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相关论文: Non Kolmogorov-like Turbulence in the Local Inters…

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We derive a new shell model of magnetohydrodynamic (MHD) turbulence in which the energy transfers are not necessary local. Like the original MHD equations, the model conserves the total energy, magnetic helicity, cross-helicity and volume…

流体动力学 · 物理学 2009-09-29 F. Plunian , R. Stepanov

Multiple space and time scales arise in plasma turbulence in magnetic confinement fusion devices because of the smallness of the square root of the electron-to-ion mass ratio $(m_e/m_i)^{1/2}$ and the consequent disparity of the ion and…

等离子体物理 · 物理学 2019-06-26 M. R. Hardman , M. Barnes , C. M. Roach , F. I. Parra

Cosmic rays (CRs) are a dynamically important component of the interstellar medium (ISM) of galaxies. The $\sim$GeV CRs that carry most CR energy and pressure are likely confined by self-generated turbulence, leading them to stream along…

We present a generic mechanism for the thermal damping of compressive waves in the interstellar medium (ISM), occurring due to radiative cooling. We solve for the dispersion relation of magnetosonic waves in a two-fluid (ion-neutral) system…

星系天体物理 · 物理学 2021-11-24 Kedron Silsbee , Alexei V. Ivlev , Munan Gong

The injection of turbulence in the circum-galactic medium at redshift z = 2 is investigated using the mesh-based hydrodynamic code Enzo and a subgrid-scale (SGS) model for unresolved turbulence. Radiative cooling and heating by a uniform…

宇宙学与河外天体物理 · 物理学 2013-06-18 Luigi Iapichino , Matteo Viel , Stefano Borgani

Interstellar space is filled with a dilute mixture of charged particles, atoms, molecules and dust grains, called the interstellar medium (ISM). Understanding its physical properties and dynamical behavior is of pivotal importance to many…

星系天体物理 · 物理学 2014-12-18 Ralf S. Klessen , Simon C. O. Glover

Previously we developed a local model for a spherically contracting/expanding gas cloud that can be used to study turbulence and small scale instabilities in such flows. In this work we generalise the super-comoving variables used in…

太阳与恒星天体物理 · 物理学 2026-01-19 Elliot M. Lynch , Guillaume Laibe

The nature of the turbulent energy transfer rate is studied using direct numerical simulations of weakly collisional space plasmas. This is done comparing results obtained from hybrid Vlasov-Maxwell simulations of colissionless plasmas,…

The genesis, growth and rupture of intracranial aneurysm (IA) are open questions in neurovascular medicine until the present moment. The complexity of aneurysm mechanobiology and pathobiology staggeringly combine intertwining biological and…

医学物理 · 物理学 2020-01-24 Simon Tupin , Khalid M. Saqr , Sherif Rashad , Kuniyasu Niizuma , Makoto Ohta , Teiji Tominaga

It is crucial to understand the extreme intermittency of ocean and lake turbulence and turbulent mixing in order to estimate vertical fluxes of momentum, heat and mass by Osborn-Cox flux-dissipation methods. Vast undersampling errors occur…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson

Observations of interstellar scintillations at radio wavelengths reveal a Kolmogorov-like scaling of the electron density spectrum with a spectral slope of -5/3 over six decades in wavenumber space. A similar turbulent density spectrum in…

空间物理 · 物理学 2015-05-13 Dastgeer Shaikh , G. P. Zank

We present results of large-scale three-dimensional simulations of weakly magnetized supersonic turbulence at grid resolutions up to 1024^3 cells. Our numerical experiments are carried out with the Piecewise Parabolic Method on a Local…

星系天体物理 · 物理学 2009-08-13 Alexei G. Kritsuk , Sergey D. Ustyugov , Michael L. Norman , Paolo Padoan

Stellar and nebular abundance indicators reveal that there exists significant abundance fluctuations in the interstellar medium (ISM) of gas-rich galaxies. It is shown that at the present observed solar level of O/H $\sim 6 \times 10^{-4}$,…

天体物理学 · 物理学 2007-05-23 Jean-Rene ROY , Daniel KUNTH

In low-density plasma environments, such as the intracluster medium (ICM), the Larmour frequency is much larger than the ion-ion collision frequency. In such a case, the thermal pressure becomes anisotropic with respect to the magnetic…

宇宙学与河外天体物理 · 物理学 2015-06-11 M. S. Nakwacki , E. M. de Gouveia Dal Pino , G. Kowal , R. Santos-Lima

We study the homogeneous isotropic turbulence of a shear-thinning fluid modeled by the Carreau model and show how the variable viscosity affects the multiscale behaviour of the turbulent flow. We show that Kolmogorov theory can be extended…

流体动力学 · 物理学 2025-06-11 Marco Edoardo Rosti

In this paper we discuss the dynamical features of intermittent fluctuations in homogeneous shear flow turbulence. In this flow the energy cascade is strongly modified by the production of turbulent kinetic energy related to the presence of…

混沌动力学 · 物理学 2007-05-23 P. Gualtieri , C. M Casciola , R. Benzi , G. Amati , R. Piva

Many scaling relations are observed for self-gravitating systems in the universe. We explore the consistent understanding of them from a simple principle based on the proposal that the collision-less dark matter fluid terns into a turbulent…

天体物理学 · 物理学 2010-02-04 Akika Nakamichi , Masahiro Morikawa

Magnetic-field generation by a relativistic ion beam propagating through an electron-ion plasma along a homogeneous magnetic field is investigated with 2.5D high-resolution particle-in-cell (PIC) simulations. The studies test predictions of…

高能天体物理现象 · 物理学 2014-11-20 Jacek Niemiec , Martin Pohl , Antoine Bret , Thomas Stroman

The neutral interstellar medium (ISM) inside the Local Bubble (LB) has been known to have properties typical of the warm neutral medium (WNM). However, several recent neutral hydrogen (HI) absorption experiments show evidence for the…

天体物理学 · 物理学 2009-06-23 Snezana Stanimirovic

The Kolmogorov flow provides an ideal instance of a virtual channel flow: It has no boundaries, but nevertheless it possesses well defined mean flow in each half-wavelength. We exploit this remarkable feature for the purpose of…

流体动力学 · 物理学 2015-06-18 S. Musacchio , G. Boffetta