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]
| 80
|
| Sun: Magnetic Fields
| 64
|
| Scattering
| 60
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 50
|
| Astrophysics
| 37
|
| Sun: Atmosphere [S]
| 32
|
| Stars: Atmospheres
| 30
|
| Sun: Photosphere [S]
| 26
|
| Line: Profiles
| 25
|
| Magnetic Fields
| 22
|
| Line: Formation
| 22
|
| Spectropolarimetry
| 22
|
| Methods: Numerical
| 19
|
| Sun: Transition Region [S]
| 15
|
| Atomic Processes
| 14
|
| Sun: Filaments [S]
| 12
|
| Stars: Magnetic Fields
| 8
|
| Techniques: Polarimetric
| 8
|
| Sun: Surface Magnetism [S]
| 7
|
| Plages
| 6
|
| Sun: UV Radiation [S]
| 6
|
| Sun: Corona [S]
| 6
|
| Solar Physics [S]
| 6
|
| Stellar Atmospheres
| 5
|
| Sun: Oscillations [S]
| 5
|
| Methods: Data Analysis
| 5
|
| Polarimetry
| 5
|
| Sun: Abundances
| 5
|
| The Sun [S]
| 4
|
| Sun: Sunspots
| 4
|
| Solar And Stellar Astrophysics
| 4
|
| Magnetohydrodynamics [S]
| 4
|
| Methods: Observational
| 4
|
| Quiet Sun
| 4
|
| Iron Lines: Solar Atmosphere
| 3
|
| Sun: Infrared
| 3
|
| Instrumentation: Polarimeters
| 3
|
| Shock Waves
| 3
|
| Quiet Solar Chromosphere
| 3
|
| Convection
| 3
|
| Molecular Processes
| 3
|
| Dynamo
| 3
|
| Solar Transition Region
| 3
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 3
|
| Sun: Prominences
| 3
|
| Radiative Transfer Simulations
| 2
|
| Techniques: High Angular Resolution
| 2
|
| Stellar Oscillations
| 2
|
| Stellar Atmospheres: Iron Lines
| 2
|
| Sun: Spectropolarimetry
| 2
|
| Photosphere [S]
| 2
|
| Numerical Analysis
| 2
|
| Stars: Magnetic Field
| 2
|
| Sun: Solar Chromosphere
| 2
|
| Stars: Chromospheres
| 2
|
| Molecular Data
| 2
|
| Missions: First
| 2
|
| Methods: Statistical
| 2
|
| Techniques: Spectroscopic
| 2
|
| Sun: Vacuum Ultraviolet
| 2
|
| Space Vehicles: Instruments
| 2
|
| Line Spectra
| 2
|
| Sun: Polarization Calibration
| 2
|
| Instrumentation And Methods For Astrophysics
| 2
|
| Instrumentation
| 2
|
| Solar Magnetic Reconnection
| 2
|
| Hydrodynamics
| 2
|
| Sun: Lyman-alpha
| 2
|
| Esa Cosmic Vision
| 2
|
| Energy Transfer
| 2
|
| Solar Atmosphere: Non-lte Analysis
| 2
|
| Solar Atmosphere: Iron Lines
| 2
|
| Sun: Faculae [S]
| 2
|
| Atomic Spectroscopy
| 2
|
| Atmospheric Stratification
| 2
|
| Sun: Clasp
| 2
|
| Astrophysics - Astrophysics Of Galaxies
| 2
|
| Sun: Activity
| 2
|
| Active Solar Chromosphere
| 2
|
| 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: Polarimetic
| 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
|
| Solar Active Region Magnetic Fields [S]
| 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
|
| Calcium
| 1
|
| Atmospheric Temperature
| 1
|
| Atmospheric Models
| 1
|
| Abundances
| 1
|