i.e. A2A_{2} and A4A_{4}) shift the maximum and minimum of the temperature profile in opposite directions, are antisymmetric around θ0\theta_{0}, and could be interpreted as a sloshing of the LSC Xi et al. (2009); Zhou et al. (2009); Brown and Ahlers (2009). Only the A2A_{2} moment was found to oscillate in cylindrical containers, and A4A_{4} has not been reported to oscillate before Brown and Ahlers (2009). Even-order BnB_{n} (i.e. B2B_{2} and B4B_{4}) and T0T0T_{0}-\langle T_{0}\rangle lead to a change in the temperature profile that breaks the symmetry around T=T0T=\langle T_{0}\rangle, and can split one of the temperature extrema into two separate extrema if B2B_{2} or B4B_{4} are large enough, similar to the jumprope oscillation Vogt et al. (2018). Our observation of small peaks in B2B_{2}, B4B_{4}, and T0T0T_{0}-\langle T_{0}\rangle confirm the existence of a weak jumprope mode, or a mode with similar symmetry for water in a cubic cell. Odd-order BnB_{n} (i.e. B3B_{3}) preserve all the symmetries of the temperature profile, but have not been reported to oscillate before. Odd-order AnA_{n} (i.e. A3A_{3}) shift the maximum and minimum of the temperature profile in the same direction by the same amount, but break the symmetry around θ0=0\theta_{0}=0, while preserving a translational antisymmetry upon shifting θ0\theta_{0} by π\pi. An illustration of this moment is given in Fig. 5. The A3A_{3} moment does not correspond to any previously reported oscillation modes.

moment A2,pA_{2,p} A3,pA_{3,p} A4,pA_{4,p} B2,pB_{2,p} B3,pB_{3,p} B4,pB_{4,p} TpT_{p} δp\delta_{p} θ0,p\theta_{0,p}
amplitude (mK) 0 28 7 3 7 2 2 0 16
Table 1: Root-mean-square oscillation amplitudes of terms of the temperature profile. All amplitude are given in units of mK, each with an error of 2 mK. The amplitude of the oscillation in A3A_{3} is significantly larger than the other terms.

To quantify the amplitude of each of the oscillating moments in Figs. 2, 3, and 4, we calculate the peak power in each power spectrum. Each peak power is obtained from the integral (P(ω)Pbg)𝑑ω\int(P(\omega)-P_{bg})d\omega, where PbgP_{bg} is a linear background which is excluded from the integral, as shown for example in Fig. 2 as the region bounded by the thin line that connects the first and last data point in the visually identified peak. According to Parseval’s Theorem, the root-mean-square (rms) amplitude of the oscillation in units of temperature is given by the square root of the integral of peak power. We define these rms oscillation amplitudes as An,pA_{n,p} for moments AnA_{n}, Bn,pB_{n,p} for moments BnB_{n}, δp\delta_{p} for δδ\delta-\langle\delta\rangle, and TpT_{p} for T0T0T_{0}-\langle T_{0}\rangle. These oscillation amplitudes are summarized in Table 1. There is an error of 2 mK on these measurements, dominated by the uncertainty in identifying the range to fit the peak and its background. The raw amplitude of θ0,p=37\theta_{0,p}=37 mrad is obtained from the power spectrum of θ0θ0\theta_{0}-\langle\theta_{0}\rangle, which is converted into mK for comparison in Table 1 by multiplying by δ=0.431\langle\delta\rangle=0.431 K. Among all the amplitudes, A3,pA_{3,p} is the largest, even larger than the well-known oscillation in θ0\theta_{0}, and B3,pB_{3,p} and A4,pA_{4,p} are tied for the next largest amplitudes. The remaining moments are near the resolution limit. The significant oscillations in the moments A3A_{3}, B3B_{3}, and A4A_{4} remain unexplained.

III.1 Asymmetries

To check for consistency of data with expected symmetries, we measured phase shifts between different oscillating moments by calculating correlation functions (not shown) as in Ji and Brown (2020). Notably, the oscillation of moment A4A_{4} is found to be in phase with θ0\theta_{0}. An in-phase superposition of these two moments results in an asymmetry between the hot and cold sides of the LSC at the mid-height where the hot side oscillates with a larger amplitude than the cold side. This asymmetry between the hot and cold sides of the flow appears to be a form of non-Boussinesq asymmetry, similar to an observation of a very weak oscillation of A2A_{2} out-of-phase by π\pi rad with θ0\theta_{0} Ji and Brown (2020). To test whether this is a non-Boussinesq effect due to the change in material parameter values with the temperature on opposite sides of the cell, or due to some other asymmetry of the setup, we compare data from a similar dataset where the cell was nearly level but tilted slightly to cancel out asymmetries so that the LSC orientation sampled all 4 corners of the container Bai et al. (2016). When calculating the phase shift between A4A_{4} and θ0\theta_{0} separately for each potential well, we find them to be in phase in 2 wells and π\pi out of phase in the other 2 wells. This difference between potential wells suggests that the existence of A4A_{4} in the long-term average is likely due to an asymmetry of the experimental setup. An alternative possibility is that it is a long-lived spontaneous-symmetry-breaking mode that did not have time to sample all of the possible phase shifts, although it was observed in a dataset that was 10 days long.

IV Fourier moments of the temperature profile in a cylindrical cell

Refer to caption
Figure 6: (color online) Power spectra of moments of the temperature profile as indicated in the legend, for a cylindrical container Brown and Ahlers (2009). A2A_{2} is the dominant oscillating mode, corresponding to a sloshing back and forth of the LSC. This lacks the strong A3A_{3} and B3B_{3} moments found for a cubic container.

To identify which moments of the oscillations observed in Sec. III are depend on container geometry, we compare to data from a cylindrical cell at Ra=1.1×1010=1.1\times 10^{10}, Pr=4.4Pr=4.4, and aspect ratio 1 Brown and Ahlers (2009). Power spectra of the AnA_{n} moments were reported in Brown and Ahlers (2009), and here we additionally report BnB_{n}, δ\delta and T0T0T_{0}-\langle T_{0}\rangle for that dataset. Power spectra were calculated according to Eq. 5, smoothed by averaging over a range of 2.15×1032.15\times 10^{-3} rad/s, and shown in Fig. 6. A2A_{2} has the largest peak, in contrast with the cubic cell data in Fig. 2 where A2A_{2} was the only term that did not oscillate at the mid-height. The oscillation in A2A_{2} in the cylinder at mid-height is known as the sloshing aspect of the n=1n=1 advected oscillation mode Brown and Ahlers (2009). B3B_{3} and δδ\delta-\langle\delta\rangle may also exhibit weak oscillations in Fig. 6, but these are near our resolution limit. The difference in oscillating moments between the cylinder in Fig. 6 and in the cube in Figs. 2 and 3 suggests that these new moments of oscillation of the temperature profile depend on container geometry; specifically the dominant A3A_{3} moment followed by the B3B_{3} moment.

V Model of the temperature profile

Refer to caption

Figure 7: Pathlength of the LSC along the top and bottom plates as a function of the orientation θf\theta_{f} of the flow and coordinate θ\theta for (a) a circular cross-section cell, and (b) a square cross-section cell. The thick solid lines with arrows indicate the central path of the LSC. The parallel lines indicate pathlengths at different θ\theta.

To understand the geometry-dependence of the oscillation of the shape of the temperature profile, we propose a minimal model. Since the LSC transfers heat to and from the thermal boundary layers near the top and bottom plates, we hypothesize that the temperature difference TT0T-T_{0} across any streamline of the LSC is proportional to the pathlength λ\lambda of that streamline along the top and bottom plates. This is the result of a simplistic approximation of the heat conduction if the boundary layer and flow are uniform along the plates, and the temperature difference between the boundary layer and the bulk is large compared to TT0T-T_{0} in the LSC. To identify these streamlines we have to imagine an average over a time and length scale large enough to remove fluctuations, but short enough that the LSC orientation has not changed much. The pathlength λ\lambda can in general be a function of both the orientation θf\theta_{f} of the flow at the edges of the top and bottom plates, and can vary around the cell with the coordinate θ\theta at the wall of the container where measurements are made. θf\theta_{f} is not necessarily the same as the LSC orientation θ0\theta_{0} from the temperature profile fit, although they are expected to be closely related. The pathlength as a function of θ\theta depends on θ0\theta_{0}, but the slosh displacement only shifts the nominal central plane of the LSC, not the pathlength as a function of θ\theta, so the pathlengths can be completely expressed in terms of θ0\theta_{0} and θ\theta. We make the approximation that the temperature profile obtained from the pathlength λ\lambda is advected vertically and retains its shape, with the hot side of the LSC (|θ|π/2|\theta|\leq\pi/2) advected upward from the bottom plate, and the cold side of the cell advected downward from the top plate. This ignores heat transfer by conduction in the bulk or turbulent mixing, as that is expected to smooth temperature profiles rather than produce higher order moments in the temperature profile. Thus this model should not be used to characterize the dependence of the mean temperature profile on height. We also ignore any modification to the heat transport by counter-rolls in corners, as we do not know the flow fields in a cubic cell, so we do not know how big an effect they would have, how it depends on θ\theta, or how much the pathlength of corner rolls should count toward the sidewall temperature profile. We approximate streamlines as straight across the plates, although even the idealized traveling wave solutions of the advected oscillation mode would have curved streamlines Brown and Ahlers (2009); Ji and Brown (2020), resulting in a slight underestimate of the pathlength by using straight lines.

With the above assumptions, the temperature profile is predicted to be

TT0λ(θ,θf)Hsign[cos(θθf)],T-T_{0}\propto\frac{\lambda(\theta,\theta_{f})}{H}sign[\cos(\theta-\theta_{f})]\ , (6)

where sign[cos(θθf)]sign[\cos(\theta-\theta_{f})] is a step function to account for whether heat is gained (+1+1) or lost (1-1) from the hot or cold plates, respectively. The pathlength λ\lambda can be calculated based on the geometry of the container, as shown for example in Fig. 7 for circular and square cross sections. The predicted temperature profile reduces to a simple known result in the case of a circular cross section container: λ(θ)/H=|cos(θθf)|\lambda(\theta)/H=|\cos(\theta-\theta_{f})|, so Eq. 6 yields TT0cos(θθf)T-T_{0}\propto\cos(\theta-\theta_{f}), which matches the shape of the measured mean temperature profile in cylindrical containers within 5% Brown and Ahlers (2007), if in this case the proportionality in Eq. 6 equals δ\delta, and θf=θ0\theta_{f}=\theta_{0}. With cylindrical symmetry, the pathlength does not depend on where θ=0\theta=0 is defined, and the flow orientation matches the extrema of the temperature profile (θf=θ0\theta_{f}=\theta_{0}).

The amplitude δ\delta of the temperature profile can be predicted from a simple extension of the approximate rate of temperature change δ˙\dot{\delta} of a parcel of fluid in the LSC due to conduction through the thermal boundary layer Brown and Ahlers (2008b), times the duration that the parcel of fluid advects past each plate 𝒯/4\mathcal{T}/4 (𝒯=141\mathcal{T}=141 s Ji and Brown (2020) is the LSC turnover time). This yields the prediction δ=3πκΔT𝒩𝒯/16L2=0.8\delta=3\pi\kappa\Delta T\mathcal{N}\mathcal{T}/16L^{2}=0.8 K (𝒩=86\mathcal{N}=86 Funfschiling et al. (2005) is the Nusselt number), about twice the measured value, which is consistent within the level of approximation of the model of Brown & Ahlers Brown and Ahlers (2008b). This supports the assumption that the temperature profile can be quantitatively estimated based on heat conduction through the boundary layer.

V.1 Predicted pathlength for a cubic cell

Refer to caption

Figure 8: (color online) Thick solid black line: Example of a predicted temperature profile based on the pathlength λ(θ)/H\lambda(\theta)/H along the top and bottom plates of a cubic cell for θf=0.3\theta_{f}=0.3 rad. Dashed blue line: cosine fit (Eq. 6) as a 1st-order approximation of the temperature profile. Dotted red line: difference between the predicted temperature profile and 1st-order cosine term. Thin solid red line: Fit of 3rd order sine moment (A3A_{3}) to the difference. The difference is dominated by the A3A_{3} moment.

In a cell without circular symmetry, changes in the orientation θ0\theta_{0} lead to a change in the pathlength with both θ\theta and θf\theta_{f} as the shape of the container changes in the reference frame of the LSC. The n=1n=1 advected oscillation mode was observed in experiments with the same cubic cell that we report data from in this paper Ji and Brown (2020). The preferred flow orientation is aligned along a diagonal, with oscillations in θ0\theta_{0} centered on a diagonal. While θ0=0\theta_{0}=0 at the center of the top and bottom plates in the n=1n=1 mode, assuming the LSC runs in a rectangular path along the inner wall of the container, the peak amplitude of the oscillation in θ0\theta_{0} at the edges of the plates is still expected to be sin[π/2×2/(1+2)]=0.79\sin[\pi/2\times\sqrt{2}/(1+\sqrt{2})]=0.79 times the amplitude at the mid-height. These hot and cold spots advect upward and downward, respectively, so that the thermal profile obtained at the top and bottom plates passes the mid-height at the same time. The hot and cold spots are also predicted to advect azimuthally Brown and Ahlers (2009), and azimuthal flow has been observed Vasiliev et al. (2019). Because the displacements in θ0\theta_{0} are in phase at the top and bottom plates for the n=1n=1 mode, the restoring force pushes them in the same direction such that they shift the entire temperature profile so that θf\theta_{f} is closer to zero at the mid-height. Thus, even with this azimuthal advection, the predicted temperature profile at the mid-height is the same as the pathlength across the plate in terms of T(θθ0T(\theta-\theta_{0}).

For a square cross-section with origin θ=0\theta=0 in a corner as shown in Fig. 7, the pathlength at the top and bottom plates is given by

λ(θ)H=1cos(π/4|θf|)\frac{\lambda(\theta)}{H}=\frac{1}{\cos(\pi/4-|\theta_{f}|)} (7)

for 0<θ<π/20<\theta<\pi/2 and [1+tan(θπ/4)]/2>tan(π/4|θf|)[1+\tan(\theta-\pi/4)]/2>\tan(\pi/4-|\theta_{f}|), which is a constant independent of θ\theta, and

λ(θ)H=1tan(θπ/4)2sin(π/4|θf|)\frac{\lambda(\theta)}{H}=\frac{1-\tan(\theta-\pi/4)}{2\sin(\pi/4-|\theta_{f}|)} (8)

for 0<θ<π/20<\theta<\pi/2 and [1+tan(θπ/4)]/2<tan(π/4|θf|)[1+\tan(\theta-\pi/4)]/2<\tan(\pi/4-|\theta_{f}|), and

λ(θ)H=1+tan(θπ/4)2cos(π/4|θf|).\frac{\lambda(\theta)}{H}=\frac{1+\tan(\theta-\pi/4)}{2\cos(\pi/4-|\theta_{f}|)}\ . (9)

for π/2<θ<0-\pi/2<\theta<0. This profile is repeated periodically every π\pi rad. An example plot is shown in Fig. 8.

To determine the proportionality coefficient in the temperature profile of Eq. 6 for a non-circular cross-section, we use the assumption of the Brown-Ahlers model that the flow velocity at the sidewall in the direction of the LSC (and thus δ)\delta) does not vary with small changes in diameter Brown and Ahlers (2008a). This choice had a significant consequence in determining the form of the potential in θ0\theta_{0}, for example with potential minima at the corners Brown and Ahlers (2008a). In contrast, allowing δ\delta to vary with the pathlength along θ0\theta_{0} would have led to a different potential, with a prediction that corners would no longer be the most preferred orientations, which disagrees with observations Zimin and Ketov (1978); Zocchi et al. (1990); Qiu and Xia (1998); Valencia et al. (2007); Liu and Ecke (2009); Bai et al. (2016); Foroozani et al. (2017); Giannakis et al. (2018); Vasiliev et al. (2016, 2019); Ji and Brown (2020). To keep consistent with the previous model assumption Brown and Ahlers (2008a) and experimental observations, the temperature profiles should be normalized by δ\delta to remove variations in δ\delta with θ0\theta_{0}, so the proportionality coefficient should be δ2/δ\langle\delta\rangle^{2}/\delta, to retain the result that the mean value of the coefficient is δ\langle\delta\rangle. However, since δ\delta is calculated from the temperature profile, this normalization is done after the shape of the temperature profile is calculated and δ\delta obtained from a fit of the temperature profile. In practice, this leads to a correction of less than 0.3% in the rms amplitudes of Fourier moments in the range of measured parameters shown in the following Figs. 11 and 12, but more importantly it eliminates a large oscillation in δ\delta that would occur if we instead assumed the proportionality in Eq. 6 were a constant.

V.2 Predicted oscillating moments for a square cross-section

In principle, oscillations in the shape of the temperature profile can occur if the pathlength of the LSC oscillates over time. Since we can analyze oscillation modes without adding noise, which would just obfuscate the results, we include the effect of the oscillation in θ0\theta_{0} as a deterministic time series θf(t)=θf,maxcos(ωt)\theta_{f}(t)=\theta_{f,max}\cos(\omega t), where θf,max\theta_{f,max} is the amplitude of the oscillation in θf\theta_{f} at the edge of the top and bottom plates.

Refer to caption

Figure 9: (color online) Time series of Fourier moments of the temperature profile predicted from the assumed pathlength in Eqs. 7, 8, 9. The A3A_{3} moment is dominant, followed by B3B_{3}. The other moments shown in the legend are not excited.

We calculate time series for the temperature profile from Eq. 6 using the pathlength of Eqs. 7, 8, and 9 for a square cross-section and oscillatory θf(t)\theta_{f}(t). The temperature was sampled at 8 equally spaced orientations, mimicking our thermistor measurements. The resulting temperature profile was fit at each time step to obtain the LSC orientation θ0\theta_{0} using Eq. 1. Fourier moments were then calculated at each time step using Eqs. 3 and 4. An example time series of Fourier moments is shown in Fig. 9 for δ=0.431\langle\delta\rangle=0.431 K and θf,max=0.3\theta_{f,max}=0.3 rad. The A3A_{3} moment has a dominant oscillation, followed by the B3B_{3} moment. The A3A_{3} moment also has the dominant oscillation in the experimental data, followed by the B3B_{3} moment (not counting A4A_{4} which violates symmetry expectations).

Refer to caption

Figure 10: (color online) Thick solid black line: Example of the predicted temperature profile at an intermediate phase of the oscillation where θf=0\theta_{f}=0 rad. Dashed blue line: cosine fit (Eq. 6) used for 1st-order approximation of the temperature profile. Dotted red line: difference between the predicted temperature profile and 1st-order cosine term. Thin solid red line: Fit of moment B3B_{3} to the difference. The difference has the symmetry of odd-order BnB_{n} moments.

The dominance of the A3A_{3} moment in the temperature profile is illustrated by comparing the predicted temperature profile (Eq. 6) at the phase where θf\theta_{f} peaks to the 1st-order approximation of the cosine profile (Eq. 1) in Fig. 8. The difference between the predicted temperature profile and 1st-order cosine profile is shown as the dotted line in Fig. 8. A fit of the A3A_{3} moment to the difference in Fig. 8 shows that it is dominated by that moment. If θf\theta_{f} oscillates, then Eq. 6 leads to oscillations of A3A_{3} as is shown in Fig. 9. Thus, the dominant A3A_{3} moment can be understood as a result of the change in pathlength in the reference frame of the LSC as it oscillates around the corner of a cubic cell.

To visualize the B3B_{3} moment, the predicted temperature profile for the intermediate phase where θf=0\theta_{f}=0 is shown in Fig. 10. It has the symmetry of odd-order BnB_{n} moments (antisymmetric around θ=±π/2\theta=\pm\pi/2 and symmetric around θ=0\theta=0). With 8 thermistors, B3B_{3} is the only odd-order BnB_{n} moment that we can detect (shown by the fit in Fig. 10) due to the Nyquist limit. The B3B_{3} moment does not capture the full difference between the predicted temperature profile and the cosine fit shown in Fig. 10, and a B5B_{5} moment with similar magnitude to the B3B_{3} moment is apparent in the predicted profile by inspection.

The details of the time series shown in Fig. 9 vary with the number and location of temperature measurements. For example, at the phase shown in Fig. 10, the arrangement of our thermistors yields a simulated measurement of B3=0B_{3}=0 at that phase even though the complete temperature profile in Fig. 10 leads to a maximum of B3B_{3} at this phase. However, this moment is still detected in the time series at other intermediate phases, suggesting different thermistor arrangements will still detect the same moments, but with different amplitudes. The model temperature profile actually predicts B3B_{3} is the strongest moment for small amplitude oscillations of θ0\theta_{0} (not shown), but our thermistors are not arranged to detect this moment optimally. At least 10 evenly-spaced thermistors would be required to detect the predicted B5B_{5} moment.

A feature of note is that the fit of the temperature profile in Fig. 8 yields the amplitude of the oscillation in θ0\theta_{0} to be 0.180.18 rad instead of the input θf,max=0.3\theta_{f,max}=0.3 rad, indicating that θ0\theta_{0} from the cosine fit of the temperature profile underestimates the flow orientation θf\theta_{f} in cubic cells. θ0\theta_{0} and θf\theta_{f} still oscillate together, and there is a one-to-one relationship between θ0\theta_{0} and θf\theta_{f}, so θ0\theta_{0} can work as a proxy for the flow direction as long as it is acknowledged that there is a conversion function between them in non-circular cross-section cells.

V.3 Phase shifts

Phase shifts between different signals can be identified from correlation functions, many of which were already reported for the cubic cell dataset Ji and Brown (2020). The observed in-phase behavior of A3A_{3} at all 3 rows of thermistors is expected from the model, as it depends on the driving θ0\theta_{0}-oscillation which is predicted to be in-phase at all 3 rows of thermistors in the n=1n=1 advected mode Ji and Brown (2020) . The observation that A3A_{3} is π\pi rad out of phase with θ0\theta_{0} Ji and Brown (2020) is consistent with the picture that azimuthal advection shifts θf\theta_{f} in Fig. 8 to 0 at the mid-height of the container so that θ0\theta_{0} is slightly negative while A3A_{3} is positive. This extra contribution to the measured θ0\theta_{0} superposed on the driving oscillation in θ0\theta_{0} may also explain why θ0\theta_{0} was not measured to be in-phase at all 3 rows of thermistors as predicted for the n=1n=1 advected mode Ji and Brown (2020).

V.4 Dependence on θf,max\theta_{f,max}

Refer to caption

Figure 11: (color online) Predicted oscillation amplitudes of Fourier moments as a function of the amplitude of the driving oscillation amplitude θ0,p\theta_{0,p}.

To test whether the model quantitatively captures the observed moment amplitudes reported in Table 1, we varied the input oscillation amplitude θf,max\theta_{f,max} and compare amplitudes of oscillating signals. Figure 11 shows the root-mean-square (rms) amplitudes of the oscillating signals vs. the rms of the oscillating component of the LSC orientation θ0,p\theta_{0,p} for δ=0.431\langle\delta\rangle=0.431 K (matching the measured value of δ\langle\delta\rangle). Generally, A3,pA_{3,p} is dominant, followed by B3,pB_{3,p}, and both moments increase nonlinearly with θ0,p\theta_{0,p}. We find an input value of θf,max=0.074\theta_{f,max}=0.074 rad matches the observation of θ0,p=0.037\theta_{0,p}=0.037 rad from Table 1. For these input parameter values, the model yields the amplitudes A3,p=17A_{3,p}=17 mK and B3,p=1.4B_{3,p}=1.4 mK, somewhat smaller than measured root-mean-squared values of A3,p=28A_{3,p}=28 mK and B3,p=7B_{3,p}=7 mK for the middle row.

We tried smoothing the pathlength function as in Ref. Song et al. (2014), and found that it did not introduce any different oscillating moments, and has less than 1% effect on the magnitudes on moment amplitudes.

V.5 Offset in θ0\theta_{0}

Refer to caption

Figure 12: (color online) Predicted oscillation amplitudes of Fourier moments as a function of the offset of the preferred orientation θp\theta_{p} from the corner for θ0,p=0.037\theta_{0,p}=0.037 rad. The offset of θp\theta_{p} leads to an increase in B3,pB_{3,p}.

The preceding model assumes that the oscillation of θ0\theta_{0} is centered around the corner of the cell. In actual experiments, the oscillation is not centered around the corner, with the preferred orientation at an angle θp=0.05\theta_{p}=0.05 rad away from the corner, mainly due to a nonuniform temperature profile in the heating and cooling plates Ji and Brown (2020). This offset can change the induced temperature profile in the coordinate θθ0\theta-\theta_{0}, leading to different Fourier moment amplitudes than found in Sec. V.4. To determine the effect of this offset on the Fourier moments, we added the preferred orientation to the model for the oscillation of the flow direction: θf(t)=θf,maxcos(ωt)+θp\theta_{f}(t)=\theta_{f,max}\cos(\omega t)+\theta_{p}. Figure 12 shows rms amplitudes of Fourier moments as a function of the preferred orientation θp\theta_{p} for θ0,p=0.037\theta_{0,p}=0.037 rad. B3,pB_{3,p} increases significantly with θp\theta_{p}, and no new moments are observed. At the measured offset of θp=0.05\theta_{p}=0.05 rad, the model yields A3,p=17A_{3,p}=17 mK and B3,p=3.9B_{3,p}=3.9 mK. This is within 50% of the observed magnitudes of 28 mK and 7 mK, respectively.

V.6 Predicted temperature profile of sloshing oscillations in a circular cross-section container

Refer to caption

Figure 13: (color online) Thick solid black line: Example of predicted temperature profile due to the n=2n=2 oscillation in a cylinder for θf=0.3\theta_{f}=0.3 rad. Thick dashed blue line: cosine fit (Eq. 6) as a 1st-order approximation of the temperature profile. Dashed-dotted red line: difference between the predicted temperature profile and 1st-order cosine term. Short-dashed red line: Fit of A2A_{2} to the difference. Long-dashed red line: Fit of A4A_{4} to the difference. Dotted orange line: difference between the predicted temperature profile and 1st-order cosine term smoothed over a range ±π/4\pm\pi/4. Thin solid orange line: fit of the A2A_{2} moment to the smoothed difference. In either case, the difference is dominated by the A2A_{2} moment, as observed in experiments. The A4A_{4} moment is highly dependent on smoothing.

Since the pathlength model can predict the existence of the new A3A_{3} and B3B_{3} moments, it is worth checking if it can recover the temperature profiles of other known oscillations in temperature profiles, in particular the sloshing oscillation in a circular cross-section container. The observed sloshing mode has peak amplitude at the mid-height Xi et al. (2009); Zhou et al. (2009); Brown and Ahlers (2009), and an oscillating A2A_{2} moment Brown and Ahlers (2009). This is part of the n=2n=2 advected oscillation mode (with 2 oscillation periods per LSC rotation) which also has a twisting component corresponding to oscillations in θ0\theta_{0} at the top and bottom rows of thermistors out of phase with each other Funfschilling and Ahlers (2004); Brown and Ahlers (2009). The twisting oscillation is π/2\pi/2 rad out of phase with the sloshing oscillation.

The pathlength-based model predicts that the cosine-shaped pathlengths on the hot and cold sides of the cell are advected upward and downward, respectively, to meet at the middle row. Both cosine profiles at the hot and cold sides are advected azimuthally by a displacement θf,max\theta_{f,max}, but for the n=1n=1 mode they advect in opposite directions in θ\theta due to the twist displacements being on opposite sides at the hot and cold plates. This results in a temperature profile where the hot and cold extrema are pushed closer together with the antisymmetry of the sloshing mode.

We show an example of this temperature profile in Fig. 13 for θf=0.3\theta_{f}=0.3 rad. At the interfaces where the hot and cold sides are pushed together or pulled apart, we do not know how the temperature profile evolves, so as a simplest model we assume there is no advection past θ=π/2\theta=\pi/2 and the temperature around π/2-\pi/2 is close to the average T0T_{0}. The non-zero moments of the temperature profile for n4n\leq 4 are A2,p0.56δθf,maxA_{2,p}\approx 0.56\langle\delta\rangle\theta_{f,max} and A4,p0.21δθf,maxA_{4,p}\approx 0.21\langle\delta\rangle\theta_{f,max}. The difference between the predicted temperature profile and its 1st-order cosine fit, as well as the A2A_{2} and A4A_{4} moments, are shown in Fig. 13. This produces a dominant A2A_{2} moment as observed, but also a significant A4A_{4} moment, which is not observed in experiments Brown and Ahlers (2009).

Since a non-smooth temperature profile is unrealistic, as there will be some turbulent mixing to smooth the temperature profile, we considered the effects of smoothing in θ\theta. Smoothing in general will have a tendency to reduce the contribution of higher order moments in the temperature profile. For example, smoothing the difference in the predicted temperature profile from the 1st-order cosine fit over a range of ±π/4\pm\pi/4 rad is shown in Fig. 13. This smoothing is even more dominated by the A2A_{2} moment with A2,p0.39δθf,maxA_{2,p}\approx 0.39\langle\delta\rangle\theta_{f,max} and A4,p0.04δθf,maxA_{4,p}\approx 0.04\langle\delta\rangle\theta_{f,max}. Due to the approximate nature of the model, we can only predict orders of magnitude for the effect of thermal mixing. Since vertical temperature gradients are comparable to horizontal temperature gradients in the bulk Brown and Ahlers (2007), the turbulent thermal mixing which is solely responsible for the vertical temperature gradient is comparable in magnitude to effects that generate the azimuthal temperature profile, and thus we cannot give a precise prediction of how much smoothing is expected from mixing. Even without a precise prediction of the effects of thermal mixing, we can still say that the temperature profile is a combination of A2A_{2} and potentially A4A_{4} terms. Note that including the effects of thermal mixing more generally in the model is expected to similarly smooth the temperature profile, reducing the magnitudes of higher order moments more severely than lower order moments, but would not fundamentally change which moments can be excited by the geometry, or the order of magnitude estimates.

To compare the magnitudes of the predicted moments with experimental measurements, we measure an amplitude from the peak power of θb,p=0.094\theta_{b,p}=0.094 rad at the bottom row of thermistors to represent the oscillation in θ0\theta_{0} for data from the cylindrical container. The amplitude of the advected oscillation in θ0\theta_{0} at the bottom row of thermistors is not as large as at the edge of the bottom plate. If we assume a rectangular pathlength around the inner edge of the aspect ratio 1 container, then θf,max=θb,psin(π/4)/sin(π/8)=0.173\theta_{f,max}=\theta_{b,p}\sin(\pi/4)/\sin(\pi/8)=0.173 rad. For this θf,max\theta_{f,max} and the observed δ=0.255\langle\delta\rangle=0.255 K, Eq. 6 predicts A2,p=1724A_{2,p}=17-24 mK and A4=29A_{4}=2-9 mK, where the range is given from zero smoothing to smoothing by ±π/2\pm\pi/2. This overestimates the measured A2,bot=11A_{2,bot}=11 mK at the mid-height in the cylindrical container by about a factor of 2, and is 1-4 times the resolution limit for measurements of the A4A_{4} moment, so is reasonably consistent with the measurement of A2A_{2} and lack of observed A4A_{4} for an approximate model.

The situation is expected to be similar for the sloshing aspect of the n=1n=1 advected oscillation mode in non-circular cross sections. The n=1n=1 mode includes sloshing at the top and bottom rows of thermistors, but not at the mid-height Brown and Ahlers (2009); Ji and Brown (2020). We expect horizontal advection of the temperature profile will move θf\theta_{f} from the in-phase twist displacement near the top and bottom plates by different amounts due to the different times it takes to reach the top and bottom rows of thermistors from the top and bottom plates, so that the two temperature extrema have moved closer together to produce a slosh displacement. Due to the conceptual similarity with the slosh profile for the cylinder, it is not shown here. Due to the ambiguity of how to define the temperature profile near the border of the hot and cold sides, any breakdown of the slosh profile into A2A_{2} and A4A_{4} components would be again highly dependent on assumptions about smoothing, and our measurement of A4A_{4} is plagued by large asymmetries of the setup, any quantitative results we could show would not be very informative.

The jumprope oscillation is the other mode that is known to cause an oscillation in the shape of the temperature profile, specifically with the symmetries of even order BnB_{n} moments and T0T_{0} Vogt et al. (2018). However, since this is known to consist of the core of the LSC oscillating around in the central plane of the LSC, it does not involve changes in pathlengths of parallel paths along the top and bottom plates in the sense discussed here, so that temperature profile oscillation should be described by a different mechanism.

VI Summary

We observe an oscillation in the shape of the LSC expressed in terms of Fourier moments of the azimuthal temperature profile relative to the LSC orientation θ0\theta_{0}. In a cubic container, the oscillation is dominated by the 3rd-order sine moment (A3A_{3}), followed by the 3rd-order cosine moment (B3)B_{3}) (Figs. 2, 3). This oscillation in the temperature profile lacks the symmetry in θ0\theta_{0} of the jumprope mode, lacks the antisymmetry in θ0\theta_{0} of the sloshing mode, and was not found in cylindrical containers like those other modes, making it distinct from those known oscillation modes.

An explanation for this new oscillation in the temperature profile is that the heat conducted from the thermal boundary layers to each streamline of the LSC is proportional to the pathlength of the streamlines along the top and bottom plates. In a non-circular-cross-section cell, the oscillation of the LSC orientation θ0\theta_{0} results in the pathlength as a function of θθ0\theta-\theta_{0} oscillating in the reference frame of the LSC, and thus oscillations in the temperature profile. The detailed collection of moments can be estimated based on the container geometry (Fig. 7). In a cubic cell, this minimal model predicts a dominant A3A_{3} moment followed by B3B_{3} (Figs. 8, 9, 10), with magnitudes about 50% larger than measured values when using experimental input for the advected oscillation amplitude in θ0\theta_{0} (Figs. 11, 12). Thus, the oscillation in the temperature profile in a non-circular cross section is not an entirely new oscillation mode, but a modification of the temperature profile due to previously known oscillations of the LSC orientation θ0\theta_{0}.

A circular-cross-section cell is special in that the pathlength along the plate is independent of θ0\theta_{0}, and so no oscillations in the shape of the temperature profile are induced as θ0\theta_{0} oscillates. In a cylindrical cell, the model produces the sinusoidal mean temperature profile with a sloshing oscillation dominated by the 2nd order sine moment (A2A_{2}) (Fig. 13), in agreement with observations in that geometry (Fig. 6)Brown and Ahlers (2007, 2009).

We also show that observation of oscillations of A4A_{4} in phase with the oscillation of θ0\theta_{0} break the symmetry between the hot and cold sides of the LSC. These are likely a consequence of asymmetries of the setup, or possibly a long-lived symmetry-breaking mode.

This work demonstrates a low-dimensional approximate model can explain the qualitative shape and order of magnitude of the LSC temperature profile and some of the major perturbations to it in Rayleigh-Bénard convection. It remains to be seen if quantitative predictions can be refined using more detailed information of the temperature and flow fields, for example to quantify the effects of corner-rolls on the temperature profile, or using local properties of the thermal boundary layer to calculate heat transport to the LSC. It also remains to be seen if the basic concept of estimating heat transport from conduction along the boundary layer pathlength can inform modeling of large-scale coherent flow structures in other systems.

VII Acknowledgements

We thank the University of California, Santa Barbara machine shop and K. Faysal for helping with construction of the experimental apparatus. This work was supported by Grant CBET-1255541 of the U.S. National Science Foundation.

VIII Author Contributions

Experimental measurements and data analysis for the cubic cell was carried out by D. Ji. Modeling, and analysis of data from the cylindrical cell was done by E. Brown. The draft was written by E. Brown.

References

  • Ahlers et al. (2009) G. Ahlers, S. Grossmann,  and D. Lohse, “Heat transfer and large-scale dynamics in turbulent Rayleigh-Bénard convection,” Reviews of Modern Physics 81, 503–537 (2009).
  • Lohse and Xia (2010) D. Lohse and K.-Q. Xia, “Small-scale properties of turbulent Rayleigh-Bénard convection,” Annual Reviews of Fluid Mechanics 42, 335–364 (2010).
  • Krishnamurti and Howard (1981) R. Krishnamurti and L. N. Howard, “Large scale flow generation in turbulent convection,” Proc. Natl. Acad. Sci. 78, 1981–1985 (1981).
  • Cioni et al. (1996) S. Cioni, S. Ciliberto,  and J. Sommeria, “Experimental study of high Rayleigh-number convection in mercury and water,” Dyn. Atmos. Oceans 24, 117–127 (1996).
  • Brown and Ahlers (2006) E. Brown and G. Ahlers, “Rotations and cessations of the large-scale circulation in turbulent Rayleigh-Bénard convection,” J. Fluid Mech. 568, 351 (2006).
  • Xi et al. (2006) H. D. Xi, Q. Zhou,  and K. Q. Xia, “Azimuthal motion of the mean wind in turbulent thermal convestion,” Phys. Rev. E 73, 056312 (2006).
  • Heslot et al. (1987) F. Heslot, B. Castaing,  and A. Libchaber, “Transition to turbulence in helium gas,” Phys. Rev. A 36, 5870–5873 (1987).
  • Sano et al. (1989) M. Sano, X. Z. Wu,  and A. Libchaber, “Turbulence in helium-gas free convection,” Phys. Rev. A 40, 6421 (1989).
  • Castaing et al. (1989) B. Castaing, G. Gunaratne, F. Heslot, L. Kadanoff, A. Libchaber, S. Thomae, X. Z. Wu, S. Zaleski,  and G. Zanetti, “Scaling of hard thermal turbulence in Rayleigh-Bénard convection,” J. Fluid Mech. 204, 1–30 (1989).
  • Ciliberto et al. (1996) S. Ciliberto, S. Cioni,  and C. Laroche, “Large-scale flow properties of turbulent thermal convection,” Phys. Rev. E 54, R5901–R5904 (1996).
  • Takeshita et al. (1996) T. Takeshita, T. Segawa, J. A. Glazier,  and M. Sano, “Thermal turbulence in mercury,” Phys. Rev. Lett. 76, 1465–1468 (1996).
  • Cioni et al. (1997) S. Cioni, S. Ciliberto,  and J. Sommeria, “Strongly turbulent Rayleigh-Bénard convection in mercury: comparison with results at moderate Prandtl number,” J. Fluid Mech. 335, 111–140 (1997).
  • Qiu et al. (2000) X. L. Qiu, S. H. Yao,  and P. Tong, “Large-scale coherent rotation and oscillation in turbulent thermal convection,” Phys. Rev. E 61, R6075 (2000).
  • Qiu and Tong (2001) X. L. Qiu and P. Tong, “Onset of coherent oscillations in turbulent Rayleigh-Bénard convection,” Phys. Rev. Lett 87, 094501 (2001).
  • Niemela et al. (2001) J. Niemela, L. Skrbek, K. R. Sreenivasan,  and R. J. Donnelly, “The wind in confined thermal turbulence,” J. Fluid Mech. 449, 169–178 (2001).
  • Qiu and Tong (2002) X. L. Qiu and P. Tong, “Temperature oscillations in turbulent rayleigh-benard convection,” Phys. Rev. E 66, 026308 (2002).
  • Qiu et al. (2004) X. L. Qiu, X. D. Shang, P. Tong,  and K.-Q. Xia, “Velocity oscillations in turbulent Rayleigh-Bénard convection,” Phys. Fluids. 16, 412–423 (2004).
  • Funfschilling and Ahlers (2004) D. Funfschilling and G. Ahlers, “Plume motion and large scale circulation in a cylindrical Rayleigh-Bénard cell,” Phys. Rev. Lett. 92, 194502 (2004).
  • Sun et al. (2005) C. Sun, K. Q. Xia,  and P. Tong, “Three-dimensional flow structures and dynamics of turbulent thermal convection in a cylindrical cell,” Phys. Rev. E 72, 026302 (2005).
  • Tsuji et al. (2005) Y. Tsuji, T. Mizuno, T. Mashiko,  and M. Sano, “Mean wind in convective turbulence of mercury,” Phys. Rev. Lett. 94, 034501 (2005).
  • Funfschilling et al. (2008) D. Funfschilling, E. Brown,  and G. Ahlers, “Torsional oscillations of the large-scale circulation in turbulent Rayleigh-Bénard convection,” J. Fluid. Mech. 607, 119–139 (2008).
  • Xi et al. (2009) H.-D. Xi, S.-Q. Zhou, Q. Zhou, T.-S. Chan,  and K.-Q. Xia, “Origin of the temperature oscillation in turbulent thermal convection,” Phys. Rev. Lett. 102, 044503–1–4 (2009).
  • Zhou et al. (2009) Q. Zhou, H.-D. Xi, S.-Q. Zhou, C. Sun,  and K.-Q. Xia, “Oscillations of the large-scale circulation in turbulent Rayleigh-Bénard convection: the sloshing mode and its relationship with the torsional mode,” J. Fluid Mech. 630, 367–390 (2009).
  • Brown and Ahlers (2009) E. Brown and G. Ahlers, “The origin of oscillations of the large-scale circulation of turbulent Rayleigh-Bénard convection,” J. Fluid Mech. 638, 383–400 (2009).
  • Zimin and Ketov (1978) V. D. Zimin and A. I. Ketov, “Turbulent convection in a cubic cavity heated from below,” Fluid Dynamics 13, 594–599 (1978).
  • Zocchi et al. (1990) G. Zocchi, E. Moses,  and A. Libchaber, “Coherent structures in turbulent convection: an experimental study,” Physica A 166, 387–407 (1990).
  • Qiu and Xia (1998) X. L. Qiu and K.-Q. Xia, “Viscous boundary layers at the sidewall of a convection cell,” Phys. Rev. E 58, 486–491 (1998).
  • Valencia et al. (2007) Leonardo Valencia, Jordi Pallares, Ildefonso Cuesta,  and Francesc Xavier Grau, “Turbulent Rayleigh-Bénard convection of water in cubical cavities: A numerical and experimental study,” International Journal of Heat and Mass Transfer 50, 3203 – 3215 (2007).
  • Ji and Brown (2020) D. Ji and E. Brown, “Low-dimensional model of the large-scale circulation of turbulent Rayleigh-Bénard convection in a cubic container,” Phys. Rev. Fluids 5, 064606 (2020).
  • Song et al. (2014) H. Song, E. Brown, R. Hawkins,  and P Tong, “Dynamics of large-scale circulation of turbulent thermal convection in a horizontal cylinder,” J. Fluid Mech 740, 136–167 (2014).
  • Vasiliev et al. (2016) A. Vasiliev, A. Sukhanovskii, P. Frick, A. Budnikov, V. Fomichev, M. Bolshukhin,  and R. Romanov, “High rayleigh number convection in a cubic cell with adiabatic sidewalls,” International Journal of Heat and Mass Transfer 102, 201 – 212 (2016).
  • Giannakis et al. (2018) D. Giannakis, A. Kolchinskaya, D. Krasnov,  and J. Schumacher, “Koopman analysis of the long-term evolution in a turbulent convection cell,” J. Fluid Mech. 847, 735–767 (2018).
  • Brown and Ahlers (2008a) E. Brown and G. Ahlers, “Azimuthal asymmetries of the large-scale circulation in turbulent Rayleigh-Bénard convection,” Phys. Fluids 20, 105105–1–15 (2008a).
  • Foroozani et al. (2019) N. Foroozani, J. J. Niemela, V. Armenio,  and K. R. Sreenivasan, “Turbulent convection and large scale circulation in a cube with rough horizontal surfaces,” Phys. Rev. E 99, 033116 (2019).
  • Vogt et al. (2018) T. Vogt, S. Horn, A. M. Grannan,  and J. M. Aurnou, “Jump rope vortex in liquid metal convection,” Proc. Nat. Acad. Sciences 115, 12674–12679 (2018).
  • Bai et al. (2016) K. Bai, D. Ji,  and E. Brown, “Ability of a low-dimensional model to predict geometry-dependent dynamics of large-scale coherent structures in turbulence,” Phys. Rev. E) 93, 023117–1–5 (2016).
  • Brown and Ahlers (2007) E. Brown and G. Ahlers, “Temperature gradients, and search for non-boussinesq effects, in the interior of turbulent Rayleigh-Bénard convection,” Euro. Phys. Lett. 80, 14001–1–6 (2007).
  • Brown and Ahlers (2008b) E. Brown and G. Ahlers, “A model of diffusion in a potential well for the dynamics of the large-scale circulation in turbulent Rayleigh-Bénard convection,” Phys. Fluids 20, 075101–1–16 (2008b).
  • Funfschiling et al. (2005) D. Funfschiling, E. Brown, A. Nikolaenko,  and G. Ahlers, “Heat transport by turbulent Rayleigh-Bénard convection in cylindrical cells with aspect ratio one and larger,” J. Fluid Mech. 536, 145–154 (2005).
  • Vasiliev et al. (2019) A. Vasiliev, P. Frick, A. Kumar, R. Stepanov, A. Sukhanovskii,  and M. K. Verma, “Transient flows and reorientations of large-scale convection in a cubic cell,” International Comunications in Heat and Mass Transfer 108, 104319 (2019).
  • Liu and Ecke (2009) Y. Liu and R. E. Ecke, “Heat transport measurements in turbulent rotating Rayleigh-Bénard convection,” Phys. Rev. E 80, 036314 (2009).
  • Foroozani et al. (2017) N. Foroozani, J.J. Niemela, V. Armenio,  and K.R. Sreenivasan, “Reorientations of the large-scale flow in turbulent convection in a cube,” Phys. Rev. E 95, 033107 (2017).