Search results for "Haze"

showing 10 items of 58 documents

Spin Trapping of Carbon-Centered Ferrocenyl Radicals with Nitrosobenzene

2015

In contrast to metal centered 17 valence electron radicals, such as [Mn(CO)5]•, ferrocenium ions [Fe(C5H5)2]+ (1+), [Fe(C5Me5)2]+ (2+), [Fe(C5H5)(C5H4Et)]+ (3+), [Fe(C5H5)(C5H4NHC(O)Me)]+ (4+), and [Fe(C5H5)(C5H4NHC(S)Me)]+ (5+) do not add to nitrosobenzene PhNO to give metal-coordinated stable nitroxyl radicals. In the presence of the strong and oxidatively stable phosphazene base tert-butylimino-tris(dimethylamino)phosphorane, the quite acidic ferrocenium ions 1+–5+ are deprotonated to give a pool of transient and persistent radicals with different deprotonation sites [1–Hx]•–[5–Hx]•. One rather persistent iron-centered radical [4–HN]•, deprotonated at the nitrogen atom, has been detected…

Spin trappingRadicalOrganic ChemistryPhotochemistryPhosphoranelaw.inventionInorganic ChemistryMetalNitrosobenzenechemistry.chemical_compoundDeprotonationchemistrylawvisual_artvisual_art.visual_art_mediumPhysical and Theoretical ChemistryElectron paramagnetic resonancePhosphazeneOrganometallics
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Adaptation of microphysical and chemical instrumentation to the airborne measuring platform Iljushin I1-18 ‘Cyclone’ and flight regime planning durin…

1997

Abstract In 1993 the joint Russian-German Research Project ‘Arctic Haze’ started (see the Introduction and editorial note of this issue, by Jaenicke, Khattatov, Jaeschke and Leiterer). Besides CAO, four German groups were involved. To the present three airborne measuring campaigns have been performed. In total 251 h of flight within altitudes up to 8.7 km were flown in the western and eastern part of the arctic leading to a comprehensive set of data of the northern arctic hemisphere. The measurements were conducted aboard the Russian research aircraft I1-18 ‘Cyclone’ which was used by CAO in numerous scientific projects mainly in the former USSR. This 4 engined turboprop aircraft is well eq…

TurbopropArctic hazeAtmospheric ScienceHazeMeteorologyArcticCycloneEnvironmental scienceInstrumentation (computer programming)Adaptation (computer science)The arcticAtmospheric Research
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Overview paper: New insights into aerosol and climate in the Arctic

2019

Motivated by the need to predict how the Arctic atmosphere will change in a warming world, this article summarizes recent advances made by the research consortium NETCARE (Network on Climate and Aerosols: Addressing Key Uncertainties in Remote Canadian Environments) that contribute to our fundamental understanding of Arctic aerosol particles as they relate to climate forcing. The overall goal of NETCARE research has been to use an interdisciplinary approach encompassing extensive field observations and a range of chemical transport, earth system, and biogeochemical models. Several major findings and advances have emerged from NETCARE since its formation in 2013. (1) Unexpectedly high summer…

[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Arctic hazeAtmospheric Science010504 meteorology & atmospheric sciencesGlobal warmingClimate change010501 environmental sciencesMineral dustAtmospheric sciences01 natural sciencesSea surface microlayerlcsh:QC1-999Atmospheric SciencesAerosollcsh:ChemistryClimate ActionDeposition (aerosol physics)lcsh:QD1-999Arctic[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology13. Climate actionMeteorology & Atmospheric Scienceslcsh:PhysicsAstronomical and Space Sciences0105 earth and related environmental sciencesAtmospheric Chemistry and Physics
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Titan's 3-micron spectral region from ISO high-resolution spectroscopy

2006

Abstract The near-infrared spectrum of Titan, Saturn's largest moon and one of the Cassini/Huygens' space mission primary targets, covers the 0.8 to 5 micron region in which it shows several weak CH 4 absorption regions, and in particular one centered near 2.75 micron. Due to the interference of telluric absorption, only part of this window region (2.9–3.1 μm) has previously been observed from the ground [Noll, K.S., Geballe, T.R., Knacke, R., Pendleton, F., Yvonne, J., 1996. Icarus 124, 625–631; Griffith, C.A., Owen, T., Miller, G.A., Geballe, T., 1998. Nature 395, 575–578; Griffith, C.A., Owen, T., Geballe, T.R., Rayner, J., Rannou, P., 2003. Science 300, 628–630; Geballe, T.R., Kim, S.J.…

[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]PhysicsSolar SystemHaze010304 chemical physicsInfraredSingle-scattering albedoAstronomyAstronomy and AstrophysicsTholin01 natural sciences7. Clean energysymbols.namesake[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]13. Climate actionSpace and Planetary SciencePlanet0103 physical sciencessymbolsMixing ratioTitan (rocket family)010303 astronomy & astrophysicsIcarus
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Titan's surface and atmosphere from Cassini/VIMS data with updated methane opacity

2013

International audience; We present an analysis of Titan data acquired by the Cassini Visual and Infrared Mapping Spectrometer (VIMS), making use of recent improvements in methane spectroscopic parameters in the region 1.3-5.2 μm. We first analyzed VIMS spectra covering a 8 × 10-km2 area near the Huygens landing site in order to constrain the single scattering albedo (ω0) of the aerosols over all of the VIMS spectral range. Our aerosol model agrees with that derived from Huygens Probe Descent Imager/Spectral Radiometer (DISR) in situ measurements below 1.6 μm. At longer wavelengths, ω0 steadily decreases from 0.92 at 1.6 μm to about 0.70 at 2.5 μm and abruptly drops to about 0.50 near 2.6 μm…

[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph][PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]Haze010504 meteorology & atmospheric sciencesOpacity[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Single-scattering albedoAstronomy and AstrophysicsTholinAstrophysicsAtmospheric sciences01 natural sciencesSpectral lineAerosolsymbols.namesake13. Climate actionSpace and Planetary Science0103 physical sciencessymbolsAtmosphere of TitanTitan (rocket family)010303 astronomy & astrophysicsGeology0105 earth and related environmental sciences
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LEAD(II) AND CADMIUM(II) REMOVAL FROM AQUEOUS SOLUTIONS USING HAZELNUT AND ALMOND SHELLS SORBENT MATERIALS

2016

Removal of toxic metal ions from natural and waste waters is of great importance for the health of living organisms and for environmental protection. Alternatively to the conventional chemical treatments, such as precipitation, reverse osmosis, etc, biosorption shows a growing interest for toxic metal ions removal from contaminated aqueous solutions. The sorption ability of every type of biomass towards metal ions depends on many variables that characterize the solution. Among these, the ionic strength (I) is one of the most important and cannot be neglected during an accurate adsorption study. For this reason and with the aim of quantitatively define the influence of I, here are reported t…

almond shellmetal ion removallead(II)remediation.Settore CHIM/01 - Chimica AnaliticaAdsorptionhazelnut shell
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Study on anther culture in hazelnut (Corylus avellana L.) .

2013

anther culture hazelnut gametic embryogenesis
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Effect of adding new phosphazene compounds to poly(butylene terephthalate)/polyamide blends. II: Effect of different polyamides on the properties of …

2006

Poly(butylene terephthalate) (PBT) and a sample of polyamide have been melt processed in the presence of two new phosphazene compounds, namely 2,2-dichloro-4,4,6,6-bis[spyro(2',2"-dioxy-1',1"-biphenyl)]cyclotriphosphazene (2Cl-CP) and 2,2-bis(2-methoxy-4-methyleneoxy-phenoxy)-4,4,6,6-bis[spyro(2',2"-dioxy-1',1"-biphenyl)]cyclophosphazene (CP-2EPOX). The blends were prepared by using polyamide 6 (PA6) and polyamide 6,6 (PA66) in 25/75 and 75/25 w/w compositions by using a co-rotating twin-screw extruder. The materials have been completely characterized from a mechanical, rheological, and morphological point of view. The results indicate that the additives used cause an increase of the ruptur…

chemistry.chemical_classificationMaterials sciencePolymers and PlasticsIzod impact strength testPolymerCompatibilizationPolymer blendCondensed Matter PhysicsCyclophosphazeneReactive compatibilizationchemistry.chemical_compoundSettore ING-IND/22 - Scienza E Tecnologia Dei MaterialichemistryPoly(butylene terephthalate)Mechanics of MaterialsPhase (matter)Polymer chemistryPolyamideMaterials ChemistryCopolymerPolyamidePolymer blendPhosphazene
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Reactions Occurring during the Melt Mixing of Nylon 6 and Oxazoline−Cyclophosphazene Units

2009

Specific reactions of amino and carboxyl end groups of Nylon 6 with the reactive oxazoline groups belonging to a cyclophosphazene compound (referred as CP20XA) were carried out at 240 °C for different times, under inert atmosphere. Ny6 polymers terminated with one specific reactive chain end (-COOH or NH2) were reacted with different amounts of CP20XA to study the kinetic order of the reactions. All Ny6-CP20XA reacted products soluble in trifluoroethanol (TFE) were well characterized by MALDI-TOF MS, FT-IR and ( 1H and 13C) NMR techniques. The MALDI-TOF results show that the oxazoline rings react with the carboxyl chain ends of Ny6 following second-order kinetics. The reactions with amino c…

chemistry.chemical_classificationOxazolineReaction mechanismPolymers and PlasticsOrganic ChemistryKineticsSide reactionPolymerOxazolineReactive BlendingInorganic Chemistrychemistry.chemical_compoundEnd-groupSettore ING-IND/22 - Scienza E Tecnologia Dei MaterialiNylon6Nylon 6chemistrycyclophosphazenes polyamide end-functionalization MALDI-TOFMaterials ChemistryOrganic chemistryInert gasMALDIMacromolecules
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Influence of polysaccharides on wine protein aggregation.

2016

Abstract Polysaccharides are the major high-molecular weight components of wines. In contrast, proteins occur only in small amounts in wine, but contribute to haze formation. The detailed mechanism of aggregation of these proteins, especially in combination with other wine components, remains unclear. This study demonstrates the different aggregation behavior between a buffer and a model wine system by dynamic light scattering. Arabinogalactan-protein, for example, shows an increased aggregation in the model wine system, while in the buffer system a reducing effect is observed. Thus, we could show the importance to examine the behavior of wine additives under conditions close to reality, in…

chemistry.chemical_classificationWineHazedigestive oral and skin physiologyfood and beveragesWine04 agricultural and veterinary sciencesGeneral MedicineProtein aggregationPolysaccharide040401 food scienceProtein Aggregation PathologicalSystem aAnalytical Chemistry0404 agricultural biotechnologyBiochemistryDynamic light scatteringchemistryPolysaccharidesFood scienceFood ScienceFood chemistry
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