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
|
|---|
| Radiative Transfer [S]
| 96
|
| Polarization
| 87
|
| Sun: Chromosphere [S]
| 79
|
| Sun: Magnetic Fields
| 64
|
| Scattering
| 59
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 50
|
| Astrophysics
| 37
|
| Sun: Atmosphere [S]
| 32
|
| Stars: Atmospheres
| 30
|
| Sun: Photosphere [S]
| 25
|
| Line: Profiles
| 25
|
| Spectropolarimetry
| 22
|
| Magnetic Fields
| 22
|
| Line: Formation
| 22
|
| Methods: Numerical
| 19
|
| Sun: Transition Region [S]
| 15
|
| Atomic Processes
| 14
|
| Sun: Filaments [S]
| 12
|
| Stars: Magnetic Fields
| 8
|
| Sun: Surface Magnetism [S]
| 7
|
| Techniques: Polarimetric
| 7
|
| Solar Physics [S]
| 6
|
| Sun: UV Radiation [S]
| 6
|
| Sun: Corona [S]
| 6
|
| Plages
| 5
|
| Methods: Data Analysis
| 5
|
| Sun: Oscillations [S]
| 5
|
| Stellar Atmospheres
| 5
|
| Sun: Abundances
| 5
|
| Quiet Sun
| 4
|
| Polarimetry
| 4
|
| Magnetohydrodynamics [S]
| 4
|
| Sun: Sunspots
| 4
|
| Solar And Stellar Astrophysics
| 4
|
| The Sun [S]
| 4
|
| Sun: Prominences
| 3
|
| Iron Lines: Solar Atmosphere
| 3
|
| Methods: Observational
| 3
|
| Instrumentation: Polarimeters
| 3
|
| Sun: Infrared
| 3
|
| Molecular Processes
| 3
|
| Dynamo
| 3
|
| Convection
| 3
|
| Shock Waves
| 3
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 3
|
| Quiet Solar Chromosphere
| 3
|
| Solar Transition Region
| 3
|
| Sun: Lyman-alpha
| 2
|
| Active Solar Chromosphere
| 2
|
| Astrophysics - Astrophysics Of Galaxies
| 2
|
| Sun: Vacuum Ultraviolet
| 2
|
| Molecular Data
| 2
|
| Esa Cosmic Vision
| 2
|
| Energy Transfer
| 2
|
| Sun: Faculae [S]
| 2
|
| Stellar Atmospheres: Iron Lines
| 2
|
| Sun: Spectropolarimetry
| 2
|
| Solar Atmosphere: Non-lte Analysis
| 2
|
| Solar Atmosphere: Iron Lines
| 2
|
| Radiative Transfer Simulations
| 2
|
| Sun: Polarization Calibration
| 2
|
| Stellar Oscillations
| 2
|
| Sun: Clasp
| 2
|
| Atomic Spectroscopy
| 2
|
| Stars: Chromospheres
| 2
|
| Numerical Analysis
| 2
|
| Atmospheric Stratification
| 2
|
| Line Spectra
| 2
|
| Stars: Magnetic Field
| 2
|
| Photosphere [S]
| 2
|
| Space Vehicles: Instruments
| 2
|
| Methods: Statistical
| 2
|
| Sun: Activity
| 2
|
| Solar Magnetic Reconnection
| 2
|
| Instrumentation And Methods For Astrophysics
| 2
|
| Instrumentation
| 2
|
| Missions: First
| 2
|
| Hydrodynamics
| 2
|
| Sun: Solar Chromosphere
| 2
|
| Calcium
| 1
|
| Atmospheric Temperature
| 1
|
| Atmospheric Models
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Astronomy Data Analysis
| 1
|
| Astronomy
| 1
|
| Astrochemistry
| 1
|
| And Gravitation
| 1
|
| Alfven Waves
| 1
|
| Waves
| 1
|
| Visible Spectrum
| 1
|
| Thermodynamic Equilibrium
| 1
|
| The Hanle And Zeeman Effects
| 1
|
| Telescopes
| 1
|
| Techniques: Spectroscopy
| 1
|
| Techniques: Spectroscopic
| 1
|
| Techniques: Polarimetic
| 1
|
| Techniques: High Angular Resolution
| 1
|
| Sunspot
| 1
|
| Sun: Ultraviolet
| 1
|
| Sun: Sun: Magnetic Fields
| 1
|
| Sun: Sun: Atmosphere
| 1
|
| Sun: Solar And Stellar Magnetic Fields
| 1
|
| Sun: Radiative Transfer
| 1
|
| Sun: Polarization
| 1
|
| Sun: Nlte Stokes Transfer
| 1
|
| Sun: Line Formation
| 1
|
| Sun: Instrumental Effects
| 1
|
| Sun: Flares [S]
| 1
|
| Sun: Active Regions
| 1
|
| Stellar Outer Astmospheres
| 1
|
| Statistics
| 1
|
| Stars: Late-type
| 1
|
| Stars: Atmosphere
| 1
|
| Stars: Abundances
| 1
|
| Spectral Line Formation
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| Solar Spicules
| 1
|
| Solar Spectra
| 1
|
| Solar Magnetic Fields: Chromosphere
| 1
|
| Solar Magnetic Field
| 1
|
| Solar Instruments
| 1
|
| Solar Dynamic Observatory
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Coronal Lines
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Solar Chromospheric Heating
| 1
|
| Solar Atmosphere: Radiative Transfer
| 1
|
| Sdo-4/iris/hinode Workshop
| 1
|
| Sdo-4
| 1
|
| Sdo Workshop
| 1
|
| Sdo 4
| 1
|
| Sdo
| 1
|
| Scattering Polarization
| 1
|
| Relaxation Time
| 1
|
| Radiation Mechanisms
| 1
|
| Polarimeters
| 1
|
| Physics - Optics
| 1
|
| Physics - Atomic Physics
| 1
|
| Physics
| 1
|
| Opacity
| 1
|
| Nucleosynthesis
| 1
|
| Nuclear Reactions
| 1
|
| Nonequilibrium Thermodynamics
| 1
|
| Mathematical Models
| 1
|
| Masers
| 1
|
| Magnetic Reconnection
| 1
|
| Magnetic Flux
| 1
|
| Magnetic Field Configurations
| 1
|
| Magnetic Field
| 1
|
| Level Crossing And Optical Pumping
| 1
|
| Iron Lines: Sunspots
| 1
|
| Iron Lines: Cool Stars
| 1
|
| Instrumentation: Spectrographs
| 1
|
| Instrumentation: Adaptive Optics
| 1
|
| Hydrogen
| 1
|
| High Energy Astrophysical Phenomena
| 1
|
| Helium Ions
| 1
|
| Galaxy: Evolution
| 1
|
| Galaxy: Abundances
| 1
|
| Fundamental Aspects Of Astrophysics
| 1
|
| Extreme Ultraviolet Astronomy
| 1
|
| Emission Spectra
| 1
|
| Eddington Approximation
| 1
|
| Cosmology And Nongalactic Astrophysics
| 1
|
| Cosmology
| 1
|
| Corona [S]
| 1
|
| Center To Limb Observations
| 1
|
| Abundances
| 1
|