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]
| 93
|
| Sun: Magnetic Fields
| 57
|
| Magnetohydrodynamics [S]
| 48
|
| Sun: Flares [S]
| 42
|
| Sun: Coronal Mass Ejections
| 29
|
| Solar Magnetic Reconnection
| 24
|
| Sun: Filaments [S]
| 22
|
| Solar Wind [H]
| 18
|
| Sun: Prominences
| 16
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 14
|
| Sun: UV Radiation [S]
| 12
|
| Magnetic Reconnection
| 12
|
| Sun: Activity
| 11
|
| Solar Physics [S]
| 11
|
| Astrophysics
| 10
|
| Coronal Loops
| 10
|
| Magnetic Fields
| 8
|
| Solar Coronal Holes [S]
| 7
|
| Sun: X-rays [S]
| 7
|
| Sun: Chromosphere [S]
| 7
|
| Sun: Magnetic Topology
| 7
|
| Boundary Conditions
| 6
|
| Stellar Models
| 6
|
| Chromosphere
| 6
|
| Stellar Coronas
| 6
|
| High Temperature Plasmas
| 5
|
| X Ray Sources
| 5
|
| Solar Magnetic Field
| 5
|
| Sun: Transition Region [S]
| 5
|
| Magnetic Field Configurations
| 5
|
| Computational Methods
| 5
|
| Solar Activity
| 4
|
| Slow Solar Wind [H]
| 4
|
| Nonequilibrium Ionization
| 4
|
| Cooling
| 4
|
| Methods: Numerical
| 4
|
| Magnetohydrodynamical Simulations
| 4
|
| Sun: Atmosphere [S]
| 4
|
| Force-free Magnetic Fields
| 4
|
| Plasma Temperature
| 3
|
| Solar Coronal Streamers
| 3
|
| Sun: Particle Emission
| 3
|
| Star Clusters
| 3
|
| The Sun [S]
| 3
|
| Late Stars
| 3
|
| Solar Filament Eruptions
| 3
|
| Heao 2
| 3
|
| Magnetohydrodynamic Stability
| 3
|
| Solar Coronal Heating [S]
| 3
|
| Radiative Transfer [S]
| 3
|
| Photosphere [S]
| 3
|
| Gamma Rays [S]
| 3
|
| Stellar Flares
| 3
|
| Convolutional Neural Networks
| 3
|
| Cold Plasmas
| 2
|
| Hydrodynamics
| 2
|
| Carbon
| 2
|
| Mathematical Models
| 2
|
| Interplanetary Magnetic Fields [H]
| 2
|
| Interplanetary Physics: Ejecta
| 2
|
| Sun: Solar Wind [H]
| 2
|
| Iue
| 2
|
| And Astronomy: Corona
| 2
|
| Sun: Active Regions
| 2
|
| Astronomical Models
| 2
|
| And Magnetic Clouds
| 2
|
| Active Solar Corona
| 2
|
| Plasmas
| 2
|
| Ultraviolet Radiation
| 2
|
| Plasma Heating
| 2
|
| G Stars
| 2
|
| Plasma Density
| 2
|
| Physics - Space Physics [H]
| 2
|
| Space Plasmas [H]
| 2
|
| Gas Pressure
| 2
|
| Solar Transition Region
| 2
|
| Driver Gases
| 2
|
| Solar Coronal Loops [S]
| 2
|
| Current Sheets
| 2
|
| Corona [S]
| 2
|
| Radiant Cooling
| 2
|
| Magnetohydrodynamic Flow
| 2
|
| Radiative Heat Transfer
| 2
|
| Stars: Jets
| 2
|
| Far Ultraviolet Radiation
| 2
|
| Dwarf Stars
| 2
|
| Heat Flux
| 1
|
| H Alpha Line
| 1
|
| General Theory And Basic Studies Of Plasma Lifetime Particle And Heat Loss Energy Balance Field Structure Etc.
| 1
|
| Gamma Ray Bursts
| 1
|
| Flares Magnetic Reconnection
| 1
|
| Flare Stars
| 1
|
| Fine Structure
| 1
|
| Fast Solar Wind
| 1
|
| Exoplanet Atmospheric Structure
| 1
|
| Evaporative Cooling
| 1
|
| Euv Lines
| 1
|
| Equilibrium Equations
| 1
|
| Energy Transfer
| 1
|
| Energy Dissipation
| 1
|
| Emissivity
| 1
|
| Emission Spectra
| 1
|
| Electron Density (concentration)
| 1
|
| Electromagnetic Radiation
| 1
|
| Eigenvalues
| 1
|
| Doppler Effect
| 1
|
| Digital Simulation
| 1
|
| Cosmology
| 1
|
| Cooling Flows (astrophysics)
| 1
|
| Computerized Simulation
| 1
|
| CMEs
| 1
|
| Calibration
| 1
|
| Boundary Value Problems
| 1
|
| Boundaries
| 1
|
| Blackbody Radiation
| 1
|
| Binary Stars
| 1
|
| Atomic Processes
| 1
|
| Asymptotic Properties
| 1
|
| Asymptotes
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| And Astronomy: Magnetic Fields
| 1
|
| And Astronomy: Flares
| 1
|
| And Astronomy: Coronal Mass Ejections
| 1
|
| Aerospace Environments
| 1
|
| X-rays
| 1
|
| X Ray Spectra
| 1
|
| Videotapes
| 1
|
| UV
| 1
|
| Ultraviolet Spectra
| 1
|
| Ultraviolet Astronomy
| 1
|
| Thermal Stability
| 1
|
| Thermal Instability
| 1
|
| Synchrotron Radiation
| 1
|
| Sun: Waves
| 1
|
| Sun: Solar Temperature
| 1
|
| Sun: Solar Magnetic Field
| 1
|
| Sun: Solar Flares
| 1
|
| Sun: Solar Corona
| 1
|
| Sun: Proper Treatment
| 1
|
| Sun: Photosphere [S]
| 1
|
| Sun: Mesh Refinement
| 1
|
| Sun: Magnetic Reconnection
| 1
|
| Sun: Magnetic Field Configurations
| 1
|
| Sun: Flux Tube
| 1
|
| Sun: Field Line
| 1
|
| Sun: Evolution
| 1
|
| Stray Light
| 1
|
| Stellar Structure
| 1
|
| Stellar Spectrophotometry
| 1
|
| Stellar Radiation
| 1
|
| Stellar Mass Ejection
| 1
|
| Stellar Magnitude
| 1
|
| Stellar Activity
| 1
|
| Spatial Resolution
| 1
|
| Spaceborne Astronomy
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| Solar Temperature
| 1
|
| Solar Spectra
| 1
|
| Solar Radio Emission
| 1
|
| Solar Magnetic Bright Points
| 1
|
| Solar Flare Spectra
| 1
|
| Solar Energetic Particles (seps)
| 1
|
| Solar Energetic Particles [H]
| 1
|
| Solar Coronal Transients
| 1
|
| Solar Activity Effects
| 1
|
| Solar Active Region Magnetic Fields [S]
| 1
|
| Shocks
| 1
|
| Shear Flow
| 1
|
| Shear
| 1
|
| Red Shift
| 1
|
| Radiant Heating
| 1
|
| Quiet Solar Corona
| 1
|
| Polarity
| 1
|
| Pleiades Cluster
| 1
|
| Plasmas (physics)
| 1
|
| Plasma Radiation
| 1
|
| Plasma Layers
| 1
|
| Plasma Jets
| 1
|
| Plasma Dynamics
| 1
|
| Perturbation Theory
| 1
|
| Optical Design Techniques
| 1
|
| Open Source Software
| 1
|
| Numerical Analysis
| 1
|
| Neutron Stars
| 1
|
| Neutral Sheets
| 1
|
| Navier-stokes Equation
| 1
|
| Methods: Data Analysis
| 1
|
| Mass Transfer
| 1
|
| Mass Flow
| 1
|
| Magnetohydrodynamics And Plasmas
| 1
|
| Magnetohydrodynamic Waves
| 1
|
| Magnetohydrodynamic Turbulence
| 1
|
| Magnetohydrodynamic Shear Heating
| 1
|
| Magnetohydrodynamic And Fluid Equation
| 1
|
| Magnetic Flux
| 1
|
| Magnetic Field Reconnection
| 1
|
| Magnetic Energy Storage
| 1
|
| Lorentz Force
| 1
|
| Loops
| 1
|
| Line Spectra
| 1
|
| Kinetic Energy
| 1
|
| Kelvin-helmholtz Instability
| 1
|
| Jets
| 1
|
| Ionization
| 1
|
| Interplanetary Physics: Solar Wind Sources
| 1
|
| Interplanetary Physics: Interplanetary Magnetic Fields [H]
| 1
|
| Interplanetary Particle Acceleration [H]
| 1
|
| Icmes
| 1
|
| High Temperature
| 1
|
| Hertzsprung-russell Diagram
| 1
|
| Acceleration Of Particles
| 1
|
| Abundance
| 1
|