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
|
|---|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 91
|
| Sun: Photosphere [S]
| 42
|
| Sun: Oscillations [S]
| 41
|
| Sun: Chromosphere [S]
| 37
|
| Magnetohydrodynamics [S]
| 25
|
| Sun: Magnetic Fields
| 18
|
| Sun: Activity
| 18
|
| Sun: Corona [S]
| 18
|
| Sun: Atmosphere [S]
| 15
|
| Sun: Evolution
| 13
|
| Sunspots [S]
| 13
|
| Sun: Flares [S]
| 11
|
| Methods: Numerical
| 8
|
| Astrophysics
| 8
|
| Magnetic Fields
| 7
|
| Waves
| 7
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 6
|
| Sun: Uv Radiation [S]
| 6
|
| Solar Atmosphere
| 6
|
| Solar Physics [S]
| 5
|
| Sun: Filaments [S]
| 4
|
| Sun: Surface Magnetism [S]
| 4
|
| Stars: Activity
| 3
|
| Heating
| 3
|
| Plasmas
| 3
|
| Shock Waves
| 3
|
| Methods: Observational
| 2
|
| Instabilities [H]
| 2
|
| Astronomy
| 2
|
| Flare Stars
| 2
|
| Sun: Atmospheric Motions
| 2
|
| Active Solar Chromosphere
| 2
|
| Sun: Fundamental Parameters
| 2
|
| Spectropolarimetry
| 2
|
| Stars: Chromospheres
| 2
|
| Sun: Transition Region [S]
| 2
|
| Sun: Granulation [S]
| 2
|
| Computational Methods
| 2
|
| The Sun [S]
| 2
|
| Radiative Transfer [S]
| 2
|
| Atomic Data
| 2
|
| Wavelet Analysis
| 2
|
| Umbra
| 2
|
| Sun: Spicules
| 2
|
| Stellar Flares
| 2
|
| Plasma Wave Heating
| 2
|
| Telescopes
| 2
|
| Optical Flares
| 2
|
| Techniques: Image Processing
| 2
|
| Sun: Coronal Mass Ejections
| 2
|
| Plages
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Penumbra
| 1
|
| Oscillations
| 1
|
| Open Clusters And Associations: Individual: α Per Ic 2391 Ic 2602
| 1
|
| Mhd Waves
| 1
|
| Methods: Statistical
| 1
|
| Methods: Data Analysis
| 1
|
| Methods: Analytical
| 1
|
| Methods - Observational
| 1
|
| Absorption
| 1
|
| Magnetohydrodynamic
| 1
|
| Magnetohy Drodynamics (mhd)
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Instrumentation: Miscellaneous
| 1
|
| Instrumentation: Adaptive Optics
| 1
|
| Instrumentation And Data Management
| 1
|
| Fitting
| 1
|
| Fast Fourier Transform
| 1
|
| Emission
| 1
|
| Emerging Flux Tubes
| 1
|
| Coronal
| 1
|
| Corona [S]
| 1
|
| Core-collapse Supernovae
| 1
|
| Chromosphere
| 1
|
| Atomic Processes
| 1
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Astrophysics - Cosmology And Nongalactic Astrophysics
| 1
|
| Astronomical Instrumentation
| 1
|
| Voigt
| 1
|
| Ultraviolet: General
| 1
|
| Type Ic Supernovae
| 1
|
| Transient Sources
| 1
|
| Techniques: Radial Velocities
| 1
|
| Techniques: Imaging Spectroscopy
| 1
|
| Supernovae
| 1
|
| Sun: Sunspots
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Incompressible Waves
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Sun: Faculae [S]
| 1
|
| Sun: Compressible Waves
| 1
|
| Sun: Alfvén Waves
| 1
|
| Sun: Abundances
| 1
|
| Sun – Corona
| 1
|
| Sun - Oscillations
| 1
|
| Sun - Atmosphere
| 1
|
| Stars: Rotation
| 1
|
| Stars: Late-type
| 1
|
| Stars: Individual: α Centauri B
| 1
|
| Stars: Individual: Eq Pegasi
| 1
|
| Stars: Flare
| 1
|
| Stars: Atmospheres
| 1
|
| Spectrum
| 1
|
| Spectrometers
| 1
|
| Spectra
| 1
|
| Solar Wind [H]
| 1
|
| Solar Spicules
| 1
|
| Solar Radiation
| 1
|
| Solar Fibrils
| 1
|
| Solar Dynamic Observatory
| 1
|
| Solar Cycle
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Transients
| 1
|
| Solar Active Region Magnetic Fields [S]
| 1
|
| Shocks
| 1
|
| Sdo-2016
| 1
|
| Sdo Workshop
| 1
|
| Sdo 2016: Unraveling The Sun's Complexity
| 1
|
| Sdo 2016
| 1
|
| Sdo
| 1
|
| Radiative Magnetohydrodynamics
| 1
|
| Quiet Sun
| 1
|
| Python
| 1
|
| Propagation
| 1
|
| Polarization
| 1
|
| Plasma
| 1
|
| Planetary Nebulae: General
| 1
|
| Active
| 1
|
| Magnetohydrodynamical Simulations
| 1
|