SPACE SCIENCE REVIEWS, ISSN 0038-6308, 10/2013, Volume 178, Issue 2-4, pp. 141 - 162
Various aspects of the magnetism of the quiet sun are reviewed. The suggestion that a small scale dynamo acting at granular scales generates what we call the...
TELESCOPE | Turbulent dynamo | PRANDTL NUMBERS | HINODE OBSERVATIONS | QUIET-SUN INTERNETWORK | HORIZONTAL MAGNETIC-FIELDS | SCALE TURBULENT DYNAMO | MAGNETOCONVECTION | ASTRONOMY & ASTROPHYSICS | CONVECTION ZONE | Quiet Sun magnetism | SIMULATIONS | POLARIZATION
TELESCOPE | Turbulent dynamo | PRANDTL NUMBERS | HINODE OBSERVATIONS | QUIET-SUN INTERNETWORK | HORIZONTAL MAGNETIC-FIELDS | SCALE TURBULENT DYNAMO | MAGNETOCONVECTION | ASTRONOMY & ASTROPHYSICS | CONVECTION ZONE | Quiet Sun magnetism | SIMULATIONS | POLARIZATION
Journal Article
Astrophysical Journal, Supplement Series, ISSN 0067-0049, 03/2017, Volume 229, Issue 1, pp. 8 - 8
Convective flows are known as the prime means of transporting magnetic fields on the solar surface. Thus, small magnetic structures are good tracers of...
methods: observational | Sun: magnetic fields | Sun: photosphere | TELESCOPE | DISPERSAL | ELEMENTS | 2-SAMPLE TRIMMED T | MOTION | QUIET-SUN | ASTRONOMY & ASTROPHYSICS | DYNAMICS | DIFFUSION | POINTS | INTERNETWORK | Confidence intervals | Photosphere | Diffusion rate | Kinematics | Emergence | Flux | Diffusion | Dispersion | Physics - Solar and Stellar Astrophysics
methods: observational | Sun: magnetic fields | Sun: photosphere | TELESCOPE | DISPERSAL | ELEMENTS | 2-SAMPLE TRIMMED T | MOTION | QUIET-SUN | ASTRONOMY & ASTROPHYSICS | DYNAMICS | DIFFUSION | POINTS | INTERNETWORK | Confidence intervals | Photosphere | Diffusion rate | Kinematics | Emergence | Flux | Diffusion | Dispersion | Physics - Solar and Stellar Astrophysics
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2012, Volume 542, p. A112
Context. Paper I presents the magnetic structure, inferred for the photosphere and the chromosphere, of a filament that developed in active region (AR) NOAA...
Sun: filaments prominences | Techniques: polarimetric | Sun: photosphere | Sun: faculae plages | Sun: chromosphere | SUPERSONIC DOWNFLOWS | MAGNETIC-FIELDS | CORONAL RAIN | Sun: faculae, plages | TWISTED FLUX TUBE | SOLAR FILAMENTS | STOKES PROFILES | Sun: filaments, prominences | HELICAL FLUX | ASTRONOMY & ASTROPHYSICS | CONVECTION ZONE | H-ALPHA FILAMENTS | techniques: polarimetric | DELTA-SUNSPOT | Physics - Solar and Stellar Astrophysics
Sun: filaments prominences | Techniques: polarimetric | Sun: photosphere | Sun: faculae plages | Sun: chromosphere | SUPERSONIC DOWNFLOWS | MAGNETIC-FIELDS | CORONAL RAIN | Sun: faculae, plages | TWISTED FLUX TUBE | SOLAR FILAMENTS | STOKES PROFILES | Sun: filaments, prominences | HELICAL FLUX | ASTRONOMY & ASTROPHYSICS | CONVECTION ZONE | H-ALPHA FILAMENTS | techniques: polarimetric | DELTA-SUNSPOT | Physics - Solar and Stellar Astrophysics
Journal Article
The Astrophysical Journal Letters, ISSN 2041-8205, 11/2010, Volume 723, Issue 2, pp. L169 - L174
Bright points (BPs) are manifestations of small magnetic elements in the solar photosphere. Their brightness contrast not only gives insight into the thermal...
Techniques: photometric | Techniques: polarimetric | Sun: photosphere | Sun: magnetic topology | Techniques: spectroscopic | MAGNETIC-FIELDS | techniques: photometric | RECONSTRUCTION | SOLAR IRRADIANCE VARIATIONS | ELEMENTS | FACULAE | CONTRAST ANALYSIS | CYCLE-23 | techniques: spectroscopic | ASTRONOMY & ASTROPHYSICS | SURFACE | techniques: polarimetric | Physics - Solar and Stellar Astrophysics | WAVELENGTHS | MAIN SEQUENCE STARS | PHOTOSPHERE | SOLAR ATMOSPHERE | STELLAR ATMOSPHERES | SUN | ATMOSPHERES | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | CHROMOSPHERE | PHYSICAL PROPERTIES | OPTICAL PROPERTIES | STARS | BRIGHTNESS
Techniques: photometric | Techniques: polarimetric | Sun: photosphere | Sun: magnetic topology | Techniques: spectroscopic | MAGNETIC-FIELDS | techniques: photometric | RECONSTRUCTION | SOLAR IRRADIANCE VARIATIONS | ELEMENTS | FACULAE | CONTRAST ANALYSIS | CYCLE-23 | techniques: spectroscopic | ASTRONOMY & ASTROPHYSICS | SURFACE | techniques: polarimetric | Physics - Solar and Stellar Astrophysics | WAVELENGTHS | MAIN SEQUENCE STARS | PHOTOSPHERE | SOLAR ATMOSPHERE | STELLAR ATMOSPHERES | SUN | ATMOSPHERES | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | CHROMOSPHERE | PHYSICAL PROPERTIES | OPTICAL PROPERTIES | STARS | BRIGHTNESS
Journal Article
The Astrophysical Journal Letters, ISSN 2041-8205, 11/2010, Volume 723, Issue 2, pp. L139 - L143
We characterize the observational properties of the convectively driven vortex flows recently discovered on the quiet Sun, using magnetograms, Dopplergrams,...
Sun: granulation | Sun: photosphere | Convection | Sun: surface magnetism | convection | BRIGHT POINTS | ASTRONOMY & ASTROPHYSICS | DYNAMICS | GRANULATION | DIVERSITY | MOTIONS | SOLAR PHOTOSPHERE | Physics - Solar and Stellar Astrophysics | ROTATION | TELESCOPES | AIRCRAFT | BALLOONS | SOLAR GRANULATION | MAIN SEQUENCE STARS | SOLAR ACTIVITY | CONVECTION | PHOTOSPHERE | SOLAR ATMOSPHERE | VORTEX FLOW | HEAT TRANSFER | STELLAR ATMOSPHERES | SUN | ATMOSPHERES | MAGNETISM | MASS TRANSFER | STELLAR ACTIVITY | ENERGY TRANSFER | MOTION | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | PROPER MOTION | STARS | FLUID FLOW
Sun: granulation | Sun: photosphere | Convection | Sun: surface magnetism | convection | BRIGHT POINTS | ASTRONOMY & ASTROPHYSICS | DYNAMICS | GRANULATION | DIVERSITY | MOTIONS | SOLAR PHOTOSPHERE | Physics - Solar and Stellar Astrophysics | ROTATION | TELESCOPES | AIRCRAFT | BALLOONS | SOLAR GRANULATION | MAIN SEQUENCE STARS | SOLAR ACTIVITY | CONVECTION | PHOTOSPHERE | SOLAR ATMOSPHERE | VORTEX FLOW | HEAT TRANSFER | STELLAR ATMOSPHERES | SUN | ATMOSPHERES | MAGNETISM | MASS TRANSFER | STELLAR ACTIVITY | ENERGY TRANSFER | MOTION | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | PROPER MOTION | STARS | FLUID FLOW
Journal Article
Nucleic Acids Research, ISSN 0305-1048, 10/2009, Volume 38, Issue 1, pp. D142 - D148
The primary mission of UniProt is to support biological research by maintaining a stable, comprehensive, fully classified, richly and accurately annotated...
ANNOTATION | ARCHIVE | BIOCHEMISTRY & MOLECULAR BIOLOGY | SEQUENCE | Genome, Viral | Computational Biology - methods | Information Storage and Retrieval - methods | Europe | Humans | Computational Biology - trends | Proteome | Algorithms | Animals | Genome, Fungal | Databases, Protein | Protein Isoforms | Proteomics | Software | Internet | Databases, Nucleic Acid
ANNOTATION | ARCHIVE | BIOCHEMISTRY & MOLECULAR BIOLOGY | SEQUENCE | Genome, Viral | Computational Biology - methods | Information Storage and Retrieval - methods | Europe | Humans | Computational Biology - trends | Proteome | Algorithms | Animals | Genome, Fungal | Databases, Protein | Protein Isoforms | Proteomics | Software | Internet | Databases, Nucleic Acid
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2013, Volume 558, pp. A30 - np
contex. Localized strongly Doppler-shifted Stokes V signals were detected by IMaX/SUNRISE. These signals are related to newly emerged magnetic loops that are...
Sun: granulation | Sun: photosphere | Sun: surface magnetism | INSTABILITY | MISSION | FLUX TUBES | SHOCKS | CONVECTIVE COLLAPSE | SOLAR PHOTOSPHERE | HORIZONTAL MAGNETIC-FIELDS | SUNRISE/IMAX | ASTRONOMY & ASTROPHYSICS | GRANULAR-CELLS | INTERNETWORK | Mathematical analysis | Small scale | Fluid flow | Linear polarization | Sunrise | Doppler effect | Temporal logic | Astronomy | Physics - Solar and Stellar Astrophysics
Sun: granulation | Sun: photosphere | Sun: surface magnetism | INSTABILITY | MISSION | FLUX TUBES | SHOCKS | CONVECTIVE COLLAPSE | SOLAR PHOTOSPHERE | HORIZONTAL MAGNETIC-FIELDS | SUNRISE/IMAX | ASTRONOMY & ASTROPHYSICS | GRANULAR-CELLS | INTERNETWORK | Mathematical analysis | Small scale | Fluid flow | Linear polarization | Sunrise | Doppler effect | Temporal logic | Astronomy | Physics - Solar and Stellar Astrophysics
Journal Article
Communications in Mathematical Physics, ISSN 0010-3616, 1/2018, Volume 357, Issue 1, pp. 77 - 123
We study entropy production (EP) in processes involving repeated quantum measurements of finite quantum systems. Adopting a dynamical system approach, we...
Quantum Physics | Mathematical Physics | Classical and Quantum Gravitation, Relativity Theory | Theoretical, Mathematical and Computational Physics | Complex Systems | Physics | MULTIFRACTAL ANALYSIS | LYAPUNOV EXPONENTS | PRESSURE FUNCTION | STATES | MECHANICS | SYMMETRY | ADDITIVE THERMODYNAMIC FORMALISM | INFORMATION | FLUCTUATION THEOREM | DYNAMICAL ENSEMBLES | PHYSICS, MATHEMATICAL | Measurement | Thermodynamics | Analysis | Probability | Mathematics | Statistics
Quantum Physics | Mathematical Physics | Classical and Quantum Gravitation, Relativity Theory | Theoretical, Mathematical and Computational Physics | Complex Systems | Physics | MULTIFRACTAL ANALYSIS | LYAPUNOV EXPONENTS | PRESSURE FUNCTION | STATES | MECHANICS | SYMMETRY | ADDITIVE THERMODYNAMIC FORMALISM | INFORMATION | FLUCTUATION THEOREM | DYNAMICAL ENSEMBLES | PHYSICS, MATHEMATICAL | Measurement | Thermodynamics | Analysis | Probability | Mathematics | Statistics
Journal Article
Astrophysical Journal, ISSN 0004-637X, 12/2015, Volume 815, Issue 1, p. 10
Our aim is to model the three-dimensional magnetic field structure of the upper solar atmosphere, including regions of non-negligible plasma beta. We use...
numerical | Sun:hotosphere | Sun: corona | Sun: magnetic fields | Sun: chromosphere | FIELD | EQUATIONS | Sun: photosphere | methods: numerical | 3-DIMENSIONAL MAGNETOHYDROSTATIC EQUILIBRIA | CYLINDRICAL GEOMETRY | ASTRONOMY & ASTROPHYSICS | SPHERICAL GEOMETRY | COMPUTATION | MINIMUM CORONA | QUIET SUN | Photosphere | Gravitation | Nonlinearity | Solar atmosphere | Sunrise | Lorentz force | Magnetic fields | Density | Physics - Solar and Stellar Astrophysics | MAGNETIC FIELDS | LORENTZ FORCE | ELECTRIC CURRENTS | PHOTOSPHERE | RESOLUTION | SUN | COMPUTERIZED SIMULATION | DENSITY | PLASMA | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | NONLINEAR PROBLEMS | CHROMOSPHERE | GRAVITATION | PRESSURE GRADIENTS
numerical | Sun:hotosphere | Sun: corona | Sun: magnetic fields | Sun: chromosphere | FIELD | EQUATIONS | Sun: photosphere | methods: numerical | 3-DIMENSIONAL MAGNETOHYDROSTATIC EQUILIBRIA | CYLINDRICAL GEOMETRY | ASTRONOMY & ASTROPHYSICS | SPHERICAL GEOMETRY | COMPUTATION | MINIMUM CORONA | QUIET SUN | Photosphere | Gravitation | Nonlinearity | Solar atmosphere | Sunrise | Lorentz force | Magnetic fields | Density | Physics - Solar and Stellar Astrophysics | MAGNETIC FIELDS | LORENTZ FORCE | ELECTRIC CURRENTS | PHOTOSPHERE | RESOLUTION | SUN | COMPUTERIZED SIMULATION | DENSITY | PLASMA | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | NONLINEAR PROBLEMS | CHROMOSPHERE | GRAVITATION | PRESSURE GRADIENTS
Journal Article
Space Science Reviews, ISSN 0038-6308, 9/2017, Volume 210, Issue 1, pp. 317 - 349
We present a contemporary view of how solar active region magnetic fields are understood to be generated, transported and dispersed. Empirical trends of active...
Astrophysics and Astroparticles | Planetology | Active region | MHD | Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics) | Magnetic fields | Aerospace Technology and Astronautics | Sun | Sunspots | Physics | TORSIONAL OSCILLATION | EMERGING FLUX TUBES | COOL STARS | MAIN-SEQUENCE | EMERGENCE | DIFFERENTIAL ROTATION | HELICITY | ASTRONOMY & ASTROPHYSICS | SOLAR CONVECTION ZONE | VECTOR MAGNETOGRAPH DATA | Atmospheric research | Analysis | Astronomy | Evolution | Solar magnetic field | Life cycles
Astrophysics and Astroparticles | Planetology | Active region | MHD | Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics) | Magnetic fields | Aerospace Technology and Astronautics | Sun | Sunspots | Physics | TORSIONAL OSCILLATION | EMERGING FLUX TUBES | COOL STARS | MAIN-SEQUENCE | EMERGENCE | DIFFERENTIAL ROTATION | HELICITY | ASTRONOMY & ASTROPHYSICS | SOLAR CONVECTION ZONE | VECTOR MAGNETOGRAPH DATA | Atmospheric research | Analysis | Astronomy | Evolution | Solar magnetic field | Life cycles
Journal Article
Astrophysical Journal, ISSN 0004-637X, 03/2012, Volume 748, Issue 1, pp. 23 - 12
The three-dimensional structure of an active region filament is studied using nonlinear force-free field extrapolations based on simultaneous observations at a...
Sun: filaments, prominences | Sun: magnetic topology | Sun: activity | CORONAL MAGNETIC-FIELDS | MHD SIMULATIONS | TWISTED FLUX TUBE | EMERGENCE | VECTOR | ROPE | MODELS | HELICAL FLUX | ASTRONOMY & ASTROPHYSICS | CONVECTION ZONE | SOLAR PROMINENCES | Extrapolation | Photosphere | Solar surface | Filaments | Magnetic structure | Deviation | Three dimensional | Ambiguity | MAGNETIC FIELDS | TELESCOPES | POLARIMETERS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | NONLINEAR PROBLEMS | SOLAR ACTIVITY | PHOTOSPHERE | SIGNALS | THREE-DIMENSIONAL CALCULATIONS | SUN
Sun: filaments, prominences | Sun: magnetic topology | Sun: activity | CORONAL MAGNETIC-FIELDS | MHD SIMULATIONS | TWISTED FLUX TUBE | EMERGENCE | VECTOR | ROPE | MODELS | HELICAL FLUX | ASTRONOMY & ASTROPHYSICS | CONVECTION ZONE | SOLAR PROMINENCES | Extrapolation | Photosphere | Solar surface | Filaments | Magnetic structure | Deviation | Three dimensional | Ambiguity | MAGNETIC FIELDS | TELESCOPES | POLARIMETERS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | NONLINEAR PROBLEMS | SOLAR ACTIVITY | PHOTOSPHERE | SIGNALS | THREE-DIMENSIONAL CALCULATIONS | SUN
Journal Article
HIV Medicine, ISSN 1464-2662, 03/2018, Volume 19, Issue 3, pp. 238 - 242
Objectives The aim of the study was to determine whether there is a relationship between social deprivation and time of HIV diagnosis in France. Methods...
deprivation | late diagnosis | key population | HIV | age | INFECTIOUS DISEASES | Heterosexuality - statistics & numerical data | Prospective Studies | Health Status Disparities | Humans | Middle Aged | Risk Factors | HIV Infections - psychology | Logistic Models | Male | Delayed Diagnosis - statistics & numerical data | Socioeconomic Factors | HIV Infections - diagnosis | Adult | Female | France | Homosexuality, Male - statistics & numerical data | Medicine, Experimental | Medical research | HIV (Viruses) | Analysis | Deprivation | Statistical analysis | Infections | Regression analysis | Gender | Patients | Data bases | Strong interactions (field theory) | Confidence intervals | Hepatitis | Sexually transmitted diseases | Databases | Men | Ecological monitoring | Quartiles | Diagnosis | Hepatitis B virus | Hepatitis B
deprivation | late diagnosis | key population | HIV | age | INFECTIOUS DISEASES | Heterosexuality - statistics & numerical data | Prospective Studies | Health Status Disparities | Humans | Middle Aged | Risk Factors | HIV Infections - psychology | Logistic Models | Male | Delayed Diagnosis - statistics & numerical data | Socioeconomic Factors | HIV Infections - diagnosis | Adult | Female | France | Homosexuality, Male - statistics & numerical data | Medicine, Experimental | Medical research | HIV (Viruses) | Analysis | Deprivation | Statistical analysis | Infections | Regression analysis | Gender | Patients | Data bases | Strong interactions (field theory) | Confidence intervals | Hepatitis | Sexually transmitted diseases | Databases | Men | Ecological monitoring | Quartiles | Diagnosis | Hepatitis B virus | Hepatitis B
Journal Article
Pediatric Rheumatology, ISSN 1546-0096, 05/2017, Volume 15, Issue S1
Journal Article
Astrophysical Journal, Supplement Series, ISSN 0067-0049, 03/2017, Volume 229, Issue 1, pp. 11 - 11
A dense forest of slender bright fibrils near a small solar active region is seen in high-quality narrowband Ca II H images from the SuFI instrument onboard...
methods: observational | Sun: magnetic fields | Sun: chromosphere | ACTIVE REGIONS | PHASE-DIVERSITY | FLUX TUBES | RADIATIVE-TRANSFER | TORSIONAL MOTIONS | K-LINE | DISK COUNTERPART | MG-I | ASTRONOMY & ASTROPHYSICS | CONVECTION ZONE | NUMERICAL SIMULATIONS | Field strength | Photosphere | Chromosphere | Computer simulation | Inversions | Sunrise | Magnetic fields | Onboard | Physics - Solar and Stellar Astrophysics | MAGNETIC FIELDS | BALLOONS | MAGNETIC FIELD CONFIGURATIONS | SOLAR ACTIVITY | CALCIUM IONS | PHOTOSPHERE | MAGNETOHYDRODYNAMICS | SUN | EXTRAPOLATION | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | IMAGES | CHROMOSPHERE | ORIENTATION | MAPPING
methods: observational | Sun: magnetic fields | Sun: chromosphere | ACTIVE REGIONS | PHASE-DIVERSITY | FLUX TUBES | RADIATIVE-TRANSFER | TORSIONAL MOTIONS | K-LINE | DISK COUNTERPART | MG-I | ASTRONOMY & ASTROPHYSICS | CONVECTION ZONE | NUMERICAL SIMULATIONS | Field strength | Photosphere | Chromosphere | Computer simulation | Inversions | Sunrise | Magnetic fields | Onboard | Physics - Solar and Stellar Astrophysics | MAGNETIC FIELDS | BALLOONS | MAGNETIC FIELD CONFIGURATIONS | SOLAR ACTIVITY | CALCIUM IONS | PHOTOSPHERE | MAGNETOHYDRODYNAMICS | SUN | EXTRAPOLATION | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | IMAGES | CHROMOSPHERE | ORIENTATION | MAPPING
Journal Article