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: Chromosphere [S]
| 39
|
| Sun: Atmosphere [S]
| 19
|
| Magnetohydrodynamics [S]
| 17
|
| Sun: Oscillations [S]
| 16
|
| Waves
| 15
|
| Sunspots [S]
| 14
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 14
|
| Sun: Flares [S]
| 11
|
| Sun: Photosphere [S]
| 10
|
| Sun: Magnetic Fields
| 10
|
| Sun: Activity
| 9
|
| Sun: Corona [S]
| 8
|
| Hydrodynamics
| 7
|
| Sun: Filaments [S]
| 6
|
| Alfven Waves
| 4
|
| Methods: Observational
| 4
|
| Line: Profiles
| 4
|
| Methods: Data Analysis
| 3
|
| Techniques: Imaging Spectroscopy
| 2
|
| Sun: UV Radiation [S]
| 2
|
| Instrumentation: Spectrographs
| 2
|
| Techniques: Image Processing
| 2
|
| Instabilities [H]
| 2
|
| Quiet Sun
| 2
|
| Solar Magnetic Reconnection
| 2
|
| Solar Activity
| 2
|
| Magnetic Reconnection
| 1
|
| Magnetic Fields
| 1
|
| Lines: Profiles
| 1
|
| Line: Formation
| 1
|
| Instrumentation: Polarimeters
| 1
|
| High Energy Astrophysical Phenomena
| 1
|
| Earth And Planetary Astrophysics
| 1
|
| Techniques: Spectroscopic
| 1
|
| Techniques: High Angular Resolution
| 1
|
| Sun: Visible
| 1
|
| Sun: Transition Region [S]
| 1
|
| Sun: Spectrum
| 1
|
| Sun: Radio Radiation [S]
| 1
|
| Sun: Pre-flare Phenomena
| 1
|
| Sun: Infrared
| 1
|
| Sun: In Flares
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Sun: Heating
| 1
|
| Sun: Coronal Mass Ejections
| 1
|
| Sun: Atmospheric Motions
| 1
|
| Sun: Active Regions
| 1
|
| Sun: Abundances
| 1
|
| Spectroscopy
| 1
|
| Solar Transition Region
| 1
|
| Solar Spicules
| 1
|
| Solar Flare Spectra
| 1
|
| Solar Filament Eruptions
| 1
|
| Solar And Stellar Astrophysics
| 1
|
| Shock Waves
| 1
|
| Radiative Transfer [S]
| 1
|
| Plasmas
| 1
|
| Neural Networks
| 1
|
| Methods: Numerical
| 1
|
| Astronomy Data Analysis
| 1
|
| Magnetohydrodynamic (mhd)
| 1
|