2018
DOI: 10.1063/1.5020555
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Intermittent fluctuations due to uncorrelated Lorentzian pulses

Abstract: Fluctuations due to a super-position of uncorrelated Lorentzian pulses with a random distribution of amplitudes and duration times are considered. These are demonstrated to be strongly intermittent in the limit of weak pulse overlap, resulting in large skewness and flatness moments. The characteristic function and the lowest order moments are derived, revealing a parabolic relationship between the skewness and flatness moments. Numerical integration reveals the probability density functions in the case of expo… Show more

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Cited by 4 publications
(4 citation statements)
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“…For example trapped electron mode turbulence with a strong dependence on collisions [16] does scale differently than ion temperature gradient (ITG) driven turbulence with adiabatic electrons in the collisionless limit [4,17]. However, when considering the influence of collisions [4,13], E × B shear [18] and β stabilisation physics [18] for ITG turbulence the expected scaling with main ion mass will change. A more complete account of the different physics mechanisms depending on the main ion mass can be found in [19].…”
Section: Introductionmentioning
confidence: 99%
“…For example trapped electron mode turbulence with a strong dependence on collisions [16] does scale differently than ion temperature gradient (ITG) driven turbulence with adiabatic electrons in the collisionless limit [4,17]. However, when considering the influence of collisions [4,13], E × B shear [18] and β stabilisation physics [18] for ITG turbulence the expected scaling with main ion mass will change. A more complete account of the different physics mechanisms depending on the main ion mass can be found in [19].…”
Section: Introductionmentioning
confidence: 99%
“…12, this is better described using a skewed Lorentzian pulse as a fit function with duration 80 and skewness parameter 1 for the x SOL = 50 case. [87][88][89][90] The slightly elevated tails of the conditional burst shape is likely due to finite pulse overlap in the turbulence simulations. 12.…”
Section: Fluctuation Statisticsmentioning
confidence: 99%
“…where A k and t k are pulse amplitude and arrival time for the pulse labeled k, respectively, and K(T) is the number of pulses present in a time interval of duration T. In the case of Lorentzian pulses, the function ϕ is given by [39][40][41] ϕ(θ) = 1 π…”
Section: Lorentzian Pulsesmentioning
confidence: 99%
“…Recently, the exponential spectrum has been attributed to the presence of uncorrelated Lorentzian pulses in the temporal dynamics. [29][30][31][32][33][34][35][36][37][38][39][40][41][42][43] This includes the Lorenz model, which describes chaotic dynamics in Rayleigh-Bénard convection. [23][24][25][26][27][28][29][30] In two-dimensional thermal convection, it is well known that the convection rolls in a horizontally periodic domain can give rise to the spontaneous formation of strong mean flows through a tilting instability.…”
Section: Introductionmentioning
confidence: 99%