Search results for "brightness temperature"

showing 10 items of 54 documents

Imaging strong blazars with space VLBI

2020

Abstract The RadioAstron mission has obtained a series of detailed multi-frequency images of the brightest blazars of the radio sky concentrated in three key science programs. We present here results of the program on powerful jets in blazars. In the first two years of the mission, observations of compact relativistic jets in 0836+710, 3C 345, 3C 273, and 4C +69.21 were made at λ λ  18, 6, and 1.3 cm. The resulting images have revealed compact emitting regions with brightness temperature in excess of 10 13  K and a complex jet structure that can be explained by plasma instability developing in a relativistic outflow. We present here some highlights of these space-VLBI observations, designed…

PhysicsAtmospheric ScienceJet (fluid)Active galactic nucleus010504 meteorology & atmospheric sciencesmedia_common.quotation_subjectAerospace EngineeringAstronomy and AstrophysicsAstrophysicsSpace (mathematics)01 natural sciencesGeophysicsAstrophysical jetSpace and Planetary ScienceSkyBrightness temperature0103 physical sciencesVery-long-baseline interferometryGeneral Earth and Planetary SciencesBlazar010303 astronomy & astrophysics0105 earth and related environmental sciencesmedia_commonAdvances in Space Research
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Probing the innermost regions of AGN jets and their magnetic fields with RadioAstron II. Observations of 3C 273 at minimum activity

2017

RadioAstron is a 10 m orbiting radio telescope mounted on the Spektr-R satellite, launched in 2011, performing Space Very Long Baseline Interferometry (SVLBI) observations supported by a global ground array of radio telescopes. With an apogee of about 350 000 km, it is offering for the first time the possibility to perform {\mu}as-resolution imaging in the cm-band. We present observations at 22 GHz of 3C 273, performed in 2014, designed to reach a maximum baseline of approximately nine Earth diameters. Reaching an angular resolution of 0.3 mas, we study a particularly low-activity state of the source, and estimate the nuclear region brightness temperature, comparing with the extreme one det…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)BrightnessActive galactic nucleus010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics - Astrophysics of Galaxies01 natural sciencesRadio telescopeSpace and Planetary ScienceBrightness temperatureAstrophysics of Galaxies (astro-ph.GA)0103 physical sciencesVery-long-baseline interferometryAstrophysics - High Energy Astrophysical PhenomenaBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesFermi Gamma-ray Space Telescope
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The limb-brightened jet of M87 down to 7 Schwarzschild radii scale

2018

M87 is one of the nearest radio galaxies with a prominent jet extending from sub-pc to kpc-scales. Because of its proximity and large mass of the central black hole, it is one of the best radio sources to study jet formation. We aim at studying the physical conditions near the jet base at projected separations from the BH of $\sim7-100$ Schwarzschild radii ($R_{\rm sch}$). Global mm-VLBI Array (GMVA) observations at 86 GHz ($\lambda=3.5\,$mm) provide an angular resolution of $\sim50\mu$as, which corresponds to a spatial resolution of only $7~R_{\rm sch}$ and reach the small spatial scale. We use five GMVA data sets of M87 obtained during 2004--2015 and present new high angular resolution VL…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Jet (fluid)010308 nuclear & particles physicsRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAstrophysics - Astrophysics of GalaxiesBlack holeSpace and Planetary ScienceBrightness temperatureAstrophysics of Galaxies (astro-ph.GA)0103 physical sciencesVery-long-baseline interferometryAngular resolutionAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]010303 astronomy & astrophysicsSchwarzschild radiusAstrophysics::Galaxy Astrophysics
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VLBI-selected sample of Compact Symmetric Object candidates and frequency-dependent position of hotspots

2011

The Compact Symmetric Objects (CSOs) are small (<1 kiloparsec) and powerful extragalactic radio sources showing emission on both sides of an active galactic nucleus and no signs of strong relativistic beaming. They may be young radio sources, progenitors of large FRII radio galaxies. We aim to study the statistical properties of CSOs by constructing and investigating a new large sample of CSO candidates on the basis of dual-frequency, parsec-scale morphology. For the candidate selection we utilized VLBI data for 4170 extragalactic objects obtained simultaneously at 2.3 and 8.6 GHz (S and X band) within the VLBA Calibrator Survey 1-6 and the Research and Development - VLBA projects. Prope…

PhysicsSpectral indexActive galactic nucleusCosmology and Nongalactic Astrophysics (astro-ph.CO)010504 meteorology & atmospheric sciencesRadio galaxyX bandFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics01 natural sciencesSpectral lineRelativistic beamingSpace and Planetary ScienceBrightness temperature0103 physical sciencesVery-long-baseline interferometry010303 astronomy & astrophysics0105 earth and related environmental sciencesAstrophysics - Cosmology and Nongalactic Astrophysics
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Long Term Radio Monitoring of SN 1993J

2007

We present our observations of the radio emission from supernova (SN) 1993J, in M 81 (NGC 3031), made with the VLA, from 90 to 0.7 cm, as well as numerous measurements from other telescopes. The combined data set constitutes probably the most detailed set of measurements ever established for any SN outside of the Local Group in any wavelength range. Only SN 1987A in the LMC has been the subject of such an intensive observational program. The radio emission evolves regularly in both time and frequency, and the usual interpretation in terms of shock interaction with a circumstellar medium (CSM) formed by a pre-SN stellar wind describes the observations rather well considering the complexity o…

PhysicsSpectral indexAstrophysics (astro-ph)FOS: Physical sciencesLocal GroupAstronomy and AstrophysicsAstrophysicsLight curveAstrophysicsShock (mechanics)SupernovaWavelengthSpace and Planetary ScienceBrightness temperatureExponential decay
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Near-Real-Time Estimation of Water Vapor Column From MSG-SEVIRI Thermal Infrared Bands: Implications for Land Surface Temperature Retrieval

2015

The Meteosat Second Generation-Spinning Enhanced Visible and Infrared Imager (MSG-SEVIRI) instrument provides observations of half the globe every 15 min, at low spatial resolution. These data are an invaluable tool to observe daily to yearly cycle of land surface temperature (LST), as well as for various early warning systems. However, advanced algorithms for LST estimation requires a previous estimation of the water vapor (WV) column above the observed pixel, for which no instantaneous retrieval methods are yet available, and therefore hinders their implementation in a near-real-time processing chain for MSG-SEVIRI data. This work analyzes three different formulations for such WV retrieva…

Propagation of uncertaintyPixelMeteorologyBrightness temperatureGeneral Earth and Planetary SciencesEnvironmental scienceAlgorithm designAtmospheric modelElectrical and Electronic EngineeringImage resolutionWater vaporRemote sensingData modelingIEEE Transactions on Geoscience and Remote Sensing
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The CoSMOS L-band experiment in Southeast Australia

2007

The CoSMOS (Campaign for validating the Operation of the Soil Moisture and Ocean Salinity mission) campaign was conducted during November of 2005 in the Goulburn River Catchment, in SE Australia. The main objective of CoSMOS was to obtain a series of L-band measurements from the air in order to validate the L-band emission model that will be used by the SMOS (Soil Moisture and Ocean Salinity) ground segment processor. In addition, the campaign was designed to investigate open questions including the Sun-glint effect over land, the application of polarimetric measurements over land, and to clarify the importance of dew and interception for soil moisture retrievals. This paper summarises the …

Radiometer010504 meteorology & atmospheric sciencesMeteorologyPASSIVE MICROWAVES[SDV]Life Sciences [q-bio]BRIGHTNESS TEMPERATURE0211 other engineering and technologiesL-BAND EMISSION MODEL02 engineering and technology15. Life on land01 natural sciencesSalinity13. Climate action[SDE]Environmental SciencesSOIL MOISTUREEnvironmental scienceRadiometryDewGround segmentInterceptionWater contentCosmosComputingMilieux_MISCELLANEOUS021101 geological & geomatics engineering0105 earth and related environmental sciences
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Ground measurements for the validation of land surface temperatures derived from AATSR and MODIS data

2005

Abstract An experimental site was set up in a large, flat and homogeneous area of rice crops for the validation of satellite derived land surface temperature (LST). Experimental campaigns were held in the summers of 2002–2004, when rice crops show full vegetation cover. LSTs were measured radiometrically along transects covering an area of 1 km 2 . A total number of four thermal radiometers were used, which were calibrated and inter-compared through the campaigns. Radiometric temperatures were corrected for emissivity effects using field emissivity and downwelling sky radiance measurements. A database of ground-based LSTs corresponding to morning, cloud-free overpasses of Envisat/Advanced A…

RadiometerBrightness temperatureRadianceEmissivitySoil ScienceEnvironmental scienceRadiometryGeologyAATSRModerate-resolution imaging spectroradiometerLand coverComputers in Earth SciencesRemote sensingRemote Sensing of Environment
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An Atmospheric Radiosounding Database for Generating Land Surface Temperature Algorithms

2008

A database of global, cloud-free, and atmospheric radiosounding profiles was compiled with the aim of simulating radiometric measurements from satellite-borne sensors in the thermal infrared. The objective of the simulated data is to generate split-window (SW) and dual-angle (DA) algorithms for the retrieval of land surface temperature (LST) from Terra/Moderate Resolution Imaging Spectroradiometer (MODIS) and Envisat/Advanced Along Track Scanning Radiometer (AATSR) data. The database contains 382 radiosounding profiles acquired over land, with nearly uniform distribution of precipitable water between 0.02 and 5.5 cm. Radiative transfer calculations were performed with the MODTRAN 4 code for…

RadiometerDatabaseMeteorologyMODTRANAATSRcomputer.software_genreBrightness temperatureRadianceNadirGeneral Earth and Planetary SciencesRadiometryEnvironmental scienceModerate-resolution imaging spectroradiometerElectrical and Electronic EngineeringAlgorithmcomputerRemote sensingIEEE Transactions on Geoscience and Remote Sensing
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ENVISAT/AATSR derived land surface temperature over a heterogeneous region

2007

Abstract In this paper a method for evaluating land surface temperature (LST) algorithms over heterogeneous areas is presented. The evaluation was made for a set of 12 algorithms derived by using the split-window (SW) and dual-angle (DA) techniques for estimating sea and land surface temperature (SST and LST) from Advanced Along-Track Scanning Radiometer (AATSR) data. A validation of the proposed algorithms was carried out over a heterogeneous region of Morocco in the framework of the WATERMED (WATer use Efficiency in natural vegetation and agricultural areas by Remote sensing in the MEDiterranean basin) project. AATSR data and in situ measurements over this heterogenous region were compare…

RadiometerPixelThematic MapperBrightness temperatureNadirSoil ScienceEnvironmental scienceGeologySpatial variabilityAATSRComputers in Earth SciencesImage resolutionRemote sensingRemote Sensing of Environment
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