Search results for "rotation"

showing 10 items of 935 documents

Rotational CARS thermometry at high temperature (1800 K) and high pressure (0.1-1.55 MPa)

2007

International audience; Dual-broadband rotational CARS (DB-RCARS) thermometry has been investigated at high temperature and high pressure. Single-shot measurements were performed at 1800 K, in air and nitrogen at pressures up to 1.55 MPa and in oxygen at pressures up to 0.5 MPa. For all conditions, the resonant signal contribution to the spectra clearly dominated over the non-resonant one, implying the high potential for DB-RCARS for temperature and concentration measurements also at the high temperatures and pressures used in the present investigation. The relative standard deviation was generally similar to 2% for single-shot data at pressures from 0.5 to 1.55 MPa. At the investigated tem…

Relative standard deviationAnalytical chemistrychemistry.chemical_element02 engineering and technology7. Clean energy01 natural sciencesOxygenSpectral lineStandard deviation010309 opticssymbols.namesakecombustion diagnostics0103 physical sciencesGeneral Materials Sciencerotational CARSSpectroscopy[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]Chemistry021001 nanoscience & nanotechnologyNitrogengas-phase thermometryHigh pressureExcited statesymbols0210 nano-technologyRaman spectroscopy
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Economic evaluation of introduction of poplar as biomass crop in Italy

2014

Abstract Lignocellulosic biomass production deriving from agro forest species, as well as poplar ( Populus spp.), has denoted an increase in last years in UE also thanks to a series of policies aimed at reducing emissions of greenhouse gases and promoting renewable sources. In Italy poplar represents the main agro forest species and it is cultivated according to two different methods: very Short Rotation Coppice (vSRC) and Short Rotation Coppice (SRC). The aim of this paper has been to evaluate the economic feasibility of poplar as energy crop in the southern Italy and specifically to consider its competitiveness with respect to conventional crops. In particular, an economic analysis in a r…

Renewable Energy Sustainability and the Environmentbusiness.industryAgroforestryBiomassLignocellulosic biomassRenewable energyEnergy cropClimate change mitigationAgricultureGreenhouse gasSettore AGR/01 - Economia Ed Estimo RuraleAnnual gross margin CAP subsidy Durum wheat Farm Market value Short Rotation CoppiceEnvironmental scienceShort rotation coppicebusiness
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NMR relaxation times of trabecular bone—reproducibility, relationships to tissue structure and effects of sample freezing

2010

Nuclear magnetic resonance (NMR) spectroscopy provides a potential tool for non-invasive evaluation of the trabecular bone structure. The objective of this study was to determine the reproducibility of the NMR relaxation parameters (T(2), Carr-Purcel-T(2), T(1ρ)) for fat and water and relate those to the structural parameters obtained by micro-computed tomography (μCT). Especially, we aimed to evaluate the effect of freezing on the relaxation parameters. For storing bone samples, freezing is the standard procedure during which the biochemical and cellular organization of the bone marrow may be affected. Bovine trabecular bone samples were stored at -20 °C for 7 days and measured by NMR spec…

ReproducibilityMagnetic Resonance SpectroscopyTime FactorsRotationTibiaRadiological and Ultrasound TechnologyChemistryCoefficient of variationRelaxation (NMR)Reproducibility of ResultsWaterX-Ray MicrotomographyNuclear magnetic resonance spectroscopyTrabecular boneNuclear magnetic resonancemedicine.anatomical_structureAdipose TissueRelaxation rateFreezingmedicineAnimalsCattleRadiology Nuclear Medicine and imagingBone marrowSpectroscopyPhysics in Medicine and Biology
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Reverse rotation of the right kidney associated with vascular anomaly producing ipsilateral ureteropelvic junction obstruction.

2009

Reverse rotation kidney ureteropelvic junction obstruction
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Meta-analytic study on the frequency and treatment of oral antral communications

2010

Objective: To determine the optimum surgical treatment for oral antral communications (OAC) and to understand the main post-operative complications.Study Design: Meta-analytical, observational and retrospective study of 1,072 cases of OAC obtained from a literature review of 15 articles. Results: OAC occur slightly more often in men and during the fourth decade of life. Its primary etiological factor is dental extraction, most often affecting the third molar. The most common treatment has been the use of Bichat's fat pad grafts, whereas the technique with the highest percentage of complications has been the use of the palatal rotation flap. The most frequent complication has been the fistul…

Rotation flapmedicine.medical_specialtybusiness.industrymedicine.medical_treatmentOral Surgical ProceduresRetrospective cohort studyOral Surgical Procedures:CIENCIAS MÉDICAS [UNESCO]Surgical FlapsFat padSurgeryOtorhinolaryngologyDental extractionMeta-analysisUNESCO::CIENCIAS MÉDICASmedicineEtiologyHumansSurgeryOroantral FistulabusinessComplicationGeneral DentistryRetrospective Studies
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Simultaneous Kepler/K2 and XMM-Newton observations of superflares in the Pleiades

2019

Flares are powerful events ignited by a sudden release of magnetic energy. With the aim of studying flares in the 125-Myr-old stars in the Pleiades observed simultaneously in optical and X-ray light, we obtained new XMM-Newton observations of this cluster during the observations of Kepler K2 Campaign 4. Our objective is to characterize the most powerful flares observed in both bands and to constrain the energy released in the optical and X-ray, the geometry of the loops, and their time evolution. We aim to compare our results to existing studies of flares occurring in the Sun and stars at different ages. We selected bright X-ray/optical flares occurred in 12 known members of the Pleiades fr…

Rotation period010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)Astrophysics01 natural scienceslaw.inventionSettore FIS/05 - Astronomia E Astrofisicalaw0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesX-rays:stars–stars:flarePhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Solar flareComputer Science::Information RetrievalAstronomy and AstrophysicsLight curveStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsPleiadesAstrophysics - High Energy Astrophysical PhenomenaSuperflareFlare
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The 2017 May 20 stellar occultation by the elongated centaur (95626) 2002 GZ32

2021

Full list of authors: Santos-Sanz, P.; Ortiz, J. L.; Sicardy, B.; Benedetti-Rossi, G.; Morales, N.; Fernández-Valenzuela, E.; Duffard, R.; Iglesias-Marzoa, R.; Lamadrid, J. L.; Maícas, N.; Pérez, L.; Gazeas, K.; Guirado, J. C.; Peris, V.; Ballesteros, F. J.; Organero, F.; Ana-Hernández, L.; Fonseca, F.; Alvarez-Candal, A.; Jiménez-Teja, Y. Vara-Lubiano, M.; Braga-Ribas, F.; Camargo, J. I. B.; Desmars, J.; Assafin, M.; Vieira-Martins, R.; Alikakos, J.; Boutet, M.; Bretton, M.; Carbognani, A.; Charmandaris, V.; Ciabattari, F.; Delincak, P.; Fuambuena Leiva, A.; González, H.; Haymes, T.; Hellmich, S.; Horbowicz, J.; Jennings, M.; Kattentidt, B.; Kiss, Cs; Komžík, R.; Lecacheux, J.; Marciniak, …

Rotation period010504 meteorology & atmospheric sciencesFOS: Physical sciencesAstrophysicsEllipse01 natural sciencesOccultationlaw.inventiontechniques: photometriclawGeometric albedo0103 physical sciencesoccultationsobservational [Methods]individual: 2002 GZ(32) [Kuiper Belt objects]methods: observational – techniques: photometric – occultations – Kuiper Belt objects: individual: 2002 GZ32.010303 astronomy & astrophysicsKuiper Belt objects: individual: 2002 GZ(32)Solar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsEarth and Planetary Astrophysics (astro-ph.EP)[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]photometric [Techniques]Astronomy and AstrophysicsCentaurAlbedoLight curveKuiper Belt objects: individual: 2002 GZ32Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science[SDU]Sciences of the Universe [physics]OccultationsHydrostatic equilibriummethods: observationalAstrophysics - Earth and Planetary Astrophysics
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The X-ray activity-rotation relation of T Tauri stars in Taurus-Auriga

2007

The Taurus-Auriga star-forming complex hosts the only population of T Tauri stars in which an anticorrelation of X-ray activity and rotation period has been observed. We have used XMM-Newton's European Photon Imaging Cameras to perform the most sensitive survey to date of X-ray emission (0.3-10 keV) from young stars in Taurus-Auriga and investigate the dependences of X-ray activity measures -- X-ray luminosity, Lx, its ratio with the stellar luminosity, Lx/Lstar, and the surface-averaged X-ray flux, Fxs -- on rotation period. We tested for differences in the distributions of Lx/Lstar of fast and slow rotators, accretors and non-accretors, and compared the dependence of Lx/Lstar on the ratio…

Rotation periodAstrophysics::High Energy Astrophysical PhenomenaPopulationFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsRotation01 natural sciencesLuminosity[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicseducation010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicseducation.field_of_studyAURIGA010308 nuclear & particles physicsAstrophysics (astro-ph)Astronomy and AstrophysicsEffective temperatureStarsT Tauri star13. Climate actionSpace and Planetary Science[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Astrophysics::Earth and Planetary Astrophysics
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Pulsations in the late-type Be star HD 50 209 detected by CoRoT

2009

The presence of pulsations in late-type Be stars is still a matter of controversy. It constitutes an important issue to establish the relationship between non-radial pulsations and the mass-loss mechanism in Be stars. To contribute to this discussion, we analyse the photometric time series of the B8IVe star HD 50209 observed by the CoRoT mission in the seismology field. We use standard Fourier techniques and linear and non-linear least squares fitting methods to analyse the CoRoT light curve. In addition, we applied detailed modelling of high-resolution spectra to obtain the fundamental physical parameters of the star. We have found four frequencies which correspond to gravity modes with az…

Rotation periodBe starHertzsprung–Russell diagramFOS: Physical sciencesAstrophysicsStar (graph theory)01 natural sciencesSpectral linesymbols.namesake0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Physics010308 nuclear & particles physicsAstronomy and AstrophysicsLight curveCiència EnsenyamentStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstronomiasymbolsAstrophysics::Earth and Planetary AstrophysicsInstability strip[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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HADES RV Programme with HARPS-N at TNG. IV. Time resolved analysis of the Ca II H&K and Hα chromospheric emission of low-activity early-type M dwarfs

2016

Context. M dwarfs are prime targets for current and future planet search programs, particularly those focused on the detection and characterization of rocky planets in the habitable zone. In this context, understanding their magnetic activity is important for two main reasons: it affects our ability to detect small planets and it plays a key role in the characterization of the stellar environment. Aims: We analyze observations of the Ca II H&K and Hα lines as diagnostics of chromospheric activity for low-activity early-type M dwarfs. Methods: We analyze the time series of spectra of 71 early-type M dwarfs collected in the framework of the HADES project for planet search purposes. The HARPS-…

Rotation periodPhysics010504 meteorology & atmospheric sciencesAstronomy and AstrophysicsContext (language use)Astrophysics01 natural sciencesK-lineSpectral lineStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science0103 physical sciencesTerrestrial planetAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary Astrophysics010303 astronomy & astrophysicsCircumstellar habitable zone0105 earth and related environmental sciencesLine (formation)
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