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]
| 89
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 44
|
| Sun: Magnetic Fields
| 35
|
| Solar Physics [S]
| 27
|
| Sun: Flares [S]
| 24
|
| Sun: Uv Radiation [S]
| 22
|
| Magnetohydrodynamics [S]
| 20
|
| Gamma Rays [S]
| 12
|
| Sun: X-rays [S]
| 12
|
| Astrophysics
| 12
|
| Sun: Activity
| 11
|
| Sun: Transition Region [S]
| 10
|
| Solar Atmosphere
| 10
|
| Solar Magnetic Field
| 10
|
| Solar Coronal Heating [S]
| 10
|
| Sun: Chromosphere [S]
| 10
|
| Hydrodynamics
| 9
|
| Solar Coronal Loops [S]
| 8
|
| Sun: Prominences
| 7
|
| Solar Active Regions [S]
| 7
|
| Physics - Plasma Physics [H]
| 7
|
| Sun: Filaments [S]
| 6
|
| Solar Activity
| 6
|
| Sun: Atmosphere [S]
| 6
|
| Solar Extreme Ultraviolet Emission [S]
| 5
|
| Doppler Effect
| 5
|
| Sunspots [S]
| 5
|
| Photosphere [S]
| 5
|
| Coronal Loops
| 5
|
| Physics - Space Physics [H]
| 5
|
| Solar Magnetic Reconnection
| 4
|
| Hydromagnetics
| 4
|
| Solar Wind [H]
| 4
|
| Coronal Heating
| 4
|
| Force-free Magnetic Fields
| 4
|
| The Sun [S]
| 4
|
| Solar Spicules
| 4
|
| Ultraviolet Spectra
| 4
|
| Sun: Atmospheric Motions
| 3
|
| Transition Region
| 3
|
| Methods: Numerical
| 3
|
| Stellar Models
| 3
|
| Solar Spectra
| 3
|
| Waves
| 3
|
| Sun: Oscillations [S]
| 3
|
| Mathematical Models
| 3
|
| Techniques: Image Processing
| 3
|
| Computerized Simulation
| 3
|
| Techniques: Spectroscopic
| 3
|
| Methods: Data Analysis
| 3
|
| Thermal Stability
| 3
|
| Solar Transition Region
| 3
|
| Velocity Distribution
| 3
|
| Magnetic Fields
| 3
|
| Magnetic Field Configurations
| 3
|
| Chromosphere
| 3
|
| Turbulence
| 2
|
| Sun: Radio Radiation [S]
| 2
|
| Sun: Photosphere [S]
| 2
|
| Sun: Particle Emission
| 2
|
| Sun: General
| 2
|
| Sun: Fundamental Parameters
| 2
|
| Stars: Coronae
| 2
|
| Spectrum Analysis
| 2
|
| Solar Temperature
| 2
|
| Shear
| 2
|
| Red Shift
| 2
|
| Methods: Observational
| 2
|
| Magnetohydrodynamic Flow
| 2
|
| Magnetic Signatures
| 2
|
| Magnetic Flux
| 2
|
| Magnetic Field
| 2
|
| Line Spectra
| 2
|
| Kinetic Energy
| 2
|
| H Alpha Line
| 2
|
| Emission Spectra
| 2
|
| Coronal Holes
| 2
|
| Corona [S]
| 2
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 2
|
| Astronomy Data Modeling
| 2
|
| Astronomical Models
| 2
|
| Solar Electromagnetic Emission
| 2
|
| Solar Coronal Loops:numerical Simulations
| 1
|
| Space Plasmas [H]
| 1
|
| Solar Coronal Lines
| 1
|
| Spatial Structure
| 1
|
| Solar Corona: Heating
| 1
|
| Solar Chromosphere:solar Coronal Loops
| 1
|
| Spectral Line
| 1
|
| Spicules
| 1
|
| Solar Active Regions:solar Filaments
| 1
|
| Statistics And Probability
| 1
|
| Soho Mission
| 1
|
| Silicon
| 1
|
| Signatures
| 1
|
| Shocks
| 1
|
| Shear Flow
| 1
|
| Asymptotes
| 1
|
| Seeing (astronomy)
| 1
|
| Rocket-borne Instruments
| 1
|
| Rocket Sounding
| 1
|
| Resonance Lines
| 1
|
| Regions
| 1
|
| X-ray And Gamma-ray Emission
| 1
|
| Radiant Heating
| 1
|
| Radial Velocity
| 1
|
| Quiet Sun
| 1
|
| Quiet Solar Corona
| 1
|
| Post-flare Loops
| 1
|
| Polarized Radiation
| 1
|
| Polarization
| 1
|
| Polarity
| 1
|
| Polar Regions
| 1
|
| Plasmas
| 1
|
| Plasma Heating
| 1
|
| Stellar Coronae
| 1
|
| Stellar Mass Ejection
| 1
|
| Physics - Data Analysis
| 1
|
| Stellar Temperature
| 1
|
| Perturbation
| 1
|
| Oxygen Spectra
| 1
|
| Observational Astronomy
| 1
|
| Observation
| 1
|
| Numerical Analysis
| 1
|
| Nonlinear Systems
| 1
|
| Non-thermal Radiation Sources
| 1
|
| Momentum Transfer
| 1
|
| Microwave Spectroscopy
| 1
|
| Acceleration Of Particles
| 1
|
| Sun: Abundances
| 1
|
| Sun: Coronal Mass Ejections
| 1
|
| Mathematical Physics
| 1
|
| Sun: Magnetic Topology
| 1
|
| Mass Transfer
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetohydrodynamic Waves
| 1
|
| Magnetohydrodynamic Stability
| 1
|
| X-ray Bright Point
| 1
|
| Magnetoacoustic Wave
| 1
|
| Magnetic Structure
| 1
|
| Astronomy Image Processing
| 1
|
| Magnetic Reconnection
| 1
|
| 96.60.tk
| 1
|
| Sun: Sunspots
| 1
|
| Symmetry
| 1
|
| 96.60.qe
| 1
|
| Lorentz Force
| 1
|
| Loop Length
| 1
|
| And Astronomy: Ultraviolet Emissions
| 1
|
| Line Of Sight
| 1
|
| And Astronomy: Transition Region
| 1
|
| Interesting Property
| 1
|
| Intensity And Diagnostics
| 1
|
| Instrumental Effects
| 1
|
| Important Implication
| 1
|
| Temperature Distribution
| 1
|
| Three Dimensional Models
| 1
|
| Heat Transfer
| 1
|
| And Astronomy: Corona
| 1
|
| Gas Pressure
| 1
|
| Time Dependence
| 1
|
| Ultraviolet Spectrometers
| 1
|
| Flow Distribution
| 1
|
| Flares
| 1
|
| Fine Structure
| 1
|
| Field Strength
| 1
|
| Field Line
| 1
|
| Extreme Ultraviolet Radiation
| 1
|
| Euv Emission
| 1
|
| Energy Transfer
| 1
|
| And Astronomy: Chromosphere
| 1
|
| Early Analysis
| 1
|
| Doppler Velocities:solar Filaments
| 1
|
| Ultraviolet: Spectra
| 1
|
| Digital Simulation
| 1
|
| Diffusion
| 1
|
| Critical Flaw
| 1
|
| Cosmology
| 1
|
| Coronal Loops Streamers
| 1
|
| Velocity Field
| 1
|
| Coronal Loop
| 1
|
| Active Region
| 1
|
| Vertical Distribution
| 1
|
| Active
| 1
|
| Cooling
| 1
|
| Convection
| 1
|
| Conduction
| 1
|
| Virial Theorem
| 1
|
| Computer Programs
| 1
|
| Viscosity
| 1
|
| Boundary Value Problems
| 1
|
| Atmospheric Circulation
| 1
|
| Solar Prominences:numerical Simulations
| 1
|
| Solar Prominences:formation
| 1
|
| Solar Probe Plus
| 1
|
| Solar Spectrometers
| 1
|
| Solar Observatories
| 1
|
| Solar Maximum Mission
| 1
|
| Solar Wind Velocity
| 1
|
| Solar X-ray Emission
| 1
|
| Solar Limb
| 1
|
| Solar Gravitation
| 1
|
| Solar Filaments:solar Active Regions
| 1
|
| Solar Filaments:doppler Velocities
| 1
|
| Sound Waves
| 1
|
| 96.60.pf
| 1
|
| Solar Coronal Loops:thermal Stability
| 1
|
| Solar Coronal Loops:solar Chromosphere
| 1
|
| Solar Coronal Loops:models
| 1
|