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
|
|---|
| Solar Physics [S]
| 13
|
| Sun: Flares [S]
| 13
|
| Sun: Corona [S]
| 13
|
| Sun: Uv Radiation [S]
| 11
|
| Sun: Transition Region [S]
| 8
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 8
|
| Sun: Atmosphere [S]
| 8
|
| Solar Maximum Mission
| 5
|
| X Ray Spectra
| 5
|
| Solar X-rays
| 5
|
| Iron
| 4
|
| Calcium
| 4
|
| Sun: Activity
| 4
|
| Magnetic Fields
| 4
|
| Sun: Abundances
| 3
|
| High Temperature Plasmas
| 3
|
| Techniques: Spectroscopic
| 3
|
| Sun: Magnetic Fields
| 3
|
| Flare
| 3
|
| Physics - Space Physics [H]
| 3
|
| Emission Spectra
| 3
|
| Solar Wind [H]
| 3
|
| Solar Spectra
| 3
|
| Line Spectra
| 3
|
| Instrumentation: Spectrographs
| 3
|
| Sun: X-rays [S]
| 2
|
| Sun: Filaments [S]
| 2
|
| Solar Activity
| 2
|
| Techniques: Imaging Spectroscopy
| 2
|
| Plasma Turbulence
| 2
|
| Magnetic Reconnection
| 2
|
| Gamma Rays [S]
| 2
|
| Germanium
| 2
|
| Coronal Loops
| 2
|
| Corona [S]
| 2
|
| Atomic Data
| 2
|
| Light Curve
| 2
|
| X Ray Imagery
| 2
|
| Chromosphere
| 2
|
| Temperature Dependence
| 2
|
| Sun: Chromosphere [S]
| 2
|
| Esa Cosmic Vision
| 2
|
| Particle Acceleration
| 2
|
| Methods: Observational
| 2
|
| Sulfur
| 2
|
| Space Vehicles: Instruments
| 2
|
| Plasma Diagnostics
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Methods: Numerical
| 1
|
| Metallicity
| 1
|
| Maximum Entropy Method
| 1
|
| Magnetohydrodynamics [S]
| 1
|
| Magnetohydrodynamic Turbulence
| 1
|
| Magnetohydrodynamic Stability
| 1
|
| Line: Profiles
| 1
|
| Labrador
| 1
|
| Kernel Functions
| 1
|
| Japanese Space Program
| 1
|
| Ionospheric Propagation
| 1
|
| Instrumentation
| 1
|
| Impulsive Phase
| 1
|
| Imaging Spectrometers
| 1
|
| Hydrodynamics
| 1
|
| High Activity
| 1
|
| Gravity Waves
| 1
|
| Gradual Phase
| 1
|
| Good Sensitivity
| 1
|
| Geophysics
| 1
|
| Gamma-rays
| 1
|
| Frequency Distribution
| 1
|
| Flares
| 1
|
| Extreme Uv Spectroscopy
| 1
|
| Extreme Ultraviolet
| 1
|
| Entropy
| 1
|
| Energy Content
| 1
|
| Emissivity
| 1
|
| Electron Energy
| 1
|
| Electron Beams
| 1
|
| Diurnal Variations
| 1
|
| Detailed Calculation
| 1
|
| Decay Phase
| 1
|
| Data Processing
| 1
|
| Crystal Optics
| 1
|
| Cosmic Rays
| 1
|
| Coronal Mass Ejections (cmes)
| 1
|
| Conjugate Gradient Method
| 1
|
| Conjugate Gradient
| 1
|
| Conductive Heat Transfer
| 1
|
| Bragg Angle
| 1
|
| Bessel Photometry
| 1
|
| Backscattering
| 1
|
| Atomic Spectroscopy
| 1
|
| Abundance
| 1
|
| X Ray Telescopes
| 1
|
| X Ray Sources
| 1
|
| X Ray Astronomy
| 1
|
| Waves
| 1
|
| Wavelengths
| 1
|
| Wavelength Range
| 1
|
| Wave Propagation
| 1
|
| Time Resolution
| 1
|
| Thermal Energy
| 1
|
| Thermal Emission
| 1
|
| The Sun [S]
| 1
|
| Temperature Interval
| 1
|
| Temperature Distribution
| 1
|
| Techniques: Spectroscopy
| 1
|
| Techniques: Polarimetic
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Coronal Mass Ejections
| 1
|
| Sun:
| 1
|
| Sulphur
| 1
|
| Stellar Models
| 1
|
| Spectrum Analysis
| 1
|
| Spectrometers
| 1
|
| Spectral Energy Distribution
| 1
|
| Spacecraft Instrumentation
| 1
|
| Space Missions
| 1
|
| Solar Temperature
| 1
|
| Solar Spectrometers
| 1
|
| Solar Radio Bursts
| 1
|
| Solar Phys
| 1
|
| Solar Maximum
| 1
|
| Solar Limb
| 1
|
| Solar Atmosphere
| 1
|
| Solar Active Regions [S]
| 1
|
| Slow Solar Wind [H]
| 1
|
| Satellite-borne Instruments
| 1
|
| Run Time (computers)
| 1
|
| Resonance Lines
| 1
|
| Radio Telescopes
| 1
|
| Radio Astronomy
| 1
|
| Radar Measurement
| 1
|
| Polar Regions
| 1
|
| Plasma Heating
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Activity Phase
| 1
|
| Active Sun
| 1
|
| Active Region
| 1
|
| X-rays
| 1
|