Search results for "COMPOSITION"

showing 10 items of 2675 documents

Forensics of birds of prey by DNA fingerprinting with 32P-labeled oligonucleotide probes.

1991

Paternity tests on confiscated families of eight species of birds of prey were carried out successfully by DNA fingerprinting with 32P-labeled oligonucleotide probes. Variations in the number of hybridized fragments, depending on the species of birds, are observed using the same probe, as well as differences of polymorphism by hybridizing the DNA samples with several oligonucleotide probes.

GeneticsMaleBase CompositionBase SequenceOligonucleotideClinical BiochemistryPhosphorus IsotopesBiologyBiochemistryDNA FingerprintingAnalytical ChemistryPredationBirdschemistry.chemical_compoundchemistryDNA profilingPolymorphism (computer science)Paternity testsAnimalsBase sequenceMolecular probeOligonucleotide ProbesDNAPolymorphism Restriction Fragment LengthRepetitive Sequences Nucleic AcidElectrophoresis
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Pulsed field gel electrophoresis and genome size estimates

2015

Pulsed field gel electrophoresis (PFGE) is a quick and reliable procedure to resolve DNA molecules larger than 30 kb by applying an electric field that periodically changes direction. This technique can be used to estimate genome size of a microorganism, to reveal if a genome is circular or linear, to indicate the presence of megaplasmids, and to show if a strain contains only one or more chromosomes.

Genome sizeDNA BacterialMaterials scienceChromosomes ArchaealSettore BIO/19 - Microbiologia GeneraleGenomePlasmidchemistry.chemical_compoundPlasmidGeneticGenome ArchaealElectric fieldPulsed-field gel electrophoresisGenome sizeMolecular BiologyElectrophoresis Agar GelBase CompositionStrain (chemistry)BacteriaMulti-repliconMedicine (all)Physical Chromosome Mappingfood and beveragesChromosomes BacterialPhysical Chromosome MappingArchaeaElectrophoresis Gel Pulsed-FieldDNA ArchaealchemistryMegaplasmidBiological systemDNAGenome BacterialGenome topology
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Lactobacillus rossii sp. nov. isolated from wheat sourdough

2005

Screening of sourdough lactic acid bacteria for bacteriocin production resulted in the isolation of a Gram-positive, catalase-negative, non-spore-forming, non-motile rod bacterium (strain CS1T) that could not be associated with any previously described species. Comparative 16S rRNA gene sequence analysis recognized strain CS1T as a distinct member of the genus Lactobacillus. By a species-specific PCR strategy, five additional strains previously isolated from sourdoughs were found to belong to the same species as strain CS1T, as confirmed by 16S rRNA gene sequence analysis. The closest related species were Lactobacillus durianis, Lactobacillus malefermentans and Lactobacillus suebicus, with …

GenotypeSequence analysisMolecular Sequence DataLactobacillus rossiae impasti acidi nuova specieBiologyDNA RibosomalPolymerase Chain ReactionMicrobiologyMicrobiologychemistry.chemical_compoundBacteriocinRNA Ribosomal 16SLactobacillusPhylogenyTriticumEcology Evolution Behavior and SystematicsBase CompositionNucleic Acid HybridizationGenes rRNABreadSequence Analysis DNAGeneral MedicineRibosomal RNAbiology.organism_classification16S ribosomal RNALactobacillusPhenotypechemistryFermentationPeptidoglycanBacteriaSettore AGR/16 - Microbiologia Agraria
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New insights into magma dynamics during last two eruptions of Mount Etna as inferred by geochemical monitoring from 2002 to 2005

2007

Two distinct eruptive events characterize the volcanic activity at Mount Etna during the 2002 to 2005 period. We identified signals of magma ascent preceding these eruptions by geochemical monitoring of both chemical composition and He-isotope ratio of gas emissions from five locations in the peripheral area of the volcano. The geochemical signals are interpreted using the models proposed by Caracausi et al. (2003a, 2003b) and allow identification of episodes of magma ascent and estimation of the pressures of degassing magma. As observed for the 2001 eruption (Caracausi et al., 2003b), magma ascent probably triggered the onset of the 2002–2003 eruption, and minor events of magma ascent were…

Geochemical monitoringMagma migrationChemical compositionHe isotope
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The Mathematical Modeling of Ca And Fe Distribution In Peat Layers

2015

Bogs have been formed by an accumulation of peat - a light brown-to-black organic material, built up from partial decomposition of mosses and other bryophytes, sedges, grasses, shrubs, or trees under waterlogged conditions. The total peatlands area in Latvia covers 698 918 ha or 10.7% of the entire territory. Knowledge’s of peat metals content are important for any kind of peat using. Experimental determination of metals in peat is very long and expensive work. Using experimental data mathematical model for calculation of concentrations of metals in different points for different layers can help to very easy and fast to find approximately concentration of metals or trace elements. The resul…

Geographygeography.geographical_feature_categoryPeatMathematical modelfinite difference method; heavy metals; peat bogMireHeavy metalsPartial decompositionSoil scienceBogEnvironment. Technology. Resources. Proceedings of the International Scientific and Practical Conference
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Basaltic Rocks Analyzed by the Spirit Rover in Gusev Crater

2004

The Spirit landing site in Gusev Crater on Mars contains dark, fine-grained, vesicular rocks interpreted as lavas. Pancam and Mini–Thermal Emission Spectrometer (Mini-TES) spectra suggest that all of these rocks are similar but have variable coatings and dust mantles. Magnified images of brushed and abraded rock surfaces show alteration rinds and veins. Rock interiors contain ≤25% megacrysts. Chemical analyses of rocks by the Alpha Particle X-ray Spectrometer are consistent with picritic basalts, containing normative olivine, pyroxenes, plagioclase, and accessory FeTi oxides. Mössbauer, Pancam, and Mini-TES spectra confirm the presence of olivine, magnetite, and probably pyroxene. The…

Geologic SedimentsExtraterrestrial EnvironmentMagnesium CompoundsMarsMineralogyPyroxeneengineering.materialFeldsparSpectroscopy MossbauerPlagioclaseComposition of MarsBasaltMineralsgeographyMultidisciplinarygeography.geographical_feature_categoryOlivineSilicatesSpectrum AnalysisWaterOxidesVolcanic rockIgneous rockvisual_artengineeringvisual_art.visual_art_mediumIron CompoundsGeologyScience
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Concept of Biogenic Ferromanganese Crust Formation: Coccoliths as Bio-seeds in Crusts from Central Atlantic Ocean (Senghor Seamount/Cape Verde)

2011

At depths of 2,000 to 3,000 m, seamounts from the Cape Verde archipelago (Central Atlantic Ocean) are largely covered with ferromanganese crusts. Here we studied 60 to 150 mm thick crusts from the Senghor Seamount (depth: 2257.4 m). The crusts have a non lamellated texture and are covered with spherical nodules. The chemical composition shows a dominance of MnO2 (26.1%) and Fe2O3 (38.8%) with considerable amounts of Co (0.74%) and TiO2 (2.1%). Analysis by scanning electron probe microanalyzer (EPMA) revealed a well defined compositional zonation of micro-layers; the distribution pattern of Mn does not match that of Fe. Analysis by high resolution scanning electron microscopy (SEM) revealed…

Geologic SedimentsIronSeamountGeochemistryPlant ScienceElectron microprobeFerromanganeseCape verdeDrug DiscoveryAtlantic IslandsDominance (ecology)Atlantic OceanChemical compositionPharmacologyManganesegeographygeography.geographical_feature_categoryFossilsHaptophytaCrustGeneral MedicineComplementary and alternative medicineArchipelagoMicroscopy Electron ScanningGeologyElectron Probe MicroanalysisNatural Product Communications
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Mineralogy at Gusev Crater from the Mössbauer spectrometer on the Spirit Rover.

2004

Mössbauer spectra measured on Mars by the Spirit rover during the primary mission are characterized by two ferrous iron doublets (olivine and probably pyroxene) and a ferric iron doublet (tentatively associated to nanophase ferric iron oxide). Two sextets resulting from nonstoichiometric magnetite are also present, except for a coating on the rock Mazatzal, where a hematite-like sextet is present. Greater proportions of ferric-bearing phases are associated with undisturbed soils and rock surfaces as compared to fresh rock surfaces exposed by grinding. The ubiquitous presence of olivine in soil suggests that physical rather than chemical weathering processes currently dominate at Gusev crat…

Geologic SedimentsMaterials scienceExtraterrestrial EnvironmentIronMineralogyMagnesium CompoundsMarsWeatheringPyroxeneengineering.materialFerric CompoundsFerrouschemistry.chemical_compoundSpectroscopy MossbauerImpact craterComposition of MarsMagnetiteMineralsMultidisciplinaryOlivineSilicatesOxidesHematiteFerrosoferric Oxidechemistryvisual_artvisual_art.visual_art_mediumengineeringIron CompoundsScience (New York, N.Y.)
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Evidences of magma mixing in the "Daly gap" of the alkaline suites: a case study from the enclaves of Pantelleria (Italy)

2006

The island of Pantelleria consists of trachytes, pantellerites and minor mildly alkaline basalts. Rocks of intermediate composition (falling in the so-called ‘Daly Gap’) such as mugearites, benmoreites and mafic trachytes occur only in the form of enclaves in trachytes and pantellerites inside the main caldera of the island (Caldera ‘Cinque Denti’), which collapsed during the ‘Green Tuff ’ ignimbrite eruption at 50 ka. The enclaves include volcanic, subvolcanic and intrusive rock types. The enclaves in host trachyte contain traces of glass; devitrified glass occurs within enclaves in host pantellerites. Minerals in the enclaves show regular compositional variations with whole-rock silica co…

GeophysicsFelsicFractional crystallization (geology)Geochemistry and PetrologyGeochemistryTrachyteCalderaMineralogyIgneous differentiationMagma chamberMaficIntermediate compositionGeology
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Chemical abundances determined from meteor spectra: I. Ratios of the main chemical elements

2003

Relative chemical abundances of 13 meteoroids were determined by averaging the composition of the radiating gas along the fireball path that originated during their penetration into the Earth's atmosphere. Mg, Fe, Ni, Cr, Mn, and Co abundances, relative to Si, are similar to those reported for CI and CM carbonaceous chondrites and interplanetary dust particles. In contrast, relative abundances of Ca and Ti in meteor spectra indicate that these elements suffer incomplete evaporation processes. The chemical composition of all meteoroids studied in this work differs from that of 1P/Halley dust.

GeophysicsInterplanetary dust cloudMeteoroidSpace and Planetary ScienceChemistryChondriteAnalytical chemistryChemical compositionSpectral lineAstrobiologyMeteoritics & Planetary Science
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