Search results for "PLASMA"

showing 10 items of 4043 documents

Sequence-Specific Repression of Cotranslational Translocation of the Hepatitis B Virus Envelope Proteins Coincides with Binding of Heat Shock Protein…

1997

AbstractThe large L envelope protein of the hepatitis B virus has the peculiar capacity to adopt two transmembrane topologies. The N-terminal preS domain of L initially remains in the cytosol while the S domain is cotranslationally inserted into the endoplasmic reticulum membrane. The preS region of about half of the L molecules is posttranslationally translocated to the lumenal space. We now demonstrate that the repression of cotranslational translocation of preS is conferred by a preS1-specific sequence. By analysis of L deletion mutants, the cytosolic anchorage determinant was mapped to amino acid sequence 70 to 94 of L. The intrinsic potential of this determinant to suppress cotranslati…

Hepatitis B virusHSC70 Heat-Shock ProteinsRecombinant Fusion ProteinsPlasma protein bindingBiologyGenes envCytosolViral Envelope ProteinsHeat shock proteinVirologyHumansHSP70 Heat-Shock ProteinsBinding sitePromoter Regions GeneticPeptide sequenceBinding SitesBase SequenceCell-Free SystemEndoplasmic reticulumHSC70 Heat-Shock ProteinsOligonucleotides AntisenseMolecular biologyTransmembrane proteinChaperone (protein)Protein Biosynthesisbiology.proteinMutagenesis Site-DirectedMetallothioneinCarrier ProteinsProtein BindingVirology
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Mosaic particles formed by wild-type hepatitis B virus core protein and its deletion variants consist of both homo- and heterodimers.

2003

AbstractCo-expression in Escherichia coli of wild-type (wt) hepatitis B virus core protein (HBc) and its naturally occurring variants with deletions at amino acid positions 77–93 or 86–93 leads to formation of mosaic particles, which consist of three dimer subunit compositions. These compositions are wt/variant HBc heterodimers and two types of homodimers, formed by wt HBc or the variant HBc themselves. Mosaic particles were found also when both HBc deletion variants 77–93 and 86–93 were co-expressed in E. coli. These findings are discussed in terms of their significance for hepatitis B virus pathogenesis and prospective use of mosaic particles in vaccine development.

Hepatitis B virusvirusesProtein subunitDimerBiophysicsExpressionPlasma protein bindingBiologymedicine.disease_causeMosaic particlesBiochemistrychemistry.chemical_compoundHepatitis B virus core proteinProtein structureStructural Biologyparasitic diseasesGeneticsmedicineHepatitis B VaccinesCloning MolecularProtein Structure QuaternaryMolecular BiologyEscherichia coliSequence Deletionchemistry.chemical_classificationHepatitis B virusViral Core ProteinsWild typevirus diseasesGenetic VariationCell BiologyHepatitis BDimer formationVirologyMolecular biologydigestive system diseasesAmino acidProtein SubunitschemistryDimerizationProtein BindingFEBS letters
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Soluble adhesion molecules correlate with liver inflammation and fibrosis in chronic hepatitis C treated with interferon-α

1998

Background: In chronic hepatitis C the relation of circulating adhesion molecules to disease features before, during and after therapy has not been completely established. Aim: To analyse the basal levels of circulating adhesins and the changes induced by interferon in these patients. Methods: We studied, using ELISA assays, the serum levels of soluble intercellular adhesion molecule-1 (sICAM-1) and vascular cell adhesion molecule-1 (sVCAM-1) in 52 patients with chronic hepatitis C on entry, prior to finalizing a 6-month course of interferon-α therapy and at the end of the follow-up. Correlations with clinical, virological and histological features, including inflammation and fibrosis, were…

HepatitisHepatologybiologybusiness.industryCell adhesion moleculeHepacivirusmedicine.medical_treatmentHepatitis C virusGastroenterologymedicine.diseasebiology.organism_classificationmedicine.disease_causeCytokineFibrosisInterferonBlood plasmaImmunologyMedicinePharmacology (medical)businessmedicine.drugAlimentary Pharmacology & Therapeutics
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The new murine hepatic 3A cell line responds to stress stimuli by activating an efficient Unfolded Protein Response (UPR)

2012

In the present study we have investigated the properties of a novel cell line (3A cells) obtained from the liver of 14.5. days post coitum (dpc) wild-type mouse embryo. 3A cells morphology was characterized by fluorescent localization of F-actin and β-catenin. The expression of specific genes and proteins essential to liver function in these cells was comparable or even more efficient then in the differentiated hepatocytic cell line MMH-D6. 3A cells also showed the capability to excrete molecules in extracellular spaces resembling functional bile canaliculi, glycogen storage activity and the ability to control retinol-binding protein 4 secretion in response to retinol deprivation. Their re…

Hepatocytes; ER stress; RBP4BiologyToxicologyCellular modelCell LineMicechemistry.chemical_compoundStress PhysiologicalExtracellularAnimalsHepatocyteSecretionActinbeta CateninAnimalReverse Transcriptase Polymerase Chain ReactionRBP4Gene Expression ProfilingTunicamycinDays post coitumCellular model; ER stress; Hepatocytes; RBP4; Actins; Animals; Cell Line; Fluorescein; Gene Expression Profiling; Glycogen; Liver; Retinol-Binding Proteins Plasma; Reverse Transcriptase Polymerase Chain Reaction; Stress Physiological; Tunicamycin; Unfolded Protein Response; beta Catenin; Mice; ToxicologyGeneral MedicineTunicamycinMolecular biologyActinsLiverchemistryCell cultureUnfolded Protein ResponseUnfolded protein responseER streFluoresceinLiver functionCellular modelRetinol-Binding Proteins PlasmaGlycogenToxicology in Vitro
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Avoiding Boundary Effects in Wang-Landau Sampling

2003

A simple modification of the ``Wang-Landau sampling'' algorithm removes the systematic error that occurs at the boundary of the range of energy over which the random walk takes place in the original algorithm.

Heterogeneous random walk in one dimensionStatistical Mechanics (cond-mat.stat-mech)Rejection samplingFOS: Physical sciencesSlice samplingSampling (statistics)Boundary (topology)Random walk01 natural sciences010305 fluids & plasmasCombinatorics0103 physical sciencesRange (statistics)Applied mathematics010306 general physicsEnergy (signal processing)Condensed Matter - Statistical MechanicsMathematics
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Atmospheric pressure plasma polymerisation of metalloporphyrins containing mesoporous membranes for gas sensing applications

2013

Abstract Metalloporphyrins are embedded in an organosilicon matrix by an easily up-scalable atmospheric pressure dielectric barrier discharge method. The integrity of the metalloporphyrins, followed by UV–visible spectroscopy, is successfully preserved and their aggregation prevented. The single molecule properties, rather than the bulk ones, are thus enhanced. Exposure to triethylamine, which reaches the metalloporphyrins through the pores of the organosilicon membrane, led to a shift in the absorption spectrum and confirms the gas sensing potential of such coatings.

HexamethyldisiloxaneMaterials scienceAbsorption spectroscopyAtmospheric pressureAtmospheric-pressure plasmaSurfaces and InterfacesGeneral ChemistryDielectric barrier dischargeCondensed Matter PhysicsSurfaces Coatings and Filmschemistry.chemical_compoundMembraneChemical engineeringchemistryMaterials ChemistryOrganic chemistryMesoporous materialOrganosiliconSurface and Coatings Technology
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The supernova remnant SN 1006 as a Galactic particle accelerator

2022

The origin of cosmic rays is a pivotal open issue of high-energy astrophysics. Supernova remnants are strong candidates to be the Galactic factory of cosmic rays, their blast waves being powerful particle accelerators. However, supernova remnants can power the observed flux of cosmic rays only if they transfer a significant fraction of their kinetic energy to the accelerated particles, but conclusive evidence for such efficient acceleration is still lacking. In this scenario, the shock energy channeled to cosmic rays should induce a higher post-shock density than that predicted by standard shock conditions. Here we show this effect, and probe its dependence on the orientation of the ambient…

High Energy Astrophysical Phenomena (astro-ph.HE)Astrophysical plasmasSHARPHorizon 2020MultidisciplinaryFOS: Physical sciencesGeneral Physics and Astronomyshock wavesGeneral ChemistryGeneral Biochemistry Genetics and Molecular BiologyHigh-energy astrophysicsSettore FIS/05 - Astronomia E AstrofisicaEuropean Union (EU)Particle astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical Phenomenacosmic rayNature Communications
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Unveiling the spatial structure of the overionized plasma in the supernova remnant W49B

2011

W49B is a mixed-morphology supernova remnant with thermal X-ray emission dominated by the ejecta. In this remnant, the presence of overionized plasma has been directly established, with information about its spatial structure. However, the physical origin of the overionized plasma in W49B has not yet been understood. We investigate this intriguing issue through a 2D hydrodynamic model that takes into account, for the first time, the mixing of ejecta with the inhomogeneous circumstellar and interstellar medium, the thermal conduction, the radiative losses from optically thin plasma, and the deviations from equilibrium of ionization induced by plasma dynamics. The model was set up on the basi…

High Energy Astrophysical Phenomena (astro-ph.HE)ISM: individual objects: W49BPhysics::Plasma PhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics - High Energy Astrophysical PhenomenaISM: individual objects: G43.3-0.2Astrophysics::Galaxy Astrophysicshydrodynamicmethods: numericalISM: supernova remnants
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Computational general relativistic force-free electrodynamics

2021

Scientific codes are an indispensable link between theory and experiment; in (astro-)plasma physics, such numerical tools are one window into the universe's most extreme flows of energy. The discretization of Maxwell's equations - needed to make highly magnetized (astro)physical plasma amenable to its numerical modeling - introduces numerical diffusion. It acts as a source of dissipation independent of the system's physical constituents. Understanding the numerical diffusion of scientific codes is the key to classify their reliability. It gives specific limits in which the results of numerical experiments are physical. We aim at quantifying and characterizing the numerical diffusion propert…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsDiscretizationWaves in plasmasFOS: Physical sciencesAstronomy and AstrophysicsContext (language use)PlasmaComputational Physics (physics.comp-ph)Numerical diffusionDissipation01 natural sciencesMagnetic fieldCurrent sheetSpace and Planetary ScienceQuantum electrodynamics0103 physical sciencesAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysics010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Physics - Computational Physics010303 astronomy & astrophysicsAstronomy & Astrophysics
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Spatial identification of the overionized plasma in W49B

2010

Recent Suzaku X-ray observations of the ejecta-dominated supernova remnant W49B have shown that in the global spectrum there is a clear indication for the presence of overionized plasma whose physical origin is still under debate. In order to ascertain the physical origin of such a rapidly cooling plasma, we focus on the study of its spatial localization within the X-ray emitting ejecta. We confirm the presence of a saw-edged excess (interpreted as a strong radiative recombination continuum) in the global spectrum above 8 keV, emerging above the ionization-equilibrium model. We produce a hardness ratio map to determine where the plasma is overionized and we perform a spectral analysis of th…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsHardness ratioAstrophysics::High Energy Astrophysical PhenomenaInterstellar cloudFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsPlasmaX-rays: ISM ISM: supernova remnants ISM: individual object: W49BSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceSpontaneous emissionSpectral analysisSpatial localizationAstrophysics - High Energy Astrophysical PhenomenaEjectaSupernova remnantISM ISM: supernova remnants ISM: individual object: W49B [X-rays]Astrophysics::Galaxy Astrophysics
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