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]
| 35
|
| Sun: Filaments [S]
| 29
|
| Sun: Magnetic Fields
| 26
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 19
|
| Solar Magnetic Reconnection
| 17
|
| Sun: Flares [S]
| 16
|
| Magnetohydrodynamics [S]
| 11
|
| Sun: Coronal Mass Ejections
| 9
|
| Magnetic Reconnection
| 8
|
| Sun: UV Radiation [S]
| 6
|
| Sun: Activity
| 6
|
| Sun: Oscillations [S]
| 6
|
| Sun: Prominences
| 5
|
| Solar Wind [H]
| 5
|
| Plasma Jets
| 4
|
| Sun: Chromosphere [S]
| 4
|
| Sun: Atmosphere [S]
| 3
|
| Current Sheets
| 3
|
| Oscillations
| 3
|
| Sun: Transition Region [S]
| 3
|
| Plasmas
| 3
|
| Solar Activity
| 3
|
| Solar Filament Eruptions
| 3
|
| Solar Magnetic Field
| 3
|
| Solar Physics [S]
| 3
|
| Turbulence
| 2
|
| The Sun [S]
| 2
|
| Sun: Solar X-rays
| 2
|
| Sun: Heliosphere [H]
| 2
|
| Sun: Astronomical Models
| 2
|
| Sun: Active Regions
| 2
|
| Stars: Jets
| 2
|
| Solar Radio Emission
| 2
|
| Solar Coronal Transients
| 2
|
| Solar Coronal Streamers
| 2
|
| Solar Coronal Holes [S]
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Methods: Numerical
| 2
|
| Magnetohydrodynamic Flow
| 2
|
| Magnetic Fields
| 2
|
| Kelvin-helmholtz Instability
| 2
|
| Jets
| 2
|
| Hydrodynamics
| 2
|
| Fast Solar Wind
| 2
|
| Coronal Loops
| 2
|
| Chromosphere
| 2
|
| Acceleration Of Particles
| 2
|
| Waves
| 2
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Coronal Waves [S]
| 1
|
| 14j60
| 1
|
| Extreme Ultraviolet Astronomy
| 1
|
| Solar Coronal Seismology
| 1
|
| Solar Coronal Plumes
| 1
|
| Solar Coronal Mass Ejection Shocks
| 1
|
| Exoplanet Atmospheric Structure
| 1
|
| Energy Dissipation
| 1
|
| Sun: Solar Magnetic Field
| 1
|
| Solar Active Region Filaments
| 1
|
| Shear Layers
| 1
|
| Shear Flow
| 1
|
| Quiet Solar Corona
| 1
|
| Quiescent Solar Prominence
| 1
|
| Sun: Thermal Radiation
| 1
|
| Sun: X Ray Spectra
| 1
|
| Plasma Heating
| 1
|
| Photosphere [S]
| 1
|
| Sun: X-rays [S]
| 1
|
| Mhd Waves
| 1
|
| Emission Spectra
| 1
|
| Mathematical Models
| 1
|
| Surges
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetohydrodynamic Turbulence
| 1
|
| Magnetohydrodynamic Stability
| 1
|
| Magnetohydrodynamic Shear Heating
| 1
|
| Videotapes
| 1
|
| Magnetic Structures
| 1
|
| Magnetic Structure
| 1
|
| Thermal Stability
| 1
|
| Astrophysics
| 1
|
| Magnetic Field Reconnection
| 1
|
| Magnetic Field Configurations
| 1
|
| Active Solar Corona
| 1
|
| Catalogs
| 1
|
| Sun: Betatrons
| 1
|
| Boundary Conditions
| 1
|
| Stellar Structure
| 1
|
| Stellar Models
| 1
|
| Hydrodynamical Simulations
| 1
|
| Spectral Index
| 1
|
| Solar X-ray Flares [S]
| 1
|
| Sun: Bremsstrahlung
| 1
|
| Solar Surges
| 1
|
| Gamma Rays [S]
| 1
|
| Solar Prominence
| 1
|
| Sun: Bursts
| 1
|
| Sun: Electron Acceleration
| 1
|
| Sun: Magnetic Topology
| 1
|
| Solar Magnetic Bright Points
| 1
|
| Solar Flare Spectra
| 1
|
| Sun: Solar Activity Effects
| 1
|
| Solar Energetic Particles [H]
| 1
|