Search results for " observations"

showing 10 items of 100 documents

G-CLASS: geosynchronous radar for water cycle science – orbit selection and system design

2019

The mission geosynchronous – continental land atmosphere sensing system (G-CLASS) is designed to study thediurnal water cycle, using geosynchronous radar. Although the water cycle is vital to human society, processes on timescalesless than a day are very poorly observed from space. G-CLASS, using C-band geosynchronous radar, could transform this. Itsscience objectives address intense storms and high resolution weather prediction, and significant diurnal processes such assnow melt and soil moisture change, with societal impacts including agriculture, water resource management, flooding, andlandslides. Secondary objectives relate to ground motion observations for earthquake, volcano, and subs…

geosynchronous protected regionscience objectives010504 meteorology & atmospheric sciencesgeosynchronous satellite0211 other engineering and technologiesc-band geosynchronous radar02 engineering and technologycomputer.software_genre01 natural scienceslaw.inventionsubsidence monitoringRadar meteorologystandard small geosynchronous satellitelawground motion observationsRadarWater cycleweather forecastingagriculturelandslidesAtmospheric techniquesRadar remote sensing[SDE.IE]Environmental Sciences/Environmental EngineeringRadarmeteorologiaGeneral EngineeringGeosynchronous orbitintense stormsGeosynchronous SARHydrological techniquessocietal impactswater cycle sciencegeosynchronous orbitflexible imaging modessize 20.0 mhigh temporal resolution imaging:Enginyeria de la telecomunicació::Radiocomunicació i exploració electromagnètica::Radar [Àrees temàtiques de la UPC]Weather forecastingEnergy Engineering and Power Technologyatmospheric techniques[SDU.STU.ME]Sciences of the Universe [physics]/Earth Sciences/MeteorologyLatitudeWeather forecastinggeosynchronous radar; water cyclefloodingsoil moisture changewater resource managementcontinental land atmosphere sensing system[SDU.STU.HY]Sciences of the Universe [physics]/Earth Sciences/HydrologyMeteorological radar021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensingStormhuman societyorbit selectionmission geosynchronousmeteorological radarsignificant diurnal processesvolcano13. Climate actionlcsh:TA1-2040SnowmeltearthquakeEnvironmental scienceSystems designsnow melthydrological techniquesdiurnal water cyclehigh resolution weather predictionesa earth explorerlcsh:Engineering (General). Civil engineering (General)computerSoftwareg-class system design
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SPI/INTEGRAL in-flight performance

2003

The SPI instrument has been launched on-board the INTEGRAL observatory on October 17, 2002. SPI is a spectrometer devoted to the sky observation in the 20 keV-8 MeV energy range using 19 germanium detectors. The performance of the cryogenic system is nominal and allows to cool the 19 kg of germanium down to 85 K with a comfortable margin. The energy resolution of the whole camera is 2.5 keV at 1.1 MeV. This resolution degrades with time due to particle irradiation in space. We show that the annealing process allows the recovery of the initial performance. The anticoincidence shield works as expected, with a low threshold at 75 keV, reducing the GeD background by a factor of 20. The digital …

media_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical scienceschemistry.chemical_elementGermaniumAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsGamma-rayObservatoryinstrument observations [gamma-ray]Observationsmedia_commonPhysicsSpectrometerINTEGRAL/SPIAstrophysics (astro-ph)DetectorAstronomy and AstrophysicsInstrumentDead timeGalactic planeINTEGRAL/SPI [space telescope]:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Gamma-ray ; Instrument ; Observations ; Space telescope ; INTEGRAL/SPIComputational physicsCrab NebulachemistrySpace and Planetary ScienceSkySpace telescopeUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Lyman break and ultraviolet-selected galaxies at z ̃ 1-I. Stellar populations from the ALHAMBRA survey

2013

We take advantage of the exceptional photometric coverage provided by the combination of GALEX data in the ultraviolet (UV) and the ALHAMBRA survey in the optical and near-infrared to analyse the physical properties of a sample of 1225 GALEX-selected Lyman break galaxies (LBGs) at 0.8 ≲ z ≲ 1.2 that are located in the COSMOS field. This is the largest sample of LBGs studied in this redshift range to date. According to a spectral energy distribution (SED) fitting with synthetic stellar population templates, we find that LBGs at z ̃ 1 are mostly young galaxies with a median age of 341 Myr and have intermediate dust attenuation, (Es(B - V)) ̃ 0.20. Owing to the selection criterion, LBGs at z ̃…

media_common.quotation_subjectLibrary scienceAstrophysics::Cosmology and Extragalactic Astrophysicsstar formation [Galaxies]high-redshift [Galaxies]ExcellenceAstrophysics::Solar and Stellar Astrophysicsobservations [Cosmology]Astrophysics::Galaxy Astrophysicsmedia_commonPhysicsGalaxies: star formationphotometry [Galaxies]Cosmology: observationsGalaxies: high-redshiftAstronomyGalaxies: evolutionAstronomy and AstrophysicsGalaxies: photometryevolution [Galaxies]Galaxygalaxies [Ultraviolet]Space and Planetary ScienceUltraviolet: galaxiesAstrophysics::Earth and Planetary AstrophysicsAdministration (government)
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ADAMTS13 and VWF activities guide individualized caplacizumab treatment in patients with aTTP

2020

Abstract Introduction of the nanobody caplacizumab was shown to be effective in the treatment of acquired thrombotic thrombocytopenic purpura (aTTP) in the acute setting. The official recommendations include plasma exchange (PEX), immunosuppression, and the use of caplacizumab for a minimum of 30 days after stopping daily PEX. This study was a retrospective, observational analysis of the use of caplacizumab in 60 patients from 29 medical centers in Germany. Immunosuppressive treatment led to a rapid normalization of ADAMTS13 activities (calculated median, 21 days). In 35 of 60 patients, ADAMTS13 activities started to normalize before day 30 after PEX; in 11 of 60 patients, the treatment was…

medicine.medical_specialtyClinical Trials and Observationsmedicine.medical_treatmentMedizinADAMTS13 Protein030204 cardiovascular system & hematology03 medical and health sciences0302 clinical medicineVon Willebrand factorFibrinolytic AgentsInternal medicinehemic and lymphatic diseasesvon Willebrand FactormedicineHumansIn patientRetrospective StudiesAcquired Thrombotic Thrombocytopenic PurpurabiologyPurpura Thrombotic Thrombocytopenicbusiness.industryImmunosuppressionRetrospective cohort studyHematologySingle-Domain AntibodiesADAMTS13Cardiovascular and Metabolic Diseases030220 oncology & carcinogenesisbiology.proteinBiomarker (medicine)Caplacizumabbusiness
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Never say never again: A bone graft infection due to a hornet sting, thirty-nine years after cranioplasty

2017

Background: Cranioplasty (CP) is a widespread surgical procedure aimed to restore skull integrity and physiological cerebral hemodynamics, to improve neurological functions and to protect the underlying brain after a life-saving decompressive craniectomy (DC). Nevertheless, CP is still burdened by surgical complications, among which early or late graft infections are the most common outcome-threatening ones. Case Description: We report the case of 48-year-old man admitted to our neurosurgical unit because of a painful right frontal swelling and 1-week purulent discharge from a cutaneous fistula. He had been undergone frontal CP because of severe traumatic brain injury (TBI) when he was 9-ye…

medicine.medical_specialtyTraumatic brain injurymedicine.medical_treatmentCranioplastylate infection management03 medical and health sciences0302 clinical medicinemedicinerisk factorsMedical historyDebridementSettore MED/27 - Neurochirurgiabusiness.industryUnique Case Observations: Case Reportmedicine.diseasesurgical complicationsCranioplastySurgerySkullStingmedicine.anatomical_structure030220 oncology & carcinogenesisVancomycinSurgeryDecompressive craniectomyRisk factorNeurology (clinical)business030217 neurology & neurosurgerymedicine.drugSurgical Neurology International
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GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

2017

On August 17, 2017 at 12-41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per 8.0×104 years. We infer the component masses of the binary to be between 0.86 and 2.26 M, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17-1.60 M, with the total mass of the system 2.74-0.01+0.04M. The source was localized within a sky region of 28 deg2 (90% probabili…

neutron star: binary[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]X-ray binaryADVANCED LIGOAstrophysicsKilonovagravitational waves; LIGO; binary neutron star inspiralspin01 natural sciencesLIGOGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Electromagnetic observationsGravitational-wave signals3100 General Physics and AstronomyPoint MassesAstrophysics - High Energy Astrophysical PhenomenaBlack-Hole MergersBinary neutron starsBlack HolesX-ray bursterCoalescing BinariesAstrophysics::High Energy Astrophysical Phenomena10192 Physics InstituteGeneral Relativity and Quantum Cosmology (gr-qc)Gravity wavesGravitational wavesNeutron starsPhysics and Astronomy (all)ddc:530Electromagnetic spectraNeutrons010308 nuclear & particles physicsVirgoGamma raysAstronomyRCUKVIRGOelectromagneticgravitational radiation: emissionStellar black holeGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Compact Binariesbinary: masscosmological modelAstronomyGeneral Physics and AstronomyAstrophysicsneutron starsGamma ray burstsGeneral Relativity and Quantum CosmologyGravitational wave detectorsUniverseDENSE MATTER010303 astronomy & astrophysicsastro-ph.HEPhysicsSignal to noise ratioSettore FIS/01 - Fisica SperimentaleGravitational effectsFalse alarm rateEQUATION-OF-STATEMergers and acquisitionsgravitational waves[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]530 PhysicsMERGERSGeneral Relativity and Quantum Cosmology; General Relativity and Quantum Cosmology; astro-ph.HEFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstgravitational radiation: direct detectionMerging[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]GAMMA-RAY BURSTLIGO (Observatory)binary: coalescenceGravitational waves neutron stars gamma-ray burst LIGO Virgo0103 physical sciencesGW151226MASSESSTFCAstrophysics::Galaxy AstrophysicsPhysiqueGravitational wavegravitational radiationPULSARgravitational radiation detectorNeutron starPhysics and AstronomygravitationRADIATIONDewey Decimal Classification::500 | Naturwissenschaften::530 | Physikbinary neutron star inspiralSignal detectionPHYS REV LETT PHYSICAL REVIEW LETTERS
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Lärarstudenter som aktörer i interaktiv observation och handledning: En studie om digitala redskap i VFU-handledning på övningsskolor

2018

Source at https://doi.org/10.23865/hu.v8.1078. Licensed CC BY-NC-ND 4.0. Syftet med denna artikel är att bidra med kunskap om hur digitala redskap kan påverka lärarstudenters deltagande i handledningsprocessen. Trots att lärarstudenter och handledare ofta befinner sig i digitala klassrumsmiljöer används digitala redskap endast i begränsad omfattning under handledningsprocessen. Med utgångspunkt i Wengers teori om lärande i en praktikgemenskap har lärarstudenter och handledare arbetat med stöd av digitala observationsunderlag. Processen har studerats på fyra övningsskolor. Information om studenternas erfarenheter av handledningen har samlats in via enkäter och fokusgruppsamtal. Resultatet vi…

responsövningsskolordigitala observationsunderlagPedagogymultimodalPedagogikAktörGeneral MedicineVDP::Samfunnsvitenskap: 200::Pedagogiske fag: 280multimodal responsVFU-handledningPolitical scienceReligious studiesVDP::Social science: 200::Education: 280övningskolor
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A Decade of GRB Follow-Up by BOOTES in Spain (2003–2013)

2016

This article covers ten years of GRB follow-ups by the Spanish BOOTES stations: 71 follow-ups providing 23 detections. Follow-ups by BOOTES-1B from 2005 to 2008 were given in a previous article and are here reviewed and updated, and additional detection data points are included as the former article merely stated their existence. The all-sky cameras CASSANDRA have not yet detected any GRB optical afterglows, but limits are reported where available.

spectroscopyArticle Subjectlcsh:Astronomy100418AFOS: Physical sciencesgamma-ray burst02 engineering and technology01 natural scienceslcsh:QB1-991emission0103 physical sciences0202 electrical engineering electronic engineering information engineeringpanchromatic observations010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsshooterenergy injectionAstronomyAstronomy and AstrophysicsBOOTEShost-galaxySpace and Planetary Science28 February 1997020201 artificial intelligence & image processingAstrophysics - High Energy Astrophysical PhenomenaafterglowGamma-ray burstAdvances in Astronomy
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THE ALHAMBRA SURVEY: EVOLUTION OF GALAXY SPECTRAL SEGREGATION

2016

arXiv:1601.03668v1

statistical [Methods]Cosmology and Nongalactic Astrophysics (astro-ph.CO)Large-scale structure of universeFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesMethods statisticalGalaxies: distances and redshiftsMethods: data analysis0103 physical sciencesdistances and redshifts [Galaxies]observations [Cosmology]data analysis [Methods]010303 astronomy & astrophysicsMethods: statisticalAstrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSPhysics[PHYS]Physics [physics]010308 nuclear & particles physicsCosmology: observationsFísicaAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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Foneettisten piirteiden ja vieraan aksentin yhteydestä suomen kielessä

2018

Tapaustutkimuksemme tarkoituksena on selvittaa muutaman foneettisen piirteen ja vieraan aksentin yhteytta suomen kielessa. Analysoimme ilmiota kuulijatestilla, akustisin mittauksin ja kirjoittajien tekemin kuulonvaraisin havainnoin. Puhujina ovat varsin edistyneet suomenpuhujat, jotka puhuvat suomea toisena tai vieraana kielenaan. Tuloksemme antavat uutta tietoa vieraan aksentin ja foneettisten piirteiden yhteyksista seka tarjoavat avauksia jatkotutkimukselle. Tutkitut piirteet ovat pitkien vokaalien etaisyydet, aannekestot, perustaajuuden (f0) vaihteluvali, f0:n vaihtelun jyrkkyys ja keskihajonta seka artikulaationopeus. Tuloksemme osoittavat, etta kaikilla piirteilla on yhteys vieraaseen …

toinen kieliLinguistics and Languageoppiminenmedia_common.quotation_subjectphoneticshavaintoL2-ääntäminenlcsh:Finnic. Baltic-Finniclcsh:PH91-98.5ta6121segmentsääntäminenperceptionPronunciationääntämisen oppiminenL2 pronunciationLanguage and Linguisticssecond languageprosodyAuditory observationspronunciation learningVowelPerceptionStress (linguistics)segmentitfonetiikkapronunciationProsodymedia_commonprosodiikkaArticulation (music)learningL2Linguisticsprosodiahavainnotaccent (linguistics)SyllablePsychologyaksenttiLähivõrdlusi. Lähivertailuja
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