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]
| 48
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 25
|
| Sun: Coronal Mass Ejections
| 21
|
| Sun: Magnetic Fields
| 20
|
| Magnetohydrodynamics [S]
| 18
|
| Solar Wind [H]
| 15
|
| Waves
| 8
|
| Solar Coronal Holes [S]
| 8
|
| Magnetohydrodynamical Simulations
| 7
|
| Sun: Flares [S]
| 7
|
| Sun: Filaments [S]
| 6
|
| Physics - Space Physics [H]
| 6
|
| Sun: Heliosphere [H]
| 5
|
| Sun: UV Radiation [S]
| 5
|
| Solar Physics [S]
| 5
|
| Solar Magnetic Flux Emergence
| 4
|
| Solar Extreme Ultraviolet Emission [S]
| 4
|
| Solar Coronal Streamers
| 4
|
| Sun: Photosphere [S]
| 4
|
| Solar Surface
| 3
|
| Solar Optical Telescopes
| 3
|
| Interplanetary Magnetic Fields [H]
| 3
|
| Coronagraphic Imaging
| 3
|
| Techniques: Image Processing
| 3
|
| Solar Activity
| 3
|
| Sun: Magnetic Topology
| 3
|
| Turbulence
| 3
|
| Solar Eclipses
| 3
|
| Sun: Physics - Space Physics
| 2
|
| Space Weather
| 2
|
| Methods: Data Analysis
| 2
|
| Sun: Evolution
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Astronomy Software
| 2
|
| Sun: Infrared
| 2
|
| Model Selection
| 2
|
| Astronomy Data Analysis
| 2
|
| Sun: Atmosphere [S]
| 2
|
| Neural Networks
| 2
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 2
|
| Sun: Particle Emission
| 2
|
| Solar Coronal Waves [S]
| 2
|
| Interplanetary Turbulence [H]
| 2
|
| Shocks
| 1
|
| Shock Waves
| 1
|
| Recombination
| 1
|
| Quiet Solar Corona
| 1
|
| Plasmas
| 1
|
| Plasma Temperature
| 1
|
| Plasma Density
| 1
|
| Plasma Alfven Waves
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Physics - Computational Physics
| 1
|
| Parallel
| 1
|
| Methods: Observational
| 1
|
| Methods: Numerical
| 1
|
| Methods: Analytical
| 1
|
| Magnetic Reconnection
| 1
|
| Magnetic Fields
| 1
|
| 7835)
| 1
|
| Interplanetary Physics: Coronal Mass Ejections (7513)
| 1
|
| Interplanetary Medium [H]
| 1
|
| Instrumentation: Spectrographs
| 1
|
| Flares
| 1
|
| Cross-validation
| 1
|
| Corona [S]
| 1
|
| Computer Science - Programming Languages
| 1
|
| Computer Science - Distributed
| 1
|
| Comets: Individual: Comet C&2011 W3 (lovejoy
| 1
|
| Comets: Individual: C/2011 W3
| 1
|
| Comets: General
| 1
|
| Chemical Abundances
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Astrophysics
| 1
|
| Astrophysical Plasma
| 1
|
| Astronomy Planetary-science, Physics, Sociology
| 1
|
| Astronomy Image Processing
| 1
|
| Ultraviolet: General
| 1
|
| The Sun [S]
| 1
|
| Techniques: Imaging Spectroscopy
| 1
|
| Sun: X-rays [S]
| 1
|
| Sun: Waves
| 1
|
| Sun: Transition Region [S]
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Sun: Shock
| 1
|
| Sun: Rotation [S]
| 1
|
| Sun: Radio Radiation [S]
| 1
|
| Sun: Radio
| 1
|
| Sun: Propagation
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: Magnetohydrodynamic
| 1
|
| Sun: Low Coronal Signatures
| 1
|
| Sun: General
| 1
|
| Sun: Fractional Charge States
| 1
|
| Sun: Euv
| 1
|
| Sun: Activity
| 1
|
| Stellar Physics
| 1
|
| Stellar Activity
| 1
|
| Stars: Magnetic Field
| 1
|
| Stars: Coronae
| 1
|
| Stars: Activity
| 1
|
| Space Plasmas [H]
| 1
|
| Solid State: Refractory
| 1
|
| Solar Storm
| 1
|
| Solar Meridional Circulation
| 1
|
| Solar Magnetism
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar K-corona
| 1
|
| Solar Filament Eruptions
| 1
|
| Solar F-corona
| 1
|
| Solar Energetic Particles [H]
| 1
|
| Solar E Corona
| 1
|
| Solar Differential Rotation
| 1
|
| Solar Cycle
| 1
|
| Solar Coronal Mass Ejection Shocks
| 1
|
| Solar Coronal Lines
| 1
|
| Solar Active Region Magnetic Fields [S]
| 1
|
| Solar Active Region Filaments
| 1
|
| Slow Solar Wind [H]
| 1
|
| And Cluster Computing
| 1
|
| And Astronomy: Magnetic Reconnection (2723
| 1
|
| And Astronomy: Corona
| 1
|
| Alfven Waves
| 1
|
| Active Solar Corona
| 1
|
| Acceleration Of Particles
| 1
|
| Ionization
| 1
|