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]
| 76
|
| Sun: Uv Radiation [S]
| 35
|
| Solar Wind [H]
| 27
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 23
|
| Solar Physics [S]
| 20
|
| Sun: Transition Region [S]
| 15
|
| Sun: Solar Wind [H]
| 15
|
| Magnetohydrodynamics [S]
| 12
|
| Sun: Magnetic Fields
| 11
|
| Sun: Activity
| 10
|
| Sun: Atmosphere [S]
| 10
|
| Sun: Coronal Mass Ejections
| 10
|
| Line: Profiles
| 7
|
| Nonequilibrium Ionization
| 7
|
| Extreme Ultraviolet Radiation
| 6
|
| Line Spectra
| 6
|
| Coronal Holes
| 6
|
| Radiative Transfer [S]
| 6
|
| Interplanetary Turbulence [H]
| 6
|
| Physics - Space Physics [H]
| 6
|
| Emission Spectra
| 5
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 5
|
| The Sun [S]
| 5
|
| Sun: Filaments [S]
| 5
|
| Coronal Heating
| 5
|
| Hydrodynamics
| 5
|
| Coronal Loops
| 5
|
| Space Plasmas [H]
| 5
|
| Sun: General
| 5
|
| Transition Region
| 5
|
| Sun: Heliosphere [H]
| 4
|
| Astrophysics
| 4
|
| Magnetohydrodynamic Flow
| 4
|
| Space Vehicles: Instruments
| 4
|
| Carbon
| 4
|
| Stellar Models
| 4
|
| Solar Activity
| 4
|
| H Alpha Line
| 4
|
| Stellar Winds
| 4
|
| Oxygen Ions
| 4
|
| Lyman Alpha Radiation
| 4
|
| Magnetic Fields
| 3
|
| Ionization
| 3
|
| Solar Atmosphere
| 3
|
| Soho Mission
| 3
|
| Velocity Distribution
| 3
|
| Ultraviolet Radiation
| 3
|
| Space Weather
| 3
|
| Sunspots [S]
| 3
|
| Coronagraphic Imaging
| 3
|
| Corona [S]
| 3
|
| Solar Spectra
| 3
|
| Sun: Chromosphere [S]
| 3
|
| Alfven Waves
| 3
|
| Mass Flow
| 2
|
| Stars: Mass Loss
| 2
|
| Early Stars
| 2
|
| Spatial Resolution
| 2
|
| Astronomy
| 2
|
| Plasma Temperature
| 2
|
| Techniques: Spectroscopic
| 2
|
| Cosmic Rays
| 2
|
| Plasma Density
| 2
|
| Steady Flow
| 2
|
| Slow Solar Wind [H]
| 2
|
| Hydrogen
| 2
|
| Ultraviolet: Stars
| 2
|
| Soho
| 2
|
| Physics - Plasma Physics [H]
| 2
|
| Methods: Data Analysis
| 2
|
| Sun: Flares [S]
| 2
|
| Solar Protons
| 2
|
| Solar Radiation
| 2
|
| Instrumentation: Detectors
| 2
|
| Condensed Matter - Materials Science
| 2
|
| Oxygen
| 2
|
| Solar X-rays
| 2
|
| Waves
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Stellar Mass
| 2
|
| Stellar Mass Ejection
| 2
|
| Stellar Spectra
| 2
|
| Atomic Processes
| 2
|
| Solar Electrons
| 2
|
| Temperature Gradients
| 2
|
| Magnesium
| 2
|
| Solar Magnetic Field
| 2
|
| Sun: Oscillations [S]
| 2
|
| Esa Cosmic Vision
| 2
|
| Radiative Heat Transfer
| 2
|
| Red Shift
| 2
|
| Sun: Particle Emission
| 2
|
| Flow Velocity
| 2
|
| Spectral Resolution
| 2
|
| Ultraviolet: Solar System
| 2
|
| Maxwell Equation
| 1
|
| Mathematical Models
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetism
| 1
|
| Magnetic Field Configurations
| 1
|
| Lyman Spectra
| 1
|
| Line Profiles
| 1
|
| Line Profile
| 1
|
| Late Stars
| 1
|
| Ionization State
| 1
|
| Ion Density (concentration)
| 1
|
| Ion Densities
| 1
|
| Ion Charge
| 1
|
| Interplanetary Space
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Interplanetary Medium [H]
| 1
|
| Interior
| 1
|
| Instrumentation: Spectrographs
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Instrumentation And Data Management
| 1
|
| Hydromagnetics
| 1
|
| Hydrogen Ions
| 1
|
| High Temperature Plasmas
| 1
|
| High Latitude
| 1
|
| Hi Ly Alpha
| 1
|
| Heating
| 1
|
| H Ii Regions
| 1
|
| Flares
| 1
|
| Flare Forecasting
| 1
|
| Fe Xii Lines
| 1
|
| Extreme Uv
| 1
|
| Euv Lines
| 1
|
| Equations Of Motion
| 1
|
| Emissivity
| 1
|
| Elemental Abundance
| 1
|
| Electron Energy
| 1
|
| Electron Distribution
| 1
|
| Electron Density (concentration)
| 1
|
| Early-type Stars: Stellar Winds
| 1
|
| Dynamo
| 1
|
| Dynamics
| 1
|
| Doppler Effect
| 1
|
| Density Distribution
| 1
|
| Coronal Plasma
| 1
|
| Coronal Loops Streamers
| 1
|
| Coronal Hole
| 1
|
| Coronal Dynamics
| 1
|
| Coronagraphy
| 1
|
| Coronagraphs
| 1
|
| Convection
| 1
|
| Circumstellar Matter:stellar Winds
| 1
|
| Chemical Abundances
| 1
|
| Charge Coupled Devices
| 1
|
| Brightness
| 1
|
| Be
| 1
|
| B Stars
| 1
|
| Atmospheric Models
| 1
|
| Astronomy Data Analysis
| 1
|
| Astronomical Spectroscopy
| 1
|
| Astronomical Photometry
| 1
|
| Astronomical Models
| 1
|
| Angular Velocity
| 1
|
| Angular Momentum
| 1
|
| X-rays
| 1
|
| X Ray Irradiation
| 1
|
| Visible-light Polarimetry
| 1
|
| Visible Spectrum
| 1
|
| Visible Continuum
| 1
|
| Uvcs
| 1
|
| Uv Spectroscopy
| 1
|
| Uv Coronagraph
| 1
|
| Ultraviolet Spectra
| 1
|
| Ultraviolet Imaging
| 1
|
| Ultraviolet Emission
| 1
|
| Ultraviolet Coronagrapf Spectrometer (uvcs)
| 1
|
| Ultraviolet Astronomy
| 1
|
| Thermal Stability
| 1
|
| Telescopes
| 1
|
| Techniques: Spectroscopy
| 1
|
| Techniques: Polarimetic
| 1
|
| Surges
| 1
|
| Supernova Remnants
| 1
|
| Supergiant Stars
| 1
|
| Sunspot-groups
| 1
|
| Sun: X-rays [S]
| 1
|
| Sun: Sunspots
| 1
|
| Sun: Solar Activity
| 1
|
| Sun: Prominences
| 1
|
| Sun: Photosphere [S]
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: Interior [S]
| 1
|
| Sun: Fundamental Parameters
| 1
|
| Sun: Corona - Sun: Solar Wind - Sun: Uv Radiation
| 1
|
| Sulfur
| 1
|
| Subsonic Flow
| 1
|
| Stellar Winds:circumstellar Matter
| 1
|
| 85-02
| 1
|
| Stellar Atmospheres
| 1
|
| Steady State
| 1
|
| Stars: Supergiants
| 1
|
| Stars: Individual Constellation Name: P Cygni
| 1
|
| Stars: Emission-line
| 1
|
| Stars: Early-type
| 1
|
| Stars: Atmospheres
| 1
|
| Spectrum Analysis
| 1
|
| Spectroscopy
| 1
|
| Spectral Line Width
| 1
|
| Spectral Line
| 1
|
| Spectral Energy Distribution
| 1
|
| Sources Of Solar Wind
| 1
|
| Solar-terrestrial Relations
| 1
|
| Solar Wind Plasma [H]
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| Solar Transition Region
| 1
|
| Solar Spectrometers
| 1
|
| Solar Rotation
| 1
|
| Solar Patrol
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Instrumentation
| 1
|
| Solar Evolution
| 1
|
| Solar Diameter
| 1
|
| Solar Cycles
| 1
|
| Solar Cycle
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Transients
| 1
|
| Solar Coronal Mass Ejection Shocks
| 1
|
| Solar Active Regions [S]
| 1
|
| Software: Simulations
| 1
|
| Software: Data Analysis
| 1
|
| Silicon
| 1
|
| Si Xii
| 1
|
| Shocks
| 1
|
| Secular Variations
| 1
|
| Reynolds Stress
| 1
|
| Radioactive Decay
| 1
|
| Radio Bursts
| 1
|
| Radiation Distribution
| 1
|
| Radiant Flux Density
| 1
|
| Radial Direction
| 1
|
| Power Spectra
| 1
|
| Positive Ions
| 1
|
| Polarimetry
| 1
|
| Polar Observations
| 1
|
| Plasmas (physics)
| 1
|
| Plasma Equilibrium
| 1
|
| Plasma Astrophysics
| 1
|
| Particles Effective Temperature
| 1
|
| Oxygen Spectra
| 1
|
| Ob Stars: Mass Loss
| 1
|
| O Vi
| 1
|
| O Stars
| 1
|
| Nitrogen
| 1
|
| Neon
| 1
|
| Momentum Transfer
| 1
|
| Mg X
| 1
|
| Methods: Observational
| 1
|
| Methods: Numerical
| 1
|
| Active Sun
| 1
|
| Active Solar Corona
| 1
|
| Accretion Disks
| 1
|
| Abundances
| 1
|
| Abundance
| 1
|
| Absolute Abundance
| 1
|
| 96.60.pf
| 1
|
| 96.50.ci
| 1
|
| Stellar Luminosity
| 1
|