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Related papers: Linear dynamics of over-expanded annular supersoni…

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An overexpanded jet in a truncated ideally contoured nozzle is found to feature a tonal behavior. The flow field is investigated to understand its origin and show how it modifies side-load properties. The temporal and spatial organization…

We study the linear stability of a planar interface separating two fluids in relative motion, focusing on conditions appropriate for the boundaries of relativistic jets. The jet is magnetically dominated, whereas the ambient wind is…

High Energy Astrophysical Phenomena · Physics 2023-07-10 Anthony Chow , Jordy Davelaar , Michael Rowan , Lorenzo Sironi

Strong observational evidence indicates that all extragalactic jets associated with AGNs move at relativistic speed up to 100 pc - 1 kpc scales from the nucleus. At larger distances, reflecting the Fanaroff-Riley radio source…

Astrophysics · Physics 2009-11-13 P. Rossi , A. Mignone , G. Bodo , S. Massaglia , A. Ferrari

A novel supersonic jet oscillating method is investigated both experimentally and numerically. A rectangular primary supersonic jet is issued into a confined chamber with sudden enlargement. Secondary control jets are issued from the top,…

Fluid Dynamics · Physics 2023-11-01 Spandan Maikap , S. K. Karthick , R. Arun Kumar

The long term magnetohydrodynamic stability of magnetized transonic/supersonic jets is numerically investigated using a spatial approach. We focus on two-dimensional linearly-unstable slab configurations where the jet is embedded in a…

Astrophysics · Physics 2007-07-26 M. Viallet , H. Baty

We investigate the Kelvin-Helmholtz instability of stratified jets. The internal component (core) is made of a relativistic gas moving with a relativistic bulk speed. The second component (sheath or envelope) flows between the core and…

Astrophysics · Physics 2007-05-23 M. Hanasz , H. Sol

We perform a linear analysis of the stability of a magnetized relativistic non-rotating cylindrical flow in the aproximation of zero thermal pressure, considering only the m = 1 mode. We find that there are two modes of instability:…

High Energy Astrophysical Phenomena · Physics 2015-06-16 G. Bodo , G. Mamatsashvili , P. Rossi , A. Mignone

This investigation aims to assess the effect of different types of actuator forcing on the feedback loop of an under-expanded Mach 1.27 planar impinging jet using a resolvent framework. To this end, we employ a Large Eddy Simulation…

Fluid Dynamics · Physics 2022-04-18 Qiong Liu , Chitrarth Prasad , Datta V. Gaitonde

Non-relativistic three-dimensional magnetohydrodynamic simulations of Poynting-flux-dominated (PFD) jets are presented. Our study focuses on the propagation of strongly magnetized hypersonic but sub-Alfv\'enic flow ($C_{\rm s}^2 << V_{\rm…

Astrophysics · Physics 2009-11-10 Masanori Nakamura , David L. Meier

We study a turbulent jet issuing from a cylindrical nozzle to characterise coherent structures evolving in the turbulent boundary layer. The analysis is performed using data from a large-eddy simulation of a Mach 0.4 jet. Azimuthal…

Fluid Dynamics · Physics 2021-08-11 Oğuzhan Kaplan , Peter Jordan , André Cavalieri , Guillaume A. Brès

Relativistic outflows represent one of the best-suited tools to probe the physics of AGN. Numerical modelling of internal structure of the relativistic outflows on parsec scales provides important clues about the conditions and dynamics of…

Astrophysics · Physics 2009-11-11 M. Perucho , A. Lobanov , J. -M. Marti , P. E. Hardee

We analyze the perturbation dynamics of a complex supersonic multi-stream rectangular jet. The dynamics are examined through application of spectral proper orthogonal decomposition (SPOD) to elicit coherent structure and linear resolvent…

Fluid Dynamics · Physics 2025-04-04 Mitesh Thakor , Datta V. Gaitonde , Yiyang Sun

The recent development of tomographic analysis of radio data shows the presence of sheaths around several extragalactic jets. We have studied the Kelvin-Helmholtz instability of such stratified jets, describing them as inner relativistic…

Astrophysics · Physics 2007-05-23 M. Hanasz , H. Sol

Many jets exhibit twisted helical structures. Where superluminal motions are detected, jet orientation and pattern/flow speed are considerably constrained. In this case modeling efforts can place strong limits on conditions in the jet and…

Astrophysics · Physics 2009-11-10 P. E. Hardee

We study, by numerical simulations, the entrainment process in a supersonic, radiative jet flow, during the evolution of Kelvin-Helmholtz instabilities, in the context of the the acceleration problem of molecular bipolar outflows, observed…

Astrophysics · Physics 2007-05-23 M. Micono , G. Bodo , S. Massaglia , P. Rossi , A. Ferrari

Flow-induced instabilities are relevant for the storage and dynamics of magnetic fields in stellar convection zones and possibly also in other astrophysical contexts. We continue the study started in the first paper of this series by…

Astrophysics · Physics 2009-11-13 V. Holzwarth , D. Schmitt , M. Schuessler

The KelvinHelmholtz (KH) instability is a fundamental wave instability that is frequently observed in all kinds of shear layer (jets, wakes, atmospheric air currents etc). The study of KH-instability, coherent flow structures has a major…

Computational Engineering, Finance, and Science · Computer Science 2015-03-29 Santosh Tirunagari

The properties of wave-like helically twisted normal mode structures on steady relativistic jets are summarized. Wave speeds are a function of the wavelength and less than the jet speed. However, normal mode interference can lead to both…

Astrophysics · Physics 2009-10-31 Philip E. Hardee

The effects of relativistic dynamics and thermodynamics in the development of Kelvin-Helmholtz instabilities in planar, relativistic jets along the early phases (namely linear and saturation phases) of evolution has been studied by a…

Astrophysics · Physics 2009-11-10 M. Perucho , M. Hanasz , J. M. Marti , H. Sol

We investigate the linear and nonlinear evolution of current-carrying jets in a periodic configuration by means of high resolution three-dimensional numerical simulations. The jets under consideration are strongly magnetized with a variable…

High Energy Astrophysical Phenomena · Physics 2014-07-09 M. Anjiri , A. Mignone , G. Bodo , P. Rossi