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: Filaments [S]
| 33
|
| Sun: Corona [S]
| 19
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 14
|
| Sun: Flares [S]
| 12
|
| Solar Physics [S]
| 10
|
| Sun: Magnetic Fields
| 7
|
| Sun: Uv Radiation [S]
| 6
|
| Sun: Transition Region [S]
| 5
|
| Sun: Oscillations [S]
| 5
|
| Very Large Array (vla)
| 4
|
| Sun: X-rays [S]
| 4
|
| Transition Region
| 3
|
| Sun: Radio Radiation [S]
| 3
|
| Sun: Activity
| 3
|
| Solar
| 3
|
| Astrophysics
| 3
|
| Gamma Rays [S]
| 3
|
| Doppler Shift
| 3
|
| Modelling
| 2
|
| Waves
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Sun: Coronal Mass Ejections
| 2
|
| Brightness Temperature
| 2
|
| Magnetohydrodynamical Simulations
| 2
|
| Sun: Chromosphere [S]
| 2
|
| Interplanetary Physics: Interplanetary Shocks
| 2
|
| Interplanetary Physics: Energetic Particles
| 2
|
| Sun: Abundances
| 2
|
| Radio Interferometers
| 2
|
| Hydrogen
| 2
|
| Radio Astronomy
| 2
|
| Radiative Transfer [S]
| 2
|
| Spectroscopy
| 2
|
| H Alpha Line
| 2
|
| Ultraviolet: Stars
| 2
|
| Sun: Prominences
| 2
|
| Flare
| 2
|
| Solar X-rays
| 2
|
| Techniques: Spectroscopic
| 2
|
| Solar Radio Emission
| 2
|
| Synchrotron Radiation
| 2
|
| Sun: Helioseismology [S]
| 2
|
| Solar Limb
| 2
|
| And Astronomy: Radio Emissions
| 2
|
| And Astronomy: Coronal Mass Ejections
| 2
|
| Physics - Space Physics [H]
| 1
|
| Physics
| 1
|
| Particle Acceleration
| 1
|
| Observational Diagnostics
| 1
|
| Numerical Analysis
| 1
|
| Non-thermal Radiation Sources
| 1
|
| Model Prediction
| 1
|
| Microwave Emission
| 1
|
| Microwave
| 1
|
| Methods: Statistical
| 1
|
| Main Phase
| 1
|
| Magnetohydrodynamics [S]
| 1
|
| Magnetohydrodynamic Waves
| 1
|
| Magnetic Field
| 1
|
| Line Shape
| 1
|
| Line Profile
| 1
|
| Imaging Spectrometers
| 1
|
| Imaging Data
| 1
|
| I.5.4
| 1
|
| I.4.6
| 1
|
| Hydrodynamical Simulations
| 1
|
| High Time
| 1
|
| High Temporal Resolution
| 1
|
| High Resolution
| 1
|
| Heat Input
| 1
|
| Absolute Intensity
| 1
|
| Gamma Ray Astronomy
| 1
|
| G.3
| 1
|
| Flux Tube
| 1
|
| Filling Factor
| 1
|
| Field Structure
| 1
|
| Field Line
| 1
|
| Emit Radiation
| 1
|
| Electron Density (concentration)
| 1
|
| Diagnostics
| 1
|
| Cyclotron Radiation
| 1
|
| Cme
| 1
|
| Circular Polarization
| 1
|
| Chromospheric Structure
| 1
|
| Charge Transfer
| 1
|
| Channel Structure
| 1
|
| Central Absorption
| 1
|
| Catalogs
| 1
|
| Bremsstrahlung
| 1
|
| Board Soho
| 1
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 1
|
| Astronomical Observatory
| 1
|
| Astronomical Observatories
| 1
|
| Very Long Base Interferometry
| 1
|
| Time Observation
| 1
|
| Three-dimensional
| 1
|
| Thermal Instability
| 1
|
| Temporal Resolution
| 1
|
| Sunspots [S]
| 1
|
| Sun:transition Region
| 1
|
| Sun: Radio
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: Infrared
| 1
|
| Sun: Euv
| 1
|
| Sun: Atmospheric Motions
| 1
|
| Sun: Active Region
| 1
|
| Stellar Models
| 1
|
| Stellar Mass Ejection
| 1
|
| Stars: Oscillations
| 1
|
| Spectral Resolution
| 1
|
| Spectral Line
| 1
|
| Specific Morphology
| 1
|
| Spatial Resolution
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| Solar Spectra
| 1
|
| Solar Radio Bursts
| 1
|
| Solar Magnetic Field
| 1
|
| Solar Flare Spectra
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Atmosphere
| 1
|
| Solar Active Region Filaments
| 1
|
| Similar Difference
| 1
|
| Resonant Condition
| 1
|
| Resonant Absorption
| 1
|
| Region Temperature
| 1
|
| Radio Spectra
| 1
|
| Radio Sources (astronomy)
| 1
|
| Radiative Transfer Simulations
| 1
|
| Radiative Processes
| 1
|
| Radiation Mechanisms: Cyclotron And Synchrotron
| 1
|
| Radiation
| 1
|
| Quiet Solar Corona
| 1
|
| Quiescent Solar Prominence
| 1
|
| Pulsed Radiation
| 1
|
| Prime Objective
| 1
|
| Plasma Radiation
| 1
|
| Alfven Waves
| 1
|
| Active Solar Corona
| 1
|
| Absorption Feature
| 1
|
| Good Explanation
| 1
|