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ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2 , Tom Chang 3 , Paul M. Kintner 4 , and Eric M. Klatt 5 1 Institute of Space, Astrophysical and Plasma Sciences, National Cheng Kung University, Tainan, Taiwan 2 Plasma and Space Science Center, National Cheng Kung University, Tainan, Taiwan 3 Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA 4 School of Electrical and Computer Engineering, Cornell University, Ithaca, NY, USA

ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

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Page 1: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global

Crossover Behavior

Sunny W. Y. Tam1,2, Tom Chang3, Paul M. Kintner4, and Eric M. Klatt5

1 Institute of Space, Astrophysical and Plasma Sciences, National Cheng Kung University, Tainan, Taiwan2 Plasma and Space Science Center, National Cheng Kung University, Tainan, Taiwan3 Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA4 School of Electrical and Computer Engineering, Cornell University, Ithaca, NY, USA5 Applied Physics Laboratory, Johns Hopkins University, Laurel, MD, USA

Page 2: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Outline

• Data

– Electric field in the auroral zone

• Multifractal Analyses and Scaling Behavior

– Traditional Structure Function Analysis

– ROMA (Rank-Ordered Multifractal Analysis)

• Individual Regimes

– ROMA for Nonlinear Crossover Behavior

• Across Regimes of Time Scales

• Summary

Page 3: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

• SIERRA sounding rocket in the nighttime auroral zone

• Time series of an electric field component perpendicular to the magnetic field

• Consider E measured between 550 km altitude and the apogee (735 km) of SIERRA

• Typically observed broadband extremely low-frequency (BB-ELF) electric field fluctuations

• Subset of the observed electric field fluctuations found to be intermittent in nature [Tam et al., 2005]

Electric Field Data

Page 4: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

• The broadband power spectrum signature of the BB-ELF fluctuations has been suggested as the manifestation of intermittent turbulence; origin of intermittent fluctuations interpreted as the result of sporadic mixing and/or interactions of localized pseudo-coherent structures [Chang, 2001; Chang et al., 2004]

• Pseudo-coherent structures (c.f. nearly 2D oblique potential structures based on MHD simulations by Seyler [1990]) nearly non-propagating, measurements due to Doppler-shifted spatial fluctuations, mixed with small fractions of propagating waves

• Time scales τ in data can be interpreted as spatial scales Δ=Uτ (horizontal speed of rocket, U ≈1.5 km/s)

Page 5: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Multifractal Analyses and Scaling Behavior

• Traditional Structure Function Analysis

• ROMA (Rank-Ordered Multifractal Analysis) [Chang and Wu, 2008]

• ROMA for Nonlinear Crossover Behavior [Tam et al., 2010]

– Double rank-ordering

Page 6: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Common procedures for the methods:

• Generate Probability Distribution Function (PDF) for different values of , where(| |, )P E ( ) ( )E E t E t

Page 7: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Traditional Structure Function Analysis

• Define the structure function of the moment order q at the time scale :

• q is required to be non-negative to avoid divergence of Sq

• One looks for the scaling behavior

max| |

0

( ) ( ) ( ) ,E

q q

qS E E P E d E

q

qS ~)(

Page 8: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

• If the “fractal dimension” is proportional to q, i.e. , all the fractal properties can be

characterized by a single number

monofractal

• The Hurst exponent

is constant if the fluctuations are monofractal; multifractals are indicated by non-constant H(q).

qqH q)(

q

1q q 1

Page 9: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Single-Parameter Scaling• Monofractal condition can be satisfied by a one-

parameter scaling with the parameter s [Chang et al., 1973]:

One can show that

• For monofractal fluctuations, the single-parameter scaling is able to provide a clear description of how the strength of the fluctuations varies with the time scale.

0 0( , ) ( ) ( )s ssP E P E

1s H 1q q

Page 10: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Structure Functions of Electric Field Fluctuations

Indication of multiple physical regimes of time scales

log Sq vs. log τ not a straight line

Page 11: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Regimes 1 2 3 4

Consider only Regime 1 in detail as an example.

Assume adjacent regimes roughly have a common time scale:

Regime 1: 5 – 80 ms (kinetic)

Regime 2: 80 – 160 ms (crossover)

Regime 3: 160 – 320 ms (crossover)

Regime 4: 320 ms and longer (MHD)

Slope ζ q

Rank-Order the time regimes into i =1 to 4

Study the multifractal characteristics of each regime separately

Page 12: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

For the electric field fluctuations, the plot of vs. q is not exactly a straight line.

q

H(q) is not a constant, varying considerably.

Indications of multifractal behaviorWith traditional structure function analysis:

Page 13: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

0 0( , ) ( ) ( )s ssP E P E

0( ) ( , )ssP Y P E where 0( ) sY E

Single-parameter scaling does not apply well to the multifractal electric field fluctuations.

Apply single-parameter scaling formula ( ms):0 5

0.69s 0.9s

Page 14: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Drawbacks of Tradition Structure Function Analysis on Multifractal Fluctuations

• Different parts of the PDF are emphasized by different moment order (larger q for larger ) and have different fractal properties (non-constant H), but characterizes only the average fractal properties over the entire PDF.

• Negative q is ill-defined.

| |E

q

Page 15: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Rank-Ordered Multifractal Analysis (ROMA) for Individual Regimes• Technique introduced by Chang and Wu [2008]

• Technique retains the spirit of structure function analysis and single-parameter scaling

• Divide (Rank-Order) the domain of (Note: s=s(Y)) into separate ranges and, for each range, look for one-parameter scaling

• Scaling function and scale invariant Y

( )0( ) s YY E

( ) ( )0 0( , ) ( ) ( )s Y s Y

sP E P E

( )0( ) ( , )s Y P E

Page 16: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

To solve for s(Y), the scaling parameter s for the range

:• construct the range-limited structure functions with

prescribed s

• Look for the scaling behavior

• The solution s will satisfy

[ , ]low highY Y Y

0

0

( )

( )

' ( ) ( ) ,

shigh

slow

Yq

q

Y

S E P E d E

'' ( ) ~ q

qS

'q qs

Page 17: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Example: Regime 1 Y1 = [0.8, 1.2]

s1 = 0.80 from this plot

With increased resolution, s1 = 0.804

1'q qs

Page 18: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Validity of the solution

Note: negative q is applicable

1'q qs

Page 19: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Plot of scaling parameter s1 for different ranges of Y1

In principle, s1=s1(Y1) a continuous spectrum; but for practical purpose, statistics reaches limitation as Y-ranges keep decreasing

Considerable variation of s1 multifractal

Page 20: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Comparison of the scaling by the two multifractal analyzing techniques

Traditional single-parameter scaling

ROMA

Page 21: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Regime 1

Persistency (s > 0.5): probably due to kinetic effects

Rapidly changing s: indication of possible developing instability and turbulence

Slowly changing s: More stable and developed turbulent state

Page 22: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Regime 2Developing turbulence at small Y seems to be of a mixture of persistent (s > 0.5) and anti-persistent (s > 0.5) nature

Effects beyond the kinetic range play a non-negligible role

Turbulence settled down to more stable and developed state

Persistent probably because kinetic effects are still more dominant than those of MHD

Page 23: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Regime 3

Similar to Regimes 1 and 2, developing turbulence at small Y

Highly unstable turbulence compared with the other 2 regimes, indicated by the wide range of s and the range of Y where s exhibits such large fluctuations

Page 24: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Regime 4

Anti-persistency (s < 0.5)

Monotonically decreasing s beyond a certain Y

Same features in the original ROMA calculations for results of 2D MHD simulations [Chang and Wu, 2008]

Signature of developing MHD turbulence?

Page 25: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Scaling Functions

Regime 1 Regime 2

Regime 3 Regime 4

Page 26: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Regime 1 Regime 2 Regime 4

Resemblance in shape between s(Y) and H(q)

Page 27: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Resemblance in shape between s(Y) and H(q)

max| |

0

( ) ( ) ,E

q

qS E P E d E

q

qS ~)( ( ) qH q q

q increases fractal property at larger |δE| is emphasized

0

0

( )

( )

' ( ) ( ) ,

shigh

slow

Yq

q

Y

S E P E d E

'' ( ) ~ q

qS 'qs q

for each Y-range

Y increases |δE| increases

Page 28: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Exception: Regime 3 Reason:

Significant decrease in s(Y) over a small range of Y

( )0( )s YE Y

• a narrow range in the domain of |δE| corresponds to a wide range in the domain of Y• Narrow range of |δE| emphasized by H(q) actually characterizes the average fractal behavior at a wide range of Y• s(Y) is a more accurate description than H(q)

Page 29: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Advantages of ROMA

1. Fractal properties at different and • is known at each range of Y

2. Scaling behavior• s is found for each range of Y; scale invariance is

determined:

3. Negative q• Applicable except for the range that includes Y = 0

| |E'q qs

( )0( ) s YY E

Page 30: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

ROMA Across Regimes of Time Scales

• Assume that crossover ranges of time scales between contiguous time regimes are narrow

• Because regimes are contiguous and scaling with the time scales is power law in nature, Yi can be mapped onto Yi-1 , and so on. Eventually, all the Yi can be mapped onto one global scaling variable Yglobal

• Correspondingly, the scaling functions of all the regimes can be mapped to a global scaling function Ps1(Yglobal)

Page 31: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

s1

s2

s3

s4

Except for highly unstable turbulence, a generally decreasing trend for si at given Yglobal as i goes from

1 to 4, with the regimes crossing over from kinetic to MHD.

Page 32: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Global Scaling Functions

Regime 1 – 4

Page 33: ROMA (Rank-Ordered Multifractal Analysis) for Intermittent Fluctuations with Global Crossover Behavior Sunny W. Y. Tam 1,2, Tom Chang 3, Paul M. Kintner

Summary• Traditional structure function analysis vs. ROMA

for time (or spatial) series of fluctuations– Both methods indicate multifractal nature of the

electric field fluctuations in the auroral zone– ROMA has the advantages of providing clearer

information regarding the fractal properties and scaling behavior of the fluctuations

• ROMA is extended to apply to fluctuations with multiple regimes in time scale– Double rank-ordered parameters: regime index i and

power-law scaling variable Yi

– Determine global scaling function and global scaling variable across different regimes

– Scaling parameter s generally decreases as the regimes cross over from kinetic to MHD

– Collapse of PDF at all time scales of all regimes