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]
| 12
|
| Sun: UV Radiation [S]
| 11
|
| Sun: Flares [S]
| 9
|
| Sun: Transition Region [S]
| 8
|
| Sun: Atmosphere [S]
| 8
|
| Sun: X-rays [S]
| 4
|
| Sun: Activity
| 4
|
| Magnetic Fields
| 4
|
| Sun: Abundances
| 4
|
| Instrumentation: Spectrographs
| 4
|
| Solar Physics [S]
| 4
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 4
|
| Techniques: Spectroscopic
| 3
|
| Sun: Magnetic Fields
| 3
|
| X Ray Spectra
| 3
|
| Techniques: Imaging Spectroscopy
| 3
|
| Calcium
| 3
|
| Sun: Coronal Mass Ejections
| 2
|
| Plasma Turbulence
| 2
|
| Space Vehicles: Instruments
| 2
|
| High Temperature Plasmas
| 2
|
| Solar Wind [H]
| 2
|
| Sun: Chromosphere [S]
| 2
|
| Esa Cosmic Vision
| 2
|
| Atomic Data
| 2
|
| Solar Maximum Mission
| 2
|
| Corona [S]
| 2
|
| Methods: Observational
| 2
|
| Magnetic Reconnection
| 2
|
| Sun: Filaments [S]
| 2
|
| Line: Profiles
| 2
|
| Sun: Solar Wind [H]
| 2
|
| Particle Acceleration
| 2
|
| Sun: Emission Spectra
| 1
|
| Sun: Electron Energy
| 1
|
| Sun: Diurnal Variations
| 1
|
| Sun: Crystal Optics
| 1
|
| Sun: Conjugate Gradient Method
| 1
|
| Sun: Calcium
| 1
|
| Sun: Bragg Angle
| 1
|
| Sun: Backscattering
| 1
|
| Sun: Active Regions
| 1
|
| Sun:
| 1
|
| Spectral Energy Distribution
| 1
|
| Solar Spectra
| 1
|
| Solar Limb
| 1
|
| Solar Flare Prediction
| 1
|
| Slow Solar Wind [H]
| 1
|
| Sharp Parameters
| 1
|
| Polarity Inversion Line
| 1
|
| Plasma Diagnostics
| 1
|
| Methods: Numerical
| 1
|
| Metallicity
| 1
|
| Magnetohydrodynamics [S]
| 1
|
| Magnetohydrodynamic Turbulence
| 1
|
| Magnetohydrodynamic Stability
| 1
|
| Machine Learning
| 1
|
| Iron
| 1
|
| Instrumentation
| 1
|
| Imaging Spectrometers
| 1
|
| Hydrodynamics
| 1
|
| Gamma Rays [S]
| 1
|
| Flares
| 1
|
| Electron Beams
| 1
|
| Cosmic Rays
| 1
|
| Coronal Loops
| 1
|
| Bessel Photometry
| 1
|
| Atomic Spectroscopy
| 1
|
| X Ray Imagery
| 1
|
| Waves
| 1
|
| Time Series Model
| 1
|
| Techniques: Spectroscopy
| 1
|
| Techniques: Polarimetic
| 1
|
| Techniques: High Angular Resolution
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| Sun: Sun
| 1
|
| Sun: Sulfur
| 1
|
| Sun: Spectrum Analysis
| 1
|
| Sun: Solar X-rays
| 1
|
| Sun: Solar Temperature
| 1
|
| Sun: Solar Spectrometers
| 1
|
| Sun: Solar Spectra
| 1
|
| Sun: Solar Physics
| 1
|
| Sun: Solar Flares
| 1
|
| Sun: Solar Atmosphere
| 1
|
| Active Sun
| 1
|
| Sun: Run Time (computers)
| 1
|
| Sun: Resonance Lines
| 1
|
| Sun: Radio Astronomy
| 1
|
| Sun: Radar Measurement
| 1
|
| Sun: Polar Regions
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: Maximum Entropy Method
| 1
|
| Sun: Line Spectra
| 1
|
| Sun: Japanese Space Program
| 1
|
| Sun: Iron
| 1
|
| Sun: Ionospheric Propagation
| 1
|
| Sun: High Temperature Plasmas
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Gravity Waves
| 1
|
| Sun: Extreme UV Spectroscopy
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Sun: Solar Activity
| 1
|