Search results for "iNOS"

showing 10 items of 2075 documents

Las guerras del agua

1997

PaisajesVidaVidal-Beneyto JoséAgriculturaPenuriaCONFLICTOSConvivencia humanaConflictoAguaDesalinizaciónCivilizaciónGuerraBien comúnUrgencias MercantilizaciónPublicaciones: Obra periodística: Columnas y artículos de opiniónLunaDeberesGeopolíticaOriente PróximoHidropolíticaDerechosBotsuanaMartePalestinos
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Reconstruction of the internal structure of the pore system of a complex dinosaur eggshell (Megaloolithus siruguei)

2013

Despite the many reconstructions of fossil material that have recently appeared in the literature, dinosaur eggshells have never been reconstructed using computing techniques. Using the EMAC 3-D modelling methodology, we reconstruct a section of the Late Cretaceous Megaloolithus siruguei eggshell, which has a particularly complex pore system, exhibiting an intricate network of vertical, oblique, and horizontal pores.

PaleontologySection (archaeology)PaleontologyMineralogyPore systemEggshellBiologyQE701-760CretaceousPaleontologíadinosaur eggshell 3-d reconstruction palaeoclimate
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Ordovician echinoderms from the Tabas and Damghan regions, Iran: palaeobiogeographical implications

2005

Abstract Two echinoderm assemblages are described in the Middle Ordovician of Iran (Darriwilian). The Simeh Kuh section (Damghan area, eastern Alborz range) has yielded a rich and diverse blastozoan fauna consisting of fistuliporite (Echinosphaerites, Heliocrinites) and dichoporite rhombiferans (cheirocrinids indet., hemicosmitids indet.), as well as aristocystitid (Sinocystis) and sphaeronitid diploporites (Glyptosphaerites, Tholocystis). Heliocrinites, cheirocrinids, hemicosmitids, Glyptosphaerites, and Tholocystis are reported for the first time in the Ordovician of Iran. A less diverse assemblage was collected in the Shirgesht section (Tabas area, Derenjal Mountains), and represents the…

PaleontologySouth chinaEchinosphaeritesEchinodermbiologyRange (biology)FaunaOrdovicianGeologyBalticabiology.organism_classificationGeologyTerraneBulletin de la Société Géologique de France
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Interactive effects of parasitism and predation on the behaviour of the amphipod Pallasea quadrispinosa

2006

Pallasea quadrispinosaPääjärvi (Hämeenlinna)springkatkatparasitismpredationEchinorhynchus borealisokakatkaPääjärvi
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Dinosauroid footprints of French Upper Triassic. Discrimination, interpretation and comparison

2005

Abstract Dinosauroid tracks are common in France. They are mainly tridactyl II–IV feet tracks, sometimes with those of hands. A lot of these latter Coelurosaurichnus grancieri Courel & Demathieu, 2000 was discovered by MG near the village of Payzac (Ardèche department) in beds belonging to the “Ensemble gréso-dolomitique gris” (= EGDG) (fig. 1. 2). They are dated Carnian from palynological data [Fauconnier et al., 1996]. C. grancieri are tracks of feet and hands respectively 10 cm and 2.5 cm long (fig. 1. 3–5, 7–21; tabl. I-1, tabl. II). From the trackways characters, it was inferred that trackmakers were long legged, bipedal-quadrupedal reptiles, 1–2 m long. New discoveries made by M…

PalynologyPaleontologyOsteologybiologyChirotheriumEubrontesDinosauromorphaGeologyCeratosauriabiology.organism_classificationIchnitesGeologySauropodaBulletin de la Société Géologique de France
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Eine einfache Methode des quantitativen Nachweises der Para-Aminosalicyls�ure im Harn

1951

Mitteilung eines einfachen quantitativen Nachweises der PAS im Urin bei Kranken, die mit diesem Medikament behandelt werden. Auf mit Ehrlich-Reagens prapariertem Filtrierpapier wird PAS-haltiger Urin aufgetropft. Der entstehende Farbniederschlag ist je nach PAS-Gehalt mehr oder weniger gelb bis braun-rot verfarbt. Diese Farbung wird mit selbst angefertigten Testfarbungen verglichen und der PAS-Gehalt in der ausgeschiedenen Urinmenge bestimmt.

Para-aminosalicylic acidChromatographyChemistryDrug DiscoveryMolecular MedicineGeneral MedicineUrineGenetics (clinical)Quantitative determinationKlinische Wochenschrift
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The energy spectrum of atmospheric neutrinos between 2 and 200 TeV with the AMANDA-II detector

2010

The muon and anti-muon neutrino energy spectrum is determined from 2000-2003 AMANDA telescope data using regularised unfolding. This is the first measurement of atmospheric neutrinos in the energy range 2 - 200 TeV. The result is compared to different atmospheric neutrino models and it is compatible with the atmospheric neutrinos from pion and kaon decays. No significant contribution from charm hadron decays or extraterrestrial neutrinos is detected. The capabilities to improve the measurement of the neutrino spectrum with the successor experiment IceCube are discussed.

Particle physicsAMANDA[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and Detectors[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Solar neutrinoAstrophysics::High Energy Astrophysical PhenomenaAMANDA; Atmospheric neutrinos; Cherenkov radiation; Neural net; Unfoldingneural netFOS: Physical sciencesAetiology screening and detection [ONCOL 5]01 natural sciences7. Clean energy[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciences010306 general physicsunfoldingPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Muon010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Cherenkov radiationHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsSolar neutrino problematmospheric neutrinosCosmic neutrino backgroundNeutrino detectorddc:540Measurements of neutrino speedHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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Search for Higgs bosons decaying to WW in e(+)e(-) stope collisions at LEP

2006

A search for Higgs bosons produced in association with a fermion pair, and decaying to WW, is performed with the data collected by the ALEPH detector at centre-of-mass energies ranging from 191 to 209 GeV. The data correspond to an integrated luminosity of 453.2 pb^-1. Thirteen exclusive selections are developed according to the different final state topologies. No statistically significant evidence for a Higgs boson decaying into a WW pair has been found. An upper limit is derived, as a function of the Higgs boson mass, on the product of the e+e- -> Hff cross section and the H -> WW branching ratio. The data on the search for H -> WW are combined with previously published ALEPH re…

Particle physicsAlephPhysics and Astronomy (miscellaneous)Electron–positron annihilationFOS: Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsEngineering (miscellaneous)BosonPhysicsLuminosity (scattering theory)010308 nuclear & particles physicsBranching fractionHigh Energy Physics::PhenomenologyFermionFunction (mathematics)3. Good healthHiggs bosonHigh Energy Physics::ExperimentHiggs Boson Invariant Mass Higgs Boson Mass Time Projection Chamber Inant VariableParticle Physics - Experiment
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Theoretical estimates of supernova-neutrino cross sections for the stable even-even lead isotopes: Charged-current reactions

2016

A detailed study of the charged-current supernova electron neutrino and electron antineutrino scattering off the stable even-mass lead isotopes $A=204$, 206, and 208 is reported in this work. The proton-neutron quasiparticle random-phase approximation (pnQRPA) is adopted to construct the nuclear final and initial states. Three different Skyrme interactions are tested for their isospin and spin-isospin properties and then applied to produce (anti)neutrino-nucleus scattering cross sections for (anti)neutrino energies below 80 MeV. Realistic estimates of the nuclear responses to supernova (anti)neutrinos are computed by folding the computed cross sections with a two-parameter Fermi-Dirac distr…

Particle physicsAstrophysics::High Energy Astrophysical PhenomenaNuclear Theoryneutrino-nucleus interactionsElectronelectron neutrino01 natural sciencesNuclear physics0103 physical sciencesNuclear Experiment010306 general physicsNeutrino oscillationsupernova neutrinosCharged currentPhysicsta114010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyscatteringelectron antineutrinoSupernovalead isotopesIsospinQuasiparticleHigh Energy Physics::ExperimentNeutrinoElectron neutrinoPhysical Review C
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Measurement of the Spin of the Ω− Hyperon

2006

A measurement of the spin of the Omega(-) hyperon produced through the exclusive process Xi(c)(0)--Omega(-)K(+) is presented using a total integrated luminosity of 116 fb(-1) recorded with the BABAR detector at the e(+)e(-) asymmetric-energy B factory at SLAC. Under the assumption that the Xi(c)(0) has spin 1/2, the angular distribution of the Lambda from Omega(-)--LambdaK(-) decay is inconsistent with all half-integer Omega(-) spin values other than 3/2. Lower statistics data for the process Omega(c)(0)--Omega(-)pi(+) from a 230 fb(-1) sample are also found to be consistent with Omega(-) spin 3/2. If the Xi(c)(0) spin were 3/2, an Omega(-) spin of 5/2 could not be excluded.

Particle physicsBABARmedia_common.quotation_subjectElectron–positron annihilationGeneral Physics and AstronomyLIFETIMELambda01 natural sciencesOmegaAsymmetryLuminosityNuclear physicsParticle decay0103 physical sciencesSDG 7 - Affordable and Clean Energy010306 general physicsmedia_commonSpin-½Physics/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energy010308 nuclear & particles physicsHyperonParticle physicsHEPHigh Energy Physics::ExperimentSLACFísica de partículesExperimentsLIFETIME; BABAR; SLAC
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