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: Oscillations [S]
| 27
|
| Sun: Atmosphere [S]
| 25
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 19
|
| Sun: Chromosphere [S]
| 12
|
| Sun: Photosphere [S]
| 9
|
| The Sun [S]
| 8
|
| Hydrodynamics
| 8
|
| Chromosphere
| 8
|
| Waves
| 8
|
| Solar Physics [S]
| 7
|
| Sun: Helioseismology [S]
| 7
|
| Photosphere [S]
| 6
|
| Stars: Atmospheres
| 6
|
| Sun: Magnetic Fields
| 5
|
| Solar Wind [H]
| 5
|
| Sdo
| 4
|
| Sdo Workshop
| 4
|
| Solar Dynamic Observatory
| 4
|
| Sun: Corona [S]
| 4
|
| Sun: Interior [S]
| 4
|
| Oscillations
| 4
|
| Corona [S]
| 4
|
| Magnetohydrodynamics [S]
| 3
|
| Sun: UV Radiation [S]
| 3
|
| Wave Propagation
| 3
|
| Soho
| 3
|
| Sun: Atmospheric Motions
| 3
|
| Convection
| 3
|
| Stellar Atmospheres
| 3
|
| Space Missions: Sun
| 3
|
| Sun: General
| 2
|
| Sun: Flares [S]
| 2
|
| Instrumentation
| 2
|
| Transition Region
| 2
|
| Sunspots [S]
| 2
|
| Iron
| 2
|
| Sun: Radio Radiation [S]
| 2
|
| Space Research: Heliosphere
| 2
|
| Brightness Distribution
| 2
|
| Sun: Magnetic Field
| 2
|
| 2013 Lws/sdo Science Workshop
| 2
|
| Space Weather
| 2
|
| Magnetic Fields
| 2
|
| Wave Reflection
| 2
|
| Stars: Oscillations
| 2
|
| Sun: Activity
| 2
|
| Sun: Velocity Fields
| 2
|
| Sun: Active Regions
| 2
|
| Solar Granulation
| 2
|
| Sun: Waves
| 2
|
| Methods: Observational
| 2
|
| Sdo 7
| 2
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 2
|
| Gravity Waves
| 2
|
| Sdo-7
| 2
|
| Solar Orbiter
| 1
|
| Solar Observing Facilities
| 1
|
| Solar Magnetic Field
| 1
|
| Solar Irradiance
| 1
|
| Solar Interior: Dynamics
| 1
|
| Solar Imaging
| 1
|
| Solar Data
| 1
|
| Solar Cycles
| 1
|
| Solar Coronal Loops: Solar Prominences
| 1
|
| Solar Coronal Holes: Solar Wind
| 1
|
| Solar Corona: Space Research
| 1
|
| Solar Corona: Space Missions
| 1
|
| Solar Corona: Mass Flow
| 1
|
| Solar Convection (astronomy)
| 1
|
| Solar Activity
| 1
|
| Soho (artificial Satellite)
| 1
|
| Shock Waves
| 1
|
| Sdo-4/iris/hinode Workshop
| 1
|
| Sdo-4
| 1
|
| Sdo-3
| 1
|
| Sdo 4
| 1
|
| Sdo 3
| 1
|
| Remote Observing Techniques
| 1
|
| Radiative Transfer [S]
| 1
|
| Quiet Sun
| 1
|
| Propagation Velocity
| 1
|
| Power Spectra
| 1
|
| Polarimetric
| 1
|
| Plages
| 1
|
| Physics
| 1
|
| Phase Diagrams
| 1
|
| Penumbras
| 1
|
| Particle Emission Solar Wind [H]
| 1
|
| P Waves
| 1
|
| Nitrides
| 1
|
| Millimeter Radiation
| 1
|
| Methods: Numerical
| 1
|
| Methods: Data Analysis
| 1
|
| Methods: Analytical
| 1
|
| Methods
| 1
|
| Magnetographs
| 1
|
| Magnetic Flux Tubes: Solar Oscillations
| 1
|
| Magnetic Flux Tubes: Solar Atmosphere
| 1
|
| Magnetic Flux
| 1
|
| Lyman Alpha Radiation
| 1
|
| Lower Corona
| 1
|
| Linear Equations
| 1
|
| Line: Formation
| 1
|
| Line Spectra
| 1
|
| Lamb Waves
| 1
|
| Instruments
| 1
|
| Instrumentation And Data Management
| 1
|
| Instrumental Effects
| 1
|
| Hypergeometric Functions
| 1
|
| Hydrodynamics Shock Waves
| 1
|
| High Resolution
| 1
|
| Heliophysics
| 1
|
| Halo Orbit
| 1
|
| H Alpha Line
| 1
|
| Fourier Transformation
| 1
|
| Fip Effect
| 1
|
| Field Strength
| 1
|
| Faculae
| 1
|
| Euv Spectroscopy
| 1
|
| Energetic Particles
| 1
|
| Diamond
| 1
|
| Detectors
| 1
|
| Data Reduction
| 1
|
| Data Archives
| 1
|
| Cosmic Rays
| 1
|
| Coronal Hole
| 1
|
| Coronagraphs
| 1
|
| Convection Zone
| 1
|
| Composition
| 1
|
| CMEs
| 1
|
| Circular Polarization
| 1
|
| Cameras
| 1
|
| Calcium
| 1
|
| Atmospheric Models
| 1
|
| Virtual Observatory Tools
| 1
|
| UV/euv
| 1
|
| UV Range
| 1
|
| UV Radiation
| 1
|
| Total Solar Irradiance
| 1
|
| Time Series Analysis
| 1
|
| Temperature Gradients
| 1
|
| Temperature Distribution
| 1
|
| Sun: UV Radiation: Sun: Oscillations: Sun: Waves: Sun: Corona
| 1
|
| Sun: Transition Region [S]
| 1
|
| Sun: Sunspot
| 1
|
| Sun: Sun
| 1
|
| Sun: Space Research: Sun
| 1
|
| Sun: Space Research
| 1
|
| Sun: Space Instrumentation: Solar Wind
| 1
|
| Sun: Space Instrumentation: Solar Interior
| 1
|
| Sun: Space Instrumentation: Solar Corona
| 1
|
| Sun: Space Instrumentation: Heliosphere
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Sun: Solar Interior
| 1
|
| Sun: Solar Corona
| 1
|
| Sun: Solar
| 1
|
| Sun: Soho
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Observations
| 1
|
| Sun: Modes
| 1
|
| Sun: Measurement
| 1
|
| Sun: Line Formation
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Granulation [S]
| 1
|
| Sun: Faculae [S]
| 1
|
| Sun: Direct Modeling
| 1
|
| Sun: Chromospheric Oscillations
| 1
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 1
|
| Stellar Models
| 1
|
| Standing Waves
| 1
|
| Spectrographs
| 1
|
| Spatial Resolution
| 1
|
| Space Vehicles: Instruments
| 1
|
| Space Vehicles
| 1
|
| Space Research: Sun
| 1
|
| Space Plasmas: Measurement
| 1
|
| Space Plasma Physics
| 1
|
| Space Missions: Improvements
| 1
|
| Space Missions
| 1
|
| Space Instrumentation: Solar Patrol
| 1
|
| Sound Waves
| 1
|
| Solar Wind: Origin
| 1
|
| Solar Velocity
| 1
|
| Solar Transition Region: Dynamics
| 1
|
| Solar Transition Region
| 1
|
| Solar Telescopes
| 1
|
| Solar Spectra
| 1
|
| Solar Space Missions
| 1
|
| Solar Physics: International
| 1
|
| Alma
| 1
|
| Lws/sdo-3/soho-26/gong-2011 Workshop
| 1
|