Search results for " methods]"

showing 4 items of 4 documents

XMM-Newton Large Program on SN1006 - I: Methods and Initial Results of Spatially-Resolved Spectroscopy

2015

Based on our newly developed methods and the XMM-Newton large program of SN1006, we extract and analyze the spectra from 3596 tessellated regions of this SNR each with 0.3-8 keV counts $>10^4$. For the first time, we map out multiple physical parameters, such as the temperature ($kT$), electron density ($n_e$), ionization parameter ($n_et$), ionization age ($t_{ion}$), metal abundances, as well as the radio-to-X-ray slope ($\alpha$) and cutoff frequency ($\nu_{cutoff}$) of the synchrotron emission. We construct probability distribution functions of $kT$ and $n_et$, and model them with several Gaussians, in order to characterize the average thermal and ionization states of such an extended s…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsElectron densityAstrophysics::High Energy Astrophysical Phenomenadata analysis cosmic rays ISM: supernova remnants X-rays: ISM [acceleration of particles shock waves methods]FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsacceleration of particles shock waves methods: data analysis cosmic rays ISM: supernova remnants X-rays: ISMSpectral lineInterstellar mediumSupernovaSpace and Planetary ScienceIonizationAstrophysics::Solar and Stellar AstrophysicsSpectroscopySupernova remnantAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Equivalent widthAstrophysics::Galaxy Astrophysics
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High-order regularization in lattice-Boltzmann equations

2017

A lattice-Boltzmann equation (LBE) is the discrete counterpart of a continuous kinetic model. It can be derived using a Hermite polynomial expansion for the velocity distribution function. Since LBEs are characterized by discrete, finite representations of the microscopic velocity space, the expansion must be truncated and the appropriate order of truncation depends on the hydrodynamic problem under investigation. Here we consider a particular truncation where the non-equilibrium distribution is expanded on a par with the equilibrium distribution, except that the diffusive parts of high-order nonequilibrium moments are filtered, i.e., only the corresponding advective parts are retained afte…

Shock waverecurrence relationspolynomialsComputational MechanicsLattice Boltzmann methods114 Physical sciences01 natural sciences010305 fluids & plasmassubspaces0103 physical sciences010306 general physicsFluid Flow and Transfer ProcessesPhysicstensor methods: shock tubesHermite polynomialsRecurrence relationta114AdvectionMechanical EngineeringpolynomitMathematical analysisCondensed Matter PhysicsDistribution functionMechanics of MaterialsRegularization (physics)shock tubes [tensor methods]Shear flowPhysics of Fluids
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Emission-Line Intensity Ratios in F[CLC]e[/CLC] [CSC]xvii[/CSC] Observed with a Microcalorimeter on an Electron Beam Ion Trap

2000

We report new observations of emission line intensity ratios of Fe XVII under controlled experimental conditions, using the National Institute of Standards and Technology electron beam ion trap (EBIT) with a microcalorimeter detector. We compare our observations with collisional-radiative models using atomic data computed in distorted wave and R-matrix approximations, which follow the transfer of the polarization of level populations through radiative cascades. Our results for the intensity ratio of the 2p6 1S0-2p53d 1P1 15.014 A line to the 2p6 1S0-2p53d 3D1 15.265 A line are 2.94 ± 0.18 and 2.50 ± 0.13 at beam energies of 900 and 1250 eV, respectively. These results are not consistent wit…

PhysicsMethods: laboratorySun: coronaDetectorTechniques: spectroscopicAstronomy and Astrophysicslaboratory; Stars: individual (Capella); Sun: corona; Techniques: spectroscopic; X-rays: general [Atomic data; Methods]PlasmaX-rays: generalIntensity ratioPolarization (waves)IonSettore FIS/05 - Astronomia E AstrofisicaStars: individual (Capella)Space and Planetary ScienceRadiative transferEmission spectrumAtomic physicsAtomic dataElectron beam ion trapThe Astrophysical Journal
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Hydrodynamic modelling of ejecta shrapnel in the Vela supernova remnant

2013

Many supernova remnants (SNRs) are characterized by a knotty ejecta structure. The Vela SNR is an excellent example of remnant in which detached clumps of ejecta are visible as X-ray emitting bullets that have been observed and studied in great detail. We aim at modelling the evolution of ejecta shrapnel in the Vela SNR, investigating the role of their initial parameters (position and density) and addressing the effects of thermal conduction and radiative losses. We performed a set of 2-D hydrodynamic simulations describing the evolution of a density inhomogeneity in the ejecta profile. We explored different initial setups. We found that the final position of the shrapnel is very sensitive …

PhysicsShock waveHigh Energy Astrophysical Phenomena (astro-ph.HE)Vela Supernova RemnantAstrophysics::High Energy Astrophysical Phenomenanumerical ISM: individual objects: Vela SNR ISM: kinematics and dynamics ISM: supernova remnants [hydrodynamics shock waves methods]AstronomyFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsThermal conductionVelahydrodynamics shock waves methods: numerical ISM: individual objects: Vela SNR ISM: kinematics and dynamics ISM: supernova remnantsSupernovaSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceRadiative transferAstrophysics::Solar and Stellar AstrophysicsDensity contrastEjectaAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::Galaxy Astrophysics
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