Search results for "FOS"

showing 10 items of 15075 documents

X-ray flare modeling in the single giant HR 9024

2005

We analyze a Chandra-HETGS observation of the single G-type giant HR 9024. The high flux allows us to examine spectral line and continuum diagnostics at high temporal resolution, to derive plasma parameters (thermal distribution, abundances, temperature, ...). A time-dependent 1D hydrodynamic loop model with semi-length 10$^{12}$cm ($\sim R_{\star}$), and impulsive footpoint heating triggering the flare, satisfactorily reproduces the observed evolution of temperature and emission measure, derived from the analysis of the strong continuum emission. The observed characteristics of the flare appear to be common features in very large flares in active stars (also pre-main sequence stars), possi…

hydrodynamic loop modelsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstrophysics::Solar and Stellar AstrophysicsAstrophysicsAstrophysics::Galaxy Astrophysicshigh resolution X-ray spectroscopy
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Changes in pore water quality after peatland restoration: Assessment of a large¿scale, replicated Before-After-Control-Impact study in Finland

2017

Drainage is known to affect peatland natural hydrology and water quality, but peatland restoration is considered to ameliorate peatland degradation. Using a replicated BACIPS (Before-After-Control-Impact Paired Series) design, we investigated 24 peatlands, all drained for forestry and subsequently restored, and 19 pristine control boreal peatlands with high temporal and spatial resolution data on hydroclimate and pore water quality. In drained conditions, total nitrogen (Ntot), total phosphorus (Ptot), and dissolved organic carbon (DOC) in pore water were several-fold higher than observed at pristine control sites, highlighting the impacts of long-term drainage on pore water quality. In gen…

hydrologiarestorationtyppipeatland hydrologypore water qualityennallistaminenvedenlaatuturvemaatfosforidrainage
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Revision of Recent and fossil Mixtacandona Klie 1938 (Ostracoda, Candonidae) from Italy, with description of a new species

2017

Although studies on ostracods dwelling in inland subterranean habitats of Italy have increased in the last decades, highlighting a considerable taxonomic diversity, available information is still far from sufficient to understand phylogenetic and biogeographic relationships. Mixtacandona Klie 1938 is one of the most common and diverse genera of ostracods in subterranean waters. Of the 20 living recognized species in the genus, all stygobiontic and restricted to the Palearctic Region, four are known for the Italian peninsula and Sardinia, one of which exclusively as fossil. Several other Recent and fossil taxa attributable to Mixtacandona, but identified at supraspecific level, have been rep…

hypogean ostracods morphology taxonomy distribution Mixtacandona idrisi n. sp.0106 biological sciencesArthropodaOstracodaSettore BIO/05 - ZoologiaBiology010603 evolutionary biology01 natural sciencesCavePeninsulaGenusCrustaceaOstracodAnimalsAnimaliaSicilyEcosystemPhylogenyEcology Evolution Behavior and SystematicsTaxonomyCandonidaegeographygeography.geographical_feature_categoryPhylogenetic treeFossilsEcology010604 marine biology & hydrobiologyBiodiversitybiology.organism_classificationPodocopidaTaxonCandonidaeAnimal Science and ZoologyTaxonomy (biology)
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Concreções calcárias da formação Santana, bacia do Araripe: uma proposta de classificação.

2007

18 pages; The calcareous concretions of the Santana Formation have been known since 1800 thanks to the work of João da Silva Feijó (1800). Their study was promoted internationally by the report of von Spix and von Martius (1823-1831), and their richness in fossil fishes led Silva Santos to name them “ichthyoliths” in 1950. Here we propose a classification for the various types of calcareous concretions that occurred in the Santana Formation (Late Cretaceous, Araripe Basin). We consider their geographic distribution and we propose a terminological uniformization for the descriptions of that material. This will serve future statistical, geographical, geochemical and taphonomical studies that,…

ichthyolithSantana FormationLate Cretaceousmacrofossils[SDU.STU.ST] Sciences of the Universe [physics]/Earth Sciences/Stratigraphy[SDU.STU.PG] Sciences of the Universe [physics]/Earth Sciences/Paleontology[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/Stratigraphysyngenetic carbonate concretions[ SDU.STU.PG ] Sciences of the Universe [physics]/Earth Sciences/Paleontology
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Figure del contagio. Dalle topografie mediche al contact tracing: trasformazioni nell’architettura e nel paesaggio urbano

2021

Ita_Il tracciamento del contagio, fra le più efficaci forme globali di difesa dal coronavirus, viene ripercorso mettendo in luce il rapporto fra pensiero architettonico e spazio delle epidemie negli ultimi due secoli. La relazione fra la diffusione delle malattie e le forme del costruito è stata infatti compresa nella seconda metà dell’Ottocento attraverso le mappature tematiche, secondo metodi ancora oggi in evoluzione. A partire dalle topografie mediche comparse per la prima volta in Francia nel XIX secolo, interpolate con le intuizioni di J. Snow sulla base delle mappe da lui elaborate nello stesso periodo in Inghilterra, si evidenziano i modi di formazione di un regime di sapere teso fr…

igienismo spazio pubblico contact tracing mapping Locative Media Social Networks LMSN GAFAMSettore ICAR/14 - Composizione Architettonica E UrbanaTony Garnier Eugène Henard Fondation Rothschild Adolphe-Augustin Rey Norman Foster Topografie medicheTony Garnier Eugène Henard Fondation Rothschild Adolphe-Augustin Rey Norman Foster Medical Topographies Hygienism Public Space contact tracing mapping Locative Media Social Networks LMSN GAFAM
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Design and performance of the prototype Schwarzschild-Couder telescope camera

2022

Journal of astronomical telescopes, instruments, and systems 8(01), 014007-1 (2022). doi:10.1117/1.JATIS.8.1.014007

imaging atmospheric Cherenkov telescopesinstrumentationPhysics - Instrumentation and Detectorsvery-high-energy gamma-ray astronomyPhysics::Instrumentation and DetectorsMechanical EngineeringSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)530Electronic Optical and Magnetic MaterialsCherenkov telescope arraySpace and Planetary ScienceControl and Systems Engineeringddc:530prototype Schwarzschild-Couder telescopeAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)silicon photomultipliers
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New Insights into the Chemistry of Imidodiphosphinates from Investigations of Tellurium-Centered Systems

2010

Dichalcogenido-imidodiphosphinates, [N(PR2E)2]− (R = alkyl, aryl), are chelating ligands that readily form cyclic complexes with main group metals, transition metals, lanthanides, and actinides. Since their discovery in the early 1960s, researchers have studied the structural chemistry of the resulting metal complexes (where E = O, S, Se) extensively and identified a variety of potential applications, including as NMR shift reagents, luminescent complexes in photonic devices, or single-source precursors for metal sulfides or selenides. In 2002, a suitable synthesis of the tellurium analogs [N(PR2Te)2]− was developed. In this Account, we describe comprehensive investigations of the chemistry…

imidodiphosphinatesimidodifosfinaatit
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Optimality of Increasing Stability for an Inverse Boundary Value Problem

2021

In this work we study the optimality of increasing stability of the inverse boundary value problem (IBVP) for the Schrödinger equation. The rigorous justification of increasing stability for the IBVP for the Schrödinger equation were established by Isakov [Discrete Contin. Dyn. Syst. Ser. S, 4 (2011), pp. 631--640] and by Isakov et al. [Inverse Problems and Applications, Contemp. Math. 615, American Math Society, Providence, RI, 2014, pp. 131--141]. In [Discrete Contin. Dyn. Syst. Ser. S, 4 (2011), pp. 631--640] and [Inverse Problems and Applications, Contemp. Math. 615, American Math Society, Providence, RI, 2014, pp. 131--141], the authors showed that the stability of this IBVP increases …

increasing stability phenomenaosittaisdifferentiaaliyhtälötinstabilityComputational MathematicsMathematics - Analysis of PDEsApplied Mathematics35J15 35R25 35R30FOS: MathematicsSchrödinger equationinverse boundary value probleminversio-ongelmatAnalysisAnalysis of PDEs (math.AP)SIAM Journal on Mathematical Analysis
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Broad-band Spectral Evolution of Scorpius X-1 along its Color-Color Diagram

2007

We analyze a large collection of RXTE archive data from April 1997 to August 2003 of the bright X-ray source Scorpius X-1 in order to study the broadband spectral evolution of the source for different values of the inferred mass accretion rate by studying energy spectra from selected regions in the Z-track of its Color-Color Diagram. A two-component model, consisting of a soft thermal component interpreted as thermal emission from an accretion disk and a thermal Comptonization component, is unable to fit the whole 3--200 keV energy spectrum at low accretion rates. Strong residuals in the highest energy band of the spectrum require the addition of a third component that can be fitted with a …

individual (Scorpius X-1); stars : neutron; X-rays : binaries; X-rays : general; X-rays : stars [accretion accretion disks; stars]PhysicsAccretion (meteorology)Component (thermodynamics)Astrophysics::High Energy Astrophysical PhenomenaX-rays : starsDiagramAstrophysics (astro-ph)FOS: Physical sciencesstars : individual (Scorpius X-1)Astronomy and AstrophysicsColor–color diagramPlasmaAstrophysicsAstrophysicsaccretion accretion diskstars : neutronSpectral lineSpace and Planetary ScienceThermalX-rays : binarieElectronic band structureAstrophysics::Galaxy AstrophysicsX-rays : general
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Sub-milliarcsecond imaging of a bright flare and ejection event in the extragalactic jet 3C 111

2020

Context. Flares in radio-loud active galactic nuclei are thought to be associated with the injection of fresh plasma into the compact jet base. Such flares are usually strongest and appear earlier at shorter radio wavelengths. Hence, very long baseline interferometry (VLBI) at millimeter(mm)-wavelengths is the best-suited technique for studying the earliest structural changes of compact jets associated with emission flares. Aims. We study the morphological changes of the parsec-scale jet in the nearby (z = 0.049) γ-ray bright radio galaxy 3C 111 following a flare that developed into a major radio outburst in 2007. Methods. We analyse three successive observations of 3C 111 at 86 GHz with th…

individual: 3C 111 [Galaxies]active [Galaxies]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesLibrary scienceAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGalaxies: individual: 3C 1117. Clean energy01 natural sciencesTechniques: high angular resolutionObservatory0103 physical sciencesVery-long-baseline interferometryAstrophysics::Solar and Stellar Astrophysicsmedia_common.cataloged_instanceEuropean union010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsVery Long Baseline Arraymedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsEuropean researchAstronomy and AstrophysicsGalaxies: activeMonitoring programRadio astronomy observatory3. Good healthhigh angular resolution [Techniques]Galaxies: jetsSpace and Planetary Sciencejets [Galaxies]Christian ministryAstrophysics - High Energy Astrophysical PhenomenaAstronomy & Astrophysics
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