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]
| 26
|
| SUN: OSCILLATIONS [S]
| 25
|
| Sun: Helioseismology [S]
| 23
|
| Chromosphere
| 22
|
| SUN: SUNSPOTS
| 21
|
| SUN: INTERIOR [S]
| 15
|
| Sun: Flares [S]
| 14
|
| Submillimeter Waves
| 12
|
| SUN: CHROMOSPHERE [S]
| 11
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 11
|
| Solar Atmosphere
| 11
|
| Radiative Transfer [S]
| 10
|
| SUN: ACTIVITY
| 9
|
| Solar Limb
| 9
|
| Flares
| 7
|
| Infrared Astronomy
| 7
|
| Sunspots [S]
| 7
|
| Far Infrared Radiation
| 7
|
| Solar Spectra
| 6
|
| Sun: Magnetic Fields
| 6
|
| Solar Granulation
| 5
|
| Astrophysics
| 5
|
| Infrared Spectra
| 5
|
| Solar Activity
| 5
|
| Magnetic Fields
| 4
|
| Limb Darkening
| 4
|
| SUN: LIMB DARKENING
| 4
|
| INFRARED: SPECTRA
| 4
|
| Brightness Temperature
| 4
|
| Infrared Radiation
| 4
|
| Power Spectra
| 4
|
| Solar Eclipses
| 4
|
| SUN: RADIO RADIATION [S]
| 4
|
| INFRARED: SOURCES
| 3
|
| Compression Waves
| 3
|
| Thermodynamic Equilibrium
| 3
|
| Sun: Corona [S]
| 3
|
| Solar Temperature
| 3
|
| Photosphere [S]
| 3
|
| Atmospheric Models
| 3
|
| Solar Active Regions [S]
| 3
|
| Limb Brightening
| 3
|
| Time Series Analysis
| 3
|
| Stellar Models
| 3
|
| Convection
| 3
|
| Solar Observatories
| 3
|
| WAVES
| 2
|
| Temperature Profiles
| 2
|
| Sunquakes
| 2
|
| Sun: Photosphere [S]
| 2
|
| Sun: Infrared
| 2
|
| Stellar Structure
| 2
|
| Stellar Spectrophotometry
| 2
|
| Spicules
| 2
|
| Space Weather
| 2
|
| Solar Radio Emission
| 2
|
| Solar Radiation
| 2
|
| Solar Phys
| 2
|
| Solar Magnetic Field
| 2
|
| Solar Flux Density
| 2
|
| Solar Dynamics Observatory
| 2
|
| Seismic Imaging
| 2
|
| Scale Height
| 2
|
| Particle Acceleration
| 2
|
| Luminous Intensity
| 2
|
| Line Spectra
| 2
|
| K Lines
| 2
|
| INFRARED: GENERAL
| 2
|
| Infrared Telescopes
| 2
|
| Infrared Sources (Astronomy)
| 2
|
| High Resolution
| 2
|
| Fine Structure
| 2
|
| Faculae
| 2
|
| Dynamics
| 2
|
| Corona [S]
| 2
|
| Continuous Radiation
| 2
|
| Computational Astrophysics
| 2
|
| Chromospheric Heating
| 2
|
| Brightness Distribution
| 2
|
| Brightness
| 2
|
| Astronomical Photometry
| 2
|
| Acoustic Emission
| 2
|
| Statistical Analysis
| 2
|
| 96.60.Na
| 1
|
| Average Power
| 1
|
| Saturn (Planet)
| 1
|
| Relaxation Time
| 1
|
| Recent Work
| 1
|
| Ramaty High Energy Solar Spectroscopic Imager
| 1
|
| Radio Telescopes
| 1
|
| Radio Spectra
| 1
|
| Radio Astronomy
| 1
|
| SUN: ECLIPSES
| 1
|
| Radiant Flux Density
| 1
|
| Radial Distribution
| 1
|
| Sun: Faculae [S]
| 1
|
| Planetary Surfaces
| 1
|
| Planetary Atmospheres
| 1
|
| Plages
| 1
|
| SUN: PLAGES
| 1
|
| Phase Deviation
| 1
|
| Periodic Variations
| 1
|
| Penumbrae
| 1
|
| Atmospheric Temperature
| 1
|
| P -Modes
| 1
|
| Oscillations:Solar Photosphere
| 1
|
| Oscillation Investigation
| 1
|
| Opposite Polarity
| 1
|
| Observations
| 1
|
| Michelson Doppler Imager
| 1
|
| Methods: Data Analysis
| 1
|
| Mercury (Planet)
| 1
|
| Mathematical Models
| 1
|
| Mars (Planet)
| 1
|
| Magnetohydrodynamic Waves
| 1
|
| Magnetic Structure
| 1
|
| Magnetic Region
| 1
|
| SUN: SPECTRA
| 1
|
| Magnetic Field Variation
| 1
|
| Venus (Planet)
| 1
|
| Atmospheric Heating
| 1
|
| LINE PROFILES
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| Sun: UV Radiation [S]
| 1
|
| Light (Visible Radiation)
| 1
|
| Atmospheric Composition
| 1
|
| Jupiter (Planet)
| 1
|
| Techniques: Interferometric
| 1
|
| Techniques: Polarimetric
| 1
|
| Atmosphere
| 1
|
| Very Large Array (Vla)
| 1
|
| Telescopes
| 1
|
| White-light Flares
| 1
|
| Temperature Gradients
| 1
|
| Infrared Detectors
| 1
|
| Temporal Distribution
| 1
|
| Impulsive Phase
| 1
|
| Imaging Techniques
| 1
|
| Hydrogen
| 1
|
| Holography
| 1
|
| ASTRONOMY
| 1
|
| Heliospheric Observatory
| 1
|
| Helioseismology Pulsations And Shock Waves
| 1
|
| Gas Mixtures
| 1
|
| Gas Ionization
| 1
|
| The Sun [S]
| 1
|
| Flare
| 1
|
| 96.60.qe
| 1
|
| Field Data
| 1
|
| Thermodynamics
| 1
|
| Astronomical Models
| 1
|
| Equations Of Motion
| 1
|
| Energy Dissipation
| 1
|
| Electron Density (Concentration)
| 1
|
| Electromagnetic Radiation
| 1
|
| Antipodes
| 1
|
| Dynamic Characteristics
| 1
|
| Doppler Effect
| 1
|
| Direction Finding
| 1
|
| Diagnostic Application
| 1
|
| Data Acquisition
| 1
|
| Airborne Equipment
| 1
|
| Convection Currents
| 1
|
| Type III Bursts
| 1
|
| Continuous Spectra
| 1
|
| Activity
| 1
|
| Active Region
| 1
|
| UV Radiation
| 1
|
| Compression Wave
| 1
|
| Acoustic Radiation
| 1
|
| Solar-terrestrial Relations
| 1
|
| Solar Wind [H]
| 1
|
| Space Infrared Telescope Facility
| 1
|
| Solar Surface
| 1
|
| Spectral Resolution
| 1
|
| Solar Rotation
| 1
|
| Velocity Distribution
| 1
|
| Solar Radio
| 1
|
| Carbon
| 1
|
| Spectrographs
| 1
|
| Calibrating
| 1
|
| Solar Photosphere: Infrared Observations
| 1
|
| STARS: ATMOSPHERES
| 1
|
| C-141 Aircraft
| 1
|
| 96.60.Ly
| 1
|
| Stellar Atmospheres
| 1
|
| Velocity Field
| 1
|
| Solar Eclipses: Sub-MM Radiation
| 1
|
| Stellar Luminosity
| 1
|
| Acoustic Field
| 1
|
| Solar Chromosphere: Sub-MM Radiation
| 1
|
| Stellar Radiation
| 1
|
| Subsurface Flow
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Solar Active Region Velocity Fields
| 1
|
| Shock Waves
| 1
|
| Seismic Source
| 1
|
| Seismic Image
| 1
|