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