Energy transfer and scale dynamics in 2D and 3D laser-driven jets DOI
Hao Yin, Jessica K. Shang, Eric G. Blackman

et al.

Physics of Plasmas, Journal Year: 2023, Volume and Issue: 30(9)

Published: Sept. 1, 2023

We demonstrate a methodology for diagnosing the multiscale dynamics and energy transfer in complex HED flows with realistic driving boundary conditions. The approach separates incompressible, compressible, baropycnal contributions to scale-transfer quantifies direction of these transfers (generalized) wavenumber space. use this compare kinetic (KE) across scales simulations 2D axisymmetric vs fully 3D laser-driven plasma jets. Using FLASH code, we model turbulent jet ablated from an aluminum cone target configuration outlined by Liao et al. [Phys. Plasmas, 26 032306 (2019)]. show that, addition its well known bias underestimating hydrodynamic instability growth, modeling suffers significant spurious energization bulk flow upscale cascade. In 2D, arises as vorticity strain instabilities near jet's leading edge KE upscale, sustaining coherent circulation that helps propel farther (≈25% 3.5 ns) keep it collimated. 3D, are absent. presented here may also help inter-model comparison validation, including future efforts alleviate some artifacts highlighted study.

Language: Английский

Global energy spectrum of the general oceanic circulation DOI Creative Commons
Benjamin A. Storer, Michele Buzzicotti, Hemant Khatri

et al.

Nature Communications, Journal Year: 2022, Volume and Issue: 13(1)

Published: Sept. 9, 2022

Advent of satellite altimetry brought into focus the pervasiveness mesoscale eddies [Formula: see text] km in size, which are ocean's analogue weather systems and often regarded as spectral peak kinetic energy (KE). Yet, understanding spatial scales has been derived mostly from Fourier analysis small "representative" regions that cannot capture vast dynamic range at planetary scales. Here, we use a coarse-graining method to analyze much larger than what had possible before. Spectra spanning over three decades length-scales reveal Antarctic Circumpolar Current global extra-tropical circulation, ≈ 104 km, previously unobserved power-law scaling 103 km. A smaller exists 300 associated with mesoscales, which, due their wider spread wavenumber space, account for more 50% resolved surface KE globally. Seasonal cycles exhibit characteristic lag-time 40 days per octave such both hemispheres, 102 peaks spring while late summer. These results provide new window multiscale oceanic circulation within Earth's climate system, including largest

Language: Английский

Citations

59

Spatio‐Temporal Coarse‐Graining Decomposition of the Global Ocean Geostrophic Kinetic Energy DOI Creative Commons
Michele Buzzicotti, Benjamin A. Storer, Hemant Khatri

et al.

Journal of Advances in Modeling Earth Systems, Journal Year: 2023, Volume and Issue: 15(6)

Published: June 1, 2023

Abstract We expand on a recent determination of the first global energy spectrum ocean's surface geostrophic circulation (Storer et al., 2022, https://doi.org/10.1038/s41467-022-33031-3 ) using coarse‐graining (CG) method. compare spectra from CG to those spherical harmonics by treating land in manner consistent with boundary conditions. While two methods yield qualitatively domain‐averaged results, are too noisy at gyre‐scales (>1,000 km). More importantly, inherently and cannot provide local information connecting scales currents geographically. shows that extra‐tropics mesoscales (100–500 km) have root‐mean‐square (rms) velocity ∼15 cm/s, which increases ∼30–40 cm/s locally Gulf Stream Kuroshio ∼16–28 ACC. There is notable hemispheric asymmetry mesoscale energy‐per‐area, higher north due continental boundaries. estimate ≈25%–50% total smaller than 100 km, un(der)‐resolved pre‐SWOT satellite products. Spectra time‐mean show most its (up 70%) resides stationary eddies characteristic (<500 This highlights preponderance “standing” small‐scale structures ocean temporally coherent forcing By space time, we compute spatio‐temporal AVISO NEMO. These every length‐scale evolves over wide range time‐scales peak ≈200 km ≈2–3 weeks.

Language: Английский

Citations

21

Particle acceleration by magnetic Rayleigh-Taylor instability: Mechanism for flares in black hole accretion flows DOI Creative Commons
Vladimir Zhdankin, Bart Ripperda, Alexander Philippov

et al.

Physical Review Research, Journal Year: 2023, Volume and Issue: 5(4)

Published: Oct. 9, 2023

This article uses magnetic Rayleigh-Taylor instability in relativistic collisionless plasma as an example of astrophysical process for nonthermal particle acceleration, and uncover the onset large-scale plumes formed by accumulation small ones via particle-in-cell simulations. is posed a potential mechanism flares.

Language: Английский

Citations

14

Kinetic energy spectrum and transfer within the near-dissipation range of compressible isotropic turbulence DOI
Guowei Yang, Zheng Yan, J. F. Wu

et al.

Physics of Fluids, Journal Year: 2025, Volume and Issue: 37(1)

Published: Jan. 1, 2025

The analysis of kinetic energy spectrum and dissipation mechanisms plays a crucial role in both theoretical examination real-world implementations within compressible turbulent flows. previous works the near-dissipation range are conducted framework incompressible flow dynamics. We investigate transfer isotropic flows via highly resolved direct numerical simulations with different Mach numbers (Mt). found that flows, model is significantly influenced by number, more pronounced tail as number increases. Within range, there exist strong local spatial fluctuations flux increase grid resolution. viscous can be decomposed into solenoidal dilatational components, its component leads to stronger intermittency range. Besides, high also dissipation, which serves an alternative factor for uncovered provides foundation prediction intense events development modelings.

Language: Английский

Citations

0

Calculating spectra by sequential filtering DOI
Dongxiao Zhao, Hussein Aluie

Journal of Renewable and Sustainable Energy, Journal Year: 2025, Volume and Issue: 17(1)

Published: Jan. 1, 2025

We expand on the method of sequential filtering for calculating spectra inhomogeneous fields. Sadek and Aluie [Phys. Rev. Fluids 3, 124610 (2018)] showed that kernel has to have at least p vanishing moments extract a power-law spectrum k−α with α&lt;p+2 by low-pass filtering. Here, we show high-pass allows extracting steeper α&lt;2p+3 using same pth order kernel. For example, field is shallower than k−5 can be extracted any first-order such as Gaussian or top-hat. Finally, demonstrate how second-order structure function fails capture spectral peaks because it cannot detect scaling too shallow.

Language: Английский

Citations

0

The role of double‐layer vortex rings with the local swirl in the rapid transition to turbulent flows in Richtmyer–Meshkov instability with reshock DOI Creative Commons
Zheng Yan, Zhu Chen, Z. Y. Li

et al.

Journal of Fluid Mechanics, Journal Year: 2025, Volume and Issue: 1003

Published: Jan. 24, 2025

In this paper, we study the rapid transition in Richtmyer–Meshkov instability (RMI) with reshock through three-dimensional double-layer swirling vortex rings. The RMI has an essential influence on evolution of supernovas and ignition inertial confinement fusion, which been confirmed numerical simulations experiments shock-tube high-energy-density facilities over past few years. Vortex to dominate late-time nonlinear development perturbed interface. However, studies have investigated characteristics interactions among structures during turbulent flows. coexistence co-rotating counter-rotating vortices is hypothesized induce successive large-scale strain fields, are main driving sources for development. effect reflected presence local motion azimuthal direction, it decreases translation velocity a ring. Large-, middle- small-scale fields employed describe process reshock, e.g. vorticity deposited by formation vortices, iterative cascade under amplification viscous dissipation internal energy. This provides theoretical suggestions designing practical applications, such as estimation hydrodynamic mixing acceleration phase fusion.

Language: Английский

Citations

0

Compressibility Effects on Mixing Layer in Rayleigh-Taylor Turbulence DOI
Cheng-Quan Fu, Zhiye Zhao, Pei Wang

et al.

Published: Jan. 1, 2025

Language: Английский

Citations

0

Atmospheric wind energization of ocean weather DOI Creative Commons
Shikhar Rai, J. Thomas Farrar, Hussein Aluie

et al.

Nature Communications, Journal Year: 2025, Volume and Issue: 16(1)

Published: Jan. 30, 2025

Abstract Ocean weather comprises vortical and straining mesoscale motions, which play fundamentally different roles in the ocean circulation climate system. Vorticity determines movement of major currents gyres. Strain contributes to frontogenesis deformation water masses, driving much mixing vertical transport upper ocean. While recent studies have shown that interactions with atmosphere damp ocean’s vortices O (100) km size, effect winds on motions remains unexplored. Here, we derive a theory for wind work vorticity strain. Using satellite model data, discover damps strain at an equal rate globally, unveil striking asymmetries based their polarity. Subtropical oceanic cyclones energize anticyclones outside strong current regions, while subpolar opposite effect. A similar pattern emerges strain, where subtropical convergent flow is damped along west-equatorward east-poleward direction energized east-equatorward west-poleward direction. These findings reveal energy pathways through shapes weather.

Language: Английский

Citations

0

Compressibility effects on mixing layer in Rayleigh–Taylor turbulence DOI
Cheng-Quan Fu, Zhiye Zhao, Pei Wang

et al.

Physica D Nonlinear Phenomena, Journal Year: 2025, Volume and Issue: unknown, P. 134643 - 134643

Published: March 1, 2025

Language: Английский

Citations

0

Rayleigh–Taylor instability-induced turbulence in lean hydrogen/air premixed flames DOI
J. Zheng, Haiou Wang, Evatt R. Hawkes

et al.

Combustion and Flame, Journal Year: 2025, Volume and Issue: 277, P. 114183 - 114183

Published: April 28, 2025

Language: Английский

Citations

0