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
|
|---|
| Magnetohydrodynamics [S]
| 37
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 37
|
| Sun: Corona [S]
| 37
|
| Sun: Oscillations [S]
| 26
|
| Waves
| 23
|
| Sun: Chromosphere [S]
| 15
|
| Solar Coronal Waves [S]
| 10
|
| Plasmas
| 10
|
| Sun: Photosphere [S]
| 10
|
| Sun: Magnetic Fields
| 9
|
| Sun: Atmosphere [S]
| 8
|
| The Sun [S]
| 7
|
| Solar Coronal Heating [S]
| 6
|
| Sunspots [S]
| 5
|
| Alfven Waves
| 5
|
| Solar Coronal Holes [S]
| 4
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 4
|
| Solar Coronal Loops [S]
| 3
|
| Solar Coronal Plumes
| 3
|
| Magnetic Fields
| 3
|
| Quiet Solar Corona
| 3
|
| Solar Extreme Ultraviolet Emission [S]
| 3
|
| Sun: Filaments [S]
| 3
|
| Sun: Active Regions
| 3
|
| Active Solar Corona
| 3
|
| Infrared Spectroscopy
| 3
|
| Sun: UV Radiation [S]
| 2
|
| Sun: Helioseismology [S]
| 2
|
| Sun: Activity
| 2
|
| Solar Wind [H]
| 2
|
| Radiative Magnetohydrodynamics
| 2
|
| Quiet Sun
| 2
|
| Methods: Observational
| 2
|
| Convolutional Neural Networks
| 2
|
| Statistics - Applications
| 1
|
| Spectropolarimetry
| 1
|
| Spectral Index
| 1
|
| Space Vehicles: Instruments
| 1
|
| Alfvén Waves (23)
| 1
|
| Solar Transition Region
| 1
|
| Solar Spicules
| 1
|
| Solar Physics [S]
| 1
|
| Solar Magnetic Flux Emergence
| 1
|
| Sun: General
| 1
|
| Sun: Incompressible Waves
| 1
|
| Solar Coronal Seismology
| 1
|
| Sun: Instrumentation And Data Management
| 1
|
| Sun: Magnetohydrodynamics (mhd)
| 1
|
| Sun: Physics - Space Physics
| 1
|
| Sun: Plasmas
| 1
|
| Solar Corona (1483)
| 1
|
| Solar Chromospheric Heating
| 1
|
| Solar Chromosphere (1479)
| 1
|
| Solar Activity
| 1
|
| Solar Active Region Magnetic Fields [S]
| 1
|
| Slow Solar Wind [H]
| 1
|
| Shock Waves
| 1
|
| Science Capital
| 1
|
| Alfvén Waves
| 1
|
| Theory Of Change
| 1
|
| Sun: Solar Photosphere
| 1
|
| Sun: Spicules
| 1
|
| Plasma Wave Heating
| 1
|
| Oscillations
| 1
|
| Monte Carlo Methods
| 1
|
| Active Sun
| 1
|
| Methods: Data Analysis
| 1
|
| Methods
| 1
|
| Magnetohydrodynamics (1964)
| 1
|
| Sun: Sun: Corona
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetic Reconnection
| 1
|
| Sun: Transition Region [S]
| 1
|
| Interplanetary Turbulence [H]
| 1
|
| Sun: Waves
| 1
|
| Fast Solar Wind
| 1
|
| Diversity
| 1
|
| Telescopes
| 1
|
| Children And Young People
| 1
|
| Careers
| 1
|
| The Sun (1693)
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Astronomy Image Processing
| 1
|
| Sun: Compressible Waves
| 1
|
| Astronomy
| 1
|
| Sun: Evolution
| 1
|
| Sun: Active
| 1
|
| Stem Education
| 1
|
| Spectroscopy
| 1
|