Search results for "otos"

showing 10 items of 857 documents

Green sulphur bacteria as a component of the photosynthetic plankton community in small dimictic humic lakes with an anoxic hypolimnion

2013

High bacteriochlorophyll (BChl) concentrations in the anoxic water layers of some humic lakes have indicated that green sulphur bacteria (GSB) may be ecologically significant. The abundance and spatial distribution of GSB were therefore addressed in 13 small humic lakes using fragment analysis and sequencing of PCR-amplified 16S rRNA genes. GSB were detected from lakes where the photosynthetically active radiation was at least 1.1 µE m �2 s �1 at the oxic� anoxic boundary layer. In these lakes, 13 to 42% of the 16S rRNA gene sequences of the anoxic water column were assigned to GSB. The spatial distribution of GSB was tightly correlated with the spectrophotometrically measured BChl concentr…

Aquatic SciencePlanktonBiologySpatial distributionPhotosynthesisAnoxic waterschemistry.chemical_compoundchemistryPhotosynthetically active radiationChlorophyllBotanyNaturvetenskapBacteriochlorophyllHypolimnionNatural SciencesEcology Evolution Behavior and Systematicsta119Aquatic Microbial Ecology
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Aparatūra “Lotoss” poliuretāna plastmasas detaļu atliešanai kosmosā

2020

1980. gadā kosmosa stacijā “Salūts” pirmoreiz kosmonautikas vēsturē tika realizēts putupoliuretāna ieguves eksperiments mikrogravitācijas apstākļos, kura rezultāta tika iegūtas jaunas atziņas par ķīmiski tehnoloģisko procesu norisi kosmosā. Kosmosā tapa Maskavas olimpisko spēļu simbola lācīša figūra. Iekārtu "Lotoss", kas pašreiz atrodas Latvijas Ķīmijas vēstures muzeja krājumā, LPSR Zinātņu Akadēmijas Koksnes ķīmijas institūtā izstrādājis latviešu ķīmiķis, ķīmijas doktors, izgudrotājs un gleznotājs Arnolds Alksnis, un tā domāta polimerizācijas reakciju pētīšanai bezsvara stāvoklī.

Arnolds Alksnispolymer chemistryweightless state1980 Summer Olympicsolimpisko spēļu talismanspoliuretāna putasThe Olympic Mishkabezsvara stāvoklispolyurethanepoliuretāns:NATURAL SCIENCES::Chemistry::Organic chemistry::Polymer chemistry [Research Subject Categories]1980. gada vasaras olimpiskās spēlesLatvijas Valsts Koksnes ķīmijas institūtsLotosspolimēru ķīmija
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H-2, H-3(+) and the age of molecular clouds and prestellar cores

2012

Measuring the age of molecular clouds and prestellar cores is a difficult task that has not yet been successfully accomplished although the information is of paramount importance to help in understanding and discriminating between different formation scenarios. Most chemical clocks suffer from unknown initial conditions and are therefore difficult to use. We propose a new approach based on a subset of deuterium chemistry that takes place in the gas phase and for which initial conditions are relatively well known. It relies primarily on the conversion of H 3 + into H 2D + to initiate deuterium enrichment of the molecular gas. This conversion is controlled by the ortho/para ratio of H2 that i…

AstrochemistryAbundance (chemistry)General MathematicsGeneral Physics and AstronomySULFUR CHEMISTRYAstrophysicsINITIAL CONDITIONS01 natural sciences7. Clean energySTAR-FORMATION0103 physical sciencesGravitational collapseProtostar010306 general physics010303 astronomy & astrophysicsAMBIPOLAR DIFFUSIONCOSMIC-RAY IONIZATION[PHYS]Physics [physics]INTERSTELLAR-MEDIUMStar formationMolecular cloudTRIPLY DEUTERATED AMMONIAGeneral EngineeringORTHO-PARA TRANSITIONSInterstellar mediumDARK CLOUDSGRAVITATIONAL COLLAPSEDeuterium13. Climate action[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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EVIDENCE OF NON-THERMAL X-RAY EMISSION FROM HH 80

2013

Protostellar jets appear at all stages of star formation when the accretion process is still at work. Jets travel at velocities of hundreds of km s -1, creating strong shocks when interacting with the interstellar medium. Several cases of jets have been detected in X-rays, typically showing soft emission. For the first time, we report evidence of hard X-ray emission possibly related to non-thermal processes not explained by previous models of the post-shock emission predicted in the jet/ambient interaction scenario. HH 80 is located at the south head of the jet associated with the massive protostar IRAS 18162-2048. It shows soft and hard X-ray emission in regions that are spatially separate…

AstrofísicaCiencias AstronómicasCiencias FísicasAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSynchrotron radiationAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsIndividual: Iras 18162-2048 [Stars]//purl.org/becyt/ford/1 [https]Herbig-Haro objects ISM: jets and outflows radiation mechanisms: non-thermal stars: individual: IRAS 18162-2048 stars: pre-main sequence X-rays: generalHigh Energy Physics - Phenomenology (hep-ph)Herbig-Haro objectsGeneral [X-Rays]jets and outflows radiation mechanisms: non-thermal stars: individual: IRAS 18162-2048 stars: pre-main sequence X-rays: general [Herbig-Haro objects ISM]Jets And Outflows [Ism]ThermalProtostarstars: individualAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsStar formationX-rayAstronomy and Astrophysics//purl.org/becyt/ford/1.3 [https]radiation mechanisms: non-thermalHerbig-Haro ObjectsAstrophysics - Astrophysics of GalaxiesAccretion (astrophysics)Non-Thermal [Radiation Mechanisms]AstronomíaInterstellar mediumHigh Energy Physics - PhenomenologyISM: jets and outflowsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASThe Astrophysical Journal
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Formation of X-ray emitting stationary shocks in magnetized protostellar jets

2016

X-ray observations of protostellar jets show evidence of strong shocks heating the plasma up to temperatures of a few million degrees. In some cases, the shocked features appear to be stationary. They are interpreted as shock diamonds. We aim at investigating the physics that guides the formation of X-ray emitting stationary shocks in protostellar jets, the role of the magnetic field in determining the location, stability, and detectability in X-rays of these shocks, and the physical properties of the shocked plasma. We performed a set of 2.5-dimensional magnetohydrodynamic numerical simulations modelling supersonic jets ramming into a magnetized medium and explored different configurations…

AstrofísicaMagnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencesRadiative coolingAstrophysics::High Energy Astrophysical PhenomenaISM: structureFOS: Physical sciencesAstrophysics01 natural sciencesISM: magnetic field0103 physical sciencesShock diamondRadiative transfer010303 astronomy & astrophysicsISM: jets and outflowSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Jet (fluid)Astronomy and AstrophysicsPlasmaAstronomy and AstrophysicThermal conductionX-rays: ISMShock (mechanics)Magnetic fieldAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceStars: protostarAstrophysics - High Energy Astrophysical Phenomena
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CSI 2264: Simultaneous optical and X-ray variability in pre-main sequence stars. I. Time resolved X-ray spectral analysis during optical dips and acc…

2017

Pre-main sequence stars are variable sources. In stars with disks, this variability is related to the morphology of the inner circumstellar region (<0.1 AU) and that of the photosphere and corona, all impossible to be spatially resolved with present day techniques. This has been the main motivation for the Coordinated Synoptic Investigation of NGC 2264. In this paper, we focus on the stars with disks. We analyze the X-ray spectral properties extracted during optical bursts and dips in order to unveil the nature of these phenomena. We analyze simultaneous CoRoT and Chandra/ACIS-I observations to search for coherent optical and X-ray flux variability in stars with disks. Then, stars are an…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesstars: pre-main sequenceAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicscircumstellar matter01 natural sciencesSettore FIS/05 - Astronomia E Astrofisicastars: rotation0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsSpectral analysis010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPhotosphere010308 nuclear & particles physicsX-rayAstronomy and AstrophysicsSpectral componentAccretion (astrophysics)StarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceExtinction (optical mineralogy)stars: variables: T Tauri Herbig Ae/BeAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaMain sequence
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Characterization and intercomparison of global moderate resolution leaf area index (LAI) products: Analysis of climatologies and theoretical uncertai…

2013

products (R 2 >0.74), with typical deviations of<0.5 for nonforest and<1.0 for forest biomes. JRC-TIP, the only effective LAI product, is about half the values of the other LAI products. The average uncertainties and relative uncertainties are in the following order: MODIS (0.17, 11.5%)<GEOV1 (0.24, 26.6%)<Land-SAF (0.36, 37.8%) <JRC-TIP (0.43, 114.3%). The highest relative uncertainties usually appear in ecological transition zones. More than 75% of MODIS, GEOV1, JRC-TIP, and Land-SAF pixels are within the absolute uncertainty requirements (� 0.5) set by the Global Climate Observing System (GCOS), whereas more than 78.5% of MODIS and 44.6% of GEOV1 pixels are within the threshold for relat…

Atmospheric Science010504 meteorology & atmospheric sciencesMeteorologyGlobal climateBiome0207 environmental engineeringSoil Science02 engineering and technologyAquatic ScienceWinter timeAtmospheric sciences01 natural sciencesSatellite dataLeaf area index020701 environmental engineeringRetrieval algorithm0105 earth and related environmental sciencesWater Science and TechnologyEcologyPaleontologyForestryVegetation15. Life on land13. Climate actionPhotosynthetically active radiationEnvironmental scienceJournal of Geophysical Research: Biogeosciences
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2015

Abstract. Atmospheric concentrations of nitrous acid (HONO), one of the major precursors of the hydroxyl radical (OH) in the troposphere, significantly exceed the values predicted by the assumption of a photostationary state (PSS) during daytime. Therefore, additional sources of HONO were intensively investigated in the last decades. This study presents budget calculations of HONO based on simultaneous measurements of all relevant species, including HONO and OH at two different measurement heights, i.e. 1 m above the ground and about 2 to 3 m above the canopy (24 m above the ground), conducted in a boreal forest environment. We observed mean HONO concentrations of about 6.5 × 108 molecules …

Atmospheric ScienceNitrous acidDaytime010504 meteorology & atmospheric sciencesMeteorologyAdvection010501 environmental sciencesNoonAtmospheric sciences01 natural sciencesTropospherechemistry.chemical_compoundchemistryPhotostationary stateAtmospheric chemistrySoil water0105 earth and related environmental sciencesAtmospheric Chemistry and Physics
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Hyperspectral response of agronomic variables to background optical variability: Results of a numerical experiment

2022

Understanding how biophysical and biochemical variables contribute to the spectral characteristics of vegetation canopies is critical for their monitoring. Quantifying these contributions, however, remains difficult due to extraneous factors such as the spectral variability of canopy background materials, including soil/crop-residue moisture, soil-type, and non-photosynthetic vegetation (NPV). This study focused on exploring the spectral response of two important agronomic variables (1) leaf chlorophyll content (Cab ) and (2) leaf area index (LAI) under various canopy backgrounds through a global sensitivity analysis of wheat-like canopy spectra simulated using the physically-based PROSAIL …

Atmospheric ScienceResilient LivelihoodsLEAF-AREA-INDEXSoil typePHOTOCHEMICAL REFLECTANCE INDEXBIOPHYSICAL PROPERTIESMeteorology & Atmospheric SciencesAdaptationLeaf chlorophyll contentGlobal and Planetary ChangeScience & TechnologyVEGETATION INDEXESSPECTRAL INDEXESGLOBAL SENSITIVITY-ANALYSISAgricultureNon-photosynthetic vegetationForestry22/4 OA procedureAgronomyHyperspectral responseGlobal sensitivity analysisITC-ISI-JOURNAL-ARTICLEPhysical SciencesLeaf area indexCHLOROPHYLL CONTENTGREEN LAILife Sciences & BiomedicineCANOPY REFLECTANCEAgronomy and Crop ScienceRADIATIVE-TRANSFER MODELAgricultural and Forest Meteorology
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Ulteriori evidenze di attività antimicrobiche in invertebrati marini

2014

The antimicrobial molecules are an abundant group of molecules that are amply distributed in nature, from plants and insects to vertebrate animals, including humans. They are an essential component of the innate immune system for host defence against pathogenic agents of different types. They are often the products of individual genes and circulating cells. In this thesis, based on a bioinformatic analysis, we identified three peptides, members to the family of cathelicidins and to the class of peptides rich in proline (PR-AMPs), that may be generally be considered as the first effectors of the interior defense, acting as natural antibiotics (Scocchi et al., 2011; Reddy et al., 2004). We in…

Attività antimicrobica attività citotossicaestrattipeptidi antimicrobici
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