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: Corona [S]
| 38
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 32
|
| Sun: Atmosphere [S]
| 23
|
| Methods: Observational
| 18
|
| Sun: Chromosphere [S]
| 17
|
| Sun: Transition Region [S]
| 14
|
| Sun: Activity
| 13
|
| Solar Wind [H]
| 11
|
| Sun: Filaments [S]
| 9
|
| Sun: Abundances
| 9
|
| Sun: Magnetic Fields
| 9
|
| Sun: Active Regions
| 7
|
| Magnetic Reconnection
| 6
|
| Solar Magnetic Reconnection
| 6
|
| Sun: Flares [S]
| 6
|
| Solar Transition Region
| 6
|
| Sun: UV Radiation [S]
| 6
|
| Solar Coronal Loops [S]
| 6
|
| Solar Coronal Heating [S]
| 5
|
| Line: Profiles
| 5
|
| Sun: Coronal Mass Ejections
| 5
|
| Magnetohydrodynamics [S]
| 4
|
| Techniques: Spectroscopic
| 4
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 4
|
| Solar Activity
| 4
|
| Sunspots [S]
| 4
|
| Physics - Space Physics [H]
| 4
|
| Solar Physics [S]
| 3
|
| Solar Cycle
| 3
|
| Solar Coronal Transients
| 3
|
| Plasma Jets
| 3
|
| Sun: Solar Wind [H]
| 3
|
| Waves
| 3
|
| Solar Coronal Waves [S]
| 3
|
| Magnetic Fields
| 2
|
| Methods: Numerical
| 2
|
| Solar And Stellar Astrophysics
| 2
|
| Spectroscopy
| 2
|
| Sun: Evolution
| 2
|
| Astronomy Data Analysis
| 2
|
| Solar Surface
| 2
|
| Sun: Oscillations [S]
| 2
|
| Methods: Data Analysis
| 2
|
| Interplanetary Magnetic Fields [H]
| 1
|
| Inner Magnetosphere
| 1
|
| High-frequency Emic Waves
| 1
|
| Emerging Flux Tubes
| 1
|
| Doppler Shift
| 1
|
| Coronal Heating
| 1
|
| Astronomy Image Processing
| 1
|
| Transition Region
| 1
|
| The Sun [S]
| 1
|
| Sun: Sun: Transition Region
| 1
|
| Sun: Sun: Corona
| 1
|
| Sun: Sun: Atmosphere
| 1
|
| Sun: Stereoscopy
| 1
|
| Sun: Sources
| 1
|
| Sun: Solar Prominence
| 1
|
| Sun: Solar Eruption
| 1
|
| Sun: Solar Cycle
| 1
|
| Sun: Solar Corona
| 1
|
| Sun: Properties
| 1
|
| Sun: Photosphere-sunspots
| 1
|
| Sun: Photosphere [S]
| 1
|
| Sun: Penumbra
| 1
|
| Active Solar Corona
| 1
|
| Sun: Methods: Statistical
| 1
|
| Sun: Method: Observational
| 1
|
| Sun: Magnetohydrodynamics
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Jets
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Heating
| 1
|
| Sun: Granulation [S]
| 1
|
| Sun: Coronal Plumes
| 1
|
| Sun: Coronal Holes
| 1
|
| Sun: Chromospheric
| 1
|
| Spectroscopic Observations
| 1
|
| Solar-terrestrial Interactions
| 1
|
| Solar Wind Dynamic Pressure
| 1
|
| Solar Spicules
| 1
|
| Solar Plasma
| 1
|
| Solar Magnetic Flux Emergence
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Coronal Plumes
| 1
|
| Small-scale Dynamics
| 1
|
| Slow Solar Wind [H]
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Multipoint Observations
| 1
|
| Methods: Statistical
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetic Field
| 1
|
| Low-energy Protons
| 1
|
| Sun: Models
| 1
|