Issue 
A&A
Volume 587, March 2016



Article Number  A120  
Number of page(s)  8  
Section  Interstellar and circumstellar matter  
DOI  https://doi.org/10.1051/00046361/201527148  
Published online  29 February 2016 
Accuracy requirements to test the applicability of the random cascade model to supersonic turbulence
École Normale Supérieure, Lyon, CRAL, UMR CNRS 5574, Université de
Lyon,
69342
Lyon,
France
email:
doris.folini@enslyon.fr
Received: 9 August 2015
Accepted: 21 January 2016
A model, which is widely used for inertial rang statistics of supersonic turbulence in the context of molecular clouds and star formation, expresses (measurable) relative scaling exponents Z_{p} of twopoint velocity statistics as a function of two parameters, β and Δ. The model relates them to the dimension D of the most dissipative structures, D = 3 − Δ/(1 − β). While this description has proved most successful for incompressible turbulence (β = Δ = 2/3, and D = 1), its applicability in the highly compressible regime remains debated. For this regime, theoretical arguments suggest D = 2 and Δ = 2/3, or Δ = 1. Best estimates based on 3D periodic box simulations of supersonic isothermal turbulence yield Δ = 0.71 and D = 1.9, with uncertainty ranges of Δ ∈ [0.67,0.78] and D ∈ [2.04,1.60]. With these 5−10% uncertainty ranges just marginally including the theoretical values of Δ = 2/3 and D = 2, doubts remain whether the model indeed applies and, if it applies, for what values of β and Δ. We use a Monte Carlo approach to mimic actual simulation data and examine what factors are most relevant for the fit quality. We estimate that 0.1% (0.05%) accurate Z_{p}, with p = 1,...,5, should allow for 2% (1%) accurate estimates of β and Δ in the highly compressible regime, but not in the mildly compressible regime. We argue that simulationbased Z_{p} with such accuracy are within reach of today’s computer resources. If this kind of data does not allow for the expected high quality fit of β and Δ, then this may indicate the inapplicability of the model for the simulation data. In fact, other models than the one we examine here have been suggested.
Key words: shock waves / hydrodynamics / ISM: kinematics and dynamics / gammaray burst: general / binaries: close / turbulence
© ESO, 2016
1. Introduction
Supersonic turbulence is a key ingredient in various astrophysical contexts, from gamma ray bursts (Lazar et al. 2009; Narayan & Kumar 2009) or stellar accretion (Walder et al. 2008; Hobbs et al. 2011) to molecular clouds and star formation (Chabrier & Hennebelle 2011; Federrath & Klessen 2012; Padoan et al. 2012; Kritsuk et al. 2013). A key question is whether this turbulence, like incompressible turbulence, is characterized by universal statistics. Results from 3D periodic box simulations of driven, isothermal, supersonic turbulence (Kritsuk et al. 2007a; Schmidt et al. 2008; Pan et al. 2009) are indeed consistent with the highly compressible variant (Boldyrev 2002) of the hierarchical structure model that was put forward by She & Leveque (1994) for incompressible turbulence and that was further scrutinized by Dubrulle (1994) and She & Waymire (1995). This model is correspondingly popular in astrophysics. It is employed, for example, in the interpretation of molecular cloud observations (Gustafsson et al. 2006; HilyBlant et al. 2008) or to derive a theoretical expression for the density distribution in supersonic turbulence (Boldyrev et al. 2002), which enters theories of the stellar initial mass function (Hennebelle & Chabrier 2008).
Nevertheless, some doubts remain whether the model really applies to simulation data of supersonic turbulence and, if so, with what parameter values. The bestfit model parameters that we are aware of (Pan et al. 2009) still come with a 5−10% uncertainty range that is only marginally compatible with theoretically predicted parameter values (see below). Here we argue that today’s computer resources should allow for 1−2% accurate parameter fits in the highly compressible regime, thereby likely settling the issue. Our claim is based on a Monte Carlo approach to mimic actual simulation data.
The hierarchical structure model predicts the ratios Z_{p} of (observable) structure function scaling exponents ζ_{p}, p = 1,2,3,... etc., of a 3D velocity field u as (1)Here, D = 3 − C is the dimension of the most intermittent structure, C = Δ/(1 − β) the associated codimension, β ∈ [0,1] measures the intermittency of the energy cascade, and Δ ∈ [0,1] measures the divergent scale dependence of the most intermittent structures. The ζ_{p} are defined in the inertial range by (2)where ⟨ ... ⟩ denotes the average over all positions x within the sample and over all directed distances r. The Z_{p} should be well defined over a larger range because of extended selfsimilarity (Benzi et al. 1993) and Eq. (1) should remain formally valid for generalized structure functions , computed from massweighted velocities v ≡ ρ^{1/3}u (Kritsuk et al. 2007a,b).
Several special cases of the model that differ in their parameter values exist in the literature (see e.g. the review by She & Zhang 2009). The original model by She & Leveque (1994) applies most successfully to incompressible turbulence with 1D vortex filaments as most dissipative structures (D = 1) and parameter values β = Δ = 2/3. For highly compressible turbulence, parameter values remain debated. Boldyrev (2002) argues that the most dissipative structures are 2D shocks, thus D = 2, and chose to keep Δ = 2/3 and set β = 1/3. By contrast, Schmidt et al. (2008) argue that Δ = 1 (implying β = 0) to be consistent with Burgers turbulence. A few studies used 3D simulation data, derived sets of Z_{p}, and attempted simultaneous fits of β and Δ (Kritsuk et al. 2007b; Schmidt et al. 2008, 2009; Folini et al. 2014). The results are inconclusive in that fits of similar quality are obtained for widely different βΔpairs. Also using 3D simulation data (1024^{3}, Mach 6) but working with densityweighted moments of the dissipation rate, Pan et al. (2009) simultaneously fitted Δ and D to their data. They find Δ ∈ [0.67,0.78] and D ∈ [2.04,1.60], with a best estimate of Δ = 0.71 and D = 1.9, thus β = 0.35. The range for Δ is not compatible with the suggested Δ = 1 (see above), and also Δ = 2/3 lies only at the lowermost bound of the inferred range. Both Δ and β may thus deviate from their incompressible values (β = Δ = 2/3) as the Mach number increases, making simultaneous determination of β and Δ a must.
The present study is motivated by this still inconclusive situation. We want to better understand what factors (accuracy/order of Z_{p}; mildly versus highly compressible turbulence) are most relevant for the fit quality and why widely different βΔpairs yield fits of similar quality. We use this insight to formulate quantitative estimates of what is needed to obtain 1% accurate estimates of β and Δ. We present results in Sect. 2, discuss them in Sect. 3, and conclude in Sect. 4.
2. Results
We first show that β and Δ can be uniquely determined from an associated (i.e. computed via Eq. (1)) pair Z_{p1} and Z_{p2}. We then illustrate how uncertainties in Z_{p} map onto the βΔplane. Finally, we give estimates on how accurate the Z_{p} have to be to achieve a desired accuracy of β, Δ, and C.
2.1. β and Δ from exact Z_{p}
Consider two values Z_{p1} and Z_{p2} that both fulfill Eq. (1) for the same values (β,Δ). In the following, we show that (β,Δ) can unambiguously (uniquely) be recovered from Z_{p1} and Z_{p2}.
We start by rewriting Eq. (1), factoring out Δ: (3)Using Z_{p1}, we can obtain an expression for Δ, (4)By now writing Eq. (3) with Z_{p} = Z_{p2}, using Eq. (4) to replace Δ, do some reordering of terms, and abbreviating p_{1}/ 3 ≡ a and p_{2}/ 3 ≡ b, we end up with the following equation for β: (5)or (6)The polynomial P_{β,x} ≡ −β^{x} + xβ + 1 − x, with x> 0 and β ∈ (0,1), is a monotonically decreasing (increasing) function for x< 1 (x> 1), as can be seen by taking the derivative of P_{β,x} with respect to β and as illustrated in Fig. 1. Consequently, Eq. (6) has a unique solution, β, from which Δ can be recovered via Eq. (4). Thus Eq. (1) defines an exact onetoone correspondence between pairs (Z_{p1},Z_{p2}) and (β,Δ).
Fig. 1 Ratio of polynomials P_{β,b}/P_{β,a}, Eq. (5), (yaxis, shown as logarithm) for selected exponents a and b as function of β (xaxis). Colors indicate b/a = 2 (red), 4 (green), 5 (blue), 6 (magenta), 7 (cyan), all with a = p_{1}/ 3 = 1/3, as well as b/a = 7/6 (black) with a = p_{1}/ 3 = 6/3. 

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Two more points deserve to be highlighted, with the help of Fig. 1. The ratio P_{β,b}/P_{β,a} = R_{a,b} is shown as a function of β for different a and b or, equivalently, p_{1} and p_{2}. From the figure it can be taken that, first, largely different values of p_{1} and p_{2} are advantageous since they result in stronger stratification of β with respect to R_{a,b} = (Z_{p2} − b)/(Z_{p1} − a). The cyan curve in Fig. 1, which represents p_{1}/p_{2} = 1/7, covers a wider range of values on the yaxis than the black curve (p_{1}/p_{2} = 6/7). Secondly, the stratification is stronger for small β. Somewhat anticipating Sect. 2.2, we thus expect uncertainties in the Z_{p} to be less important if Z_{p} are available for largely different p and if they are associated with (yet to be determined) small values of β.
2.2. Uncertainty of Z_{p} in the βΔplane
2.2.1. Single Z_{p}
From Eq. (4) it is clear that each Z_{p} defines a curve in the βΔplane. If Z_{p} is derived from model data or observations, it will typically come with an uncertainty estimate, e.g. δZ_{p}/Z_{p} ≤ 5%, with δ indicating the uncertainty. In the βΔplane, this uncertainty range translates into an area around the Z_{p} curve. An illustration is given in Fig. 2. The following points may be made.
One value of Z_{p} (a line of constant Z_{p} in the βΔplane) is compatible with a (large) range of β and/or Δ that always includes Δ = 1 and β = 0. The range tends to be smaller for Z_{p} associated with small β and large Δ (i.e. the lower right corner of βΔplane). Uncertainties associated with Z_{p} (5% in Fig. 2, white curves) augment the range, especially for p = 2 and p = 4, as well as for small Δ and large β (top left corner of the plane). Also apparent from Fig. 2 (or from taking the derivative with respect to Δ of Eq. (1)): for fixed β and p< 3 (p> 3), Z_{p} is a monotonically increasing (decreasing) function of Δ. A similar statement holds for Z_{p} as a function of β for fixed Δ.
In summary, we expect uncertainties in the Z_{p} to be more of an issue if only low orders of p (up to about 4) are available and/or if the (yet to be determined) β is large.
Fig. 2 Z_{p} in the βΔplane, role of p. Shown is Z_{p} (color coded) for p = 1 (top left), p = 2 (top right), p = 4 (bottom left) and p = 10 (bottom right). For β = 1/3 and Δ = 2/3 (red dot), the curve of constant Z_{p} (black) is shown, as well as curves of ± 5% different Z_{p} (white). 

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2.2.2. Multiple Z_{p}
We now turn to multiple Z_{p} and their associated uncertainty ranges δZ_{p}, and ask what area they define in the βΔplane. An illustration is given in Fig. 3. Starting from one specific pair of β = 1/3 and Δ = 2/3 and computing Z_{p} for p = 1,...,5 (left) or p = 1,...,7 (right), we show pairs of 5% perturbed Z_{p} curves, i.e. 1.05·Z_{p} and 0.95·Z_{p}.
As can be seen, only a small fraction of the βΔplane lies between all pairs of perturbed curves. Yet this area comprises a wide range of (β,Δ) values or codimensions. The 5% uncertainty in the Z_{p} translates into a much larger uncertainty (in per cent) for β and Δ. Closer inspection reveals that the area is actually defined by only two sets of curves: those for p = 1 and p = 5 (left panel) or p = 7 (right panel). The latter area is smaller, which indicates that higher order structure functions constrain the problem of finding β and Δ from a set of Z_{p} more strongly. Also apparent from Fig. 3 is the dominant role of the p = 1 curve for narrowing down the composite area between all curves. All this is in line with the expectation (see Sect. 2.1) that Z_{p} for largely different p are advantageous for the determination of β and Δ.
Fig. 3 Part of βΔplane (color coded in codimension C = Δ/(1 − β), 0 <C< 3) within joint reach of (at most) 5% perturbed Z_{p}, starting from Z_{p} for Δ = 2/3 and β = 1/3 (red dot). Left panel: curves of 5% perturbed Z_{p} values for p = 1 (white), p = 2 (blue), p = 4 (red), and p = 5 (green) and part of the βΔplane enclosed by all of them. Right panel: same as left panel but also including p = 6 (purple) and p = 7 (black). 

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Fig. 4 Same as Fig. 3, left, but for β = Δ = 2/3 (top left), β = Δ = 1/3 (top right), β = 0.048 and Δ = 1/3 (bottom left), as well as and β = 0.048 and Δ = 2/3 (bottom right). 

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The relevance of the overall location in the βΔplane is illustrated in Fig. 4. Again, the area shown is contained within 5% perturbed Z_{p} curves for two additional (β,Δ) pairs. As can be seen, smaller values of β (lower panels) result in smaller areas, independent of Δ. The crucial role of the p = 1 (white) and p = 5 (green) curves for confining the area persists. Table 1 gives a quantitative idea of the relevance of β, Δ, δZ_{p}, and p_{max} for the uncertainty range ± δC of the codimensions C. A small δC basically requires a small δZ_{p}, a large p_{max}, a small β, and a large Δ. The concrete numbers highlight the difficulty (or illposedness) of the problem. The situation is worse for larger β (bottom rows in Table 1) and better for smaller values of β (not shown).
We emphasize that the above considerations serve only as illustration. We looked at the area confined by a set of Z_{p} ± δZ_{p} curves. We have not yet considered the problem of estimating bestfit β_{f}, Δ_{f}, and thus C_{f} for a set of given Z_{p}. Such a bestfit solution may lie outside the area considered here.
In summary, very accurate Z_{p} are needed to derive reliable best estimates for β, Δ, and C, and smaller values of β help.
2.3. Bestfit β_{f} and Δ_{f} from uncertain Z_{p}
We now turn to our actual problem of interest: given a set of perturbed (uncertain) , what are associated bestfit estimates for β_{f} and Δ_{f}? Different techniques exist to cope with this kind of question (e.g. Najm 2009; Le Maître & Knio 2010). We use a simple Monte Carlo approach.
We start with a pair (β,Δ) and a maximum order p_{max}, then use Eq. (1) to obtain a set of Z_{p} = Z_{p}(β,Δ) for p = 1 to p = p_{max}. Each of these Z_{p} we perturb randomly (uniformly distributed random numbers) by, at most, α%, which gives us a perturbed set of . For this set of we then seek to find bestfit β_{f} and Δ_{f}. In the following, we do not consider one set of , as would be the case in a real application (unless multiple time slices are available, see Sect. 3). Instead, we take a statistical view for the problem by looking at a large number (1000 to 100 000, see below) of randomly generated sets of perturbed . This enables us, in a statistical sense, to relate the accuracy of the with the accuracy of the fitted parameters. Our approach leaves us with two free parameters, the uncertainty α and the maximum order p_{max}.
Fig. 5 Bestfit β_{f} and Δ_{f} from 5% perturbed Z_{p}. Left: 2D histogram (contours, log10, spacing 0.5, spanning three orders of magnitude) of bestfit βΔvalues from 100 000 perturbed data sets. We note that the 2D histogram shows two peak values (indicated by cyan dots), none of them colocated with the unperturbed (β = 1/3,Δ = 2/3) pair (red dot). Right: underestimation of Z_{5} favors Δ_{f} = 1. Shown is, for a subset of 1000 perturbed data sets, Δ_{f} as function of , again for an unperturbed pair (β = 1/3,Δ = 2/3). Colors indicate . 

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Illustration of range δC of codimension C for given order p and uncertainty δZ_{p} of structure functions for two βΔ pairs.
2.3.1. Minimization of least square error in Z_{p}
A straightforward way to determine bestfit β_{f} and Δ_{f} for any given set of , p = 1,...,p_{max} is to minimize (7)over the βΔplane. To find the minimum, we compare the with precomputed values Z_{p}(β,Δ) on a fine βΔgrid (β,Δ ∈ (0,1); gridspacing 0.002). The associated codimension is given by C_{f} = Δ_{f}/ (1 − β_{f}).
To capture the range of potential outcomes for a range of similarly perturbed data sets , we produced 100 000 perturbed data sets, for each of which we determined β_{f} and Δ_{f}. For initial values (β,Δ) = (1/3,2/3) and (at most) 5% perturbed Z_{p} for p = 1,...,5, the result is summarized in Fig. 5.
Shown in the left panel of Fig. 5 is a 2D histogram (contours) of our 100 000 bestfit (β_{f},Δ_{f}) pairs. Two points are noteworthy. First, the overall area defined by the histogram is similar to the area in Fig. 3, left panel. This is remarkable since the area in Fig. 3 is strictly defined by the 5% uncertainty of the Z_{p}, whereas the area in Fig. 5 is defined through a minimization problem. Second, the 2D histogram has an interior structure with two peaks, around (β,Δ) = (0.1,0.4) or C = 0.4 and (β,Δ) = (0.45,1.0) or C = 1.8 (cyan dots). None of them is colocated with the initial, unperturbed (β,Δ) = (1/3,2/3) pair (red dot, C = 1).
Three questions come to mind. Where do the two peaks in the 2D histogram come from? Do other (β,Δ) pairs result in a qualitatively different picture? Can the minimization procedure be improved to better recover the initial, unperturbed (β,Δ) pair? We address the first two questions in the following while postponing the third question for Sect. 2.3.2.
The existence and location of the two peaks can be understood, at least qualitatively, from two observations. First, minimization via Eq. (7) gives more weight to larger p, as they are associated with larger values of Z_{p}. Roughly speaking, the bestfit (β_{f},Δ_{f}) pair tends to lie on or close to the curve defined by . Moving away from that curve results in a large penalty in the form of a large contribution to the sum in Eq. (7). Second, this translates the minimization problem into the question of where the curves for p< 5 come closest to the curve defined by . For illustration, we consider two extreme values of . To stay on the lower green curve in the left panel of Fig. 3, () and, at the same time, be as close as possible to any of the white curves (p = 1) results in a (β_{f},Δ_{f}) pair to the right, at Δ_{f} ≈ 1. By contrast, the upper green curve (105% of the exact Z_{5} curve) only comes closest to (intersects) any white curve between 95% Z_{1} and 105% Z_{1} in a region further to the left. Clearly, the full problem is more intricate, with also curves for Z_{2} and Z_{4}, and the Z_{5} curve not necessarily adopting one of its two extreme values. Nevertheless, Fig. 5, right panel, suggests the full data to be in line with the above reasoning. For 1000 randomly picked data sets from the left panel, we show Δ_{f} as a function of , with Z_{5} the exact value. Colors indicate . As can be seen, Δ_{f} = 1 indeed tends to be associated with small and small (lower green and upper white curve in Fig. 3, left panel). Particularly low values of Δ_{f} (e.g. Δ_{f} ≈ 0.4) tend to occur for large and any (upper green curve and any white curve in Fig. 3, left panel).
Concerning other initial values (other exact (β,Δ) pairs), a similar situation arises in the sense that double peaked histograms emerge. Details depend, however, on the concrete values of β and Δ, on the assumed uncertainty (5% or more/less), and on p_{max}. An illustration is given in Fig. 6, by means of 1D histograms of C_{f} = Δ_{f}/ (1 − β_{f}). These 1D histograms are less intricate than the 2D histogram in Fig. 5, left, yet still capture the essentials. We show histograms for Δ = 2/3 and different values of β ∈ [0.0476,2/3] (corresponding to C ∈ [0.7,2]) and accuracies between 0.1% and 20%. Five points may be made. First, the doublepeaked structure that is apparent in the βΔ plane in Fig. 5 reappears as a double peak in the 1D C_{f}histograms of Fig. 6 (panel in row three, column three). Second, the doublepeak vanishes as β and the uncertainty both become small (lower left corner of the figure). For the same uncertainty, the doublepeak exists for large β but not for small β (third row in Fig. 6). For the same β, the doublepeak exists for large uncertainties but not for small ones (second column of Fig. 6). Third, going to really small values of β and the uncertainty, the histogram becomes symmetric with one central peak. Fourth, only for these really small values is the codimension of the initially prescribed (β,Δ) pair (show in red) colocated with the peak of the histogram. Fifth, for β = Δ = 2/3 (right column) the histogram peaks at C_{f} = 3 instead of C = 2, unless the accuracy is really high (0.1%, last row). This is understandable from the arguments presented above, with regards to the origin of the two peaks in the 2D histogram in Fig. 5, and from looking at the green (p = 5) and white (p = 1) curves in Fig. 4, upper left panel.
In summary, unless both, δZ_{p} and β are small, bestfit values will preferentially reside in either one of the two peaks of the histograms in Figs. 5 or 6 instead of merely scattering around the correct solution, as in Fig. 6, lower left panel.
Fig. 6 Role of β (columns) and accuracy (rows) of associated Z_{p}, for fixed Δ = 2/3. Shown are PDFs (yaxis) of C_{f} (xaxis), 1000 random data sets, powers p = 1,...,5 for β = 0.0476 (first column), β = 0.17 (second column), β = 1/3 (third column), and β = 2/3 (fourth column). Corresponding exact codimensions (red lines) are, from left to right: C = 0.7, C = 0.8, C = 1, and C = 2. Individual rows from top to bottom contain accuracies of 20%, 10%, 5%, 2%, 0.5%, and 0.1%. As can be seen, the larger β, the more severe are the consequences of inaccuracies in the Z_{p}. Histograms in the upper right (large β, low accuracy of the Z_{p}) look worst. We note that axis ranges differ among panels, to best capture the shape of each histogram. 

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2.3.2. Alternative ways to obtain bestfit β_{f} and Δ_{f}
A number of ideas come to mind on how one may improve the bestfit approach detailed in Sect. 2.3.1.
Recalling the findings in Sect. 2.2.1, including higher values of p in the bestfit estimate should improve the situation. From Fig. 7 it can be taken that this is indeed the case, at least for the example shown (β = 1/3, Δ = 2/3, accuracy of 5%). However, the improvement may be regarded as rather modest. Going from p = 5 to p = 10, as is illustrated in the figure, has about the same effect as staying with p = 5 but going from an accuracy of 5% to an accuracy of 2%. From a practical point of view it also seems questionable whether high order structure functions can meet the accuracy requirements. In numerical simulations, higher order structure functions are probably more prone to the bottleneck effect (Dobler et al. 2003; Kritsuk et al. 2007a).
Another way to improve the situation could be to go to weighted root mean squares instead of the unweighted sum in Eq. (7). Hopefully this breaks the dominant role of the highest order Z_{p} available (see Sect. 2.3.1) and, ultimately, leads to more accurate bestfit β_{f} and Δ_{f}. Two weightings come to mind. On the one hand, weights proportional to the inverse of the Z_{p} with the goal of giving equal weight to each term in the sum, thus reducing the “overweight” of larger p in the sum. On the other hand, we could try to give more weight to p terms with a higher accuracy (smaller δZ_{p}). Corresponding information may be available, e.g. from the numerical determination of the Z_{p}. We tried both ideas but neither choice of weights decidedly improved the bestfit values. Weighting tends to change the relative height of the two peaks in the double peaked histograms of Fig. 6, but it does not get rid of the double peaked structure.
We interpret this finding in the following way. First, there are likely always several Z_{p} that do not have their exact values and thus draw the solution in different directions, away from its exact value. Second, the different curve shapes are important so that, even for weighted sums, the terms p = 1 and p = p_{max} are of crucial importance for the overall fit.
In summary, none of the above alternative ways of fitting simultaneously for β and Δ provides clearly superior results to what can be obtained from the straightforward minimization of Eq. (7). We conclude that, for successful twoparameter fits of β and Δ, highly accurate Z_{p} are a must. A quantitative estimate of “highly accurate”is given in the next section.
Fig. 7 Role of higher order moments. Inclusion of higher order ESS scaling exponents (from p = 5, top left, to p = 10, bottom right) gradually reduces the erroneous peak in the bestfit codimension (around C_{f} = 2.5). Shown are PDFs of C_{f} for at most 5% perturbed Z_{p} values (100 000 random data sets) and exact pair (β = 1/3,Δ = 2/3). Spacing of the βΔgrid for fitting is 0.002. 

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2.3.3. Required accuracy of Z_{p} for “good” bestfit β_{f} and Δ_{f}
We now ask how accurate the Z_{p} have to be in order to reach a prescribed accuracy of C_{f} = Δ_{f}/ (1 − β_{f}) via fitting β_{f} and Δ_{f}.
We formulate our accuracy goal in terms of only C_{f}, since we illustrated in Sect. 2.3.1 that a single peaked and roughly symmetric distribution of C_{f} goes hand in hand with high accuracy, not only of C_{f} but also of the underlying two parameter fit, β_{f} and Δ_{f}. If the latter is not accurate enough, a double peaked distribution for C_{f} results. We find, as a rule of thumb, a single peak distribution if 2/3 of all C_{f} lie within 10% or better of the exact C. We use Eq. (7) for the two parameter fit, as the more elaborate attempts of Sect. 2.3.2 gave no decidedly better results. As theoretical arguments suggest Δ = 2/3 or larger (Dubrulle 1994; Schmidt et al. 2008), we concentrate on that part of the βΔplane.
In practical terms, we define a grid of exact pairs (β,Δ) via a (nearly) equidistant grid of C = 0.4,...,2 and Δ = 0.7,...,0.99 plus, in addition, Δ = 2/3. We equally define some fixed levels of perturbations: δZ_{p}/Z_{p} (in %) ∈ [0.05,0.1,0.2,0.5,1,2,5,10,15,20]. For each exact pair and each perturbation, we created 1000 perturbed sets of , p = 1,...,5 (see Sect. 2.3). Each perturbed set is fitted via Eq. (7). For each initial pair (β, Δ) and for each prescribed δZ_{p}/Z_{p} this yields 1000 fitted pairs (β_{f},Δ_{f}) and derived codimensions C_{f}. These can, in principle, be arranged in histograms, as in Fig. 6. Finally, we identify the largest δZ_{p}/Z_{p} for which 2/3 of all C_{f} lie within the demanded accuracy of the exact, initial C.
Fig. 8 Required accuracy (color coding) of perturbed Z_{p}, p = 1,...,5, such that for at least 2/3 of the bestfit pairs (β_{f}, Δ_{f}) the associated C_{f} are within 10% (top) or 5% (bottom) of the C associated with the initial, unperturbed (β, Δ) pair. As can be seen, the required accuracy depends crucially on the location within the βΔ plane. Gray lines indicate the range within which 2/3 of the actual β_{f} (vertical direction) and Δ_{f} (horizontal direction) lie. Black lines indicate constant C = 1 (lower line) and C = 2 (upper line). For details see text. 

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Figure 8 illustrates the result. Obviously, the accuracy of the (colored squares, in %) that is needed to get at least 2/3 of bestfit C_{f} to lie within 10% (top panel) or 5% (bottom panel) of the exact (initial) C depends on the position within the βΔplane. In the lower right parts, δZ_{p}/Z_{p} ≥ 1% is sufficient to get 10% accurate C_{f}, and δZ_{p}/Z_{p} ≥ 0.5% yields 5% accurate C_{f}. By contrast, in the upper left parts of the plane (β ≥ 0.5) one needs δZ_{p}/Z_{p} ≤ 0.1% to get 10% accurate C_{f}. Gray lines in Fig. 8 (for clarity only shown for a subset of the colored squares) indicate the range within which at least 2/3 of the actually fitted β_{f} and Δ_{f} lie. The range is larger for Δ (horizontal lines) than for β (vertical lines). This is plausible from Fig. 4, from the area confined by multiple Z_{p} curves. Repeating Fig. 8 but demanding 10% accuracy for Δ_{f} instead of C_{f} yields a similar pattern in the βΔplane (not shown), while demanding 10% accuracy for β_{f} gives a much more homogeneous pattern (0.2% to 0.5% accuracy for , not shown).
For highly compressible turbulence, bestfit β_{f} and Δ_{f} are expected to lie in the lower part of the βΔplane in Fig. 8, roughly β ≤ 1/3 and Δ ≥ 2/3 (Boldyrev 2002; Padoan et al. 2004; Pan et al. 2009). Here, accuracies of 0.5%, 0.1%, and 0.05% for the translate into accuracies of 10%, 2%, and 1% for β_{f} and Δ_{f} (not shown). Fits of similar quality require much more accurate in the mildly compressible regime, where β> 1/3 (upper part of panels in Fig. 8) and ultimately β = 2/3 in the incompressible limit. We note that in practical applications, bestfit values may be further improved by combining, for example, data from different time slices (Pan et al. 2009).
In summary, a 2% (1%) accurate simultaneous fit for β_{f} and Δ_{f} should be possible in the highly compressible regime if the Z_{p} are 0.1% (0.05%) accurate. If no satisfying fit is possible for such Z_{p}, this may indicate that the model is not applicable to the turbulence data under examination.
3. Discussion
We address three topics. First, can the necessary accuracy for the Z_{p} be met in practical applications? Second, if we had this type of accurate simulation data, what could be learned about the hierarchical structure model and its applicability or nonapplicability to driven, isothermal, supersonic turbulence in a 3D periodic box? Third, we want to briefly revisit the frequently used one parameter fits.
We start with the question whether 0.1% or even 0.05% accurate Z_{p} for p = 1,...,5 are achievable, as are needed to get 2% (1%) accurate fits for β and Δ. The answer is probably yes, at least in the context of 3D periodic box simulations. Schmidt et al. (2008) estimate the accuracy of their Z_{p}, p = 1,...,5, to 1% (3D box simulations, 1024^{3}). Kritsuk et al. (2007a) estimate 1% accuracy or better for absolute scaling exponents ζ_{p}, p = 1,...,3 (3D box simulations, 1024^{3}). Meanwhile, 3D box simulations with 4096^{3} exist (e.g. Federrath 2013; Beresnyak 2014). A first order estimate suggests the four times better resolution to translate into four times (first order scheme) or 16 times (second order scheme) more accurate structure functions, thus accuracies of 0.25% or even 0.0625%. Moreover, if the accuracy of the Z_{p} is good enough to avoid double peaked histograms as in Fig. 6, accuracy may be further enhanced by exploring multiple time slices. Pan et al. (2009; 3D box simulations, 1024^{3}) used data from nine time slices for their two parameter fit. Their work is comparable although they rely on dissipation rates instead of velocity structure functions, since the involved scaling exponents (τ_{p} for the dissipation rate) are structurally similar according to Kolmogorov’s refined similarity hypothesis (Kolmogorov 1962), ζ_{p} = p/ 3 + τ_{p/ 3}. The tests we carried out using ratios of τ_{p} instead of ζ_{p} indeed show a similar behavior. From the quality of their fit and based on our results, we estimate their τ_{p} to be about 1% accurate, which is plausible given their numerical resolution. A reliable two parameter fit to 3D periodic box data of highly supersonic turbulence that is based on velocity structure functions thus appears feasible with today’s data.
What could be learned from better simulation data (4096^{3} or better) and associated, more accurate Z_{p}? Each Z_{p} defines a curve with associated uncertainty in the βΔ plane, the curves for different p may or may not intersect to within uncertainties. If they intersect, the model by She & Leveque (1994) may indeed carry over to highly compressible turbulence. It is then interesting to see whether the fitted range for Δ, currently estimated as (0.67−0.78) by Pan et al. (2009), remains compatible with Δ = 2/3, the value tacitly assumed in a large body of literature. It is also interesting to check whether β = 1/3, as theoretically anticipated by Boldyrev (2002). If indeed (β,Δ) = (1/3,2/3), results from one parameter fits that quantify the transition to incompressible turbulence (β = Δ = 2/3) with decreasing Mach number likely apply (Padoan et al. 2004). If Δ ≠ 2/3, two parameter fits for β and Δ would also be needed in the mildly compressible regime. However, the analysis in Sect. 2.3.3 suggests that these kind of fits are likely beyond reach of today’s computer resources.
The latter of the above cases, where the Z_{p} curves do not intersect to within their uncertainty, would imply that the model by She & Leveque (1994) does not carry over to 3D periodic box simulations of driven, isothermal, highly compressible turbulence. A simple reason here could be that theoretical results are based on the assumption of an infinite Reynolds number, a criterion clearly violated by numerical simulations. More importantly, She & Waymire (1995) already pointed out that there is no reason why only one dimension should be associated with the most dissipative structure. They argued that in such a large portion of space as is typically analyzed, a variety of most dissipative structures may coexist with different codimensions. Hopkins (2013) suggests a slightly different model based on work by Castaing (1996), which is more compatible with not strictly lognormal density PDFs as observed in isothermal supersonic turbulence. Finally, yet other models exist, (e.g. via multifractals Macek et al. 2011; Zybin & Sirota 2013), as well as other perspectives on the fractal character of a turbulent medium (see e.g. Kritsuk et al. 2007a).
Lastly, we briefly come back to the one parameter fits that are often used in the literature. Fixing the value of Δ by hand greatly reduces the impact of uncertainties in the Z_{p} on the accuracy of the estimated bestfit codimension C_{f}. Folini et al. (2014) found 5% uncertain Z_{p}, p = 1,...,5, to translate into roughly 10% uncertainty of the C_{f} for fixed Δ = 2/3. Fig. 3 offers a qualitative understanding of this reduced “error propagation”, which suggests some sensitivity to the specific location in the βΔplane, and indicates that fixing C or β instead of Δ has a similar effect. Fixing β seems questionable at first sight since there is, to our knowledge, little theoretical understanding of what numerical value β might have (see e.g. Dubrulle 1994). On the other hand, She et al. (2001) presented a theoretical framework that allows for an independent determination of only β from the relative scaling exponents Z_{p} (see also HilyBlant et al. (2008), their Appendix A3). One could thus imagine breaking the two parameter fit for β and Δ into a two step procedure: first, fix the value of β, then use this value and do a one parameter fit for Δ. Hopefully this type of a two step approach is more robust against uncertainties in the Z_{p}, but this question is beyond the scope of the current paper and we are unaware of corresponding attempts in the literature.
4. Summary and conclusions
This study was motivated by the overarching question of whether or not the random cascade model (She & Leveque 1994; Dubrulle 1994; She & Waymire 1995; Boldyrev 2002) applies to simulation data of highly compressible isothermal turbulence and, if so, with what parameter values for β and Δ. If applicable, the model offers a theoretical link between observable properties of the turbulence, namely ratios Z_{p} of scaling exponents of the structure functions, and nonobservable turbulence characteristics, for example the dimension D of the most dissipative structures. To date, applicability of the model is assumed in much of the literature with Δ = 2/3, a value just marginally compatible with simulationbased best estimates (Pan et al. 2009): Δ = 0.71 with an uncertainty range Δ ∈ (0.67,0.78).
We examine how uncertainties in the Z_{p} translate into uncertainties of bestfit βΔpairs and discuss what bestfits, consequently, seem achievable with today’s computer resources. A Monte Carlo approach is used to mimic actual simulation data. The results can be summarized in six main points.

Simultaneous fitting of β and Δ to sets of substantially (5%) perturbed (uncertain) Z_{p} yields a “double peaked ridge” of bestfit values in the βΔ plane. None of the two peaks is colocated with the initial (β,Δ) pair.

The highest and lowest order p are particularly relevant for simultaneous fitting of β and Δ. A somewhat optimal choice is p = 1,...,5. Yet higher order structure functions add comparatively little to the quality of the fit, while they tend to be afflicted with larger uncertainties in real applications.

A simultaneous, 2% (1%) accurate fit of β and Δ should be possible if the Z_{p}, p = 1,...,5, are 0.1% (0.05%) accurate and if the (yet to be determined) value of β is about 1/3 or less.

Applicability of the model thus may be best tested in the highly compressible regime, where β ≈ 1 /3 is expected, and not in the mildly compressible regime where β ultimately must approach its incompressible value of 2/3.

We argue that today’s computer resources likely allow to reach this accuracy. Existing simulations of 4096^{3} (Federrath 2013; Beresnyak 2014) probably allow for at least 2%, possibly 1% accurate estimates of β and Δ.

Should the ambiguity in the determination of β and Δ persist despite such highly accurate Z_{p}, this may indicate that the notion of She & Waymire (1995; β and Δ take a continuum of values) or Hopkins (2013; a different model for the statistics of the inertial range) is correct or that yet a different turbulence model is needed in this regime.
Acknowledgments
R.W. and D.F. acknowledge support from the French National Program for High Energies PNHE. We acknowledge support from the Pôle Scientifique de Modélisation Numérique (PSMN), from the Grand Equipement National de Calcul Intensif (GENCI), project number x2014046960, and from the European Research Council through grant ERCAdG No. 320478TOFU.
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All Tables
Illustration of range δC of codimension C for given order p and uncertainty δZ_{p} of structure functions for two βΔ pairs.
All Figures
Fig. 1 Ratio of polynomials P_{β,b}/P_{β,a}, Eq. (5), (yaxis, shown as logarithm) for selected exponents a and b as function of β (xaxis). Colors indicate b/a = 2 (red), 4 (green), 5 (blue), 6 (magenta), 7 (cyan), all with a = p_{1}/ 3 = 1/3, as well as b/a = 7/6 (black) with a = p_{1}/ 3 = 6/3. 

Open with DEXTER  
In the text 
Fig. 2 Z_{p} in the βΔplane, role of p. Shown is Z_{p} (color coded) for p = 1 (top left), p = 2 (top right), p = 4 (bottom left) and p = 10 (bottom right). For β = 1/3 and Δ = 2/3 (red dot), the curve of constant Z_{p} (black) is shown, as well as curves of ± 5% different Z_{p} (white). 

Open with DEXTER  
In the text 
Fig. 3 Part of βΔplane (color coded in codimension C = Δ/(1 − β), 0 <C< 3) within joint reach of (at most) 5% perturbed Z_{p}, starting from Z_{p} for Δ = 2/3 and β = 1/3 (red dot). Left panel: curves of 5% perturbed Z_{p} values for p = 1 (white), p = 2 (blue), p = 4 (red), and p = 5 (green) and part of the βΔplane enclosed by all of them. Right panel: same as left panel but also including p = 6 (purple) and p = 7 (black). 

Open with DEXTER  
In the text 
Fig. 4 Same as Fig. 3, left, but for β = Δ = 2/3 (top left), β = Δ = 1/3 (top right), β = 0.048 and Δ = 1/3 (bottom left), as well as and β = 0.048 and Δ = 2/3 (bottom right). 

Open with DEXTER  
In the text 
Fig. 5 Bestfit β_{f} and Δ_{f} from 5% perturbed Z_{p}. Left: 2D histogram (contours, log10, spacing 0.5, spanning three orders of magnitude) of bestfit βΔvalues from 100 000 perturbed data sets. We note that the 2D histogram shows two peak values (indicated by cyan dots), none of them colocated with the unperturbed (β = 1/3,Δ = 2/3) pair (red dot). Right: underestimation of Z_{5} favors Δ_{f} = 1. Shown is, for a subset of 1000 perturbed data sets, Δ_{f} as function of , again for an unperturbed pair (β = 1/3,Δ = 2/3). Colors indicate . 

Open with DEXTER  
In the text 
Fig. 6 Role of β (columns) and accuracy (rows) of associated Z_{p}, for fixed Δ = 2/3. Shown are PDFs (yaxis) of C_{f} (xaxis), 1000 random data sets, powers p = 1,...,5 for β = 0.0476 (first column), β = 0.17 (second column), β = 1/3 (third column), and β = 2/3 (fourth column). Corresponding exact codimensions (red lines) are, from left to right: C = 0.7, C = 0.8, C = 1, and C = 2. Individual rows from top to bottom contain accuracies of 20%, 10%, 5%, 2%, 0.5%, and 0.1%. As can be seen, the larger β, the more severe are the consequences of inaccuracies in the Z_{p}. Histograms in the upper right (large β, low accuracy of the Z_{p}) look worst. We note that axis ranges differ among panels, to best capture the shape of each histogram. 

Open with DEXTER  
In the text 
Fig. 7 Role of higher order moments. Inclusion of higher order ESS scaling exponents (from p = 5, top left, to p = 10, bottom right) gradually reduces the erroneous peak in the bestfit codimension (around C_{f} = 2.5). Shown are PDFs of C_{f} for at most 5% perturbed Z_{p} values (100 000 random data sets) and exact pair (β = 1/3,Δ = 2/3). Spacing of the βΔgrid for fitting is 0.002. 

Open with DEXTER  
In the text 
Fig. 8 Required accuracy (color coding) of perturbed Z_{p}, p = 1,...,5, such that for at least 2/3 of the bestfit pairs (β_{f}, Δ_{f}) the associated C_{f} are within 10% (top) or 5% (bottom) of the C associated with the initial, unperturbed (β, Δ) pair. As can be seen, the required accuracy depends crucially on the location within the βΔ plane. Gray lines indicate the range within which 2/3 of the actual β_{f} (vertical direction) and Δ_{f} (horizontal direction) lie. Black lines indicate constant C = 1 (lower line) and C = 2 (upper line). For details see text. 

Open with DEXTER  
In the text 
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