The table below shows the most common keywords used by the author. The letters in brackets after some keywords denote if the keyword corresponds to Solar Physics (S) or Heliospheric Physics (H).
| Keyword
| Occurrences
|
|---|
| Sun: Corona [S]
| 87
|
| Solar Wind [H]
| 38
|
| Astrophysics
| 33
|
| Solar Physics [S]
| 31
|
| Sun: Solar Wind [H]
| 23
|
| Sun: Filaments [S]
| 21
|
| And Astronomy: Corona
| 17
|
| Interplanetary Physics: Solar Wind Plasma [H]
| 16
|
| Coronal Holes
| 16
|
| Interplanetary Physics: Sources Of The Solar Wind
| 11
|
| Sun: Magnetic Fields
| 10
|
| Sun: UV Radiation [S]
| 10
|
| Sun: Coronal Mass Ejections
| 9
|
| Magnetohydrodynamic Waves
| 9
|
| Solar Eclipses
| 9
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 9
|
| Eclipses
| 8
|
| And Astronomy: Coronal Holes
| 8
|
| Particle Emission Solar Wind [H]
| 8
|
| Solar Coronal Streamers
| 7
|
| Sun: Solar Corona
| 6
|
| Sources Of Solar Wind
| 5
|
| Space Plasma Physics: Wave/particle Interactions
| 5
|
| Electron Energy
| 5
|
| Solar Wind Plasma [H]
| 5
|
| Space Plasma Physics: Numerical Simulation Studies
| 5
|
| Line: Profiles
| 5
|
| Solar Optical Telescopes
| 4
|
| Sun: Chromosphere [S]
| 4
|
| Solar Magnetic Field
| 4
|
| Magnetohydrodynamics [S]
| 4
|
| Interplanetary Physics: Mhd Waves And Turbulence
| 4
|
| Solar Cycle
| 4
|
| Stellar Winds
| 4
|
| Sun: Heliosphere [H]
| 4
|
| Sun: Activity
| 4
|
| Lyman Alpha Radiation
| 3
|
| Solar Limb
| 3
|
| Visible
| 3
|
| Interplanetary Turbulence [H]
| 3
|
| Solar Electromagnetic Emission
| 3
|
| Interplanetary Physics: Plasma Waves And Turbulence
| 3
|
| Interplanetary Medium [H]
| 3
|
| Interplanetary Magnetic Fields [H]
| 3
|
| Sun: Spatial Distribution
| 3
|
| Solar Coronal Holes [S]
| 3
|
| Solar Activity
| 3
|
| Shock Waves
| 3
|
| Shock Wave Propagation
| 3
|
| Space Plasmas [H]
| 3
|
| And Astronomy
| 3
|
| Space Plasma Physics: Turbulence
| 3
|
| Total Eclipses
| 3
|
| Plasma Heating
| 3
|
| Solar Wind Velocity
| 3
|
| Sun: Extreme Ultraviolet Radiation
| 3
|
| Chromosphere
| 3
|
| The Sun [S]
| 3
|
| Mathematical Models
| 3
|
| Solar Radio Emission
| 3
|
| Astronomical Models
| 3
|
| Magnetohydrodynamic Flow
| 3
|
| Extreme Ultraviolet Radiation
| 3
|
| Helium Abundance
| 2
|
| Sun: Abundances
| 2
|
| Polarization
| 2
|
| Sun: Transition Region [S]
| 2
|
| Plasmas
| 2
|
| Sun: Temporal Distribution
| 2
|
| Astronomical Techniques
| 2
|
| Coronas
| 2
|
| Instabilities [H]
| 2
|
| Sun: Line Spectra
| 2
|
| Magnetohydrodynamic And Fluid Equation
| 2
|
| Plasma Dynamics
| 2
|
| Plasma Density
| 2
|
| Ultraviolet Emission
| 2
|
| Waves
| 2
|
| Iron Isotopes
| 2
|
| Ism: Dust
| 2
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 2
|
| Nanocrystals And Nanoparticles
| 2
|
| Line Spectra
| 2
|
| Temperature
| 2
|
| Centimeter Waves
| 2
|
| Solar Temperature
| 2
|
| Sun: Atmosphere [S]
| 2
|
| Methods: Numerical
| 2
|
| Loops
| 2
|
| Sun: Particle Emission
| 2
|
| Techniques: Image Processing
| 2
|
| Line Of Sight
| 2
|
| Extinction
| 2
|
| Sun: Infrared
| 2
|
| Remote Observing Techniques
| 2
|
| Radio Astronomy
| 2
|
| Electronic Structure Of Nanoscale Materials: Clusters Nanoparticles Nanotubes And Nanocrystals
| 2
|
| Transonic Flow
| 2
|
| Magnetic Fields
| 2
|
| Space Plasma Physics: Transport Processes
| 2
|
| Sun: Oscillations [S]
| 2
|
| Spectroscopy
| 2
|
| Propagation Modes
| 2
|
| Radio Science: Remote Sensing
| 1
|
| Radio Science: Radio Wave Propagation
| 1
|
| Radio Radiation:solar Corona
| 1
|
| Radiative Transfer [S]
| 1
|
| Quiet Solar Corona
| 1
|
| Publicly Available Software
| 1
|
| Proton Energy
| 1
|
| Polytropic Processes
| 1
|
| Polar Regions
| 1
|
| Plasma-particle Interactions
| 1
|
| Plasma Temperature
| 1
|
| Plasma Jets
| 1
|
| Physics - Space Physics [H]
| 1
|
| Photosphere [S]
| 1
|
| Numerical Integration
| 1
|
| Neutral Gases
| 1
|
| Momentum
| 1
|
| Methods: Statistical
| 1
|
| Methods: Observational
| 1
|
| Methods: Data Analysis
| 1
|
| Mapping
| 1
|
| Magnetohydrodynamics And Plasmas
| 1
|
| Magnetohydrodynamic Stability
| 1
|
| Magnetic Flux
| 1
|
| Magnetic Fields:solar Corona
| 1
|
| Magnetic Field Configurations
| 1
|
| Magnetic Dipoles
| 1
|
| Lines Of Force
| 1
|
| Linear Polarization
| 1
|
| Line: Identification
| 1
|
| Iue
| 1
|
| Isothermal Processes
| 1
|
| Ism: Reflection Nebulae
| 1
|
| Ism: Molecules
| 1
|
| Ism: Lines And Bands
| 1
|
| Interplanetary Space
| 1
|
| Interplanetary Physics: Solar Wind Sources
| 1
|
| Interplanetary Physics: Neutral Particles
| 1
|
| Interplanetary Physics: Mhd Waves And Turbulence (2752
| 1
|
| Interplanetary Physics: Instruments And Techniques
| 1
|
| Interplanetary Physics: Ejecta
| 1
|
| 2-d Mhd Solar Wind Model
| 1
|
| Image Processing
| 1
|
| Image Enhancement
| 1
|
| Hydrogen Plasma
| 1
|
| Hydrodynamic Equations
| 1
|
| Helium Ions
| 1
|
| Heating
| 1
|
| Galactic Nuclei
| 1
|
| Flux Density
| 1
|
| Flow Characteristics
| 1
|
| Fine Structure
| 1
|
| Field Theory (physics)
| 1
|
| Field Strength
| 1
|
| Fast Solar Wind
| 1
|
| Fast Fourier Transform
| 1
|
| Equations Of Motion
| 1
|
| Energy Transfer
| 1
|
| Energy Distribution
| 1
|
| Electron Distribution
| 1
|
| Electron Density (concentration)
| 1
|
| Electric And Magnetic Fields Solar Magnetism
| 1
|
| Eigenvectors
| 1
|
| Driver Gases
| 1
|
| Discontinuity
| 1
|
| Direct Imaging
| 1
|
| Diffusion
| 1
|
| Diagnosis
| 1
|
| Density Distribution
| 1
|
| Critical Point
| 1
|
| Coronal Plumes
| 1
|
| Coronagraphs
| 1
|
| Conservation Equations
| 1
|
| Conductive Heat Transfer
| 1
|
| Computational Methods
| 1
|
| Computational Astrophysics
| 1
|
| Composition
| 1
|
| Comets: Individual: C/2012 S1 Ison
| 1
|
| Comets: General
| 1
|
| Collisional Plasmas
| 1
|
| Circular Polarization
| 1
|
| Ccd Observation
| 1
|
| Brightness Temperature
| 1
|
| Brightness Distribution
| 1
|
| Atmospheric Heating
| 1
|
| Astronomy Software
| 1
|
| Astronomical Observations
| 1
|
| And Magnetic Clouds
| 1
|
| And Astronomy: Radio Emissions
| 1
|
| And Astronomy: Magnetic Fields
| 1
|
| And Astronomy: Energetic Particles (2114)
| 1
|
| And Astronomy: Coronal Mass Ejections
| 1
|
| X-ray
| 1
|
| Very Large Array (vla)
| 1
|
| Variability
| 1
|
| Ultraviolet Spectrometers
| 1
|
| Ultraviolet Spectra
| 1
|
| Ultraviolet Astronomy
| 1
|
| Two Fluid Models
| 1
|
| Two Dimensional Flow
| 1
|
| Topology
| 1
|
| Time-resolved Optical Spectroscopies And Other Ultrafast Optical Measurements In Condensed Matter
| 1
|
| Thermal Instability
| 1
|
| Thermal Emission
| 1
|
| Theoretical Physics
| 1
|
| Temperature Measurement
| 1
|
| Sun: X-rays [S]
| 1
|
| Sun: UV Spectroscopy
| 1
|
| Sun: UV Coronagraph
| 1
|
| Sun: Sunspots
| 1
|
| Sun: Sun: Magnetic Field
| 1
|
| Sun: Sun: Filaments
| 1
|
| Sun: Sun: Coronal Holes
| 1
|
| Sun: Sun
| 1
|
| Sun: Standing Waves
| 1
|
| Sun: Spectral Line
| 1
|
| Sun: Solar Radiation
| 1
|
| Sun: Solar Phys
| 1
|
| Sun: Solar Minimum
| 1
|
| Sun: Solar Magnetism
| 1
|
| Sun: Solar Limb
| 1
|
| Sun: Solar Atmosphere
| 1
|
| Sun: Solar Activity
| 1
|
| Sun: Skylab Program
| 1
|
| Sun: Shock Wave Propagation
| 1
|
| Sun: Shock Formation
| 1
|
| Sun: Rotation [S]
| 1
|
| Sun: Reconnection Rate
| 1
|
| Sun: Radial Gradient
| 1
|
| Sun: Prominences
| 1
|
| Sun: Physics - Space Physics
| 1
|
| Sun: Opposite Effect
| 1
|
| Sun: Mass Flux
| 1
|
| Sun: Magnetohydrodynamic Waves
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Magnetic Flux Tube
| 1
|
| Sun: Magnetic Field Configurations
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: Magnetic Element
| 1
|
| Sun: Luminous Intensity
| 1
|
| Sun: Low Coronal Signatures
| 1
|
| Sun: Large Error
| 1
|
| Sun: Interplanetary Space
| 1
|
| Sun: Interior [S]
| 1
|
| Sun: Intensity Measurement
| 1
|
| Sun: Initiation And Propagation
| 1
|
| Sun: High Velocity
| 1
|
| Sun: Heliocentric Distance
| 1
|
| Sun: Flux Tube
| 1
|
| Sun: Flares [S]
| 1
|
| Sun: Eclipse
| 1
|
| Sun: Dispersion Relation
| 1
|
| Sun: Coronal Mass Ejection
| 1
|
| Sun: Coronal Loops
| 1
|
| Sun: Collisionless Plasmas
| 1
|
| Sun: Automatic Detection And Classification
| 1
|
| Sun: Atmospheric Heating
| 1
|
| Sun: Astrophysics
| 1
|
| Sun: Anisotropy
| 1
|
| Sun: Active Regions
| 1
|
| Stellar Models
| 1
|
| Spicules
| 1
|
| Spatial Resolution
| 1
|
| Space Weather: Forecasting (1922
| 1
|
| Space Plasma Physics: Wave/particle Interactions (2483
| 1
|
| Space Plasma Physics: Plasma Energization
| 1
|
| Space Plasma Physics: Nonlinear Phenomena
| 1
|
| Space Plasma Physics: Kinetic Waves And Instabilities
| 1
|
| Space Plasma Physics: Kinetic And Mhd Theory
| 1
|
| Space Plasma Physics: General Or Miscellaneous
| 1
|
| Space Plasma Physics: Charged Particle Motion And Acceleration
| 1
|
| Solar Transition Region
| 1
|
| Solar Spectra
| 1
|
| Solar Rotation
| 1
|
| Solar Radio Bursts
| 1
|
| Solar Protons
| 1
|
| Solar Particle Emission
| 1
|
| Solar K-corona
| 1
|
| Solar K Corona
| 1
|
| Solar Instruments
| 1
|
| Solar Heliosphere And Cosmic Rays
| 1
|
| Solar Granulation
| 1
|
| Solar F-corona
| 1
|
| Solar F Corona
| 1
|
| Solar E Corona
| 1
|
| Solar Differential Rotation
| 1
|
| Solar Coronal Plumes
| 1
|
| Solar Coronal Lines
| 1
|
| Solar Corona:magnetic Fields
| 1
|
| Solar Corona:heating
| 1
|
| Solar Chromosphere:solar Corona
| 1
|
| Solar Chromosphere:helium Lines
| 1
|
| Small Scale Structures
| 1
|
| Shock Wave Interaction
| 1
|
| Rankine-hugoniot Relation
| 1
|
| Analytical Mathematics
| 1
|
| Alpha Particles
| 1
|
| Algorithms
| 1
|
| Adiabatic Demagnetization Cooling
| 1
|
| Accretion Disks
| 1
|
| 7836)
| 1
|
| 6984)
| 1
|
| 2722)
| 1
|
| Image Resolution
| 1
|