Search results for "Millimeter"

showing 10 items of 44 documents

Radio observations of active galactic nuclei with mm-VLBI

2017

Over the past few decades, our knowledge of jets produced by active galactic nuclei (AGN) has greatly progressed thanks to the development of very-long-baseline interferometry (VLBI). Nevertheless, the crucial mechanisms involved in the formation of the plasma flow, as well as those driving its exceptional radiative output up to TeV energies, remain to be clarified. Most likely, these physical processes take place at short separations from the supermassive black hole, on scales which are inaccessible to VLBI observations at centimeter wavelengths. Due to their high synchrotron opacity, the dense and highly magnetized regions in the vicinity of the central engine can only be penetrated when …

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsEvent Horizon TelescopeSupermassive black holeActive galactic nucleusOpacityFOS: Physical sciencesAstronomyAstronomy and AstrophysicsAstrophysics01 natural sciencesInterferometrySpace and Planetary Science0103 physical sciencesVery-long-baseline interferometryRadiative transferMillimeterAstrophysics - High Energy Astrophysical Phenomena010306 general physics010303 astronomy & astrophysicsThe Astronomy and Astrophysics Review
researchProduct

Experimental study of bubble detection in liquid metal.

2017

International audience; Bubble detection in liquid metal is an important issue for various technological applications. For instance, in the framework of Sodium Fast Reactors design, the presence of gas in the sodium flow of the primary and secondary loops is an issue of crucial importance for safety and reliability. Here, the two main gas measurement methods in sodium are ultrasonic testing and eddy-current testing; we investigate the second method in our study. In a first approach, we have performed experiments with liquid metal galinstan containing insulating spherical beads of millimeter size. The liquid metal is probed with an Eddy-current Flowmeter (ECFM) in order to detect the beads a…

Liquid metalMaterials science[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]MHDBubbleFlow (psychology)Ultrasonic testingGeneral Physics and AstronomyMechanicsSignal01 natural sciencesFlow measurementGalinstan010305 fluids & plasmas010309 opticschemistry.chemical_compoundchemistry0103 physical sciencesPhysique Nucléaire ThéoriqueMillimeterElectrical and Electronic Engineering
researchProduct

Seedless assembly of colloidal crystals by inverted micro-fluidic pumping

2018

We propose a simple seedless approach to assemble millimeter sized monolayer single colloidal crystals with desired orientations at predetermined locations on an unstructured charged substrate. This approach utilizes the millimeter-ranged fluid flow on the bottom glass substrate induced by an ion exchange resin (IEX) fixed on top of the closed sample cell. This fluid flow increases with decreasing height of the sample cell and increasing radius R of the IEX. For a single inverted pump, millimeter sized monolayer single crystals of hexagonal close packing can be obtained. For two closely spaced (D ~ 4R) pumps, the formed crystals have a predefined orientation along the line connecting the tw…

Materials sciencebusiness.industryClose-packing of equal spheresFOS: Physical sciences02 engineering and technologyGeneral ChemistrySubstrate (electronics)RadiusCondensed Matter - Soft Condensed MatterColloidal crystal010402 general chemistry021001 nanoscience & nanotechnologyCondensed Matter Physics01 natural sciences0104 chemical sciencesMonolayerFluid dynamicsSoft Condensed Matter (cond-mat.soft)OptoelectronicsMillimeter0210 nano-technologybusinessIon-exchange resinSoft Matter
researchProduct

Advances in Microwave and Submillimeter-Wave Dielectric Spectroscopic Techniques and their Applications

2007

Measurement methodOpticsLiquid stateSpectrometerChemistrybusiness.industryDielectric lossDielectricbusinessRefractive indexMicrowaveSubmillimeter wave
researchProduct

Dust Production and Particle Acceleration in Supernova 1987A Revealed with ALMA

2013

Supernova (SN) explosions are crucial engines driving the evolution of galaxies by shock heating gas, increasing the metallicity, creating dust, and accelerating energetic particles. In 2012 we used the Atacama Large Millimeter/Submillimeter Array to observe SN 1987A, one of the best-observed supernovae since the invention of the telescope. We present spatially resolved images at 450um, 870um, 1.4mm, and 2.8mm, an important transition wavelength range. Longer wavelength emission is dominated by synchrotron radiation from shock-accelerated particles, shorter wavelengths by emission from the largest mass of dust measured in a supernova remnant (>0.2Msun). For the first time we show unambig…

MetallicityAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSynchrotron radiationAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSubmillimeter ArrayEARLY UNIVERSEindividual (1987A) [supernovae]Magellanic CloudsAstrophysics::Solar and Stellar AstrophysicsEjectaSupernova remnantSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsQBHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsISM [galaxies]supernova remnants [ISM]Astronomy and AstrophysicsOPTICAL-PROPERTIESHUBBLE-SPACE-TELESCOPEAstrophysics - Astrophysics of GalaxiesEVOLUTIONGalaxyParticle accelerationEJECTASupernovaPhysics and AstronomyAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)REVERSE SHOCKREMNANTAstrophysics::Earth and Planetary AstrophysicsEMISSIONAstrophysics - High Energy Astrophysical PhenomenaMASSIVE STARSSN 1987A
researchProduct

Spectral and morphological analysis of the remnant of Supernova 1987A with ALMA and ATCA

2014

We present a comprehensive spectral and morphological analysis of the remnant of Supernova (SN) 1987A with the Australia Telescope Compact Array (ATCA) and the Atacama Large Millimeter/submillimeter Array (ALMA). The non-thermal and thermal components of the radio emission are investigated in images from 94 to 672 GHz ($\lambda$ 3.2 mm to 450 $\mu$m), with the assistance of a high-resolution 44 GHz synchrotron template from the ATCA, and a dust template from ALMA observations at 672 GHz. An analysis of the emission distribution over the equatorial ring in images from 44 to 345 GHz highlights a gradual decrease of the east-to-west asymmetry ratio with frequency. We attribute this to the shor…

PARTICLE-ACCELERATIONAstrophysics::High Energy Astrophysical PhenomenaLIGHT-CURVEAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsPulsar wind nebulaSubmillimeter ArrayGALACTIC RADIO EMISSIONlaw.inventionneutron [stars]Far infraredPulsarlawQCAstrophysics::Galaxy AstrophysicsQBPhysicsSN-1987ANEUTRINO BURSTsupernova remnants [ISM]RAY-EMISSIONMAGNETIC-FIELDAstronomy and AstrophysicsPULSARnon-thermal [radiation mechanisms]SynchrotronEVOLUTIONSupernovaPhysics and Astronomyindividual (SN 1987A) [supernovae]Space and Planetary Sciencethermal [radiation mechanisms]Spectral energy distributiongeneral [radio continuum]MillimeterAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaSN 1987A
researchProduct

Permittivity Measurements of Lossy Liquids at Millimeter-Wave Frequencies

1983

A measurement system is described which allows the determination of the complex permittivity of high-loss liquids at millimeter waves. Basically, the setup consists of a waveguide interferometer whose unknown arm embodies a liquid holder irradiated by an open-ended rectangular waveguide. The sample thickness is varied by means of a piston driven by a micrometer screw. The bridge output then is read as a function of the liquid thickness. Best fitting between experimental and computed data through a suitable model of the system enables the permittivity to be determined. The system can operate, with high sensitivity, over the whole frequency range of the dominant mode propagating in the wavegu…

PermittivityRadiationMaterials sciencebusiness.industrySystem of measurementRelative permittivityCondensed Matter PhysicsWaveguide (optics)law.inventionInterferometryOpticslawExtremely high frequencyMicrometerMillimeterElectrical and Electronic EngineeringbusinessIEEE Transactions on Microwave Theory and Techniques
researchProduct

PRECISE LABORATORY MEASUREMENTS OF TRANS-DCOOH AND TRANS-HCOOD FOR ASTROPHYSICAL OBSERVATIONS

2011

The rotational spectra of the mono-deuterated isotopologues of trans-formic acid, trans-DCOOH and trans-HCOOD, were investigated. In the millimeter- and submillimeter-wave frequency regions the Lamb-dip technique was exploited to obtain sub-Doppler resolution and to resolve the hyperfine structure due to the deuterium and hydrogen nuclei, thus enabling the accurate determination of the corresponding hyperfine constants. The experimental determination was supported by high-level quantum-chemical calculations at the coupled-cluster level of theory using large atomic-orbital basis sets. The Lamb-dip measurements were also supplemented by THz Doppler- limited measurements in order to extend the…

PhysicsHydrogenTerahertz radiationResolution (electron density)LAMB-DIP TECHNIQUEchemistry.chemical_elementAstronomy and AstrophysicsISM: moleculeHYPERFINE STRUCTURESpectral linechemistryDeuteriumrotational spectroscopySpace and Planetary ScienceMillimeterIsotopologuePhysics::Atomic PhysicsAtomic physicsQUANTUM-CHEMICAL CALCULATIONSHyperfine structureThe Astrophysical Journal Supplement Series
researchProduct

A Method to Measure the Characteristics of Biological Materials at Millimeter Waves

1976

A new method of biological sample characterization at millimeter waves has been studied to verify and extend Webb's experimental results. This method, based on interferometric measurements, is suitable to obtain an absorption spectrum of a living bacterial sediment with a high sensitivity. It has been applied in the frequency range 66-73 GHz. Some experimental results are reported.

PhysicsInterferometryOpticsAbsorption spectroscopybusiness.industryAttenuationAstrophysics::Instrumentation and Methods for AstrophysicsMeasure (physics)Range (statistics)MillimeterSensitivity (control systems)businessCharacterization (materials science)6th European Microwave Conference, 1976
researchProduct

THE HYPERFINE STRUCTURE of the ROTATIONAL SPECTRUM of HDO and ITS EXTENSION to the THz REGION: ACCURATE REST FREQUENCIES and SPECTROSCOPIC PARAMETERS…

2015

The rotational spectrum of the mono-deuterated isotopologue of water, HD16O, has been investigated in the millimeter- and submillimeter-wave frequency regions, up to 1.6 THz. The Lamb-dip technique has been exploited to obtain sub-Doppler resolution and to resolve the hyperfine (hf) structure due to the deuterium and hydrogen nuclei, thus enabling the accurate determination of the corresponding hf parameters. Their experimental determination has been supported by high-level quantum-chemical calculations. The Lamb-dip measurements have been supplemented by Doppler-limited measurements (weak high-J and high-frequency transitions) in order to extend the predictive capability of the available s…

PhysicsNuclear and High Energy PhysicsHydrogenmolecular dataTerahertz radiationResolution (electron density)chemistry.chemical_elementAstronomy and AstrophysicsISM: moleculechemistry.chemical_compoundHydrofluoric acidDeuteriumchemistrySpace and Planetary ScienceMillimeterIsotopologuePhysics::Atomic PhysicsAtomic physicsHyperfine structuremethods: data analysiAstrophysics::Galaxy Astrophysicsline: identification
researchProduct