Search results for "GALA"

showing 10 items of 3348 documents

Study of uniformity of plasmas produced in a wall-stabilized arc

2003

In this contribution the plasma of an arc discharge in a mixture of helium and argon is studied. The gas mixture is introduced uniformly along the arc column between each of the stabilizing plates. From the measured lateral distribution of radiation (HeI, HI, ArI, ArII, NI, FI line intensity and width measurements), after Abel inversion, the radial temperature distributions were obtained at various positions of the arc column. Beside the expected radial temperature gradients, a distinct temperature gradient along the arc column was found.

ArgonMaterials sciencechemistry.chemical_elementPlasmaRadiationCondensed Matter PhysicsElectric arcTemperature gradientPlasma arc weldingchemistryPlasma diagnosticsAtomic physicsAstrophysics::Galaxy AstrophysicsHeliumContributions to Plasma Physics
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Preamble Transmission Prediction for mMTC Bursty Traffic : A Machine Learning based Approach

2020

The evolution of Internet of things (IoT) towards massive IoT in recent years has stimulated a surge of traffic volume among which a huge amount of traffic is generated in the form of massive machine type communications. Consequently, existing network infrastructure is facing challenges when handling rapidly growing traffic load, especially under bursty traffic conditions which may more often lead to congestion. By proactively predicting the occurrence of congestion, we can implement necessary means and conceivably avoid congestion. In this paper, we propose a machine learning (ML) based model for predicting successful preamble transmissions at a base station and subsequently forecasting th…

Artificial neural networkComputer sciencebusiness.industryComputerSystemsOrganization_COMPUTER-COMMUNICATIONNETWORKS05 social sciences050801 communication & media studies020206 networking & telecommunicationsComputingMilieux_LEGALASPECTSOFCOMPUTING02 engineering and technologyMachine learningcomputer.software_genrePreambleBase station0508 media and communicationsRecurrent neural networkTransmission (telecommunications)Traffic volume0202 electrical engineering electronic engineering information engineeringArtificial intelligencebusinesscomputerVDP::Teknologi: 500::Informasjons- og kommunikasjonsteknologi: 550
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Enzyme replacement therapy for mucopolysaccharidosis VI: evaluation of long-term pulmonary function in patients treated with recombinant human N-acet…

2010

Pulmonary function is impaired in untreated mucopolysaccharidosis type VI (MPS VI). Pulmonary function was studied in patients during long-term enzyme replacement therapy (ERT) with recombinant human arylsulfatase B (rhASB; rhN-acetylgalactosamine 4-sulfatase). Pulmonary function tests prior to and for up to 240 weeks of weekly infusions of rhASB at 1 mg/kg were completed in 56 patients during Phase 1/2, Phase 2, Phase 3 and Phase 3 Extension trials of rhASB and the Survey Study. Forced vital capacity (FVC), forced expiratory volume in 1 s (FEV1) and, in a subset of patients, maximum voluntary ventilation (MVV), were analyzed as absolute volume in liters. FEV1 and FVC showed little change f…

Arylsulfatase BAdultmedicine.medical_specialtyVital capacityAdolescentMucopolysaccharidoses (MPS)N-Acetylgalactosamine-4-SulfataseMucopolysaccharidosis type VIClinical SciencesUrologyPulmonary function testingPlacebos03 medical and health sciencesFEV1/FVC ratio0302 clinical medicineRare DiseasesDouble-Blind MethodClinical ResearchmedicineGeneticsHumansGenetics(clinical)Longitudinal StudiesChildPreschoolLungGenetics (clinical)Genetics & Heredity0303 health sciencesLungMucopolysaccharidosis VIbusiness.industry030305 genetics & heredityEvaluation of treatments and therapeutic interventionsMucopolysaccharidosis VIEnzyme replacement therapyRecombinant Proteins3. Good healthSurgeryRespiratory Function Testsmedicine.anatomical_structureCross-Sectional StudiesResearch DesignChild Preschool6.1 PharmaceuticalsOriginal Articlebusiness030217 neurology & neurosurgery
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Zvaigžņotā Debess: 2009, Rudens (205)

2009

Contents: I.Daube. Jānis Ikaunieks ; A.Balklavs. Mountains on the Venus ; TASS and “Pravda” materials. Soviet Automatic Stations “Venera-5” and “Venera-6” Reach Venus ; A.Alksnis. Gathering of Astronomers at the University ; A.Alksnis, M.Ābele, I.Eglītis, B.Rjabovs, K.Salmiņš, I.Pundure. Directions of Scientific Research of the UL Institute of Astronomy Assessed ; D.Docenko. Meteorite Fallen in Sudan Recovered ; A.Alksnis. How Asteroids Will Disturb Observation with Extremely Large Telescopes ; M.Gills. Daily in Network with Astronomy ; I.Pundure. Arturs Balklavs and Astronomy of Latvia (continued) ; M.Sudārs. IXV – Step towards Reusable Space Vehicles ; V.Kalniņš. Hyperdrive and Heim’s Qua…

Asteroīdi un novērošana ar lielajiem teleskopiemAlfrēds Štrauss – dzīvesstāsta meklējumiAndromedas galaktika M31Vienošanās starp Latvijas valdību un Eiropas Kosmosa aģentūruMeteorīts Almahatta SittaArturs Balklavs “Latvijas astronomija pēc Trešās atmodas”IXV – Eiropas daudzkārt izmantojams kosmosa kuģisLatvijas atklātā matemātikas olimpiādeRainis – kosmosa dzejnieksJānis IkaunieksAstronomu salidojums UniversitātēSiltumnīcas uz MarsaAstronomiskās parādības - 2009Latvijas astronomija - vēstureStarptautiskais Astronomijas gads 2009 – plakātsAstronomijas institūts - zinātniskā pētniecībaJaunākie žurnāli “Zvaigžņotās Debess” bibliotēkāEduards Riekstiņš – 90LU fizikas docents Ludvigs Jansons – 100Hiperdzinējs – Heima kvantu teorijaAgreement between the Government of the Republic of Latvia and the European Space AgencyAstronomija - tīmeklīRīgas Politehnikuma Astronomijas kabinets – 130Latvijas atklātā skolēnu astronomijas olimpiāde
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Oxygen depletion in dense molecular clouds: a clue to a low O2 abundance?

2011

Context: Dark cloud chemical models usually predict large amounts of O2, often above observational limits. Aims: We investigate the reason for this discrepancy from a theoretical point of view, inspired by the studies of Jenkins and Whittet on oxygen depletion. Methods: We use the gas-grain code Nautilus with an up-to-date gas-phase network to study the sensitivity of the molecular oxygen abundance to the oxygen elemental abundance. We use the rate coefficient for the reaction O + OH at 10 K recommended by the KIDA (KInetic Database for Astrochemistry) experts. Results: The updates of rate coefficients and branching ratios of the reactions of our gas-phase chemical network, especially N + C…

AstrochemistryChemical models[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Analytical chemistrychemistry.chemical_elementFOS: Physical sciencesAstrophysicsAstrophysicsKinetic energy01 natural sciencesOxygen[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesSolar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysics010304 chemical physics[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Molecular cloudAstronomy and Astrophysicsastrochemistry; ISM; abundances; ISM; molecules; ISM; individual objects; L134N; ISM; individual objects; TMC-1[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]NitrogenchemistryAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceMolecular oxygenChemical network
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The hyperfine structure in the rotational spectrum of CF+

2012

Context. CF+ has recently been detected in the Horsehead and Orion Bar photo-dissociation regions. The J=1-0 line in the Horsehead is double-peaked in contrast to other millimeter lines. The origin of this double-peak profile may be kinematic or spectroscopic. Aims. We investigate the effect of hyperfine interactions due to the fluorine nucleus in CF+ on the rotational transitions. Methods. We compute the fluorine spin rotation constant of CF+ using high-level quantum chemical methods and determine the relative positions and intensities of each hyperfine component. This information is used to fit the theoretical hyperfine components to the observed CF+ line profiles, thereby employing the h…

AstrochemistryFOS: Physical sciencesContext (language use)Astrophysics010402 general chemistryRotation01 natural sciencesISM: clouds0103 physical sciencesSpin (physics)010303 astronomy & astrophysicsHyperfine structureAstrophysics::Galaxy AstrophysicsLine (formation)PhysicsNebularadio lines: ISMastrochemistryAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesISM: molecules0104 chemical sciences[PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Space and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)ISM: individual objects: Horsehead nebula[SDU.ASTR.GA]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Atomic physicsBar (unit)
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A KInetic Database for Astrochemistry (KIDA)

2012

We present a novel chemical database for gas-phase astrochemistry. Named the KInetic Database for Astrochemistry (KIDA), this database consists of gas-phase reactions with rate coefficients and uncertainties that will be vetted to the greatest extent possible. Submissions of measured and calculated rate coefficients are welcome, and will be studied by experts before inclusion into the database. Besides providing kinetic information for the interstellar medium, KIDA is planned to contain such data for planetary atmospheres and for circumstellar envelopes. Each year, a subset of the reactions in the database (kida.uva) will be provided as a network for the simulation of the chemistry of dense…

Astrochemistry[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Interstellar cloudFOS: Physical sciencesAstrophysicsKinetic energycomputer.software_genreAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesmiscellaneous [astrochemistry; astronomical databases]010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysics010304 chemical physicsDatabaseKinetic informationAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesInterstellar mediumSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)computerChemical databaseGalaxy Astrophysics
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Minidisk dynamics in accreting, spinning black hole binaries: Simulations in full general relativity

2021

We perform magnetohydrodynamic simulations of accreting, equal-mass binary black holes in full general relativity focusing on the impact of black hole spin on the dynamical formation and evolution of minidisks. We find that during the late inspiral the sizes of minidisks are primarily determined by the interplay between the tidal field and the effective innermost stable orbit around each black hole. Our calculations support that a minidisk forms when the Hill sphere around each black hole is significantly larger than the black hole's effective innermost stable orbit. As the binary inspirals, the radius of the Hill sphere decreases, and minidisk sconsequently shrink in size. As a result, ele…

Astrofísica010504 meteorology & atmospheric sciencesGeneral relativityastro-ph.GAgr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyLuminosityGravitationGeneral Relativity and Quantum CosmologyBinary black hole0103 physical sciences010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Accretion (meteorology)Astronomy and AstrophysicsMass ratioAstrophysics - Astrophysics of Galaxies3. Good healthBlack holeSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Hill sphereAstronomiaAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Astrophysics with the Laser Interferometer Space Antenna

2023

Full list of authors: Amaro-Seoane, Pau; Andrews, Jeff; Sedda, Manuel Arca; Askar, Abbas.; Baghi, Quentin; Balasov, Razvan; Bartos, Imre; Bavera, Simone S.; Bellovary, Jillian; Berry, Christopher P. L.; Berti, Emanuele; Bianchi, Stefano; Blecha, Laura; Blondin, Stephane; Bogdanovic, Tamara; Boissier, Samuel; Bonetti, Matteo; Bonoli, Silvia; Bortolas, Elisa; Breivik, Katelyn; Capelo, Pedro R.; Caramete, Laurentiu; Cattorini, Federico; Charisi, Maria; Chaty, Sylvain; Chen, Xian; Chruslinska, Martyna; Chua, Alvin J. K.; Church, Ross; Colpi, Monica; D'Orazio, Daniel; Danielski, Camilla; Davies, Melvyn B.; Dayal, Pratika; De Rosa, Alessandra; Derdzinski, Andrea; Destounis, Kyriakos; Dotti, Massi…

AstrofísicaACTIVE GALACTIC NUCLEICosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)Black holeAstronomyStellar remnantFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)TIDAL DISRUPTION EVENTSGeneral Relativity and Quantum CosmologyGravitational wavesMOCCA-SURVEY DATABASESettore FIS/05 - Astronomia e AstrofisicaStellar remnantsSoftware ScienceMulti-messengerGRAVITATIONAL-WAVE SOURCESInstrumentation and Methods for Astrophysics (astro-ph.IM)Extreme mass ratio in-spiralsSolar and Stellar Astrophysics (astro-ph.SR)High Energy Astrophysical Phenomena (astro-ph.HE)Black holes; Extreme mass ratio in-spirals; Gravitational waves; Multi-messenger; Stellar remnantsBlack holesData ScienceAstrophysics::Instrumentation and Methods for AstrophysicsExtreme mass ratio in-spiralAM-CVN STARSAstrophysics - Astrophysics of GalaxiesWHITE-DWARF BINARIESDOUBLE NEUTRON-STARSAstrophysics - Solar and Stellar Astrophysics[SDU]Sciences of the Universe [physics]Astrophysics of Galaxies (astro-ph.GA)AstronomiaMASSIVE BLACK-HOLEAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsX-RAY BINARIESCOMMON-ENVELOPE EVOLUTIONGravitational waveAstrophysics - Cosmology and Nongalactic Astrophysics
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Absolute kinematics of radio-source components in the complete S5 polar cap sample: IV. Proper motions of the radio cores over a decade and spectral …

2016

We have carried out a high-precision astrometric analysis of two very-long-baseline-interferometry (VLBI) epochs of observation of the 13 extragalactic radio sources in the complete S5 polar cap sample. The VLBI epochs span a time baseline of ten years and enable us to achieve precisions in the proper motions of the source cores up to a few micro-arcseconds per year. The observations were performed at 14.4 GHz and 43.1 GHz, and enable us to estimate the frequency core-shifts in a subset of sources, for which the spectral-index distributions can be computed. We study the source-position stability by analysing the changes in the relative positions of fiducial source points (the jet cores) ove…

AstrofísicaActive galactic nucleusAstrometriaAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsKinematics01 natural sciencesStability (probability)Radio continuum: generalBinary black hole0103 physical sciencesVery-long-baseline interferometry010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsJet (fluid)general [Radio continuum]general [BL Lacertae objects]Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicsgeneral [Quasars]BL Lacertae objects: generalAstrometryAstrometryAstrophysics - Astrophysics of GalaxiesQuasars: generalGravitational lensSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Techniques: interferometricinterferometric [Techniques]Astrophysics - Instrumentation and Methods for Astrophysics
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